Anti-parallel versus Component Reconnection at the Magnetopause
Tutorial Lecturecedarweb.vsp.ucar.edu/wiki/images/7/70/1992_CEDAR... · 2015. 1. 8. · 20U...
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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la. - 5i_ =
u 05 co(\siler r>€eiei fe (TNoke. E;=0^or ^\f, (<\V rrf^ arA =50aT ,aasojn*^ "lO^e^^V (^ SCq(\ \Wr> use a r'\ole\ (T^<^oefk5 "V87 nck\)\b co(npttfe J_ As
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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
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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
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^southward turning
• northward turning
"k
09:00 12:00 15:00
Magnetic Local Time
/•\
18:00
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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
![Page 35: 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](https://reader034.fdocuments.in/reader034/viewer/2022052103/603e63315cf64148193c83e6/html5/thumbnails/35.jpg)
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)
![Page 38: 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](https://reader034.fdocuments.in/reader034/viewer/2022052103/603e63315cf64148193c83e6/html5/thumbnails/38.jpg)
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)
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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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(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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fVlorVKtoard XfOF SulssVorms(a)
uiAi 0i'=^n=O
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>0
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0V =0
(b)
(c)
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merging gap
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boundary motion
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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,
lO-.ZSOTaV r<\c^t\^oj>q06€.
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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0 pc
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