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Oien, A. H., Alendal, G. (1993) A model of solar coronal heating by classical inverse bremsstrahlung and generation of the solar wind. The Astrophysical Journal, 412. 827pp. doi:10.1086/172965

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Reference TypeJournal (article/letter/editorial)
TitleA model of solar coronal heating by classical inverse bremsstrahlung and generation of the solar wind
JournalThe Astrophysical Journal
AuthorsOien, A. H.Author
Alendal, G.Author
Year1993 (August)Volume412
PublisherIOP Publishing
DOIdoi:10.1086/172965Search in ResearchGate
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Mindat Ref. ID3333378Long-form Identifiermindat:1:5:3333378:8
GUID0
Full ReferenceOien, A. H., Alendal, G. (1993) A model of solar coronal heating by classical inverse bremsstrahlung and generation of the solar wind. The Astrophysical Journal, 412. 827pp. doi:10.1086/172965
Plain TextOien, A. H., Alendal, G. (1993) A model of solar coronal heating by classical inverse bremsstrahlung and generation of the solar wind. The Astrophysical Journal, 412. 827pp. doi:10.1086/172965
In(1993) The Astrophysical Journal Vol. 412. IOP Publishing

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Wang, Y.-M. (1993) Flux-tube divergence, coronal heating, and the solar wind. The Astrophysical Journal, 410. doi:10.1086/186895
Sandbaek, Ornulf, Leer, Egil (1995) Coronal Heating and Solar Wind Energy Balance. The Astrophysical Journal, 454. 486pp. doi:10.1086/176500
Schwadron, N. A., McComas, D. J., DeForest, C. (2006) Relationship between Solar Wind and Coronal Heating: Scaling Laws from Solar X‐Rays. The Astrophysical Journal, 642 (2). 1173-1176 doi:10.1086/501066
Benford, G. (1983) Turbulent resistive heating of solar coronal arches. The Astrophysical Journal, 269. 690pp. doi:10.1086/161078
Heyvaerts, J., Priest, E. R. (1992) A self-consistent turbulent model for solar coronal heating. The Astrophysical Journal, 390. 297pp. doi:10.1086/171280
Habbal, S. R., Leer, E. (1982) Electron heating by fast mode magnetohydrodynamic waves in the solar wind emanating from coronal holes. The Astrophysical Journal, 253. 318pp. doi:10.1086/159637
Zhang, T. X. (2003) Preferential Heating of Particles by H-Cyclotron Waves Generated by a Global Magnetohydrodynamic Mode in Solar Coronal Holes. The Astrophysical Journal, 597 (1). doi:10.1086/379798
Bravo, S., Stewart, G. A. (1997) Fast and Slow Wind from Solar Coronal Holes. The Astrophysical Journal, 489 (2). 992-999 doi:10.1086/304789
Grossmann, William, Smith, Robert A. (1988) Heating of solar coronal loops by resonant absorption of Alfven waves. The Astrophysical Journal, 332. 476pp. doi:10.1086/166671
Shoda, Munehito, Yokoyama, Takaaki, Suzuki, Takeru K. (2018) A Self-consistent Model of the Coronal Heating and Solar Wind Acceleration Including Compressible and Incompressible Heating Processes. The Astrophysical Journal, 853 (2). 190pp. doi:10.3847/1538-4357/aaa3e1
Sandbaek, Onulf, Leer, Egil, Hansteen, Viggo H. (1994) On the relation between coronal heating, flux tube divergence, and the solar wind proton flux and flow speed. The Astrophysical Journal, 436. 390pp. doi:10.1086/174913
 
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