Abstract
We have studied a flare (GOES class: M2.3) on the west limb (H- alpha: N18, W78) on 1993 March 23 using microwave (17GHz) and Soft X-ray imaging data and also hard X-ray spectrum data. This flare has typical properties of “gradual-hard flares”.
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References
Kosugi, T. et al. (1991) Solar Phys., 136, 17
Kundu, M. et aI. (1984) Adv. Space Res., 4, No.7,157
Nakajima, H. et aI. (1991) in Flare Physics in Solar Activity Maximum, 22, 77
Nakajima, H. et aI. (1994) Pmc. IEEE, 82,705
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© 1996 Kluwer Academic Publishers
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Yaji, K., Kosugi, T., Nishio, M. (1996). Nonthermal Emissions In The Hard X-Ray And Microwave Ranges From Flaring Loops. In: Uchida, Y., Kosugi, T., Hudson, H.S. (eds) Magnetodynamic Phenomena in the Solar Atmosphere. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0315-9_130
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DOI: https://doi.org/10.1007/978-94-009-0315-9_130
Publisher Name: Springer, Dordrecht
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