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*Depressed density and temperature as well as decreasing velocity are indicative of a flux rope, but with the weak magnetic field it may just be the flank passing through the Earth. Clear shock signatures in temperature and velocity and total B, more of a gradual increase in density. (Hess) | *Depressed density and temperature as well as decreasing velocity are indicative of a flux rope, but with the weak magnetic field it may just be the flank passing through the Earth. Clear shock signatures in temperature and velocity and total B, more of a gradual increase in density. (Hess) | ||
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| + | "This event must have impacted Messenger at Mercury, which is roughly 30 west of the Sun-Earth line." (Moestl) | ||
=Image Data= | =Image Data= | ||
Revision as of 07:18, 19 October 2015
Contents
Comment Section
- This is a varSITI campaign event for ISEST and SPeCIMEN.
At the Sun the event had an M1.1 flare, erupting filament, type IV radio burst, fast halo CME. At Earth a shock, possible MC, SEP, and strong storm, Dst=-132. A TB case. Modeled by C-C Wu. [Added by D. Webb]
- Depressed density and temperature as well as decreasing velocity are indicative of a flux rope, but with the weak magnetic field it may just be the flank passing through the Earth. Clear shock signatures in temperature and velocity and total B, more of a gradual increase in density. (Hess)
"This event must have impacted Messenger at Mercury, which is roughly 30 west of the Sun-Earth line." (Moestl)
Image Data
In-Situ Data
A combination of SWEPAM and MAG data from the ACE Satellite:
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The blue lines are an approximation of the CME cloud and the red line denotes the shock.
Heliospheric Imager Data
