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EUV Observations of the Structure and Dynamics of the Plasmasphere Bill R. Sandel, Jerry Goldstein, Dennis Gallagher, & Don Carpenter.

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Presentation on theme: "EUV Observations of the Structure and Dynamics of the Plasmasphere Bill R. Sandel, Jerry Goldstein, Dennis Gallagher, & Don Carpenter."— Presentation transcript:

1 EUV Observations of the Structure and Dynamics of the Plasmasphere Bill R. Sandel, Jerry Goldstein, Dennis Gallagher, & Don Carpenter

2 The Plan EUV Measurements Trough Formation Plasmasphere Erosion Bite-Outs (Low Density Regions) Flux Tube Refilling

3 The scattering rate or “g-value”: g = ~1.1  10 -4 sec -1 for He + at 1 AU The light detected by EUV comes from Resonant Scattering

4 Surface Brightness of the Plasmasphere The surface brightness is a line integral along the line of sight for each pixel:

5 Mapping image field points to the equatorial plane

6 To Sun Earth’s Shadow

7 Aurora Imperfect Flat-Fielding Between Cameras

8 Plasma Tail Plasmapause Plasmasphere

9 Extended Plasmasphere

10 Small Plasmasphere

11 (Thanks to Mark Moldwin)

12 Trough Forms by Wrapping a Tail 9 May 2001 2001-129

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19 Plasmasphere Erosion Events 10 July 2000

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21 Distance, Content vs. Time

22 Plasmasphere Erosion Events 2 June 2001

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25 Bite-Outs in the Plasmasphere

26 CRRES Results Carpenter et al., JGR 105, 23,323 (2000)

27 Green et al., JGR in press

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30 2001-097 & 098 (7 & 8 April) 87% CoR

31 2000-187 to 189 (5-7 July) 84% CoR

32 2000-176 to 177 (24-25 June) 98% CoR

33 Same as inner cavities observed by e.g. CRRES? CRESS*EUV Frequency13%less frequent Contrast5-10x2-4x Azimuthal Extentup to 20°10-18° Inner BoundaryL < 3~same LT Distribution< morning ? *Carpenter et al., JGR, 2000

34 2000-176 2001-097 RealModelled

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39 from Wilson et al., Adv. Space Res., 1993. Flux Tube Refilling--Expectations Latitude (degrees) H + Density (cm -3 )

40 26 August 2000 Isolated Refilling Flux Tube

41 20 August 2000 08:26 UTC Model of an Isolated Filled Flux Tube Range7.9 R E Latitude49 N

42 ?

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