Abstract
The rapid dissipation of flare energy has been observed in the transition-zone line of C iv at 1548.2 Å using the University of Colorado spectrometer aboard OSO-8. Impulsive brightenings have been resolved with characteristic risetimes as low as 3.5 s. One event is analyzed in detail, in which it is inferred that the electron density is greater than 2 × 1011 cm−3 at T = 60 000 K, and that the flare energy is deposited at a rate of 2 ergs cm−3 s−1 or greater. The temporal behavior of the intensity at the center of the C iv line is consistent with a non-equilibrium ionization of C iii through C v. If this event is a result of the multiple tearing mode instability as the primary energy release mechanism, then the observations indicate a pre-flare magnetic field of about 175 G.
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The National Center for Atmospheric Research is sponsored by the National Science Foundation.
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Lites, B.W. Transition-zone observations of rapid flare events as observed by OSO-8. Sol Phys 71, 329–336 (1981). https://doi.org/10.1007/BF00167555
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DOI: https://doi.org/10.1007/BF00167555