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SUMMARY:Possible Role of Transients on the Energy Spectum of Energetic Par
 ticles at Solar wind Termination Shock
DTSTART;VALUE=DATE-TIME:20070710T160600Z
DTEND;VALUE=DATE-TIME:20070710T161800Z
DTSTAMP;VALUE=DATE-TIME:20260418T190943Z
UID:indico-contribution-1118@cern.ch
DESCRIPTION:Speakers: CUMMINGS\, A. C. (California Institute of Technology
 )\nWe examine the Voyager 1 (V1) and Voyager 2 (V2) intensity vs. time \np
 rofiles in several energy bands of low-energy particle populations \ndurin
 g the period 2005 through early 2007. There appear to be a set \nof propag
 ating structures with ~1 year duration that appear first at \nV2\, which i
 s upwind of the solar wind termination shock\, and then ~115 \ndays later 
 at V1 in the heliosheath. We will discuss these observations \nin the cont
 ext of the source and transport of the termination shock \nparticles and a
 nomalous cosmic rays. \n\nThis work was supported by NASA under contract N
 AS7-03001.\n\nhttps://indico.nucleares.unam.mx/event/4/session/88/contribu
 tion/1118
LOCATION:Merida\, Mexico Yucatan I (Fiesta Americana)
URL:https://indico.nucleares.unam.mx/event/4/session/88/contribution/1118
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