Advanced Ionospheric Sounding with Vertical Incidence ...
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Advanced Ionospheric Sounding with Vertical Incidence Pulsed Ionospheric Radar Dr. Terry Bullett University of Colorado Boulder Cooperative Institute for Research in Environmental Sciences [email protected] In Cooperation with: National Oceanic and Atmospheric Administration National Geophysical Data Center Solar and Terrestrial Physics Division For: LISN Workshop November 2011
Transcript of Advanced Ionospheric Sounding with Vertical Incidence ...
AdvancedIonospheric Sounding
withVertical Incidence
Pulsed Ionospheric Radar
Dr. Terry BullettUniversity of Colorado Boulder
Cooperative Institute for Research in Environmental [email protected]
In Cooperation with:National Oceanic and Atmospheric AdministrationNational Geophysical Data CenterSolar and Terrestrial Physics Division
For:LISN WorkshopNovember 2011
Outline
● Vertical Incidence Pulsed Ionospheric Radar ● Impulse Response and Precision Range● O/X Polarization● Shuffle Mode● Meteor Trails● Shuttle Modified Ionosphere● Daily Summaries● Autoscaling● VIPIR Locations● Resources
Research Ionosonde: Wallops Island, USA Vertical Incidence Pulsed Ionospherc Radar (Dynasonde)
VIPIR Receive Array
Transmit Antenna (simulated)
Typical LPA Radiation Pattern
Wallops Tx Antenna Performance
Puerto Maldonado Tx Antenna
WI937 Signal and Noise Spectrum
50 dB
PM91K Signal and Noise Spectrum
35dB
Receive Antennas: San Juan4m dipoles , 5m high
San Juan ObservatoryPuerto Rico
Vertical Gain vs Frequency
Circular Polarization Example
● Two orthogonal antennas
● Separate receivers
● O and X mode signals
● Magnitude [dB]
● Phase [deg]
● -90 for O-mode
● +90 for X-mode
● Phase shift even receiver data +90 and – 90 and sum with odd receiver data
SJJ18_2010308180508.RIQ
+90
-90
Rx2-X
Rx1-X
Rx1-O
Rx2-O
Equatorial O/X Polarizations are orthogonal linear!
Polarization Example
Receive Array: San Juan
Antennas at locations: -9 -3 -1 0 +4Gives separations of 1 2 3 4 5 6 7 8 9 13Units of 7m
Can use any 8 antennassimultaneously
Precision Range● Use the high SNR and precise receiver response● Properly sampled receiver output● Fit a raised cosine function to the amplitude data
● Ao, Ro, W Ax =Ao [ 12 1cos
x−RoW ]
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Impulse Response Fitting
Ao=58.6 ; Ro=166.7Ax=53.3 ; Rx=176.9
Precision is about 0.1 range gate (150m)Depending on SNR and echo separation
Measuring Es Thickness
● Precise echo range from VIPIR Receiver impulse response
● Fit parabolic layer● foEs= 2.37 MHz● hmEs= 104.6 km● ymEs= 3.84 km
N h=N m 1−h−H m
2
Y m2
Wallops Island30Oct07 03:47UT
Interferometry● The phase difference
between spaced antennas related to the angle of arrival of a plane radio wave
● Issues:
● 2π ambiguity ● Non-plane wave● Mutual Coupling
● Multiple spacings aid to resolve this problem
● Room for Improvement
D
1 2
k
2−2=∣k∣D sin
Shuffle ModeInterleave a sweep frequency ionogram with a fixed frequency HF radar observation on a pulse-by-pulse basis
Sweep Pulse 1Sweep Pulse 2Sweep Pulse 3
Sweep Pulse N
Tim
e
Fixed Pulse 1Fixed Pulse 2Fixed Pulse 3
Fixed Pulse N
Tim
e
Sweep Pulse 1Fixed Pulse 1
Sweep Pulse 2Fixed Pulse 2
Sweep Pulse 3Fixed Pulse 3
Sweep Pulse NFixed Pulse N
Tim
e+
● More efficient use of radar resources
● Addresses rapid scale dynamics
200GB per day!
Shuffle Mode Ionogram
Shuffle Mode Fixed Frequency
Meteor Trails at 18.6 MHz
Meteor Trail Data
q
Meteor Trails at 5.8 MHz
12 3
Meteor Signals
Vlos= 41 m/s
Shuttle Modified Ionosphere
300 km
T+08:00T+04:00
105 km
113 km
STS-135 Trajectory
Modified IonosphereSignature
Shuttle Modified Ionosphere
Detailed View
PM91K 3D Power Spectrum
WI937 3D SNR Spectrum: E-Layer
Autoscaling: ESIR● Expert System for Ionogram Reduction● URSI Characteristics● Electron Density Profiles
ESIR Scaled Ionogram
5-day foF2 Plot
VIPIR Facilities
Planned (11)Current (7)
Updated August 2011
Credits
● LISN Program
● Boston College
● NOAA National Geophysical Data Center
● NASA Wallops Island Flight Facility
● NASA Heliospheric Division
● US Geological Survey
● US Air Force Research Laboratory
● US Naval Research Laboratory
● Scion Associates
● Jicamarca Radio Observatory
● All ionosonde data producers who freely share their data!
Questions?
SpaceWeather?
Internet Resources
● World Data Center A, Boulder: http://www.ngdc.noaa.gov/stp/IONO/ionohome.html
● Digisondes and ARTIST : http://ulcar.uml.edu/
● Autoscala: http://roma2.rm.ingv.it/en/facilities/software/18/autoscala
● ESIR : http://www.spacenv.com/
● Dynasonde21: [email protected] ; [email protected]
● Low-latitude Ionospheric Sensing System: http://jro.igp.gob.pe/lisn/
● Vertical Incidence Pulsed Ionosphere Radar (VIPIR): [email protected]
● Canadian Advanced Digital Ionosonde (CADI): http://cadiweb.physics.uwo.ca/
● Ionospheric Prediction Services (IPS): http://www.ips.gov.au/
● Ionosonde Network Advisory Group (INAG) http://www.ips.gov.au/IPSHosted/INAG/
● SPIDR: http://spidr.ngdc.noaa.gov/spidr/index.jsp
