Abstract
Numerical simulations of energy depositions in the middle and upper solar chromosphere result in ejection of chromospheric material into the corona and heating of the chromospheric gas. These simulations may be capable of describing some of the features seen by the soft X-ray telescope on board theYohkoh satellite.
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Sterling, A.C., Shibata, K. & Mariska, J.T. Jets and brightenings generated by energy deposition in the middle and upper solar chromosphere. Space Sci Rev 70, 77–80 (1994). https://doi.org/10.1007/BF00777845
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DOI: https://doi.org/10.1007/BF00777845