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1. Magnetopause moving at extreme velocity Knut Stanley Jacobsen, University of Oslo. 2. Magnetopause moving at a speed of 800 km/s. 3. The velocity is perpendicular to the magnetic field. 4. Ground signatures were observed. DRBY H. DRBY D. DRBY Z. PINE H. PINE D. PINE Z. 5. THD V.
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1 Magnetopause moving at extreme velocity Knut Stanley Jacobsen, University of Oslo
2 Magnetopause moving at a speed of 800 km/s
3 The velocity is perpendicular to the magnetic field
4 Ground signatures were observed DRBY H DRBY D DRBY Z PINE H PINE D PINE Z
5 THD V ACE B THB B Density V_x V_y V_z Temp. Ppla+ Pmag Ppla+ Pmag+ Pram Hot Flow Anomaly
6 The magnetosheath first hits D, then E, then A TH <-B <-B <-A <-D <-E
7 The order of magnetosheath encounters indicate something moving tailward GSM position at 14:05 -0.43 -30.45 4.20 2.16 -11.45 1.67 1.19 -11.57 1.55 -0.28 -14.10 1.93 Separation of D and A in XY-plane ~= 3.6 R_E To close this distance in ~60 secs requires a speed of ~380 km/s
8 Example of similar event: 2007-09-04 - No esa data for Themis B and E, and no high-resolution data for Themis A. - Magnetopause velocity exceeds 600 km/s
9 Example of similar event: 2007-08-28 - All spacecraft have high-resolution data. - They are located inside the magnetopause at different distances. - Magnetopause velocity exceeds 600 km/s