Abstract
The Neupert effect is commonly interpreted as evidence that the energetic electrons causing the hard X-ray flare emission are the main source of heating and mass supply of the soft X-ray emitting hot coronal loop plasma. RHESSI and GOES data are used to test the Neupert effect by comparing the beam power supply inferred from hard X-ray spectra and the actual power required to explain the observed soft X-ray emission.
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Veronig, A., Brown, J., Dennis, B., Schwartz, R., Sui, L., Tolbert, A. (2005). Testing the Neupert Effect. In: Hanslmeier, A., Veronig, A., Messerotti, M. (eds) Solar Magnetic Phenomena. Astrophysics and Space Science Library, vol 320. Springer, Dordrecht. https://doi.org/10.1007/1-4020-2962-4_31
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DOI: https://doi.org/10.1007/1-4020-2962-4_31
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-2961-5
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