Origin of strong interplanetary shocks

Details Origin of strong interplanetary shocks Origin of strong interplanetary shocks

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985natur.314..137h&link_type=abstract

Nature (ISSN 0028-0836), vol. 314, March 14, 1985, p. 137-140.

Astronomy and Astrophysics

Astronomy

54

Interplanetary Medium, Radio Sources (Astronomy), Shock Wave Generators, Solar Atmosphere, Coronal Holes, Plasma Density, Solar Wind, Space Plasmas

Scientific paper

Observations of 900 radio sources have been used to study the shape and motion of large-scale interplanetary transients associated with shock disturbances at 1 AU. The variations of plasma density and speed and the zones in the solar atmosphere from which the transients originate suggest an origin related to intermittent flows of enhanced speed from coronal holes at mid-latitudes on the Sun.

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