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Calculations on the Solar Spectrum from 1 to 60 Å

Published online by Cambridge University Press:  12 April 2016

R. Mewe
R. Mewe*
Affiliation:
Space Research Laboratory, Utrecht, The Netherlands

Extract

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Over two hundred spectral line intensities between 1 and 60 Å from ions in the solar corona have been computed for electron temperatures ranging between 105 and 109 K (Mewe, 1972a). Also the continuum (ff+fb) radiation intensity has been computed. The calculations were set up to interprete soft X-ray measurements aboard the ESRO 2B satellite (IRIS): Wavelength bands 44–55 Å (experiment of Space Research Laboratory, Utrecht) and 1–3, 3–9, 6–18 Å(expt. of University College, London) (Brinkman and Shaw, 1972).

Type
Section IV / The Solar Soft X-Ray Spectrum
Information
International Astronomical Union Colloquium , Volume 14: Special Issue: Ultraviolet and X-Ray Spectroscopy of Astrophysical and Laboratory Plasmas , November 1972 , pp. 666 - 667
Copyright
Copyright © Reidel 1972

References

Brinkman, A. C. and Shaw, M. L.: 1972, Solar Phys. 23, 120.Google Scholar
Burger, M. and Dijkstra, J. H.: 1972, Solar Phys. 24, 395.CrossRefGoogle Scholar
Freeman, F. F. and Jones, B. B.: 1970, Solar Phys. 15, 288.Google Scholar
Landini, M. and Monsignori Fossi, B. C.: 1970, Astron. Astrophys. 6, 468.Google Scholar
Manson, J. E.: 1967, Astrophys. J. 147, 703.Google Scholar
Mewe, R.: 1972a, Solar Phys. 22, 459.Google Scholar
Mewe, R.: 1972b, to be published in Astron. Astrophys.Google Scholar
Noyes, R. W.: 1971, Ann. Rev. Astron. Astrophys. 9, 209.Google Scholar
Tousey, R., Austin, W. E., Purcell, J. D., and Widing, K. G.: 1965, Ann. Astrophys. 28, 755.Google Scholar
Widing, K. G. and Sandlin, G. D.: 1968, Astrophys. J. 152, 545.Google Scholar