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The stationary post-flare arch of May 21/22, 1980
Authors:Paul Hick  Zdeněk ?vestka
Institution:(1) Laboratory for Space Research, Utrecht, The Netherlands
Abstract:On May 21/22, 1980 the Hard X-Ray Imaging Spectrometer aboard the SMM imaged an extensive coronal structure after the occurrence of a two-ribbon flare on May 21, 20:50 UT. The structure was observed from 22:20 UT on May 21 until its disappearence at 09:00 UT on May 22.At 22:20 UT the brightest pixel in the arch was located at a projected altitude of 95 000 km above the zero line of the longitudinal magnetic field. At 23:02 UT the maximum of brightness shifted to a neighbouring pixel with approximately the same projected altitude. This sudden shift indicates that the X-ray structure consisted of (at least) two separate arches at approximately the same altitude, one of which succeeded the other as the brightest arch in the structure at 23:02 UT.From 23:02 UT onwards the maximum of brightness did not change its position in the HXIS coarse field of view. With a spatial resolution of 32Prime this places an upper limit of 1.1 km s-1 on the rise velocity of the arch. Thus, contrary to a similar arch observed on November 6/7, where rise velocities of the order of 10 km s-1 were measured in the same phase of development, the May 22 arch was a stationary structure at an altitude of ap 145000 km.The following values were estimated for the physically relevant quantities of the May 21/22 arch at the time of its maximum brightness (ap23:00 UT): temperature T ap6.3 × 106 K, electron density n e ap 1.1 × 109 cm-3, total emitting volume V ap5 × 1029 cm3, energy density epsiv ap2.9 erg cm–3, total energy contents E ap 1.4 × 1030 erg, total mass M ap 9 × 1014 g.The top of the arch was observed at ap 145 000 km altitude within 1.5 hr after the flare occurrence. Since it seems unlikely that the structure already existed prior to the flare at 20:50 UT, the arch must have risen to its stationary position with an average velocity exceeding 17 km s–1 (possibly much faster). We speculate that the arch was formed very fast at the flare onset, when (part of) the active region loop system was elevated within minutes to the observed altitude.
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