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Paper: Coronal Waves: Coronal Heating and Coronal Seismology
Volume: 325, The Solar-B Mission and the Forefront of Solar Physics
Page: 253
Authors: Nakariakov, V.M.
Abstract: SOHO and TRACE missions have demonstrated that wave phenomena are abundant in the corona and provided us with an observational basis for MHD coronal seismology. This review covers the recent observational finding of coronal wave phenomena and their theoretical models. The relevance of these observational and theoretical efforts to the coronal heating is discussed. Possible observability of these phenomena with EIS and XRT instruments is discussed.
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