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Published byErica Barker Modified over 9 years ago
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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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The Plan EUV Measurements Trough Formation Plasmasphere Erosion Bite-Outs (Low Density Regions) Flux Tube Refilling
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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
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Surface Brightness of the Plasmasphere The surface brightness is a line integral along the line of sight for each pixel:
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Mapping image field points to the equatorial plane
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To Sun Earth’s Shadow
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Aurora Imperfect Flat-Fielding Between Cameras
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Plasma Tail Plasmapause Plasmasphere
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Extended Plasmasphere
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Small Plasmasphere
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(Thanks to Mark Moldwin)
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Trough Forms by Wrapping a Tail 9 May 2001 2001-129
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Plasmasphere Erosion Events 10 July 2000
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Distance, Content vs. Time
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Plasmasphere Erosion Events 2 June 2001
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Bite-Outs in the Plasmasphere
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CRRES Results Carpenter et al., JGR 105, 23,323 (2000)
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Green et al., JGR in press
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2001-097 & 098 (7 & 8 April) 87% CoR
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2000-187 to 189 (5-7 July) 84% CoR
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2000-176 to 177 (24-25 June) 98% CoR
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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
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2000-176 2001-097 RealModelled
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from Wilson et al., Adv. Space Res., 1993. Flux Tube Refilling--Expectations Latitude (degrees) H + Density (cm -3 )
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26 August 2000 Isolated Refilling Flux Tube
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20 August 2000 08:26 UTC Model of an Isolated Filled Flux Tube Range7.9 R E Latitude49 N
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