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Volumn 77, Issue 37, 1996, Pages

The case for electron dominance in solar flare energy transport

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EID: 0038830895     PISSN: 00963941     EISSN: None     Source Type: Journal    
DOI: 10.1029/96eo00246     Document Type: Review
Times cited : (5)

References (11)
  • 1
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    • Electron time of flight distances and flare loop geometries compared from CGRO and YOHKOH observations
    • in press
    • Aschwanden, M. J., M. J. Wills, H. S. Hudson, and R. A. Schwartz, Electron time of flight distances and flare loop geometries compared from CGRO and YOHKOH observations, Astrophys. J., in press, 1996.
    • (1996) Astrophys. J.
    • Aschwanden, M.J.1    Wills, M.J.2    Hudson, H.S.3    Schwartz, R.A.4
  • 2
    • 0001009909 scopus 로고
    • The Ha spectral signatures of solar flare nonthermal electrons
    • Canfield, R. C., T. A. Gunkler, and P. J. Ricchiazzi, The Ha spectral signatures of solar flare nonthermal electrons, Astrophys. J., 282, 296, 1984.
    • (1984) Astrophys. J. , vol.282 , pp. 296
    • Canfield, R.C.1    Gunkler, T.A.2    Ricchiazzi, P.J.3
  • 4
    • 0005292442 scopus 로고
    • Hard x-ray Bremsstrahlung production in solar flares by high-energy proton beams
    • Emslie, A. G., and J. C. Brown, Hard x-ray Bremsstrahlung production in solar flares by high-energy proton beams, Astrophys. J., 295, 648, 1985.
    • (1985) Astrophys. J. , vol.295 , pp. 648
    • Emslie, A.G.1    Brown, J.C.2
  • 5
    • 4243261079 scopus 로고
    • Discrepancies between theoretical and empirical models of the flaring solar chromosphere and their possible resolution
    • Emslie, A. G., J. C. Brown, and M. E. Machado, Discrepancies between theoretical and empirical models of the flaring solar chromosphere and their possible resolution, Astrophys. J., 246, 337, 1981.
    • (1981) Astrophys. J. , vol.246 , pp. 337
    • Emslie, A.G.1    Brown, J.C.2    Machado, M.E.3
  • 6
    • 34250122571 scopus 로고
    • The excitation of the iron Kα feature in solar flares
    • Emslie, A. G., K. J. H. Phillips, and B. R. Dennis, The excitation of the iron Kα feature in solar flares, Sol. Phys., 103, 89, 1986.
    • (1986) Sol. Phys. , vol.103 , pp. 89
    • Emslie, A.G.1    Phillips, K.J.H.2    Dennis, B.R.3
  • 8
    • 21344442185 scopus 로고    scopus 로고
    • Testing the impulsiveness of solar flare heating through analysis of dynamic atmospheric response
    • Newton, E. K., A. G. Emslie, and J. T. Mariska, Testing the impulsiveness of solar flare heating through analysis of dynamic atmospheric response, Astrophys. J., 459, 804, 1996.
    • (1996) Astrophys. J. , vol.459 , pp. 804
    • Newton, E.K.1    Emslie, A.G.2    Mariska, J.T.3
  • 9
    • 0029471116 scopus 로고
    • Solar atmospheric abundances and energy content in flare-accelerated ions from gamma-ray spectroscopy
    • Ramaty, R., N. Mandzhavidze, B. Kozlovsky, and R. J. Murphy, Solar atmospheric abundances and energy content in flare-accelerated ions from gamma-ray spectroscopy, Astrophys J., 455, L193, 1995.
    • (1995) Astrophys J. , vol.455
    • Ramaty, R.1    Mandzhavidze, N.2    Kozlovsky, B.3    Murphy, R.J.4
  • 11
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    • On the production of hard X-rays in solar flares
    • Simnett, G. M., and M. G. Haines, On the production of hard X-rays in solar flares, Sol. Phys., 130, 253, 1990.
    • (1990) Sol. Phys. , vol.130 , pp. 253
    • Simnett, G.M.1    Haines, M.G.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.