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An eruptive prominence of June 10, 1973

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Abstract

An eruptive prominence of June 10, 1973, showing ascending and expanding motions, has been recorded spectroscopically at Oslo Solar Observatory.

The Ca ii H line yields broadening velocities ranging from 5 km s-1 to 20 km s-1. An extreme ratio of 1/30 was measured for line-broadening to expansion velocity.

Flare activity succeeded the start of the observed disparition brusque phase of the prominence. The eruption is related to coronal disturbances recorded approximately 1 hr later by ATM, Skylab.

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Authors and Affiliations

  1. Institute of Theoretical Astrophysics, University of Oslo, Blindern, Norway

    O. Engvold & B. M. Rustad

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  1. O. Engvold
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  2. B. M. Rustad
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Engvold, O., Rustad, B.M. An eruptive prominence of June 10, 1973. Sol Phys 35, 409–417 (1974). https://doi.org/10.1007/BF00151964

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  • DOI: https://doi.org/10.1007/BF00151964

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