Observation of flare-generated shock waves by Helios-2 near the sun |
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Authors: | P M Volkmer F M Neubauer R Schwenn |
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Institution: | (1) Institut für Geophysik und Meteorologie der Technischen Universität Braunschweig, D-3300 Braunschweig, Germany;(2) Max-Planck-Institut für Aeronomie, D-3411 Katlenburg-Lindau 3, Germany |
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Abstract: | We present the observation of three flare generated shock waves which were measured by Helios-2 at a radial distance from the Sun of 0.476 AU, 0.444 AU, and 0.297 AU. These results show that two of the shocks fulfill the classification scheme of F-events stated in the past while the third shock profile is that of a R-event being interpreted as a driven wave. Because of the close distance to the Sun a flare-association was possible. Only in one case there is some evidence for a piston in the downstream region of the shock. One of the shocks is characterized by a distinct hole in the frequency distribution of directional discontinuities in the downstream region.An invited paper presented at STIP Workshop on Shock Waves in the Solar Corona and Interplanetary Space, 15–19 June, 1980, Smolenice, Czechoslovakia. |
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