Abstract
We analyze properties of small scale events observed by the Soft X-ray Telescope (SXT) aboard the Yohkoh satellite. The analysis focuses on a sequence of highest resolution SXT images of the quiet Sun. Non-standard methods were used in order to correct images for dark current and hot pixels. Basic properties of weak X-ray events found in the data are discussed.
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References
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Gburek, S., Sylwester, J. (2005). Small Scale Events Seen in SXT Observations. 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_29
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DOI: https://doi.org/10.1007/1-4020-2962-4_29
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-2961-5
Online ISBN: 978-1-4020-2962-2
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