Difference between revisions of "12/25/2013 05:00:00 UTC"

From heliophysics
Jump to: navigation, search
(Comment Section)
(Comment Section)
 
Line 1: Line 1:
 
=Comment Section=
 
=Comment Section=
*Weak but clear magnetic cloud structre. Velocity profile shows gradual decline indicating expansion and magnetic field shows signs of rotation in both x and y directions (Hess)
+
*Weak but clear magnetic cloud structre. Velocity profile shows gradual decline indicating expansion and magnetic field shows signs of rotation in both x and y directions. The solar counterpart for this event isn't obvious, but given the rather slow bulk speed at 1 AU (< 300 km/s) a Halo CME on the 19th is a possibility. (Hess)
  
 
=Image Data=
 
=Image Data=

Latest revision as of 14:11, 29 August 2014

Comment Section

  • Weak but clear magnetic cloud structre. Velocity profile shows gradual decline indicating expansion and magnetic field shows signs of rotation in both x and y directions. The solar counterpart for this event isn't obvious, but given the rather slow bulk speed at 1 AU (< 300 km/s) a Halo CME on the 19th is a possibility. (Hess)

Image Data

In-Situ 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