Three-dimensional properties of interplanetary disturbances in 1978-1981

Details Three-dimensional properties of interplanetary disturbances in 1978-1981 Three-dimensional properties of interplanetary disturbances in 1978-1981

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..153w&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

1

Interplanetary Medium, Scintillation, Shock Wave Propagation, Solar Wind, Directivity, Propagation Velocity, Solar Corona, Solar Flares

Scientific paper

This paper presents the average three-dimensional configuration of solar flare- or disappearing filament-associated interplanetary disturbances on the basis of IPS (interplanetary scintillation) and spacecraft observations in 1978 - 1981. The angular distribution of the propagation speed at 1 AU is largely isotropic over the range of 110° in solar longitude centered at the normal of the solar source. In the latitudinal direction, the characteristic angular extent is about 60°. Thus, the three-dimensional shape of an interplanetary disturbance can be approximated by a half of an ellipsoid having an axial ratio of about 1.8.

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