Abstract
A limb flare is described that occurred above a complex and very active sunspot. Four stages can be distinguished: the flash-phase, the spray-phase, the surge-phase and the loop-phase. Each of them had a duration that was longer than that of the preceding one. In the spray ascending speeds up to 745 km s−1 and accelerations up to 1.3 km s-2 were recorded. The loop-phase has been observed in the coronal lines 5303 and 5694 Å. The yellow line, being very weak before the flare, became extremely strong in the loop and surpassed five times the intensity of the green line. X-ray bursts and ionospheric disturbances of long duration demonstrate that not only the flare itself but also the loop was a source of X-rays. Most of the radio-bursts can be ascribed to specific features in the Hα-records of the event.
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Astronomishe Mitteilungen der Eidgenössischen Sternwarte Zürich Nr. 318.
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Waldmeier, M. The limb flare of August 11, 1972. Sol Phys 30, 129–137 (1973). https://doi.org/10.1007/BF00156181
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DOI: https://doi.org/10.1007/BF00156181