4.7 Article

Varying Calcium Abundances in Solar Flares Seen by the Solar Maximum Mission

Journal

ASTROPHYSICAL JOURNAL
Volume 946, Issue 1, Pages -

Publisher

IOP Publishing Ltd
DOI: 10.3847/1538-4357/acc016

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We studied the calcium abundance A(Ca) during the decay phases of 194 solar X-ray flares using data from the Bent Crystal Spectrometer on the Solar Maximum Mission. The calcium abundance was found to be about 3 times the photospheric abundance, indicating a first ionization potential effect. We observed variations in A(Ca) during the flare decay, with some segments showing a decrease and others showing an increase in A(Ca).
We report on calcium abundance A(Ca) estimates during the decay phases of 194 solar X-ray flares using archived data from the Bent Crystal Spectrometer (BCS) on the Solar Maximum Mission (operational 1980-1989). The abundances are derived from the ratio of the total calcium X-ray line emission in BCS channel 1 to that in neighboring continuum, with temperature from a satellite-to-resonance line ratio. Generally, the calcium abundance is found to be about 3 times the photospheric abundance, as previously found, indicating a first ionization potential (FIP) effect for calcium, which has a relatively low FIP value. The precision of the abundance estimates (referred to hydrogen on a logarithmic scale with A(H) = 12), is typically similar to +/- 0.01, enabling any time variations of A(Ca) during the flare decay to be examined. For a total of 270 short time segments with A(Ca) determined to better than 2.3% accuracy, many (106; 39%) showed variations in A(Ca) at the 3 sigma level. For the majority, in 74 (70%) of these 106 segments A(Ca) decreased with time, and for 32 (30%) A(Ca) increased with time. For 79 out of 270 (29%) we observed constant or nearly constant A(Ca), and the remaining 85 (31%) with irregular time behavior. A common feature was the presence of discontinuities in the time behavior of A(Ca). Relating these results to the ponderomotive force theory of Laming, we attribute the nature of varying A(Ca) to the emergence of loop structures in addition to the initial main loop, each with its characteristic calcium abundance.

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