No CrossRef data available.
Article contents
Atomic Data Needed for Solar Astronomy from Space
Published online by Cambridge University Press: 30 March 2016
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
The UV and X-ray wavelength ranges are rich in emission unes from the transition region and the corona, formed at temperatures from 104 K to 107 K. Fortunately, these emission lines, absorbed by the earth upper atmosphere, can be observed by some solar space observatories. In particular, the NASA SMM satellite, from 1980 to 1990, has obtained very interesting spectra from which important solar results were derived. In a close future, they will be again observed but with improved spectral, spatial and temporal resolution by SOLAR-A and SOHO.
- Type
- Joint Commission Meetings
- Information
- Copyright
- Copyright © Kluwer 1992
References
Bitter, M., Hill, K.W., Sauthoff, N.R., Efthimion, P.C., Meservey, E., Roney, W., von Goeler, S., Horton, R., Goldman, M., and Stodiek, W.: 1979, Phys. Rev. Lett., 43, 129
CrossRefGoogle Scholar
Bitter, M., von Goeler, S., Hill, K.W., Horton, R., Johnson, D., Roney, W., Sauthoff, N.R., Silver, E., and Stodiek, W.: 1981, Phys. Rev. Lett, 47, 921
CrossRefGoogle Scholar
Culhane, J.L., Gabriel, A.H., Acton, L.W., Rapley, C.G., Phillips, K.J., Wolfson, C.J., Antonucci, E., Bentley, R.D., Catura, R.C., Jordan, C., Kayat, M.A., Kent, B.J., Leibacher, J.W., Parmar, A.N., Sherman, J.C., Springer, L.A., Strong, K.T., and Veck, N.J.: 1981, Astrophys J., 244, L141
CrossRefGoogle Scholar
Bely-Dubau, F., Gabriel, A.H., and Volonté, S.: 1979, Mon. Not. R. astr. Soc, 186, 405
CrossRefGoogle Scholar
Bely-Dubau, F., Dubau, J., Faucher, P., and Gabriel, A.H.: 1982, Mon. Not. R. aitr. Soc, 198, 239
CrossRefGoogle Scholar
You have
Access