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- W1989338317 abstract "The Yohkoh Soft X-Ray Telescope has observed numerous transient brightenings of compact active-region coronal loops (microflares). Shimizu (1995) found that the distribution function of the total energy of transient brightenings is a decreasing power-law with an index (1.5 ~ 1.6) in the energy range greater than 1027 erg, suggesting that the large number of small brightenings is energetically less important than the few large ones. However, the distribution function for smaller brightenings (< 1027 erg) is still unknown. This paper performs a deep search for smaller brightenings (termed nanoflares, Parker 1988) using the soft X-ray position-dependent time profiles. For details, please refer to the full-length paper published in the 1997 September issue of the Astrophysical Journal with the same title (Shimizu and Tsuneta 1997)." @default.
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- W1989338317 date "1997-09-10" @default.
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- W1989338317 title "Deep Survey of Solar Nanoflares with<i>Yohkoh</i>" @default.
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- W1989338317 doi "https://doi.org/10.1086/304542" @default.
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