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Machado, M. E., Emslie, A. G. (1979) A comparison of high-temperature flare models with observations and implications for the low-temperature flare. The Astrophysical Journal, 232. 903pp. doi:10.1086/157353

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Reference TypeJournal (article/letter/editorial)
TitleA comparison of high-temperature flare models with observations and implications for the low-temperature flare
JournalThe Astrophysical Journal
AuthorsMachado, M. E.Author
Emslie, A. G.Author
Year1979 (September)Volume232
PublisherIOP Publishing
DOIdoi:10.1086/157353Search in ResearchGate
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Mindat Ref. ID3313687Long-form Identifiermindat:1:5:3313687:5
GUID0
Full ReferenceMachado, M. E., Emslie, A. G. (1979) A comparison of high-temperature flare models with observations and implications for the low-temperature flare. The Astrophysical Journal, 232. 903pp. doi:10.1086/157353
Plain TextMachado, M. E., Emslie, A. G. (1979) A comparison of high-temperature flare models with observations and implications for the low-temperature flare. The Astrophysical Journal, 232. 903pp. doi:10.1086/157353
In(1979) The Astrophysical Journal Vol. 232. IOP Publishing

See Also

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Emslie, A. G. (1981) A comparison of the height distributions of solar flare hard X-rays in thick target and thermal models. The Astrophysical Journal, 245. 711pp. doi:10.1086/158846
Emslie, A. Gordon (1985) The structure of high-temperature solar flare plasma in non-thermal flare models. Solar Physics, 98 (2). 281-291 doi:10.1007/bf00152461
Sandlin, G. D., Brueckner, G. E., Scherrer, V. E., Tousey, R. (1976) High-temperature flare lines in the solar spectrum 171 A-630 A. The Astrophysical Journal, 205. doi:10.1086/182087
Machado, M. E., Avrett, E. H., Vernazza, J. E., Noyes, R. W. (1980) Semiempirical models of chromospheric flare regions. The Astrophysical Journal, 242. 336pp. doi:10.1086/158467
Gordon Emslie, A. (1986) The structure of high-temperature flare plasma. Solar Physics, 103 (1). 103-110 doi:10.1007/bf00154861
Machado, Marcos E., Emslie, A. Gordon, Brown, John C. (1978) The structure of the temperature minimum region in solar flares and its significance for flare heating mechanisms. Solar Physics, 58 (2). 363-387 doi:10.1007/bf00157282
Emslie, A. G., Li, Peng, Mariska, John T. (1992) Diagnostics of electron-heated solar flare models. III - Effects of tapered loop geometry and preheating. The Astrophysical Journal, 399. 714pp. doi:10.1086/171964
Peres, G., Reale, F., Serio, S., Pallavicini, R. (1987) Hydrodynamic flare modeling - Comparison of numerical calculations with SMM observations of the 1980 November 12 17:00 UT flare. The Astrophysical Journal, 312. 895pp. doi:10.1086/164936
Hawley, Suzanne L., Fisher, George H. (1992) X-ray-heated models of stellar flare atmospheres - Theory and comparison with observations. The Astrophysical Journal Supplement Series, 78. 565 doi:10.1086/191640
Emslie, A. G. (1981) On the importance of reverse current ohmic losses in electron-heated solar flare atmospheres. The Astrophysical Journal, 249. 817pp. doi:10.1086/159339
Haisch, B. M., Linsky, J. L., Lampton, M., Paresce, F., Margon, B., Stern, R. (1977) Extreme-ultraviolet observations of a flare on Proxima Centauri and implications concerning flare-star scaling theory. The Astrophysical Journal, 213. doi:10.1086/182422
 
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