Superposed epoch analysis of corotating interaction regions at 0.3 and 1.0 AU - A comparative study

Details Superposed epoch analysis of corotating interaction regions at 0.3 and 1.0 AU - A comparative study Superposed epoch analysis of corotating interaction regions at 0.3 and 1.0 AU - A comparative study

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986jgr....91.5873r&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 91, May 1, 1986, p. 5873-5878. BMFT-supported research.

Physics

13

Interplanetary Medium, Plasma Density, Solar Wind, Space Plasmas, Field Strength, Interplanetary Magnetic Fields, Leading Edges, Solar Wind Velocity, Velocity Distribution

Scientific paper

Applying the superposed epoch analysis technique to 16 and to 31 well-defined, nonshock-associated stream-stream interaction regions observed by the Helios spacecraft in the distance ranges 0.3 to 0.4 AU and 0.9 to 1.0 AU, respectively, the authors obtain the average azimuthal variation in the solar wind density, velocity and temperature, in the magnetic field strength, and in the total proton plasma plus magnetic field pressure across CIRs at these two radial distances separately.

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