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Direct observations of a flare related coronal and solar wind disturbance (1975)

Gosling, J. T. ; Hildner, E. ; Macqueen, R. M. ; [et al.]

Springer

Solar physics 40 (1975), S. 439-448

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ISSN: 1573-093X

Source: Springer Online Journal Archives 1860-2000

Topics: Physics

Notes: Abstract Numerous mass ejections from the Sun have been detected with orbiting coronagraphs. Here for the first time we document and discuss the direct association of a coronagraph observed mass ejection, which followed a 2B flare, with a large interplanetary shock wave disturbance observed at 1 AU. Estimates of the mass (2.4 × 1016 g) and energy content (1.1 × 1032 erg) of the coronal disturbance are in reasonably good agreement with estimates of the mass and energy content of the solar wind disturbance at 1 AU. The energy estimates as well as the transit time of the disturbance are also in good agreement with numerical models of shock wave propagation in the solar wind.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1007/BF00162390

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