Radiation Belt Storm Probes and Space Weather D. G. Sibeck LWS Geospace Project Scientist.
1 Dynamic Motion of Bow Shock and Magnetopause Observed by THEMIS Hui Zhang (BU) Q.-G. Zong (Umass...
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Transcript of 1 Dynamic Motion of Bow Shock and Magnetopause Observed by THEMIS Hui Zhang (BU) Q.-G. Zong (Umass...
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Dynamic Motion of
Bow Shock and MagnetopauseObserved by THEMIS
Hui Zhang (BU)
Q.-G. Zong (Umass Lowell)
D. G. Sibeck (GSFC)
T. A. Fritz (BU)
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Magnetopause Bow shock
?
13.5
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3Magnetopause Bow shock
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Normal directions of boundaries
UT boundary Normal direction (GSE)
Method
05:50 Magnetopause (0.980,-0.103,-0.169) MVA
07:52 Magnetopause (0.996,-0. 080,-0.044) MVA
07:54 Magnetopause (0.985,-0. 077,-0.153) MVA
07:59 Bow shock (0.813,-0. 292,-0.504) Coplanarity
08:01 Bow shock (0.292,-0. 550,-0.782)* Coplanarity
11:06 Bow shock (0.956, -0.142, 0.256) CoplanarityShock normal from coplanarity method: n=(BuxBd)x(Bu-Bd)/|(BuxBd)x(Bu-Bd)|
*question: why the shock normal at 08:01 is different from others?
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Magnetopause Discontinuity
Timing analysis shows:Both the magnetopause and the discontinuity move anti-sunward but at different speed.Magnetopause: ~30 km/s; discontinuity: ~ 90km/s.
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Vx ~ 90 km/s Vx ~ 30 km/s
Discontinuity
Magnetopause
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• Magetospheric population peaks at ~ 6 keV, and this peak is not present in
the magnetosheath from 0755 to 0757, suggesting these ions are not from
magnetosphere.
Where are the energetic ions (~10 keV) from?
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• Not from the sun
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Theta Bn:
Angle between the
IMF direction and the
shock normal
where Shock normal
is (0.956, -0.142,
0.256)GSE
(from THEMIS B
observation at
~1106UT)
Time difference is
2 hours!However…
Shock acceleration?
Quasi-Para Shock Quasi-Perp Shock
WIND data
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Summary• The magnetopause was found moving anti-sunward at ~30 km/s.
• Two subregions have been observed by all 5 THEMIS spacecraft
in the magnetosheath associated with a discontinuity. This
discontinuity traveled from the bow shock to the magnetopause at
Vx ~ 90 km/s.
• Both low and higher energy ions are observed in the first region
and only low energy ions are observed in the other subregion.
• What caused the shock, magnetopause moving anti-sunward?
• Where are the energetic ions (~10keV) from?
– Not from the solar wind
– May not from the magnetosphere
– Quasi-Parallel shock acceleration? Has problem to correlate the IMF
with the discontinuity marked by red arrows on slide 5.