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The Solar Wind - Inner Heliosphere
Authors:Suess  S. T.  Phillips  J. L.  McComas  D. J.  Goldstein  B. E.  Neugebauer  M.  Nerney  S.
Affiliation:(1) NASA Marshall Space Flight Center/ES82, Huntsville, AL 35812, USA;(2) Los Alamos National Laboratory, Los Alamos, NM 87545, USA;(3) Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USA;(4) Ohio University, 1570 Granville Pike, Lancaster, Ohio 43130, USA
Abstract:
The solar wind in the inner heliosphere, inside ~ 5 AU, has been almost fully characterized by the addition of the high heliographic latitude Ulysses mission to the many low latitude inner heliosphere missions that preceded it. The two major omissions are the high latitude solar wind at solar maximum, which will be measured during the second Ulysses polar passages, and the solar wind near the Sun, which could be analyzed by a Solar Probe mission. Here, existing knowledge of the global solar wind in the inner heliosphere is summarized in the context of the new results from Ulysses.
Keywords:Solar wind  Heliosphere  Ulysses  SOHO  MHD waves  Turbulence
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