RELATION BETWEEN RING CURRENT, IONOSPHERE AND PLASMASPHERE - PowerPoint PPT Presentation

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RELATION BETWEEN RING CURRENT, IONOSPHERE AND PLASMASPHERE

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I = integrated region 2 FAC (Iridium) U = Sub-auroral potential drop (DMSP) ... Outward or poleward E-field required to brake drift. Two possibilities: ... – PowerPoint PPT presentation

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Title: RELATION BETWEEN RING CURRENT, IONOSPHERE AND PLASMASPHERE


1
RELATION BETWEEN RING CURRENT, IONOSPHERE AND
PLASMASPHERE
  • P. C. Brandt

2
KEY EFFORTS
  • John Foster
  • Phil C. Anderson
  • Jerry Goldstein
  • Mei-Ching Fok and Y. Ebihara
  • R. A. Wolf
  • T. Immel

3
E-FIELD OF THE INNER MAGNETOSPHERE
CONVECTION COROTATION
SELF-CONSISTENT
SUB-AURORAL E-FIELD
4
  • How and when is the sub-auroral electric field
    formed?

5
REGION 1
REGION 2
EXTENDING TO PLASMASHEET
6
HOW AND WHEN?
  • Duskside R2-FAC close poleward through
    low-conductance gap
  • Significant E-fields
  • Moderate R2-FAC

AURORAL OVAL
LOW CONDUCTANCE
7
TEST
I integrated region 2 FAC (Iridium) U
Sub-auroral potential drop (DMSP) R Resistance
between Region 2 and Region 1 RconstD,
Dseparation ? U/(DI)constant?
I
R
U
8
CURRENT
ALL IRIDIUM DATA FROM H. KORTH AND B. J. ANDERSON.
9
RELATION TO RING CURRENT
  • Proton pressures from HENA ? Current
  • Underestimating
  • 10 min resolution

10
SUB-AURORAL POTENTIAL
ALL DMSP DATA PROVIDED BY P. C. ANDERSON
11
SEPARATION?
MLAT1 EQUATORWARD EDGE OF OVAL MLAT2 90
VALUE OF SAPD
MLAT2
I
D
D
R
MLAT1
U
12
I VERSUS U
13
D VERSUS U
14
DI VERSUS U
15
  • How does the sub-auroral E-field affect the inner
    magnetosphere?

16
  • PLASMASPHERE

17
UNDULATION
Courtesy of J. Goldstein
18
SUB-AURORAL E-FIELD?
HENA CURRENTX 70
IRIDIUM CURRENT
SEPARATION
POTENTIAL
1936 UT UNDULATION
1900 UT AURORAL ONSET
19
SUMMARY
  • Sub-auroral E-field depends more on size of
    low-conductance gap, than FAC intensity.
  • Expected for a low-conductance gap
  • Sub-auroral field modifies E-field of inner
    magnetosphere

20
  • EQUATOR?

21
EQUATORIAL FOUNTAIN
E-FIELDS LIFT PLASMA ACROSS B-FIELD
NEUTRAL WINDS FROM SUB-SOLAR POINT
22
IONOSPHERIC BUBBLES
DRIFT
BUBBLE
23
DRIFT VERSUS DST
  • Eastward drift correlates with Dst.
  • Outward or poleward E-field required to brake
    drift.
  • Two possibilities
  • Direct high-latitude electric field effects.
  • Reversal of thermospheric neutral wind, through
    high latitude heating.

Fejer et al., 1993
Immel et al., JGR, submitted, 2003.
24
CLUSTER-IMAGE
25
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