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Detailed Reference Information |
Burlaga, L.F., Ness, N.F., Stone, E.C., McDonald, F.B. and Richardson, J.D. (2005). Voyager 2 observations related to the October–November 2003 solar events. Geophysical Research Letters 32: doi: 10.1029/2004GL021480. issn: 0094-8276. |
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A transient flow system observed at 1 AU from October 24--November 7, 2003 (consisting of several shocks, ejecta and possibly other flows) moved away from the Sun for ≈180 days to 73 AU, where Voyager 2 (V2) observed a large Merged Interaction Region (MIR) associated with a fast (560 km/s) stream that followed a forward shock and moved past V2 for ≈1.5 solar rotations. The MIR and stream were associated with a large decrease in the cosmic ray intensity and an exceptionally large enhancement in the flux of ≈2.5 MeV protons. The speed and the cosmic ray profiles observed by V2 were very simple, resembling the profiles of a shock/sheath/ejecta flow and a Forbush decrease, respectively, at 1 AU, but rescaled by a factor by a factor of ≈10. The onset of the MIR-associated decrease in the cosmic ray intensity occurred 10 days after the shock, lasting several days, with a full recovery ≈70 days after the onset. |
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Abstract |
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Keywords
Interplanetary Physics, Energetic particles, Interplanetary Physics, Interplanetary magnetic fields, Interplanetary Physics, Interplanetary shocks, Interplanetary Physics, Solar wind plasma |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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