Solar and interplanetary observations of the mass ejection on 7 May, 1979

Details Solar and interplanetary observations of the mass ejection on 7 May, 1979 Solar and interplanetary observations of the mass ejection on 7 May, 1979

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..115..327j&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 115, no. 2, 1988, p. 327-343. Research supported by NSF and Polska Akademia Nauk.

Physics

14

Interplanetary Space, Solar Instruments, Solar Wind, Space Observations (From Earth), Stellar Mass Ejection, Chromosphere, H Alpha Line, Photosphere, Solar Corona, Velocity Distribution

Scientific paper

Observations of mass ejection obtained on May 7, 1979 by five different instruments from the solar surface out to more than 100 solar radii are used to produce a three-dimensional density reconstruction of the mass ejection and to fit the best velocity curve for its propagation. The results show higher speeds at greater distances from the sun. The plasma acceleration was found to continue beyond the outer limit of the coronagraph view at about 8 solar radii.

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