shine_2006 the 20 january 2005 flare/ cme is associated with a very energetic (and prompt) sep....
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SHINE_2006
The 20 January 2005 flare/ CME is associated with a very energetic (and prompt) SEP.
Ulysses .
20 January 2005 CME
LASCO C2
SMEIB.V. Jackson P.P. Hick and A. Buffington, Center for Astrophysics and Space Sciences, UCSD
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20 January 2005 CME
SMEI
Ulysses
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The bulk of the 3 x 1017 g of material reached 1 AU in about one day indicating an average speed for this mass of approximately 1600 km s-1, or a total kinetic energy for the CME of ~2 x 1033 ergs.
20 January 2005 CME
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10/26
10/28
10/29
11/2
11/4
4/21/02 ∆
∆ - UCSD total estimate
Although there are large uncertainties, it appears that large SEP eventsextract ~10% of the CME kinetic energy.
A similar efficiency has been estimated for cosmic ray acceleration by supernova shocks.
(Mostly from Dick Mewaldt – SHINE 2005)
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∆ - 1/20/05
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20 January 2005 CME
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20 January 2005 CME - caveat
20 January 2005 CME
UCSD CASS orbit-orbit subtraction analysis
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20 January 2005 CME - caveat
20 January 2005 CME
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