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Pallavicini, R., Vaiana, G. S., Tofani, G., Felli, M. (1979) The coronal atmosphere above solar active regions - Comparison of high spatial resolution soft X-ray and centimetric observations. The Astrophysical Journal, 229. 375pp. doi:10.1086/156963

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Reference TypeJournal (article/letter/editorial)
TitleThe coronal atmosphere above solar active regions - Comparison of high spatial resolution soft X-ray and centimetric observations
JournalThe Astrophysical Journal
AuthorsPallavicini, R.Author
Vaiana, G. S.Author
Tofani, G.Author
Felli, M.Author
Year1979 (April)Volume229
PublisherIOP Publishing
DOIdoi:10.1086/156963Search in ResearchGate
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Mindat Ref. ID3313188Long-form Identifiermindat:1:5:3313188:9
GUID0
Full ReferencePallavicini, R., Vaiana, G. S., Tofani, G., Felli, M. (1979) The coronal atmosphere above solar active regions - Comparison of high spatial resolution soft X-ray and centimetric observations. The Astrophysical Journal, 229. 375pp. doi:10.1086/156963
Plain TextPallavicini, R., Vaiana, G. S., Tofani, G., Felli, M. (1979) The coronal atmosphere above solar active regions - Comparison of high spatial resolution soft X-ray and centimetric observations. The Astrophysical Journal, 229. 375pp. doi:10.1086/156963
In(1979) The Astrophysical Journal Vol. 229. IOP Publishing

See Also

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Pallavicini, R., Vaiana, G. S. (1976) The spatial structure of a solar flare in soft X-rays and centimetric wavelengths. Solar Physics, 49 (2). 297-313 doi:10.1007/bf00162454
Pallavicini, R., Peres, G., Serio, S., Vaiana, G. S., Golub, L., Rosner, R. (1981) Closed coronal structures. III - Comparison of static models with X-ray, EUV, and radio observations. The Astrophysical Journal, 247. 692pp. doi:10.1086/159081
Peres, G., Serio, S., Vaiana, G., Acton, L., Leibacher, J., Rosner, R., Pallavicini, R. (1983) Closed coronal structures. V - Gasdynamic models of flaring loops and comparison with SMM observations. The Astrophysical Journal, 270. 270pp. doi:10.1086/161120
Poletto, G., Vaiana, G. S., Zombeck, M. V., Krieger, A. S., Timothy, A. F. (1975) A comparison of coronal X-ray structures of active regions with magnetic fields computed from photospheric observations. Solar Physics, 44 (1). 83-99 doi:10.1007/bf00156848
Pallavicini, R., Serio, S., Vaiana, G. S. (1977) A survey of soft X-ray limb flare images - The relation between their structure in the corona and other physical parameters. The Astrophysical Journal, 216. 108pp. doi:10.1086/155452
Giampapa, M. S., Golub, L., Peres, G., Serio, S., Vaiana, G. S. (1985) Closed coronal structures. VI - Far-ultraviolet and X-ray emission from active late-type stars and the applicability of coronal loop models. The Astrophysical Journal, 289. 203pp. doi:10.1086/162880
Lang, K. R., Willson, R. F., Felli, M. (1981) VLA Observations of Solar Active Regions - Part Two - Solar Bursts. The Astrophysical Journal, 247. 338pp. doi:10.1086/159042
Warmuth, A., Mann, G., Aurass, H. (2005) First Soft X-Ray Observations of Global Coronal Waves with the G O E S Solar X-Ray Imager. The Astrophysical Journal, 626 (2). doi:10.1086/431756
Nitta, N., White, S. M., Kundu, M. R., Gopalswamy, N., Holman, G. D., Brosius, J. W., Schmelz, J. T., Saba, J. L. R., Strong, K. T. (1991) Coronal magnetic structures observing campaign. I - Simultaneous microwave and soft X-ray observations of active regions at the solar limb. The Astrophysical Journal, 374. 374pp. doi:10.1086/170128
Rosner, R., Vaiana, G. S. (1977) Hydrostatic and dynamic models of solar coronal holes. The Astrophysical Journal, 216. 141pp. doi:10.1086/155455
Felli, M., Lang, K. R., Willson, R. F. (1981) VLA observations of solar active regions. I - The slowly varying component. The Astrophysical Journal, 247. 325pp. doi:10.1086/159041
 
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