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A S CAD E S T MO S P HERI C E SO URCE S RO G RAM Prepared for U.S. DEPARTMENT OF THE INTERIOR BUREAU OF RECLAMATION DIVISION OF ATMOSPHERIC WATER RESOURCES MANAGEMENT DENVER, COLORADO UNDER CONTRACT NO. 14-06-D-6999 STATE OF WASHINGTON DANIEL J. EVANS GOVERNOR DEPARTMENT OF ECOLOGY JOHN A. BIGGS DIRECTOR INTERIM REPORT JANUARY TO JUNE 30, 1972

Transcript of SO ROG - carg.atmos.washington.edu

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ASCADESTMOSPHERIC

ESOURCESROGRAM

Prepared forU.S. DEPARTMENT OF THE INTERIOR

BUREAU OF RECLAMATIONDIVISION OF ATMOSPHERIC WATER RESOURCES MANAGEMENT

DENVER, COLORADOUNDER CONTRACT NO. 14-06-D-6999

STATE OF WASHINGTONDANIEL J. EVANS

GOVERNOR

DEPARTMENT OF ECOLOGYJOHN A. BIGGS

DIRECTOR

INTERIM REPORTJANUARY TO JUNE 30, 1972

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STATE OF WASHINGTON

DUPAI^TMEOT @F IS(C)@1L@(C)YDANIEL J. EVANS JOHN A. BIGGS

GOVERNOR DIRECTOR335 GENERAL ADMINISTRATION BUILDING OLYMPIA 98501

August 10 19 72

Dr. Archie M. Kahan ChiefDivision of Atmospheric Water

Resources ManagementBureau of ReclamationBuilding 6 7 Denver Federal CenterDenver Colorado 802 25

Attention D-1200

Dear Dr. Kahan

According to the provisions of the U. S Bureau ofReclamation Contract No. 14-06-D-6999 dated 1 July 19 70Subparagraph 7b we are herewith forwarding five copies ofan Interim Progress Report This report covers researchefforts on the Cascades Atmospheric Water Resources Programduring the period 1 January to 30 June 1972

Sincerely

Office of Technical Services

<^.S-^- o^--^" ^’. -"^,^L^^ -yStuart E Shumway MeteorologistTechnical Assistance Division

SES ss

Enclosures ( 5 )

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Section 1

Activity for the Report Period in Each of the Topics

Stated in the Work Plan

January 1 to June 30, 1972

Task #1: Aircraft Research Instrumentation

This task’s projected goals were largely met in the previous

report period. During the present period the storage monitor scope for the

5 cm weather radar was installed in the rear of the aircraft near the flight

scientist’s transparent observation dome. The experimental telemetry

system continues to be postponed due to budgetary limitations and licensing

difficulties.

Considerable progress has been made in other areas of aircraft

improvement which were not specifically listed under this task. For example:

(1) The Mee Industries ice nucleus counter which was intermittent

at best during the last report period was substantially

improved by a series of minor modifications. While considerable

doubt still remains concerning the reliability of the actual

numerical values of the counts recorded, the mechanical

reliability is much improved. Studies continue into the

reasons for the large variations in count which can be obtained

with preconditioning adjustments.

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(2) To augment the Mee ice nucleus measurements millipore

filters can now be exposed from the aircraft during a flight.

The filters are developed in the laboratory using a modification

of the Bigg-Stevenson technique.

(3) The radar altimeter, which was previously somewhat intermittent,

has been greatly improved since we acquired complete test

and calibration sets. It now operates reliably up to 10,000

feet above terrain.

(4) The airborne wind speed and direction sensor is nearing the

airborne test stage. During this report period "bread-board"

versions have been flown and aircraft ground speed and drift

have been calculated. The further electronic calculation of

wind speed and direction is not expected to provide any great

difficulties although considerable testing is anticipated

before the unit’ is fully operational.

We expect this device to improve our targeting and

evaluation of seeding effects since the winds at flight level

will be monitored in real time. In addition, the ability to

obtain wind speed and direction over a wide area and in the

vertical anywhere the DME-VOR signals can be received will

add a valuable dimension to the aircraft’s capability.

(5) The aerosol conditioning chamber has been substantially

enlarged and improved and the sample inlet has been modified

to provide both deicing and isokinetic sampling. However,

the large heated venturi, which is also necessary for

isokinetic sampling, remains to be installed.

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The B-23 aircraft continued to operate faultlessly throughout

the remainder of the 1971-72 winter field program.

Tasks #2 and #7: Operation and Maintenance of the Ground Stations

The network of manned and automatic ground meteorological stations

remained as described in the previous report. Operational reliability was

very good throughout the winter largely due to the careful preparation and

calibration of the instruments during the previous summer together with a

regular program of service in the field.

Task #4: Rawinsonde Measurements

The rawinsonde tracker (on loan from NCAR) and launch facility

at Greenwater, Washington, operated satisfactorily during this report

period. As before, the BuRec small computer terminal was an important link

in the rapid analysis of the rawinsonde raw data.

Tasks #3 and #8: Radar Development and Operations

Introduction

The mission of the radar portion of the Cascade Project is

(1) To obtain remote measurements of precipitation, its intensity and fall

velocity spectra and to relate these measurements to the physical structure of

the cloud systems and (2) To study "control conditions" and compare them

with the seeded situations in order to define adequately the effects of

seeding on hydrometeor size^and trajectories in a storm system. In pursuit of

these goals a low power pulse Doppler radar system with a single range gate

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was interfaced -to an incoherent radar (a T-9) so that a common receiving

antenna and receiver hardware could be used.

System Operation

Pulse Doppler operation began early in January after the development

of solid state pulse control features. These were interfaced to the

incoherent radar synchronizer. Tests showed that the peak power of 20 watts

developed by the traveling wave tube was not sufficient to fire the transmit-

receiver switch in the T-9 therefore, operation of two antennas was necessary.

A 6-foot parabolic dish was installed on the ground approximately 3 meters from

the incoherent radar and was equipped with a heater for snow removal. This

arrangement proved satisfactory and was used the remainder of the winter

season. Both radar systems the high power incoherent and the low power pulse

Doppler, could be operated simultaneously when the pulse repetition rate was

harmonically related.

Data Processing

One of the most important developments during the period was the

evolution of the data processing system. Early observation of spectra from

CW and pulse Doppler returns showed the variability of the raw spectra of

the fall-velocities of the hydrometeors. The spectra had a phase flicker with

a time constant around 16 ms due to the shuffling of the scatterers in and out

of the beam. Slower variations due to meteorlogical changes were observed

over a period of minutes. The problem of reducing this type of data is a

critical one because internal variables must be found that are independent of

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the randomness of the signal. In order to do this some specialized electronics

were developed that could be used with available pieces of equipment to put

the raw spectra on digital tape. Once the link with the large digital

CDC-6400 computer had been established the raw spectra could be averaged and

processed using standard Fortran programs. This provided a great advance

in both the reduction and interpretation of the data.

Video Processing

Early video processing with CW used a Burr Brown instrumentation

amplifier and fourth order active filter’s. With the advent of pulse Doppler

work in early January the system was found inadequate to accept the wide band

signals of pulse operation and a redesign proved necessary. Later, with the

use of higher power and a reduced pulse repetition rate, simple video amplification

and filtering was too insensitive and a further modification was installed. This

is a "box car" type of detector adapted from the AFCRL "Porcupine" radar

circuits which were kindly supplied by Dr. Ken Hardy. The use of the pulse

integration scheme enormously increases the detector sensitivity.

Installation of the High Power Klystron

With suitable modification of wave guide plumbing, cooling and

mounting hardware a V-82, 7 kW pulse klystron has been adapted to replace the

magnetron of the incoherent radar. Modification of the support electronics

resulted in a simplification of peripheral equipment and gives more reliable

operation.

Future Plans

The next major improvement in the radar operation will be the

installation of the digital data recording system in the radar van. This will

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allow instantaneous observations of spectra and eliminate the re-recording

step. Furthermore data reduction will be greatly improved as the digital

tape can be brought from the radar site to the University computer center

and reduced within 24 hours or less of the data acquisition. This type of

operation would greatly improve the "feed back" between measurement and

interpretation.

Task #5: Theoretical Models

We are continuing to use two rather different computer models as a

guide to both field operations and the analysis of the measurements. The

more detailed model, which attempts to model both the airflow and microphysics

over the Cascades, has been described in a recent report to the Bureau (see

"A Theoretical Model for Orographic Precipitation and its Modification by

Artificial Seeding with Ice Nuclei" by A. B. Fraser, P. V. Hobbs and R. C.

Easter, April 1972). Since this report was written most of the developments

have centered on the microphysics portion of the model, although some efforts

are being directed toward the inclusion of the capability to handle a layer of

air with neutral stability.

The most recent improvement to the cloud microphysics part of the

model has been the addition of the aggregation process to the crystal growth

equations. Previously, only growth by riming and by diffusion from the vapor

phase had been considered in the model, but observational evidence shows

aggregation to be a common occurrence in winter storms over the Cascades. The

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model now computes the percentages of crystal mass due to riming and

aggregation to provide information on the relative importance of these

two growth mechanisms and to classify the crystal for determination of its

fall speed. A fourth-order Runge-Kutta scheme has been employed to solve the

growth equations. The debugging of the new computer program has just been

completed so that new results will soon be available.

While our goal is to use our field measurements as input data in

our sophisticated airflow and microphysics model in order to obtain outputs of

the effects of seeding of precipitation in real-time, most of the operational

targeting and decision making during this report period made use of our simpler

operational model.

The operational model, in its present form, uses rawinsonde data and

surface observations of snow crystal type to construct backward trajectories

of rimed and unrimed snow crystals. The model is based upon experimental

observations which indicate that specific crystal types (e.g. dendrites

needles etc. ) grow only in particular temperature regimes. Thus if, for

example, a dendrite is sampled at the surface, the observer can be quite

confident that the crystal grew from the vapor phase at temperatures between

-12 and -17C. The operational model assumes that any additional increase in

the mass of the crystal below the -12C isotherm is due solely to riming.

Diffusive growth of the ice crystals is not considered in the computations.

The computer program simply identifies the level where diffusive growth is

assumed to stop and then calculates trajectories from the surface to that

height. Thus only a segment of the entire trajectory is actually calculated.

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SELECT TARGET

oescftveo CWSTALTYPC AT

SJKfACC STATIONS

SURFACE WINDVELOCITY AT

TAWCT

SOUNOWeDATAP.T.V

CONPUTCR

CirrSTAL TKAJCCTORYfttON WOWTM WE610NfOK ^ARTCULAOWTAt MWTO SUfff’ACC

TIMI^HATUHl WHCW:XCONC A^NT

tyrccnyc

MNtMUM ALLWA8LCAtTITUOC Or AlftCNAFT

fLIWT PATN

AN:tCCT $eCON POSITIONAS CLOSI TO TAROCT AS

POSSIBLE

iHADIO COOWNATCS

TO AIUCKAFT

Fig. 1 Chart showing input and output data for the Cascade Operational Model

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Fall velocities of the ice crystals are assumed to be constant

if the crystals are unrimed. If riming is occurring, the fall velocities

of the rimed crystals are assumed to increase linearly from the unrimed

value at the base of diffusive growth region to twice the unrimed fall speed

at the surface. Effects of topography are ignored in the computations and

ice crystals are assumed to be displaced horizontally by the wind.

The size of the observed surface crystals is implicitly incorp.orated

into the calculations. Estimates of reasonable minimum and maximum fall

velocities have been associated with each crystal type in an attempt to

bracket all likely fall velocities. Trajectories are calculated based upon

each of these extreme fall velocities and it is assumed that the trajectories

of the observed crystals will be bracketed by these computed extreme paths.

On a typical operational day, raw rawinsonde data, surface observations

of crystal type, and surface wind direction at the target is fed into the

computer. Data output includes coordinates of trajectory paths for rimed and

unrimed snow crystals the height of the trajectory at each coordinate, and

fall time from the coordinate height to the surface. The selection of a seeding

position is based upon the temperature where the seeding agent is effective and

nearness to the target. Generally about 40 minutes is required to receive the

raw rawinsonde data by telephone, punch the data on paper tape, compute the

trajectories and radio the seeding coordinates to the waiting aircraft.

The flow of information for the operational model is shown as a

flow chart in Fig. 1. The program, as executed on the CSS computer, and its

internal flow diagram is given in Appendix A. It should be noted that the

programing of both input and output is done in such a straight forward manner

that the program can be run by non-scientific staff.

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Task #6: Aircraft Flight Operations

During this report period the aircraft flew in 14 storm situations.

In addition 8 were made when full operational support was not available but

either airborne observations were made or instruments tested. A complete list

of flights made from January 1 June 30, 1972 under this contract is contained

in Appendix C.

Tasks #9 and #10: Contingency Seeding Program

During this report period the airborne seeding program remained

fully operational and the contingency programs were not activated.

Task #11: Preliminary Data Analysis

Only slight improvements were made in reducing the time required to

analyze in detail the data collected in the field. Substantially more raw data

is still produced each storm day than can be reduced in the interval between

storms. However, many of the operational and decision making advantages of rapid

data analysis were achieved on the basis of an improved priority indexing scheme.

In this scheme a list of storm periods was compiled and given a priority score on

the basis of their importance to the project. This list was updated throughout

the winter and enabled the group to stay abreast of the "important" storm days.

The only means of further closing this gap seems to be direct linkage

of the field equipment to the computer which is not feasible within the present

budget. Some limited air-to-ground and ground-to-ground telemetry is still

planned as an operational aid.

The small computer reduction system for the aircraft data that was

worked out during the winter was in operation by the close of our storm

modification period. This system, which can convert up to 30 channels of

analog tape data into digital format, makes the necessary arithmetic

adjustments to engineering units. Table 1 shows a segment of the data

obtained from an operational flight in Texas on June 7, 1971. The data is

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10

being time averaged and printed every minute. The format has proven very

useful in studying parameters that have a long time constant and it has

greatly speeded their reduction and analysis. Illustrating this format

the first line of data in Table 1 is translated as follows:

2_3 The time is 17:23

3ft 1.74E -1 The liquid water content is 0.174 gm/m

6. 79E 2 The static pressure is 679 nib

-2.67E 00 The dew point is -2.67C

7.12E 00 The total temperature is 7.12C

2/32. 39E 00 The turbulence index is 2. 39e

6. 88E 00 The static temperature is 6. 88C

7.6 8E 1 The true airspeed is 76. 8 m/sec

4.00E 1 The cloud condensation nuclei concentration is 40cc

6.01E -1 The atmospheric aerosol scattering coefficient. During

this period the device was out of calibration.

Task #12:______Data Analysis and Interpretation

At the present time analysis and interpretation of the 1971-72 winter’s

research is still in progress. It is expected that the presentation format

will follow that of Research Report VI (Hobbs et al. 1971). Consequently, the

present section of the report consists of a progress report with some analysis

of completed work plus illustrative examples of events and techniques not

previously fully reported.

ftSpread between dewpoint and temperature suggests as does the analog record

that this value is a zero offset. The aircraft was not in cloud at this time.

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TABLE 1

Lrt- ^’c-AT DF:W ’-’’" T TURfi ;S A-1 ^T ST-AT/^TAS CCN b

SCAT

23 1 74E23 7. 68E84 2.28E64 7.05E25 2. 14E85 7. 50E 126 1 .43E26 7.08K27 .0SIS7 6. 53EW .08E28 6. 56E29 1 .28E29 7.08E30 1 31 E30 7.06E31 1 .42E31 7. 6E 132 1 1HE32 6.41 E33 1 1 1 E33 6.31E34 .09E34 6. 40E35 1 .24E35 6. 57E36 .29E36 6. 76E37 74E37 6.85E38 1 78E38 7. 38E39 1 65E39 7. 72E40 67E40 7. 38E41 2.36E41 7. 35E42 2.32E42 7.28E43 3. 51 E43 7.42E44 3. 41 E -144 7.91 E45 3. 73E45 8. 51 E46 .97E46 8. 60E47 70E47 8. 14E

6. 79E 2 -2. 67E 00 7. 2E 00

4.00E 1 6.0 1E6. 67E 2 4.25E 00 8.40E 003.99E 1 5.83E 16. 78E 2 4.97E 00 9. 44E 003.94E 1 5. 65E -16. 73E 2 -8. 77E 00 9.90E 003.90E 1 5. 58E -l6. 73E 2 -2.47E 00 9.43E 003.88E 1 5. 52E6. 73E 2 9.48E -8 9.2 E 003.85E 1 5.49E -16.81E 2 2. 18E 00 1 .01E3. 78E 1 5. 47E -16.82E 2 -2.05E 00 10E3. 72E 1 5. 46E6.83E 2 -4.05E 00 2E3. 68E 1 5. 43E6. 77E 2 -4. 33E 00 .0 E3. 68E 5. 41 E6. 77E 2 76F 00 9 40E 003. 56E 5.40E

6. 72E 2 4. 4RE 9.07E 00

3. 50E 5. 39E6. 69E 2 -4. 27E 00 9. 32E 003.46E 1 5. 37E -16. 69E 2 27E 00 9. 29E 003.40E 5. 35E -16. 68E 8 31 E 00 9. 29E 003. 37E l 5. 35E6. 68E 2 30E 00 9.42E 003. 33E 5. 34E -16. 73E 2 2.84E 00 .02E3.28E 1 5. 30E -16. 69E 8 4.0 E 00 9. 65E 003.26K 5. 24E -16. 67E 2 3. 66E 00 9. 7E 003.26E l 5. 9E -l6. 61E 2 3. ME 00 H .05E 00

3.27E 5. 10E6.49E 2 3 64E 00 7. 22E 003.27E 5.0^lE -16. 47E 2 3. 60E 00 7. 6E 003. 25E 4.9RE6. 55E 2 3. 29E 00 R. 61 E 003.23E 4.91 E6. 67E 2 3. 40E 00 9. 90E 00

3.21 E 4.90E6.83E 8 4. 92E 00 3E3. 1 8E 4.92E -1

2. 39E 00 6.88E 00

2. 30E 00 7.81 E 00

2. 32E 00 8. 38E 00

2.28E 00 9. 74E 00

1 57E 00 1 .05E

1 73E 00 9. 1 7E 00

.99E 00 9. 36E 00

2.00E 00 1 .02E

1 .05E 00 .04E

68E 00 9.83E 00

1 .97E 00 9.03E 00

41 E 00 8. 71 E 00

30E 00 8. 77E 00

40E 00 8. 69E 00

80E 00 8. 78E 00

.47E 00 8. 55E 00

1 32E 00 .OOE

1 71 E 00 1 .26E

2. 52E 00 9. 70E 00

2. 3 6E 00 7. 46E 00

2.29E 00 7. 45E 00

3.08E 00 6. bfc; 00

2. 30E 00 7.09E 00

2. 47E 00 8.28E 00

2.05E 00 1 .07E

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1. Aircraft Data: Table 2 shows that the general state of the operations

requiring detailed individual reduction is essentially complete. However,

the interactive correlation of this data is only about 50% completed and its

correlation with the ground and radar measurements has only just begun

(except for some of the priority storm days).

2. Surface Data: Progress on analyzing the ground data is summarized in Table 3.

Most of the meteorological data from the 1971-72 winter season has been

reduced and, where possible, put on computer cards for tabulation and other

uses. The format used in putting the data on cards was the one suggested by

the Bureau of Reclamation with modifications to fit our particular project.

Accordingly each instrument location was assigned a station number and each

weather parameter a card number. These are shown in Appendix B. The specific

formats we used for each card number are also given in Appendix B. It is

impractical to put replica data, snow sample weights and silver concentrations

on cards.

Once on cards these data were put into a form which could easily

be used during analyses. This was done using computer print-out with replica

data and snow sample weights being added by hand. Data on precipitation (from

the weighing bucket gauges) temperature, wind, and pressure were all

tabulated according to storm date and time of day, based on a one hour time

interval. Data on precipitation rates (from the tipping bucket gauges and

snow sample wieghts) optical snow rate sensor and replica information were

tabulated for 15 minute intervals for a period of 7 hours beginning 2 hours

before seeding commenced.

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TABLE 2

STATE OF ANALYSIS OF AIRCRAFT DATA COLLECTED DURING WINTER 1971-72

AS OF JUNE 30. 1972

(0 No data taken; Data taken but not analyzed; / Data analyzed;

F Data faulty and not analyzed. )

FlightNo.

76

77

78

79

80

81

82

83

84

85

86

87

88

89

90

91

92

93

94

95

Date

9/29/71

10/13/71

11/1/71

11/3/71

11/8/71

11/16/71

11/19/71

11/24/71

11/29/71

12/2/71

12/3/71

12/9/71

12/10/71

12/13/71

12/15/71

12/22/71

1/5/72

1/6/72

1/7/72

1/12/72

Typeof

Flight

Test

Test

Storm

Test

Storm

Storm

Storm

Storm

Storm

Storm

Storm

Storm

Storm

Storm

Storm

Test

Storm

Storm

Storm

Storm

MagneticTape

Run-off

/

/

/

/

/

/

/

/

/

/

/

/

/

/

/

VoiceTracks

Transcribed

/

/

/

/

/

/

/

/

/

/

/

/

/

/

ContinuousParticleReplicator

/

/

/

/

/

/

/

/

/

/

/

/

/

/

0

0

0

0

FoilSampler

0

0

0

/

0

0

0

0

0

0

0

0

0

0

0

0

0

0

0

0

Optical IceCrystalCounter

0

0

0

0

/

F

/

/

/

/

0

0

0

/

/

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TABLE 2 (Cont)

FlightNo.

96

97

98

99

100

101

102

103

104

105

106

107

108

109

110

112

Date

1/13/72

1/14/72

1/17/72

1/25/72

1/26/72

1/31/72

2/14/72

2/15/72

2/22/72

2/23/72

3/1/72

3/2/72

3/3/72

3/19/72

3/16/72

3/27/72

Typeof

Flight

Storm

Storm

Storm

Test

Other

Storm

Storm

Storm

Storm

Storm

Storm

Storm

Storm

Test

Test

Test

MagneticTape

Run-off

/

/

/

/

/

/

/

/

/

/

/

/

/

0

VoiceTracks

Transcribed

/

/

/

/

/

/

/

/

/

/

/

/

/

0

ContinuousParticleReplicator

/

/

/

0

0

/

/

/

/

/

/

/

/

/

0

0

FoilSampler

0

0

0

0

0

0

0

/

/

/

0

/

0

0

Optical IceCrystalCounter

/

F

/

/

/

/

/

F

0

0

0

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TABLE 3

STATE OF ANALYSES OF GROUND DATA COLLECTED DURING WINTER 1971-72

AS OF JUNE 30, 1972

(S Seeded storm; U Unseeded Storm; S’’’ Top priority seeded storm for

analysis; / Data done; x data not done; t Weighing bucket, barograph,

thermograph, wind velocity all on hourly basis and tipping bucket, optical

snow rate sensor,, all on 15 min., bas is, reduced; xx no results are available)

Date

11/1/7111/8/7111/1611/1911/2411/2912/212/312/912/1012/1312/151/5/721/61/71/121/131/141/171/312/142/152/222/233/13/23/3

SSSUSSyys*yyy^y

uyusyys*syysusysfc

Meteorological DataPunched on Computer

Cards

-t-++x

+++//////x/

x///////////

SilverAnalysis

XX

XX

XX

XX

XX

XX

ShippedXX

ShippedXX

XX

XX

XX

XX

XX

XX

XX

XX

ShippedXX

ShippedXX

XX

XX

XX

ShippedShipped

DropFreezing

To be done

Finished

To be done

FinishedTo be doneFinishedTo be doneFinished

^o precip.FinishedFinishedFinished

CrystalTypes

All

data

are

reduced

CrystalSizes

All data for

Hyak

and about half

for the top of

Alpental

is completed.

Bottom of

Alpental

and

Keechelus Dam

are not yet

started,

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16

Special techniques for the reduction of freezing nucleus and

silver concentrations and replica information remained the same as reported

previously (Hobbs et al. 1971). Freezing nucleus concentrations were

determined by the drop freezing technique. Replicas of snow crystals were

examined with a stereomicroscope and the dominant crystal type(s) present

were recorded along with the degree of riming and an estimate of aggregation.

Special effects were also noted. The replicas which were collected on

2 x 2 inch glass slides were then projected and the crystals sized. Silver

concentrations are to be determined by the Bureau of Reclamation using an

atomic absorption spectrophotometer.

3. A review and preliminary evaluation of the effects of seeding on

March 3, 1972.

As an example of our methods for evaluating the effects of seeding

we describe here the results of a preliminary analysis of results obtained

on March 3, 1972.

Aircraft operations

Prior to any seeding extensive measurements were made from the

aircraft of the extent and structure of the clouds. The clouds were continuous

only over the Cascades. Over the Puget Sound Basin there was 8/10 broken

cumuliform cloud, and there were no clouds further east than 15 miles west of

Ellensburg. Over the Cascades the cloud tops were initially from 11,000 to

12,000 feet and they contained comparatively high liquid water contents at

8,000 ft west of the crest.

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17

The theoretical model predicted that artificial ice nuclei should

be dispersed about 7 miles west of Hyak at an altitude of 8 ,000 ft. Therefore,

the aircraft flew at an altitude of 10 ,000 ft along a roughly square track

with sides 7 miles long centered on this point and 10 gm Agl ejection flares

with 2,000 ft delay and 3,000 ft dispersal distances, were ejected at each

corner of the square. Seeding began at 1251 and ended at 1440 PST and total

of 340 gm of Agl was ejected during this period.

From 1250 to 1330 PST there was a general decrease in cloud height

in the region of seeding but by 1400 PST the cloud height was increasing

again in this region. At 1420 PST the first ice particles of the day were

observed visually from the aircraft and detected with the optical ice crystal

counter in the downwind leg of the seeded track. Following seeding the

aircraft flew further downwind and over Kechellus Dam where the clouds appeared

to be glaciated since a subsun was observed.

Subsequent analysis of the continuous particle sampler showed that

prior to seeding the clouds west of the Cascade crest were composed almost

entirely of water droplets with only occasional rimed irregular ice particles

and frozen droplets. Samples taken in the seeded area from 1249-1405 PST were

also only droplets. However, after 1410 PST the particles collected were

predominately ice, irregular crystals and hexagonal plates dominated but

occasional stellars and broad-branched crystals were also found.

The data strongly suggests that the artificial seeding on this

occasion caused glaciation. Moreover, the plume-of-effect was roughly as

predicted by the theoretical model.

Radar operations:

The radar measurements at Hyak on March 3, 1972 began at 1020 PST

when the incoherent radar was turned on to survey the sky. At that time there

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18

was no precipitation at the radar station. At 1052 PST the Doppler radar

was switched on and vertical probing began. At this time a few heavily rimed

dendrites were falling at Hyak. Very light precipitation continued until

1200 PST when the incoherent radar was again used for a sky survey.

Precipitation was observed at altitude to the northwest. By 1207 PST the

first weak signals were observed on the Doppler and the range gate was set

out to 500 m. Particles with fall-velocities from 1. 5 to 2.0 m sec were

observed while heavily rimed stellars and graupel fell at the station. By

1225 PST the average fall-velocity had decreased substantially and lightly

rimed stellars and dendrites predominated at ground level.

Subsequently, heavily rimed fast-falling crystals were observed at

the station until 1430 PST. At 1315 PST and 1330 PST the Doppler measurements

indicated that the average fall velocity fell below 1 m sec for short time

periods (see Fig. 2). However, these low fall velocities may have been due to

a data processing problem associated with small returned signals in very light

snow. However, at 1330 PST the slide replicas did indicate some decrease in

riming which would have caused lower fall velocities.

Starting at 1350 PST there was a steady increase in the average

reflected power from the precipitation (Fig. 2). This marked the beginning

of a rather unique event in the winter’s radar studies which is now described.

At 1415 PST the incoherent radar was turned on for another survey.

Snow generating areas could be seen and wide spread precipitation was observed.

At 1420 PST heavily rimed columns and dendrites 1 mm in size were collected

at the ground. The Doppler velocities appeared to be lower and the range gate

was probed for different velocities with height. However, there appeared to be

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1300 1400 1500

Time PST)

^ - ’^X;^^^^^^- rw

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19

little change with height at this time, indicating little growth over the

range surveyed (1300 m). By 1448 PST the spectral characteristics had

stabilized and appeared as a nearly single fall velocity of about 0. 75 in sec

(Fig. 3). At about 1518 PST the range gate on the pulse Doppler was moved

out to the region of snow generation which appeared to be between 1. 8 and

1.95 km above the radar. By about 1540 PST the fall. velocities had increased

again (Fig. 3) and an observation of the generation layer showed that it

had moved down to about 0. 5 km above the ground. Conditions remained fairly

stable until 1655 when the radar was switched off.

The marked shift to small fall velocities observed between about

1432 and 1529 PST (see Fig. 3) was accompanied by largely unrimed crystals

reaching the ground at Hyak (Fig. 4). Similar changes in riming characteristics

were observed during this period at Alpental and Keechelus Dam which are

within the target area (Fig. 4). It should be noted that the predicted

effect of our heavier seeding is to reduce the riming and therefore the fall

velocity of precipitation particles and that seeding was carried out from the

aircraft situated about 7 miles upwind of Hyak between 1251 and 1440 PST.

It can also be seen from Fig. 4 that very sharp increases in precipitation

occurred at Hyak Alpental and Keechelus Dam from about 1430 to 1600 PST.

According to our transport model the time period during which snowfall in our

target area should have been affected by the artificial seeding was from about

1300 to 1515 PST.

Freezing nuclei in precipitation

Snow samples collected on the ground at Hyak, Alpental and Keechelus

Dam on March 3, 1972 were analyzed for their freezing nuclei concentrations in

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2

Foi Velocity (m/)

F a 3--L; ep; eati-i i.ci;. ^;-; ^: Dopp Sei- ,jJa’ .e iuci ty spect ra ofpreci pi tat ion elements from \H08 to 1608 PST on March 3 1972The radar was located at Hyak and ai rborne seeding wi th Agwas carried out. 7 mi les upwi nd (west) of Hyak between 125and 4^0 PST Note the shi ft to smal ler fal veloci t ies

between about 1432 and 1528 PST

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"’-’"’’-"-

K i*-(R) .\(R) (R) >t X X(R)<

n(R) (C) x

(R) A A X X^(R)0 (C) (R)(5

^HYAK

^x ^ ^G>@ (j) (R) ^ X

FDA(R)^7 A A A

* * ?K D:+ n n X

K ^ ;^ A (j"^(C) C?(R)

ALPENTAL

N

A+ FDPO

A

* "^ X ^(R) X A (R) K X (C) (R) ^ (R) A ^(R)(R)N H N H333e

^^m-noo 1200 1300 1400

Pocific Stondord Time

1500 1600

Fig. 4 Preci pi tat ion rates and characteri st cs of preci pi tat ion observedat three ground stat ions n the target area on March 3 1972 (SeeT,-ih)p ^ fnr 1-p,, m cwmhnic

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TABLE h

KEY TO SYMBOLS IN FIGURE k

Symbol

0(53^B Densely rimed

XA*7

<(R)Dn+(R)

Explanation

Unrimed

Light riming

Moderate riming

Dendri tes

Radiating assemblageof dendri tes

Stel lars

Side planes

Assemblages of sectors

Columns

Capped columns

Broad branched crystals

Undetermi ned

Symbol

G

GS

FD

MD

HD

N

A

Explanati on

Graupel

Graupel -l ike snow

Few crystals on sl idethat are composed oftwo paral lei planecrystals separated bya water drop at thei rcenter.

- Half crystals ons ide are composed oftwo paral lei planecrystals separated bya water drop at thei rcenter.

^A1 crystals ons ide are composed oftwo paral lei planecrystals separated bya water drop at thei rcenter.

Nothing on sl de

Aggregates of icecrystals

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20

the manner described by Hobbs et al. (1970). The results are shown in Figs.

5 7. It can be seen that increases in the concentrations of freezing nuclei

were observed at all three ground stations during the predicted time of

arrival (1300 to 1515 PST) of the plume-of-effect due to the artificial

seeding. It seems likely that this increase was due to the Agl dispersed upwind.

However, final confirmation of this conclusion must await analysis of the

concentration of silver in the snow samples on March 3. (Silver analysis is

being carried out by the Bureau but the results have not been received at

the time of writing. )

Distribution of precipitation:

It can be seen from Fig. 4 that there were marked increases in

precipitation at Hyak, Alpental and Keechelus Dam between about 1400 and

1800 PST. The predicted period of the direct effects due to seeding on

precipitation at these ground stations was 1300 to 1515 PST. The observed

precipitation pulses at several stations in the Cascades and their relationship

to the predicted period of the plume-of-effect due to seeding are shown in

Fig. 8. It would appear from these results that the increases in the rate of

precipitation which started at about 1400 PST was fairly widely spread and

may not have been due entirely to the seeding. For example, Nagrom is situated

about 10 miles south of the predicted plume-of-effect due to seeding, but

it shows an increase in precipitation between 1300 and 1700 PST. We plan to

obtain precipitation records from stations in the North and South Cascades

which are well-removed from our target area in Snoqualmie Pass in order to

further elucidate any effects which may have been due to seeding on March 3.

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Kwm_y

I

1100 1200 1300 1400 1500 1600

Poclfic Stondord Tim*

Concentrations of freezing nuclei per gram of snow collected atHydk on March 3, 1972. The time period during which artificialseeding upwind was predicted to affect the snowfall was 1300 to

1515 PST.

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""TO

1200 1300 1400 1500

PocHIc Stondard Time

1600

-24*C

-21C

:: i8c

S’C

12*C

Fig. 6 Concentrations of freezing nuclei per gram of snow collected at

Alpenta) on March 3, 1972. The time period during which arti ficial

seeding upwind was predicted to affect the snowfal was 1300 to

15)5 PST,

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Concen^.ons of .e^,n. ^^,^r ^ ^^^^e^S^al^ed?^^ ^ predicted to affec. the sno.fal

^s 1300 to 1515 PST.

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^^^TwG^^^^i

.04

oo^^ ;i^^.V^^/^>’7

BANDERA

.08 r-

04 F%^00

ALPENTAL

^^^ JZZZZZZZZ^ Z^^^y^7

HYAK

00 ^^^fazzzzzz

.08 KEECHELUS DAM

^7^77777

.08 KACHESS DAM

.04

00 jzzzzEza JZZZZZZZZL1000 1100 1200 1300 1400 1500 1600

Pacific Standard Time

1700 1800

Fig. 8. Precipi tat ion rates at s ix s tations n the Cascades on March 3 1972. The pred ctedperiods of the piume-of-effect due to ai rborne seeding wi th s lver-iodide upwind areenclosed between the arrows

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21

Conclusions

A final conclusion on effects due to seeding on March 3, 1972

must await retrieval of further data (e.g. silver content of snow samples

precipitation records from more stations in Washington State) and more

detailed analysis. However, the following features do indicate successful

artificial modification:

(a) Aircraft observations documented a substantial increase in

ice in the clouds over the target area following seeding.

(b) The fall velocities of precipitation particles in the target

area, as measured by Doppler radar, showed a substantial

decrease during the predicted period-of-effect of seeding.

Moreover, the fall velocities increased again at almost

the same time the plume-of-effect from seeding was predicted

to cease. These changes are exactly those predicted to

occur due to glaciation of the clouds by artificial seeding.

Such sharp changes in the fall velocities of precipitation

particles have not been observed previously by Doppler

radar in the Cascades.

(c) The ice crystals collected on the ground in the target area

were heavily rimed before and after the predicted period-of-

effect due to seeding, but during most of the period-of-effect

they were unrimed. This observation also shows that the clouds

were glaciated during the seeding period.

(d) Measurements of the concentrations of freezing nuclei in

snow collected in the target area show increased concentrations

during the predicted period-of-effect of seeding.

Page 33: SO ROG - carg.atmos.washington.edu

22

(e) Snowfall in the target area increased during the predicted

period-of-effect of seeding.

On the other hand, the following features indicate that some natural

changes might have been taking place during the period of seeding:

(a) Changes in cloud height were observed from the aircraft.

(b) The barograph trace at Alpental indicates that a weak post-

frontal impulse might have passed through our target area

at about the time of seeding, although this does not appear

on the synoptic charts.

(c) The increases in snowfall rate in the target area extended

beyond the predicted period-of-effect due to seeding.

(d) Increases in snowfall rates occurred at some stations

outside the predicted area-of-effect of seeding.

This case study illustrates some of the difficulties encountered

in attempting to ascribe effects to artificial seeding even when (perhaps

particularly when) very careful measurements and analysis are made.

4. Observations of seeding effects with the Continuous Particle Sampler

on January 31, 1972.

On a number of occasions the effects of artificial seeding on cloud

structure were traced with the aircraft. The seeded regions are most often

detected by the real-time measurements of large increases in crystal concentrations

with the University of Washington’s Optical Ice Crystal Counter (OIC) or

by visual observation of the glaciated region. However, in thick cloud optical

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23

effects are often difficult to observe and the crystals may be too small to be

detected by -theOIC. In these cases the effects can often by traced by a post-

flight analysis of the Formvar replicas from the continuous particle sampler

(CPS).

In our experience the seeded areas can often be distinguished from

even naturally glaciated areas by the predominance of regular crystals. In

addition, in recently seeded areas the crystals are smaller than average and

are present in high concentrations.

Flight 101 on January 31, 1972 (CPS Run No. 20) provides a good

example of a penetration of a recently seeded area. Agl seeding with both

drop flares and flares fixed to the aircraft had been in progress for 51

minutes as the aircraft flew a triangular pattern. CPS Run No. 20 was made on

the downwind leg of the seeding pattern. From the wind speed and the length

of the seeded legs it is estimated that the volume had been seeded about

5 minutes prior to CPS Run No. 20.

The observations which comprised about 1000 meters of cloud, are

summarized schematically in Fig. 9. The ice crystals found were very thick

plates and short columns with occasional irregular crystals. The ice crystal

areas contrasted strongly with sections of unglaciated cloud where the crystal

count went essentially to zero and the droplet concentration rose sharply.

The ice crystals were almost entirely between 50 and 150 ym in size

and the droplets from 10 to 30 pm in diameter. Only occasional counts

were observed on the QIC due to the small size of the crystals.

This run is especially valuable for the determination of ice crystal

concentrations due to seeding. The CPS can only rarely be used to obtain

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Gtocifd Oroptt Gtociofdora -<

Oraprtfa

400 500 600

Ortonce ( mtrs

Fig. 9 Fl ight No. 10i on January 31 1972Fl ight al ti tude 10,600 feet.

Run No. 20. 13^5 PST Ai r Temperature-21 .3C

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24

accurate measurement of concentration. Generally, the CPS is fitted with one

of our decelerators in order to reduce crystal fragmentation but in this case

the collection efficiency is unknown. On Flight 101 a decelerator was not

used but the crystals were sufficiently small and robust that virtually all

of them were collected intact. Thus on this occasion we estimate that our

deduced concentrations of ice crystals are correct to within +/- 20%. The value

of 2500 ice crystals per liter (Fig. 9) should provide an interesting starting

point in estimating the nucleating activity of our Agl flares using standard

plume diffusion theory from a time source.

5. Measurements of fall-velocities of snow crystals

One of the major problems in modelling the trajectory behavior of

snowflakes is the lack of detailed data on their fall speeds. Our model

requires this information not only as a function of the type and size of the

frozen hydrometeors but also as a function of their degree of aggregation

and riming.

To help remove these uncertainties a field project was begun last

winter to measure the sizes masses and velocities of frozen hydrometeors. A

brief description of this work is given below.

Instrumentation:

The instrument used for measuring the fall speeds of the ice

crystals is shown in Fig. 10. It consists of a transmitter and a receiver.

The transmitting section uses lights and fiber optics to transmit two planes

of parallel light separated vertically by 4.1 cm to similar fiber optics

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PtWtOBMittlpitWtub

F g ,0 instruct for n^asuri ng fal veloci ties of preci pi tat ion parti cles (Dimens ions in en,.

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25

in the receiving section. Light from the receiving fiber optics is passed

into photomultiplier tubes. Any decrease in the transmitted light caused by

a snow particle falling through the two planes of light is detected by the

photomultiplier tubes and can be displayed on a storage oscilloscope. The

time difference between signals from the upper and lower fiber optics is

recorded and can be used to determine the fall velocity of the snow particle,

Operational procedures

The instrument is located at the bottom of a tower at Keechelus

Dam which is designed to minimize horizontal wind effects. When a snow

particle falls between the two sets of fiber optics it is caught on a piece

of plastic wrap suspended on a frame. This frame is then taken from the

instrument, positioned under a microscope where a microphotograph is taken

of the particle. During this time the section of plastic having the particle

on it is stretched over a cold plate to keep the particle from melting. After

the microphotograph is taken the particle is melted into a water drop which

is also photographed. The mass of the original snow particle is then determined

from the droplet diameter.

Results

During the past few months the fall velocities sizes and masses

have been measured of over 400 snow particles. These data are sufficient to

give a fair determination of size versus mass and size versus velocity for the

following types of particles lump cone and hexagonal grauple, grauple-

like snow of lump and hexagonal type, radiating assemblages of dendrites

densely rimed columns, aggregates of sideplanes radiating assemblages of

dendrites sideplanes columns and bullets and dendrites. For the following

example, lump graupel is chosen to illustrate data handling methods and results.

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26

Fig. 11 shows a log-log plot of mass versus diameter for lump

grauple. The data points are divided into six groups of similar density

types numbered 1 through 6 in Fig. 11, with group 1 having the lowest

average density and group 6 the highest. The empirical equation relating

mass M (in 10 grams ) with diameter D (in mm) for group 3 is

M 6. 5D3

Fig. 12 shows a plot of fall velocity versus diameter for lump

graupel. This data is also divided by density with some groupings combined.

First a line was established for the group containing the largest number

of data points (group 3). Then on the assumption that the velocity of grauple

in the other density groups would be a similar function of the diameter,

lines for the other groups were drawn in parallel to the line for group three.

The table in Fig. 12 lists the different groups the average density of the

particles in the groups and the equations of velocity versus diameter.

Fig. 13 is a plot on linear paper of fall velocity versus diameter

for lump graupel in the different density groups. For comparison the dashed

line shows a curve of velocity versus diameter for lump graupel of density

0.12 gm cm drawn from results obtained by Nakaya.

When the data collected so far is combined with similar measurements

which we expect to obtain next winter, we should be able to provide detailed

information of the kind given above for lump graupel for a wide variety of

crystal types and also to show the effect of riming and aggregation on the

fall velocity.

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LiJ------- *--’ * ’ "J-------I---I--I--I I lii.i------I---I--I- > t *.tJK) 100 1000

M ( to uftif < io’5 m)

Fig. Di ameter versus mass for lump graupel <,

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Oiawter 0 mm)

Fi q. 12 Fd vc ioci t-’y ,’t-i’su-a d dme ie. or Limp qraupe

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3.0

uQ

"5

2.5

s.6 2.0>

. 1.5

1.0

0.5

0 2 3

04mtr Oirnrn)

5

13 Fal veloci ty versus cii ariiei.er or lump graupe p s the average dens ty (in gm cm

of the crystals n eaci-! group

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27

Task #13: Instrument Research and Development

1. The University of Washington Optical Ice Crystal Counter

A description of the University of Washington’s Optical Ice Crystal

Counter (QIC) in its present form is given in Appendix D, which is an

extended abstract of a paper accepted for oral presentation to the International

Cloud Physics Conference, London, August 21-26, 1972.

While this device is already providing us with very valuable

real-time data on ice crystals in clouds the minimum size of crystal which it

can detect is still not known precisely. During late March 1972, Mr. F. Turner

of our research group visited Elk Mountain Observatory in Wyoming with the

intention of obtaining ground-based measurements of ice crystals in cap clouds

with the QIC and correlating these with slide replicas of the crystals.

Unfortunately, cap clouds were absent during the period of his stay so no

measurements were obtained. Efforts to simulate cloud conditions in our cold

laboratory have generally produced either very small (< 100 pm) crystals which

are generally not detected by the QIC, or rather larger aggregates which are

counted. Presently we are making aircraft measurements in natural clouds and

correlating the observations with the crystals collected by the continuous

particle sampler. The problem is complicated by the fact that we expect the

minimum detectible size to be somewhat dependent on crystal habit and degree

of riming. At the present time we can only say that it counts practically no

crystals smaller than 100 urn and practically all crystals larger than about

700 pm. Water droplets, even as large as several mm in size, are not counted.

A good example of the useful data provided by the University of

Washington’s Optical Ice Crystal Counter and the Mee fast response Ice

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28

Nucleus Counter (INC) in delineating the effects of artificial seeding

occurred on February 23, 1972.

During this flight (Flight No. 105) a short isolated seeding

experiment was performed near cloud tops. The absence of ice crystals in the

clouds prior to seeding was verified by the QIC, post-flight analysis of

formvar replicas and by the presence of strong water droplet optics in the

form. of a glory and cloud bow. 180 grams of Agl were injected into the

cloud tops between 1237 and 1255 PST from pryrotechnic flares fixed to the

aircraft. Ice crystals were first observed in the seeded volume at 1250 PST,

and after 1252 PST a sub-sun was almost continuously visible. Fig. 14 shows

a portion of the flight record from 1313 to 1321 PST when the aircraft was

flying in and out of the seeded volume near cloud tops. The correlation

between the measured bursts of ice crystals and ice nuclei as detected by

the QIC and the INC is gratifying. Post-flight analysis of the formvar

replicas made at 1318 and 1321 PST showed primarily hexagonal plates and

plate-like fragments.

2. A Ground-based Snowflake Counter

A prototype snowflake counter was constructed and tested during the

winter of 1971-72. This was intended to be a simple approach to the problem

of measuring the number of snowflakes per unit volume of air. The sensor

(Fig. 15) consists of a horizontal sliding trap door located 20 cm above a

planar light source and photo transistor array. An electric motor pulls the door

open allowing saowflakes to fall into the volume below. The door is held open

for 2 3 seconds after which a spring pulls it rapidly closed. The light

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Illnl ^(b) Ice nucleus counts

(o) Ice crystal concentration

1321 1319 1317 1315

Time

Fig. 1A Simultaneous ice nucleus counts Mee Counter) and ice crystal concentrations

(U. of W. Optical Counter) in a cloud seeded with Agl over Cascade

Mountains on February 23. 1972.

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To Electronics

DriveMotor

--i ser

^Open closesense switch

Sliding’Trop door

"9WOReturnspring

Worm

20 cm

Reguloted ^ \Supply / \

Light

To Electronics

Phototronsistor

Snowflokesdetected inthis region(area 50 cm2)

Fig 15 Schemati c representation of prototype snowflake counter

Page 47: SO ROG - carg.atmos.washington.edu

29

source and photo sensor are mounted on the underside of an aluminum plate on

2opposite sides of a rectangular cutout (Area 50 cm through which the snow

is allowed to fall. Immediately the door closes the electronics are activated,

thereby counting the number of flakes within the enclosed volume (1 liter).

This procedure is repeated every 37 seconds. The electronics (Fig. 16) used in

this design consist of the photo transistor feeding a high-gain amplifier which

triggers a one-shot multivibrator which provides a constant pulse-width signal

for each particle sensed. A long-term integrator is allowed to sum all the

pulses encountered during the time that the door is closed, but is reset to

zero each time the door is opened. After a suitable time to count all the

particles within the volume has elapsed, the total number of snowflakes counted

is recorded, the trap-door opens again, and the cycle is repeated.

Figure 17 shows an example of the data obtained with the snowflake

counter on March 3, 1971, averaged over 15 minute intervals. Also shown in this

figure are measurements obtained with the heated tipping bucket and the E.

Bollay Assoc. optical snow rate sensor. It can be seen that on this occasion

the results are in reasonable agreement as far as fluctuations with time are

concerned. However, it should be noted that in general it is not to be

expected that the precipitation rate will vary as the concentration of snow

crystals in the air since the former quantity also depends on the mass and

fallspeeds of the crystals.

Despite reasonably encouraging results with this device in its present

form it has proved to be mechanically too complex and despite weatherproofing

and heating not sufficiently robust for severe winter environments. Several

alternatives for obtaining the concentrations of snowflakes at ground level

are being considered.

3. Keilly Probe

We have built, with some changes, the NCAR-modification of the Keilly

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Photo-transistor

CD-) )-

Open-closeswitch

1

High ^\.

7^----U----------------------------------n

gain .>----amp. ^"

OneShot

Long-termIntegrator

reset

Sample andHold

&.4 secDelay

’Gote--1---o To

J Recorder

Fi g. 16 Schemati c of e lectroni cs for snowflake counter

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Concentration of snowflakes from Universityof Washington counter

Precipitation rate from tipping bucket

Snow rate from E. Bollay Assoc. opticalsnowrote sensor

60

40

30

ou(A

0

8?o

o00)

0A

(A

.C0

0

0

1430 1445 1500 1515 1530

Pacific Standard Time

1545 1600

Compari son of concentration of snowflakes determined by Uni versi ty of Washington ’s counter

itit^^ate^^m t^ajng ^udtet^nd sno^. ate__>m ^_o1 1ay_ so__ pt_lfr?m^\lDe^Bl o^^rcrr^^ 19^W ^^ ^* ^^ ^* ^^ ^^

Page 50: SO ROG - carg.atmos.washington.edu

electrostatic probe for counting cloud droplets in the range 5 50 pm

from an aircraft. The probe was test-flown during June and the preliminary

results are encouraging, although the signals from the 5 10 pm droplets are

lost in mechanically-induced electrical noise. Various techniques of

vibrational damping and electronic redesign are underway in an attempt to

eliminate this problem.

4. Continuous Particle Sampler

During the past few years as a result of various redesigns and

improvements the MRI continuous particle sampler (on loan from the Navy)

has been made to function fairly reliably. However, the device still remains

overly complex and troublesome and requires an experienced operator. These

considerations plus the fact that the Navy wants its sampler back, have

encouraged us to begin building a greatly simplified continuous particle

sampler. It is expected that airborne testing of this device will begin

during the next report period.

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31

Section 2

Work Planned for the Next Period

From July 1 through October 31, 1972, the emphasis will be on

analyzing all of the data collected during winter 1971-72 and preparing the

ground stations instruments and aircraft for the winter 1972-73 season.

The winter program should be fully operational by November ’1, 1972,

and will continue through December 31, 1972, as described in the work plans.

Page 52: SO ROG - carg.atmos.washington.edu

32

Section 3

Professional and Technical Personnel

Prof. P. V. Hobbs Principal Investigator .(Two weeks)

Dr. L. F. Radke: Research Assistant Professor (Full time)

F. Turner: Graduate Research Assistant (1/2 time)

C. Robertson: Meteorologist (Full time)

J. Locatelli: " ( " " )

D. Atkinson: ( )

J. Frost: ( " )

L. Engel: Electronics Engineer (Full Time)

H. West: Instrumentation technician (Full time)

B. Simon: " " (Full time)

J. Russell: Field Assistant (Full time)

D. Willott: " " ( " " )

K. Moore: Office Assistant (3/4 time)

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33

Principal Items of Equipment Purchased

Item Cost From Date Ordered

J/W Liquid Water Probe $482.00 Bacharach Instr. 6/5/71

Vortex Temperature Probe 450.00 MRI 6/12/72

Pulsed Klystron Amplifier Tubes 750.00 Radio Research 5/26/72

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34

Papers Presented for Publication and at Conferences

1. "Fragmentation of Ice Particles in Clouds" by P. V. Hobbs and R. J. Farber.

Accepted for Publication in J. Rech. Atmosph. (Invited paper).

2. "Collection of Ice Particles from Aircraft Using Decelerators" by P. V. Hobbs

R. Joppa and R. J. Farber. To be submitted to J. App. Met.

3. "Ice in the Atmosphere: A Review of the Present Position" by P. V. Hobbs.

Proc. Intern. Conf. on Ice Physics, Ottawa, Canada, 1972. (Invited paper).

4. "Aircraft Observations and Measurements in Pacific Northwest Storms" by

P. V. Hobbs and L. F. Radke. Presented at Joint Pacific Div. AAAS AMS

Session at Eugene, Oregon, June 1972. (Invited paper).

5. "Studies of the Microstructure of Clouds and the Development of Precipitation

in Cyclonic Storms over the Cascade Mountains." by P. V. Hobbs. Accepted

for presentation at Intern. Conf. on Cloud Physics, London, August 1972.

6. "An Airborne Optical Ice Crystal Counter" by -F. M. Turner and L. F. Radke.

Accepted for publication at Intern. Conf. on Cloud Physics London 1972.

7. "Studies of Winter Cyclonic Storms Over the Cascade Mountains (1970-71)"

by P. V. Hobbs et al. Contributions from the Cloud Physics Group, Res.

Rpt. VI.

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35

APPENDIX A

Flow Diagram for Cascade Operational Computer Model

G>

Determine Crystal Characteristi csCal subroutine SNOCAR

Use Hydrostati c Equationto Compute Height at Baseof Crystal Growth Layer

Interpolate to ComputeAverage Wi nd Vectors at

150 Meter Intervals

Convert Wi nd Vector to UV Components at 150 Meter

ntervals

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APPENDIX A (continued)

Compute Fal Veloci tyfor Rimed Crystals in

150 Meter Steps

Compute Trajectory .e.t, x, y Components n 150Meter Vertical Step Sizes

Convert Al Trajectory Poi ntsTo Range from Surface Stationand to Height Above MSL Cal

Subrouti ne Angle

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37

APPENDIX A (continued)

SUBROUTINES

Subrouti ne SNOCAR Subrouti ne Angle

Match Crystal Typewi th Data Listi ng

Return a Max. andMin. Fal Veloci ty,and Max. Temperaturefor Growth Habi t

Take X, Y Componentsof Trajectory andConvert to Range,

Azimuth from TargetArea Based on 0 Equals

True North

Subrouti ne Head

Takes Azimuth RangeData from SubroutineAngle and Converts toAi rcraft Headi ng andRange from Seattlefor Each Trajectory

Poi nt

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38

APPETTOIX A (Cont

Computer Program for the Cascade Operational

Model Executed on the CSS Computer

00 DIMSffSION Vr<tOO)*U< aOO) V< 200 T( 75 > * rv< 75 ) *V^ 7b1 101 AZ(200)*ZAF( 6)* R(200)*X(200) *Y(200)*P( 75 ) ^( 200) <

1209, TD( 75)* D( 75)S< 75)-VTERMt 2)* ZZ( 75)* TO TALC 200 )

1 30 DIMENSION HED(200)<AR( 100)

1 40 INTEGER DO1 50 REAL K1 , IN1 60 LMAX-01 70 I RUN-01 80 IRIME-01 90 HAXVO200 JSAVE-02 10 IFIN-0220 I DATA-0330 KI-2.8704E+6/980.665840 PRINT*"THIS PROGRAM COMPUTES THE TRAJECTORIES OF RIMED AND"250 PRINT*"UNRIMED SMOV CRYSTALS OF VARIOUS TYPES."260 1 16 PRlNT*"ENTiai THE STATION HEIGHT IN METERS"870 READ* ZSFC280 1 FORMAT( F6. 1 )

290 GO TO 4000300 PRINT*"ENTER THE OBSERVED CRYSTAL TYPE ACCORDING TO THE"310 PRINT*"FQLLQIMNfl LEGEND,"}20 PRINT*"IF OENDRITES PUNCH 1"i30 PRINT* "IF STELLARS PUNCH 2"140 PRINT* "IF PLATES PUNCH 3"150 PRINT* "IF SCROLLS PUNCH 4"160 PRINT* "IFSHEATHS/NEEDLES PUNCH 5"i70 PRINT* "IF BULLETS PUNCH 6"180 PRINT* "IF COLUMNS PUNCH 7"190 PRINT* "IF SIDE PLANES PUNCH 8"00 PRINT* "IF PRISMS PUNCH 9"l0 PRINT*"IF ASSEMBLEflES OF"20 PRINT*" PLATES430 PRINT*"IF ASSEMBLEGES OF"440 PRINT*" SECTORS450 PRINT*" IF SECTORS460 PR I NT*"IF GRAUPEL465 PRINT*"IF AQOREQATES_____470 4000 PRINT*"CRYSTAL TYPE?"480 READ* I TYPE

PUNCH 10"

PUNCH 1 1"PUNCH 12"PUNCH 13"PUNCH 14"

490 CALL SNOCAR(VTERM*TMAX* ITYPE)500 IFIN-05 10 IF( IDATA ,OT. 0) GO TO 134520 PRINT* "IS THE SOUNDING DATA FROM UIL?"530 READ 6* IDAD540 6 FORMAT(A3>

550 PRINT* "ENTER THE NAME OF THE FILE WHERE SOUNDING DATA IS560A STORED^570 READ 2* ZAF< 1 )

580 IF( IDAD .Efl. "YES" ) GO TO 132590 PRINT*"ENTER THE LOWEST PRESSURE IN THE SOUNDING"600 READ* PLOW610 PLOV-PLOV+80,’on n n taPi on

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04U tje *-*650 CALL OPEWFO^ IH)

660 DO 3 J-l*76 39

670 LMAX"J680 IJ690 1F( 1DAD *EQ. "NO" ) GO TO 1 35

700 READd ^ ) P( J),ZZ( J)T( J)-TD( J) *D( J)< S( J)- IFIN

7 10 IFdDAD .EQ. -YES" ) GO TO 1 33

720 135 LMAX-J-1730 IF< J *EQ. 1 ) READd 2) B740 IF< J .EQ. 1 ) GO TO 3750 I-J-1760 READC H5) Pd )<ZZd )<Td )-TDd ) <Dd ) ,Sd )

770 5 FORMAT<2F7.0-F6.1 l8X,F5. l <9X,F4.0, lX,F4.0)

780 JLOV-Pd )

790 IFC JLOW- *LE. ILO^) GO TO 4

800 133 TD< I )"T< I ) -TD( I )

810 T< I )"T< D+273. 16820 S( I )S< I )*514830 Z( I )ZZ( I )

840 ZZ( I )"ZZ< I )*100.850 E-6. l l*( lO<0**< 7.5*( TD( I ) )/(TD( I )+237.3) ) )

860 < I )0.622*E/<P( I )-E)870 IF< IFIM OT 0) CALL CLOSEF< 1 )

880 IF< IFIN .GT. 0) GO TO 134890 3 CONTINUE900 4 CALL CLOSEFC 1 )

?20 ^PRTSr^ENTER THE OBSERVED SURFACE ^IND AZIMUTH IN DEGREES-

940 PRINT"ENTER THE OBSERVED SURFACE WIND SPEED IN KNOTS-

960 PR^NT^I^A COMPLETE TRAJECTORY WITH 300M STEPS IS DESI^D"970 PRIMT^PUNCH A OWE. IF A REDUCED PRINTOUT IS DESIRED, PUNCH-

980 PHIMT<**A ZERO***990 READ* I FLAG1 000 Z( l )"ZSFC1 010 S( 1 )"S( 1 )*.5l41020 1 18 DO 100 N-l^LMAX1030 IN1 040 IF( T<M) .LT. TMAX) GO TO 101

1050 100 CONTINUE1 060C TMAX IS BETWEEN T( I ) AND Td-D1070 101 TLAPSE"( T< I )-T( I-1 ) )/(ALOG<P< I )/P< I -1 ) ) >1080 XLNP-CTMAX-T< l-l ) )/TLAPSE+ALOG<P< I-D )

1090 PP-EXP<XLMP)100C COHPUTE HEIGHT AT TMAX (M) HEIGHTZSTOP1 10 TV( I )-T< I >-*-( I )<"166.667120 TV( I-l )T( I-l >*<< I-l )*166.667

130 TBAR"(TV( I )TV< 1-1 /2.140 ZSTOP-(K1*TBAR*ALOG(P< I-1 >/PP)+ZZ( I-1 ) >*.01

Ito PRiMT^TSE’HT. (FT) OF THE BASE OF THE CRYSTAL GROWTH LAYER-

170 PR1NT ZSl80 IFdDATA GT. 0) 60 TO 109190 DO 102 K>140200 L-K1210 IF<P(K) .GT* 841 . .AMD. P<K) .LT. 859. ) GO TO 103

220 IF<K EQ. 40) PRIMT^ERROR IN INPUT PRESSURE-1230 IF(K EQ. 40) 00 TO 10001240 102 CONTINUE1250C L IS INDEX OF 850 MB WIND,260C COMPUTE WIND COMPONENTS IN 150 METER INTERVALS,270 103 DZ-1 50.280 HZ-ZSPC-DZ/2.

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,i:)ft<W tm Httf^HVU13M U-K336 KWUC-K 40

340 HZ-HZ+DZ350 TOP-2( I )

360 H2-HZ370 IF(HZ .OT. TOP) HZ-HZ-DZ380 IF(H8 .GT. TOP) GO TO 104390 U<K)-0.0400 V<K)-0.0

410 LOV-I-l420 IFC I EQ. L) LOV^ 1430 DDI-Dd )-D(LOV)440 SSI-Sd )-S(LOy)

450 ADDI-ABS(DDI )

460 IFCADDI Eft* 180. ) GO TO 105470 IFCDDI LT. 180* ) GO TO 810480 DDI-DDI-360.490 GO TO 819500 818 IF(DDI+180) 817,819,819510 817 DDI-DDI+360*580 819 DD"D(LOV)*(DD1*(HZ-Z(LOV) ) )/( Z< I ) -Z(LCV) >530 ZF(OD .GT. 0) GO TO 822540 DD-DD+360.550 GO TO 823560 822 IFCDD .LT. 360) 80 TO 823570 DD-DD-360580 823 SS"S(LOlir)^<SSl*(HZ-Z(LOW) ) )/( Z( I )-Z(LOV) )

590 DX-DD600 IFCDX LT. 90 AND* DX .GE. 0. ) GO TO 106610 IFCDX LT* 180 AND* DX GE* 90* > GO TO 107620 IFCDX .LT* 270* AND* DX GE* 180 ) GO TO 108630 THETA-(DX-870. )/57.284640 U(K) "SS*COS< THETA)650 V(K)-SS<dSiN( THETA)660 GO TO 105670 106 THETA-(90.-DX)/57.284680 U<t()-SS*COS< THETA)690 V<K>-SS*SIM(TKETA)700 80 TO 105710 107 THETA-(DX-90 )/57.284720 U(K)--SS*COS( THETA)730 V(K)SS*SIN(THETA)740 GO TO 105750 108 THETA-(870.-DX)/57.a84760 IKK)"SS*COS(THETA)770 V(K)-SS*8IN(THETA)780 105 CONTINUE790 104 CONTINUE800C COMPUTE FALL VELOCITIES FOR LARGE AND SHALL CRYSTALS810 109 DO 1 10 I-l-S820 IF( I EQ 2 AND ITYPE EQ* 13) GO TO 1 10830 HZ-ZSFC-DZ/8.840 DO 1 12 K-1,KMAX850 HZ-HZ+DZ860 MAXVI870 IF(HZ GT. ZSTOP) GO TO 1 19880 IFC IRIHE EQ* 1 ) QO TO 1 1 1890C HERE IS THE UNRIMED FALL VELOCITY900 VT-VTERM( I )

910 GO TO 1 12920 1 1 1 VLAPSE-VTERM( p/(ZSTOP-ZSFC)930 VT"VLAPSE*< ZSTOP-HZ ) t-VTERM< I )

940 1 12 VF(K)fVT9Kf r rnNOirrip T .nprT^ ’Y

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..-^^WWffVumw90 ZO-6. 41

aobo DO 1 15 j-i^aoo

8010 X(J)-0.aoao Y( J)-O.2030 Z( J)08040 1 15 TOTAL<J)-0.8050 00 1 13 J-l^KMAX8060 HT"HT+D28070 DA-DZ8000 K-J8090 IptHT .OT. ZSTOP) DA-ZSTOP-HT+2 .*DZ8 100 IF(HT .GT. ZSTOP) KJ-18 1 10 DELTAT-DA/VF(K)8 180 TOTAL(K)"TOTAL(K-l )+DELTAT8 130 IF( J EQ* 1 ) TOTALd )-DELTAT8140 X(K)XO-DELTAT*U(K)8 150 Y(K>"YO-DELTAT*V(K)8 160 2(K)-HT8 170 IF(K EQ. < J-l Z(K)ZSTOP8 180 XQ-X<K)8190 YO"Y(K)8800 JSAVE-K8810 IF<HT .OT. ZSTOP) 60 TO 1 148880 1 13 CONTINUE8230C CONVERT ALL POINTS TO RANGE AND HEIGHT8840 1 14 CALL ANGLE(X*YJSAVE AZ*R)8850 IFC IRIME .EG. 0) PRINT 808860 IFC IRIME .Ett. 1 ) PRINTS 18870 80 PORMATdH ,/^-IF THERE IS NO RIMING* THE TRAJECTORY FOR" )

8880 83 PORMATC IH ^"THE SMALLER ICE CRYSTALS ORIGINATE A’T’*F8.2 )

8890 84 FORMATC IH SMILES- AND*** IX<F7.2, IX,"DEGREES FROM THE2300A SURFACE STATION")8310 81 FORMATC 1H *4X/<"IF THERE IS RIMING* THE TRAJECTORY FOR" )

8380 88 FORMATdH ^-THE LARGEST ICE CRYSTALS ORIGINATE AT^ IX,8330AF7.2)8340 IFCMAXV S6 l > PRINT63, R( JSAVE)8350 IFCMAXV .EQ* 8) PRINT 82, R< JSAVE)8360 PRINT 84 AZ( JSAVE)8370 IFC IFLAG BQ l > PRIMT 858380 IFC IFLAG E 0) PRINT 888390 88 FORNATdHO^-FOR THE ABOVE CONDITIONS* THE TRAJECTORY’S /8400&-POSITIONS ABE AS FOLLOWS--//)8410 85 FORMATC IHO*-FOR THE ABOVE CONDITIONS* THE TRAJECTORY*’^/*8480**’POSITIONS AT 300 M INTERVALS ARE AS FOLLOWS*"*//)8430 PRINT 878440 87 FORMATdH *2X,"AZI FROM"*4X*"NA MI"*4X*"MSL HT"*4X*8450A-FALL TIME"*8X*"A/C MAG<’*8X*MA/C RANGE** */*3X*"TAR6Er’*8460A4X*"TO TARGET <FEET) (MIN) HEADING"*2X*8470A-FROM SEACN Ml )-*/)8480 DO 810 J-1 *JSAVE8490 CALL AKGLC(X*YJ*AZ*R)8500 TOTAL( J)-TOTAL< J)/60.8510 Z( J)-Z<J)*3.288580 810 CONTINUE8530 CALL HEAO(AZR*JSAVE*HED*AR)8540 iFdFLAG .EQ* 0) GO TO 1808550 213 DO 181 J-l^JSAVE-28560 181 PRINT 886AZ< J)R( J)Z( J)TOTALC J)*HED( J)AR( J)

8570 886 FORMATdH ,6F10.1 )

8580 GO TO 1318590 180 K-28600 IS-58610 DO 183 11-1,36- IS

n TffT T I -1

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1 :^M9^W.^SlW9!^mw^^v^6W l[t<Dist LT. IKJ-I ) ) 90 TO 123 4Z

’BAtO’ lrdK JSAVB) LT 1 ) GO TO 813

8660 IFCRCJSAVE) .LT. 5. ) IS"1I 8690 IPCDIST .GT R( JSAVE) ) GO TO 123

9 2700 K*J2710 IFCDIST .LT. R( J> .AMD. DIST .OT. R( J-D > GO TO 185

1 2720 124 CONTINUE2730 125 ZLAPSE-( Z<K)-Z<K-l ) )/<R(K)-R( K-l ) )

2740 RSTEPR(K>-R<K-1 )

2750 STEP"D1ST-R(K-1 )

2760 HZZLAPSE*STEP+Z(K-1 )

2770 AZM--12780 ALOV-AZ(K-l )

1 2790 DDIAZCK}-AZ(K-1 )

2800 21 1 2FCDOI LT 180. ) GO TO 1262810 DDI-DDI -360.

1 2820 GO TO 1278830 126 IF(DDI+180. ) 188^ 127^ 1272840 128 DDI-DDI+360.2850 127 AZI"ALOIK-DDI*STEP/RSTEP

| 2860 IF(AZI .GT. 0. ) GO TO 1292870 AZI-AZ1*360.2880 GO TO 130

1 2890 129 IF<AZX .LT. 360. > GO TO 1302900 AZI-AZI-360.2910 130 TLAPSB"CTOTAL(K>-TOTAL<K-1 ) )/RSTEP

2920 ALOV-HED(K-l )

| 2930 IF(AZM .OT. 0.) QO TO 2122940 AZH-AZI2950 DDI-HED(K)-HED<K-1 )

1 2960 GO TO 21 1B970 212 DAC-(AR(K)-AIl(K-l ) )/RSTEP

2980 ACR-DAC*STEP+AR(K-1 )

1 2990 TI0;"TLAPSE*STEP*TOTAL<K-l )

3000 PRINT 886AZMOISTHZTIHEAZIACR3010 IFCK OT JSAVC> GO TO 131

, 3020 123 CONTIWE| 3030 131 CONTINUE

3040 1 10 CONTINUE3050 86 FORHATC IK 4CF826X

1 3060 IRIME-IHIHE+l3070 IPdTYPE EQ. 13) IRIME-03080 IFdHlHE .EQ. 1 ) 00 TO 109

1 3090C AMY MORE TRAJECTORIES TO BE CALCULATED?3100 PRINTS IF MORE TRAJECTORIES ARE TO BE CALUCUALTED* PUNCH A"

31 10 PRINT-THO* IF NO MORE- PUNCH A ONE."3120 READ* IRUN3 130 IFC IRUN EQ. 1 ) GO TO 10003140 PRINT*" IF THE SAME iTIND DATA IS TO BE USED< PUNCH A ONE-"3190 PRINT*"IF NEW IMD DATA IS TO BE INPUT PUNCH A ZERO."

1 3160 READ* I DATA3170 IF< IRUM .OT. l > GO TO 1 163180 1000 END3 190 SUBROUTINE SNOCAR<VTERM*TMAX, I TYPE)

| 3800 DIMENSION VTERMC2)3210 109 IFdTYPE .Sa. D GO TO 1003220 IFdTYPE EQ. 2> 00 TO 101

1 3230 IFdTYPE Efl. 3) 80 TO 1023240 IFdTYPE EO. 4) 00 TO 1033250 IFdTYPE Ett 5) QO TO 104

1 3260 IFdTYPE EQ 6) GO TO 1053270 IPdTYPB Btt 7) 00 TO 1063280 IFdTYPE .EQ. 8) 00 TO 107

’ K > tir/ ITVP’f .’ ^ Ql FQ TO

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3318 (y< ITYPe BB. 14> BO TO 1 15 433330C SECTORS3340 TMAX-261 .3350 VTERM( 1 >-.243360 VTERM(2).A93370 00 TO 1083380C DENDRITES3390 100 TMAX-2613400 VTERM( D- .243410 VTERM(2)-.493480 GO TO 1083430C STELLARS3440 101 TMAX-2613450 VTERMC D-.243460 VTERM(2 )-1 .03470 GO TO 1083480C PLATES3490 102 PRINT*"PUNCH .MAX TEMPERATURE FOR CRYSTAL HABIABASED3500 PRINT<"ON SOUNDING AND AIRCRAFT DATA"3510 READjTMAX

3520 TMAX-273.+TMAX3530 VTERM( 1 )-.243540 VTERM(8>.83550 00 TO 1083560C SCROLLS3570 103 TMAX-265.3580 ITYPE-03590 GO TO 1083600C SHEATHS/NEEDLES3610 104 TMAX-269.3680 VTERM( l )-.243630 VTERM<2)1 .03640 GO TO 1083650C BULLETS3660 105 TMAX-248.3670 VTERM( 1 )-.53680 WERM(2>"1 .03690 GO TO 1083700C COLUMNS3710 106 TMAX-S68.3720 VTERMC D-.53730 VTERM(2)"1 .53740 GO TO 1083750C SIDE PLANES3760 107 TMAX2533770 VTERM( D-.243780 VTERM(2)493790 GO TO 1083800C PRISMS3810 1 1 1 TMAX-248.3820 ITYPE-03830 GO TO 1083840C ASSEMBLEQES OF PLATES3850 1 12 TMAX-255.3860 VTERM( 1 >>.243870 VTERM(2)-.49

3880 00 TO 1083890C ASSEMBLEGES OP SECTORS3900 1 13 TMAX-255.3910 VTERM( 1 ).243920 VTERM(2)493930 GO TO 1083940C ORAUPEL3950 1 14 C2"-.01930

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,; .-3990 Bl.363 44

4000’ 0-9806554010 XNEV-.1424020 RHO-1 15E-34030 XK2 .*G/(RHO*XNEW’-XNEW)4040 S-1 .274050 PRINT,"WAT IS 8RAUPEL DIAMETER IN CM?"

4060 REA’D^ 04070 IF( D .GT. .3 .OR. D .LT. .02) ITYPE0

4080 IFdTYPE .EO. 0) PRINT, "NOT VALID DIA. RANGE"

4090 IFdTYPE .EQ. 0) GO TO 1084100 XLOGM-ALOGCD/AD/B141 10 XM-EXPCXLOGM)4120 C0l4130 BE"XK*XM*S*CO4140 RE’EXP(C2^tALOO(BE)**2.+C3*ALOG(BE)+C4)4150 VXNEW*RE/D4160 VTERMd )"V

4170 PRINT^’GRAUPEL FALL SPEED (CM/SEC )"

4180 PRINT 9, VTERM( l )

4190 9 FORMATdOX^F6.1 >4191 VTERMd 5-VTERMd )*.01

4200 TMAX-258.4210 GO TO 1084212C AGGREGATES4213 1 1 5 TMAX-258*

VTERMC D-.54214421 5421642204230424042504260427042804290430043104320433043404350436043704380439044004410442044304440445044604470448044904500451045204530

VTERM<2)2GO TO 108108 IF< ITYPE .8T. 0) GO TO 1 10

PRINTS-NO DATA AVAILABLE- TRY ANOTHER CRYSTAL

READ- I TYPEGO TO 1091 10 RETURNENDSUBROUTINE ANGLE<X,Y-K,AZ,RANGE)DIMENSION X(200)-Y(200>- AZ(200)-RANGE(200)TANfl"ABS<Y<K)/X(KTHETA-ATAN(TANG)*57.284IF<Y(K) .LT. 0. .AND. X(K) .LT>. 0. ) GO TO 100

AND. X(K) .GT. 0. ) GO TO 101IF<Y(K) .LT. 0.IF(Y(K) GT. O.PHI-870.+7HETA00 TO 103100 PHI-270.-THETAGO TO 103101 PHI-90.+THETAGO TO 103102 PHI-90.-THETA103 AZ(K)PHITHETA-THETA/57.284RANGE( K)-Y< 10/SIBK THETA)/1852RANGE< K) <*ABS< RANGE( K) )

RETURNENDSUBROUTINE HEAD(AZ-R<JSAVE-HED-AR)DIMENSION AZ(200)-R<200)HED(200)-AR( 100)

PSI0.B-36.+36.BB36.X.5

AND. X(K> .GT. 0. ) GO TO 102

4540C PS I"ANGLE BETWEEN SEA AND ALPENTAL=0 DEGREES4550C AZ-AZIMUTH ANGLE COMPUTED BY VATRAJ4560C PHI"INTERIOR ANGLE AT ALPENTAL

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4596. IFtAZd ) .LT. 90. .AND. AZ( I ) .GT. 0. ) PHIAZ( I )+90.-PSI4600 IFCAZ( I ) .LT. 180. .AND. AZ( I ) .GT. 90. ) PHI-270.-AZ( I )+PSI

4610 IF<AZ( I ) .LT. 270. .AND. AZ< I ) .GT. 180. ) PHI270.-AZ( I )+PSI

4620 IF(AZ< I ) .LT. 360. .AND. AZ< I > .GE. 270 ) PHI=AZ( I )-270.-PSI4640 PHI-PHI/57.2844650C COMPUTE DISTANCE FROM ALP TO SEA4660 C"R( I )

4670 A-B+CC-2.*BBC*COS<PHI )

4680 A-SORT(A)

4690 ARC I )"A4700 H-R( I )*10.4705 IFCPHI EQ. 0. ) GO TO 1074710C COMPUTE ETA4720 C-C*SIN(PHI )/A

4730 CSC-l ./C4740 COT"SQRT(CSC*CSC-l )

4750 106 XTANl ./COT4760 ETAATAN(XTAN)4770 ETA"ETA*57.2844780 107 IF(PHI .EO. 0. ) ETA0.4790 IF(AZ( I ) .GT. 180. .AND. AZ( I ) .LT. 360. ) HBB/COS( PHI )

4800 IF(R( D GT. H) ETA-180.-ETA4810 X2"270.*PSI4820 H-l4830 ABAZ( I >4840 IF<AB .LT. (90.+PSI+X) .AND. AB .GT. ( 90 .+PSI -X) ) H=90.+PSI

4850 IF(AB .LE. (X2+X) .AND. AB .GE. (X2-X) ) H=90.+PSI

4855 IF<H .GT. 0. ) GO TO 1034860 IF(AB LT. 270. .AND. AB .GT. 90. ) H90.+PSI*ETA

4870 IF(H .GT. 0. ) GO TO 1034880 IF<AB .LT. 90. AMD. AB .GT. 0. ) GO TQ 101

4890 IF(AB .LT. 360. .AND. AB .GT. X2 ) GO TO 101

4900 IF<H .LT. 0. ) GO TO 1024910 101 H-90.+CPSI-ETA)

4920 IF<ETA .GT. PSI ) H90.-(ETA-PSI )

4930 IF(H .LT. 0. ) H"360.-<ETA-( 90 .+PSI ) )

4940 103 HED( I )H-224950 IF(HED< D LT. 0. ) HEDt I )=360.+HED< I )

4960 100 CONTINUE4970 RETURN4980 102 PRINT^’HEADING ERRORS"4990 HEDC D-999.5000 RETURN5010 END5020X,"AZIMUTH-* 10X^"RANGE*’-//)

READYBXVE

READYSAVE

READYRUNBIG

VATRAJ 1 5148 CSS WED.07/05/72

THIS PROGRAM COMPUTES THE TRAJECTORIES OF RIMED ANDUNRIMED SNOW CRYSTALS OF VARIOUS TYPES.ENTER THE STATION HEIGHT IN METERSINPUTS 00270? 900

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46

APPENDIX B

Format for Putting Ground Data on Computer Cards

All cards will contain the following information in columns 1 12.

Column 1 2:

Column 3 5:

Bureau of Reclamation site number. State of Washington

assigned code number 60.

Station number

001 North Benc

002 Bandera

003 Denny Creek

004 Alpental, bottom

005 Alpental, middle

006 Alpental, top

007 Hyak

008 Keechelus Dam

009 Cabin Creek

010 Kachess Dam

011 Stampede Pass

012 Nagron or Maywood

013 Greenwater

014 Mobile Van

015 University of Washington

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47

Column 6 7 Year

8 9 Month

10 11 Day

12 Card number

Card 0 Station description

Column 13 16 Do not use

17 79 Station description, latitude longitude, altitude,

instrumentation.

Card 1 Weighing bucket precipitation gauges

Column 13 16 Start time (PST) using 24 hour clock

17 20 Initial precipitation, each day started at zero inches.

21 24 Time internal for coincident precipitation (use 0060

for 1 hour intervals)

25 28 Total precipitation for day. Not necessarily the sum of

the hourly totals.

29 76 Precipitation amount falling in a one hour time interval

0000-0100, 0100-0200, etc. Record to nearest hundredth

of an inch using 2 digits.

Card 2 Tipping bucket precipitation gauge

Column 13 16 Start time (PST)

17 18 Time interval, in minutes for coincident precipitation,

use 15 minutes when possible

18 78 Number of tips of the bucket in the time interval, 2 digits

per observation

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48

Note: Conversion from tips to inches of precipitation is done by use of

proper conversion factors which, in turn, depend on the particular

gauge.

Card 3 Optical snow rate sensor

Column 13 Blank

14 17 Start time, PST

18 Blank

19 20 Time interval used for averaging

21 78 Average scale reading in time interval, recorded as

percent of full scale deflection, 2 digits per observation

Card 4 Ice nucleus data

Column 13 16 Start time, PST

17 18 Time interval for totalizing ice nucleus counts

19 78 Number of ice nucleus counts in time interval, 2 digits

per observation

Card 5 Freezing nucleus information

Column 13 16 Time sample collection started

17 20 Time sample collection ended

21 22 Temperature at which first drop froze. Since all

temperatures are negative record whole degrees Celsius

(e.g. -7C is 07, -14C is 14)

23 79 Number of drops frozen in each whole degree Celsius

interval, separate each value by a comma. Example: First

drop froze by -12C, at -13C there were 3 drops frozen,

at -14C there were 10, etc. Record as 121, 3, 10, etc.

Page 69: SO ROG - carg.atmos.washington.edu

49

Note: Conversion from number of drops frozen to the number of nuclei/gram

of precipitation is done by a computer program.

Card 6 Temperature

Column 13 16 Time of first observation (PST) start at 0000

17 19 Time interval between observations. If temperatures are

in F put a minus in column 17.

20 67 Temperature to nearest tenth of a degree, 4 digits per

observation, negative temperatures should be indicated by

a minus sign.

Note: Terminating readings in column 67 allow 12 observations per card.

Card 7 Wind speed and direction

Column 13 16 Start time (PST)

17 19 Time interval for averaging, in minutes.

20 67 Average wind direction and speed in time interval.

Four digits per observation. The first two digits

indicates direction in 10’s of degrees and the second

two digits indicates speed in mph.

68 71 Blank

72 75 Direction and speed of maximum wind for time on card

76 79 Time of maximum wind.

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50

Card 8 Pressure

Columns 13 16 Time of first observation (PST) start at 0000

17 19 Time interval between observations

20 67 Pressure in mb to nearest 0.1 mb for pressures

1000 mb or greater, drop the 1. (e.g. 1005.2 nib is

recorded 0052) Four digits per observation

Note: Terminating readings in column 67 allow 12 observations per card.

Card 9 Remarks

Column 13 16 Time to which remark is referenced

17 Card number to which remark is referenced.

18 19 Blank

20 79 Plain language remark indicating missing data, wind

direction shifts or other pertinent information.

Note: If remarks are to be made, record nines in the observation spaces on

cards 1 8.

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51

APPENDIX C

Aircraft Flights During Period January 1 to June 30, 1972

FlightNo.

92

93

94

95

96

97

98

99

100

101

102

103

104

105

106

107

108

109

110

112

115

116

Date

1/5/72

1/6/72

1/7/72

1/12/72

1/13/72

1/14/72

1/17/72

1/25/72

1/26/72

1/31/72

2/14/72

2/15/72

2/22/72

2/23/72

3/1/72

3/2/72

3/3/72

3/10/72

3/16/72

3/27/72

4/3/72

5/4/72

StartTime

1105

1142

1111

1123

1105

1153

1115

9251334

1107

1125

1125

1123

1057

1115

1132

1125

1112

1216

1210

1435

1200

1058

EndTime

1456

1251

1420

1432

1432

1443

1510

10251440

1245

1510

1547

1423

1444

1508

1349

1545

1532

1354

1258

1609

1250

1145

SeedingMaterial

CO,

None

CO, Agl

None

CO, 6 Agl

CO, S Agl

Agl

None

None

Agl

CO, S Agl

CO,

CO,

CO, & Agl

None

Agl

Agl

None

None

None

None

None

SeedingTime

1303-1355

1257-1315

1245-1313

1302-1330

1333-1441

1254-1406

1315-1411

1320-1349

1245-1252

1238-1402

1320-1455

1251-1440

Remarks

Storm Day, Orographic

Storm day danceled due to warm

temperature.

Storm Day, Post-frontal.

Avalanche hazard, no seeding.

Storm Day, Orographic

Storm Day, Orographic

Storm Day, Middle trough.

Test flight

Examined NE flow.

Storm Day, Upper trough.

Storm Day, Prefrontal

Storm Day, Postfrontal

Storm Day, Postfrontal

Storm Day, Postfrontal

Storm Day, Prefrontal

Storm Day, Postfrontal

Storm Day, Upper trough

Test flight

Hyak radar test with chaft

Test flight

Hyak radar test with chaft

Hyak radar test with chaft

Page 72: SO ROG - carg.atmos.washington.edu

52

APPENDIX D

(Abstract of paper accepted for presentation at the International Conference

On Cloud Physics London, August, 1972)

An Airborne Optical Ice Crystal Counter

by

F. M. Turner and L. F. Radke

The measurement of the concentration of ice particles in clouds

remains a significant problem in cloud and precipitation physics. Previous

devices designed for this task have generally provided either data of extremely

limited spatial resolution or data which required lengthy post-flight analysis

(e.g. continuous particle samplers). During the last few years we have

developed an automatic counter for use on an aircraft which detects ice

particles in the air but does not count even large water drops. This device

provides a continuous recording in real-time of the concentrations of ice

particles in clouds.

The present instrument (Figure 1) is an improvement on an earlier

design of the authors (see Hobbs and Ryan, 1969) and consists of two polarizers

set for maximum extinction through which a narrow beam of light is directed.

An ice crystal passing between the polarizers causes a slight rotation of the

incident plane polarized beam either by the optical activity of the crystal

or by scattering from its anisotropic shape and results in a light pulse being

detected by a photomultiplier. Cloud droplets being spherical and not

optically active, do not produce a rotation of the plane polarized beam.

Extensive laboratory and field tests have established that ice crystals with

maximum dimensions, in excess of 100 pm are detected with this device. The

sample area is adequately de-iced and the flow through it is isokinetic.

Page 73: SO ROG - carg.atmos.washington.edu

53

The signal from the photomultiplier is processed through two signal

conditioners, a pulse height discriminator and a pulse rate integrator. Both

of these signal paths are routed to logarithmic amplifiers and analog tape

recorded. The integrated signal is displayed to give direct read-out of the

concentration of ice crystals in the air. The results of recent measurements

in natural clouds will be presented along with other studies designed to

determine the minimum detectible size for different types of ice crystals.

Page 74: SO ROG - carg.atmos.washington.edu

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