Tutorial Lecturecedarweb.vsp.ucar.edu/wiki/images/7/70/1992_CEDAR... · 2015. 1. 8. · 20U...

51
1992 CEDAR Workshop Boulder, CO June 21-26, 1992 Tutorial Lecture by Michael Lockwood Rutherford-Appleton Laboratory Time-Varying Convection

Transcript of Tutorial Lecturecedarweb.vsp.ucar.edu/wiki/images/7/70/1992_CEDAR... · 2015. 1. 8. · 20U...

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1992 CEDAR WorkshopBoulder, CO

June 21-26, 1992

Tutorial Lecture

by Michael LockwoodRutherford-Appleton Laboratory

Time-Varying Convection

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i-

B

•. > •. .

vV-- V

Bow shock

Plasmasphere

Plasma sheet

Magnetopause

Plasmoid

Tail lobe

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m,

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1973.)

Merging Convective trcnsporl

do. "i^tside X-lineReccnrection

• Solar wind particleo Plasma sheet

The history uf a Jlclcl line. (After S.-I. Akasofu, Chapman Memorial Ucturc

3!nVerp\aneVoj^ F»e\i Line (^^<0)Clo§)e(Si GeofiQ^netic FieUOpen Ficli

.\m

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Co(ol^ ,1^^

(a)

(b)

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f UDlOb THE<^f\G-NET0S9H£^e.

ELECTRIC EQUIPOTENTIALS OR FLOW LINES

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OPEN MAGNETOSPHERE CLOSED MAGNETOSPHERE

Fig. 1. Electric equipotencials (or ExBflow lines) in the equatorial plane of idealized compleielyopen and completely closed magnetospheres.

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Fig. 2. Electric and magnetic fields measured belore andafter a dusk magnetopause crossing.

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(^02er

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MAGNETOSHEATH B^ . GAMMASFig. 4. Scatter plot of the viscous interaction potentialversus B, for 28 ma^etopause crossings within 2 hours oflocal dusk.

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^vaVggar aosarov

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APPLIED PHYSICS LABORATORYLaurel marviano

— 500 m/s

75

(a)

Goose Bay HF radar22 Apr 1988

1531:17 to 1540:38 UT12.4 MHz

65 j I I I i_

-80

S"

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Fig. 6

ft. ^>0

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Laurel maryiano

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c

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(a)

500 m/s

(b)..I i_

1100

Halley HF radar22 Apr 1988

_i L

1457:4610 1508:58 UT12.2 MHz

1200

Magnetic local lime

Fig. 7

1

1300

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1H€ JOHNS HOPKINS UMIVERSIIV

APPLIED PHYSICS LABORATORYU*UA€l

S 75 \ s

Goose Bay HF radar22 Apr 1988

1446:57 to 1448:18 UT •12.4 MHz

- ^

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0) *

• 1

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Magnetic local lime

500 m/S —

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Page 19: Tutorial Lecturecedarweb.vsp.ucar.edu/wiki/images/7/70/1992_CEDAR... · 2015. 1. 8. · 20U IMPLICATIONS CF THE 1100 UT Magnetopause GOES-3 MAGNETIC FIELD COMPONENTS «GEOS-2 SCATHA

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Inferred convection patterns in the Northern hemisphere

By< 0

0 02= Northward< By= Dawn-to-duskj of IMF

Component

Bv,>0

Bjr < InT /-y.

A - 50 Auroral oval

^InT

LT = Ohrs

sVeajly - paWerits \)«cao6C fto acoounli UKcn IHF or n^neVosj^eiic

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\r\

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0

, cCFj(Eii ne^liaikie)

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30SOUTHERN HEMISPHERE

1T T

R = 16.9 - 0.62

CO

5 20oc

-10.0 -6.0 -2i) 2.0 6.0 10IMF

Fio. 3. ComparisonOF CIRCLE RAOimft FMMf THIS STUDY ANDPREVIOUS SnjDY.

H012WORTH J^ AND MENG 1975

Polar Cop Flux^ F=bj If R®"R= 16-1-0-62fe2 (k.)

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e)2=T5nT, Fa. 5-fc*\o'Co\5foz=-5nT, F a ?>-2.xlO'(0b

AF/At ~ laokV = \ (Jor AU 1W.)

Page 23: Tutorial Lecturecedarweb.vsp.ucar.edu/wiki/images/7/70/1992_CEDAR... · 2015. 1. 8. · 20U IMPLICATIONS CF THE 1100 UT Magnetopause GOES-3 MAGNETIC FIELD COMPONENTS «GEOS-2 SCATHA

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~ 1 h

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e Central PC Voltage

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_L_

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V

Decay

Time

i(\ onli^Ja .eien a(hi koe rCSOonM tiif> ^cciusyiL

ir

Page 24: Tutorial Lecturecedarweb.vsp.ucar.edu/wiki/images/7/70/1992_CEDAR... · 2015. 1. 8. · 20U IMPLICATIONS CF THE 1100 UT Magnetopause GOES-3 MAGNETIC FIELD COMPONENTS «GEOS-2 SCATHA

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IVfon -S^eo^ani ^ solar locni e\et^ric '\eW (iocofi ojaf\

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la. - 5i_ =

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' •^i \fF

For 'bWri Gop qV = folO'^mTrVz

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= 0-01aTs-'

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i un voVick•lu (f)"

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^\o(Of g^rox^ ^Wite las'if^(vOksVea^ I^a^(\e\\c e(\€^^ ib koc^^ \(\ l:l\e Wil)

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20U IMPLICATIONS CF THE 1100 UT

Magnetopause GOES-3

MAGNETIC FIELD COMPONENTS

«GEOS-2

SCATHA c

30l 1 ' ' 1

JS77-007

QOES-3

S/C POSITIONS

AT 1IKK) UT

MARCH 22. 1979

60

h-

S 20.0

Q

-20

X J\y

! ! 1 1 1 1 1 1 1 1

to

P -50c

>-90^ v1 ! 1 1 1 1

iseE-2

\ISEE-1 I0<00

Figure 1. Location of seven spacecraft during theCDAW-6 substormof 11UTon March 22. 1979. Note the radial alignment offoor satellites along the 0200 LT 3 Magnetic field measurements made by the magnetometer on sateflimeridian-with lSEE-l ataGSE positionof(-13.6 R,.-7.2 Rj, 0.6 R.) and ISEE-2 gOES-3 during the CDAW-6 substorm of11 UT on March 22. i979. See tcat(-12.1 Rj. -7.1Jlj,OJRe). The relative positions ofthese satellites changed very definition ofV, D, and Hcomponents.little during the event discussed here.

11=00

MARCH 22.1979

I2=0C

FRITZ ET AL. 205

tMAGN£TIC FIELD IS6E-1MARCH 22. 1-979

1 1 1 1 1 1 i 1 1 1 1 i-)- ^

1 1 1 1 1 1 1 1 1 1 1 1

1 RECONFIGURATION AT'IIgegstatignary orbit1—

1 1 1

>i-nr^ • I— f I 1 f—

1 1 1 1 1 1 fi 1 1 1 1 1 1 t 1

Universal Time

fi?"" ^®8netic field measurements in GSE coordinates made by the magnetometer on satellite ISEE-1 during the CDAW-6 substorm of 11UT on March 22.1979.

FnkcVQ\. (\SS4;)

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SB 'BM

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ElSCATSCiEMlI-IC

P.O. Box 812

S-98I 28 KIRL'NA. Sweden

Phone +46-980-79150/79153

Telex 8778 EISSWES

Fax +46-980-79161

-• •• • .

ElSCATTroniso

Ramfjordmoen\-^(127 R.AMRIORDBOTN . N.ar\va> •

Phone +^"-.S3-^Clfi''-'A>21W " '\EiSNO v

l-ax -=-ii''-S3-«23S0

FIS( AT Kiriin:!

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HISCAT SouiinkylaGeoph\sicat ()hser\iai>r\SF-9961H) SODANKYK.A. Finlatul

Phone-^?5S-693-I2462

Telex 37254 C'.KFSO Si-

Fax -A^S-^g.-1252S

1\

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Phil. Trans. R. Soc. Lond. A,

Ivoo Isoo |900 liooo IllOO I 1200 §1300 |

12h00 UT

respectively), observed by AMPTE-UKS when locaEd immediately mThe simuhaneous observaiions by the eiscat radar Thp now , "^ard ot the Earth s bow shock, i)avoid congestion of the plot; hence north3 flow iJhown K 90^and westward flow by vectors directed uoward ^^i e fh ^vectors directed to the right of the figureThe vectors are superim^sJd oi acdouHfn^ithe vectors are mthe direction of the electric field).Willis a/. 1986.) ^ two-mmute averages of the ion temperature, T, (From

Page 32: Tutorial Lecturecedarweb.vsp.ucar.edu/wiki/images/7/70/1992_CEDAR... · 2015. 1. 8. · 20U IMPLICATIONS CF THE 1100 UT Magnetopause GOES-3 MAGNETIC FIELD COMPONENTS «GEOS-2 SCATHA

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Page 33: Tutorial Lecturecedarweb.vsp.ucar.edu/wiki/images/7/70/1992_CEDAR... · 2015. 1. 8. · 20U IMPLICATIONS CF THE 1100 UT Magnetopause GOES-3 MAGNETIC FIELD COMPONENTS «GEOS-2 SCATHA

M

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^southward turning

• northward turning

"k

09:00 12:00 15:00

Magnetic Local Time

/•\

18:00

Page 34: Tutorial Lecturecedarweb.vsp.ucar.edu/wiki/images/7/70/1992_CEDAR... · 2015. 1. 8. · 20U IMPLICATIONS CF THE 1100 UT Magnetopause GOES-3 MAGNETIC FIELD COMPONENTS «GEOS-2 SCATHA

a)

b)

Polar Cap Boundary

Old Polar CapBoundary

Phase Motion

Reconnection X-line

mapped to ionosphere

Pkase 10k« nu

Oire<^ O^^soveA ^ Lockwood e'al.baol\Aers eVal

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9(jliaro\c se^nenVs ^open /c\osed boun^a^t(^ean'»^ " Qcross") - InVna^ocei ^S\scoe qoA Wuan^ (\Sft5)«Operv /closed \:>oua^Qnj, OlM j\E^T fWRfHE

v=iE>^e>yb'-

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VoWa^e, 0^^= ^E!j.il ^Oft

^ Forai^s Laio 0' is a jlux Vran^r ra^e1>'7ft(

j

Pkfevo\\^e across covresjion^"*^ rccon(\€^or\ X-lioe

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r7ovift0 Open /OosedDounAai^ Sjieexi 'jrx EBKTH'Sf ll>ecQwse polar cap cxpQtJis/conVroicW )

>\plastna speei^ ^ A i Et

Y V V V y e>

T ploswoL speeA ^ -V|

VJ V.

V

fti\aro\c EB yP

Et =-

Vo\Va^e^ 0^p^= ^-\6|Al=K-v,)6,.

-

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//

/

flow streamline

adiaroic open/closed boundary

boundary motion

CoJW^ (nn)

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FaraAa 'S Laco appVieA. fe polar cap:

§ E.Al =a(E).ftp,Vat=

Expanding Polar Cap Contracting Polar Cap

d ' n(b)ti>d =0 ci>, =8A

(d)J)^j=2Ai^>n=4A

flow equipotential (A kVoport)ionosptieric projection ofreconnectionneutral line (merging gop)adioroic polar cap boundaryboundary motion _ v . i , ^

^iscoe ond nuarjgLocVwooA ai>ji Cowl^ (.¥^88)LocVvcOooA eVa\.?lo5be\\ <.^71)

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Zero -j^\o(o ec^u'iVibnuA^Of^lOVl 'oVlOOS (,Co(oW QO^ LocWool^

12 mi)

18-

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iWiom co(\ i^uraVlon?) onlj assorncji drcJar here... V ^or lUoaravwe purposes

jlox (iF woM (\oV Wojieoe^ \(\^\afVaoeoublLo^vooo\ eV 0^. (mo) e^mVe Af/F ^0-05ir* rcai aneoo^

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Page 41: Tutorial Lecturecedarweb.vsp.ucar.edu/wiki/images/7/70/1992_CEDAR... · 2015. 1. 8. · 20U IMPLICATIONS CF THE 1100 UT Magnetopause GOES-3 MAGNETIC FIELD COMPONENTS «GEOS-2 SCATHA

(a) 24(b)

06- Flux F - 18

•3°f'ao \oc«iV>ot\

(c) (d)

F + dF

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Zero -J-\0(0

(XnVxAoce^ 1Cou)»eu afva ko^vooodi.

mlf

over <».\<^tW Sc^ <in^

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:. Lo^VtrtO aMero<^ o«e

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sVtflX^

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fVlorVKtoard XfOF SulssVorms(a)

uiAi 0i'=^n=O

i>i-^0n' 'O

>0

9^0 >0

0V =0

(b)

(c)

adiaroic open / closed boundary

merging gap

» flow streamline

boundary motion

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Vart viscoi)^()r\>itf\ cc\W.

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li

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celU are no \o

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laVcrflM^ioO.

Lo^woA an^ Cot^^ (Wi)

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WVOANT CT AL.: POLAR CAI' rOTCmiAL ANU RCCONNECTION MODELS

B^>0

„._3456703

•* HOURS Bg > 0Fig. 6. The cross polar cap polenlini Uu.ing |)erioils wlicn tf/' ''was northward versus the number of hours previousto the measurement of the polarcap potential that v/as northward.

]or \:^0ra(\^ AonA ^ ^rv/X.

Aecojs over t ' lokrs

5731

|)c I >ecau%e.

- ^ -v lOkV?

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1.5. ra<^Q,rt f<\a^neVor<>^€r

bservaViorNS^ivel(^oi co(\v/€^ior\ _ •

\ye

^n»cj,ue:-

Knipp ct al.: Ionospheric Convection Response

If^oipp dr al.(Gcopn^».Pi«>. \*W\}

Vk

. JULY2S, W83INTE JPLAKETARY MAGNETIC FIELD

iT'

vJ>j!

By'iaSflTtSJwIytS 8v»20.5«T OJiHySS It By*jO^OOUT^"" -^>.^j.-64nT lOSO OT'f T —

y SO- >•< V

^ ^^-40 "ZO ^a

00

f>OTOfnAL DiFFEKENCe • 1194 kV FOTOmAL OtFFEKEKK* • 94.1 hV

tS Ally 69 By-S.ZnT U July63 12 6Y*2SnTlO'40aT^^ T 2l.6ftT K>50 UT^" —T*Vt.Xv 62*fl6«T

SO* ^SO-

106 Ml

17.4 nT

00 02 04 06 06 10 12 »4 « M 20 22 00

1. IMP-8 IMFdata (GSMcoordinates) for 23 July 1983. K>TCMTVU. OtTFCftCNCC • 63 8 kV WTNTUU. DtPFKNCNCC • crV kV

WorWioaA

\0-.15 UT c\ --e,

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I- !.• •, A,U r \]'\<]\)

23 Jvly 631109 OT

s-id^

By-10.6aT 23Ally 63Bj*l92nT IfSC UT

POTtlfnAL 0#FtH£NCE • 75.6 kV FOTENTUL0<FTERE>ICE • 474 kV

Fig. 3. Fitted electric potential patterns for selected timesbetween 1000 UT and 1130 UT on 23 July 1983. Thecontour inteival is 10 kV, The IMF values are shown at theupper right. Inregions where the uncenainty in the large-scaleelectric field is 50% or gre;aer the contours are dashed.

•tokv

2)5 KV

0^ Qfti\Omia

aaX jUoAeco^ *ii\ wcroi\ kootb

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2-^

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Ex

:J". ^qc 'iAc QfiA ^Qotn'toVarvn.

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5^

61 U40

portsioo

:c'ELECTRIC POTENTIAL

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F

ELECTRIC POTENTIAL

12

me\Vo\C0F\(0-6

XX l*)orcU971

CONTOUR

INTERVAL

15 KV

CONTOUR

interval

15 KV

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0d'

0-

0

0,

^max~' o''"^^^max^®pc (^pc~0/)

/

/

/

//

I (growthphase)

^ < »

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c (onset) ^«K= roo««

d (convection bay)

(expansion/recovery phase)

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0 pc

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A

\

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r

0,

/

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i

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/#

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9

/

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'' d (expansion phose)

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Circular Polar Cap

w /i+4'0 pc

uV ACoto^ dm)

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-Q

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' max/I

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Adapted from Hairstonand Heelis(1990)

mm

1

20 40 60 80 100 120 140 160

Transpolar Voltage, </) (KV)pc

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Sumcuir3

c

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• V^O(<\PQn5on ^ ionospWric

Ex' diftS of>A 00 conviecHofx

VansjiAir vc^lc^C/ w)iH\ie<]tton is ore^oKirMi«UvottQQe QcroQb i-UDL sWocos convedion, *5 predoKiOanj^

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• t^Vi. e(«Yncal c- <jonvi€<^i»of\ afv^ fOOST coocejilyolones QS6oroe yeoiu stfe

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ioes cro&Ss no(\

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v\5coys -\^e vleraclroa \s \n res"\(^oc^ft\^side, veoor>ne<^(oa

~TrarvS|)lQr \j^(xc\t Qfv^ piar cap size \/aru vo ar^v)ior vo^ aofi^ (;ke subsom c^c\e

ft.loio PaUerns