03/31/2015 07:31:49 UTC

From heliophysics
Revision as of 12:55, 16 September 2017 by Ytchi (talk | contribs) (Created page with "=Comment Section= *Clear shock, followed by most of the standard MC signatures (low beta, low density, rotating magnetic field, etc.), but a fairly weak total magnetic field s...")
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
Jump to: navigation, search

Comment Section

  • Clear shock, followed by most of the standard MC signatures (low beta, low density, rotating magnetic field, etc.), but a fairly weak total magnetic field strength. The CME probably wasn't passing near the nose (Hess)

Image Data

A combination of SWEPAM and MAG data from the ACE Satellite:

Error creating thumbnail: File missing
Error creating thumbnail: File missing
Error creating thumbnail: File missing


The blue lines are an approximation of the CME cloud and the red line denotes the shock.

Video Data

References