Abstract
Center of disk EUV line intensities from quiet and active regions are used for determining an analytical expression for the variation of temperature with height in the lower corona, including the corona-chromosphere transition region. This approach imposes two coronal temperature regimes in both quiet and active regions. In each case the lower temperature regime is a continuation of the transition region, reaching a maximum of about 1.4 million deg in the quiet and 1.7 million deg in the active region. In the quiet region the high temperature regime, assumed isothermal, has a temperature of about 2.4 million deg, and in the active region, about 4.2 million deg.
Similar content being viewed by others
References
Allen, J. W. and Dupree, A. K.: 1969, Astrophys. J. 155, 27.
Athay, R. G.: 1966, Astrophys. J. 145, 784.
Athay, R. G.: 1971, in C. J. Macris (ed.), Physics of the Solar Corona, D. Reidel Publ. Co., Dordrecht, Holland, p. 36.
Athay, R. G., and Roberts, W. O.: 1955, Astrophys. J. 121, 231.
Batstone, R. M., Evans, K., Parkinson, J. H., and Pounds, K. A.: 1970, Solar Phys. 13, 389.
Billings, D. E.: 1959, Astrophys. J. 130, 961.
Dollfus, A.: 1971, in C. J. Macris (ed.), Physics of the Solar Corona, D. Reidel Publ. Co., Dordrecht, Holland, p. 97.
Dupree, A. K.: 1972, Astrophys. J. 178, 527.
Dupree, A. K. and Goldberg, L.: 1967, Solar Phys. 1, 229.
Dupree, A. K., Huber, M. C. E., Noyes, R. W., Parkinson, W. H., Reeves, E. M., and Withbroe, G. L.: 1973, Astrophys. J. 182, 321.
Evans, K. and Pounds, K. A.: 1968, Astrophys. J. 152, 319.
Jordan, C. and Wilson, R.: 1971, in C. J. Macris (ed.), Physics of the Solar Corona, D. Reidel Publ. Co., Dordrecht, Holland, p. 219.
Kopp, R. A.: 1972, Solar Phys. 27, 373.
Noyes, R. W.: 1971, in C. J. Macris (ed.), Physics of the Solar Corona, D. Reidel Publ. Co., Dordrecht, Holland, p. 192.
Pottasch, S. R.: 1963, Astrophys. J. 137, 945.
Pottasch, S. R.: 1964, Space Sci. Rev. 3, 816.
Waldmeier, M.: 1956, Z. Astrophys. 39, 219.
Walker, A. B. C., Jr.: 1972, Space Sci. Rev. 13, 672.
Walker, A. B. C., Jr., Rugge, H. R., and Weiss, K.: 1974, Astrophys. J. 188, 423.
Widing, K. G. and Sandlin, G. D.: 1968, Astrophys. J. 152, 545.
Withbroe, G. L.: 1970a, Solar Phys. 11, 42.
Withbroe, G. L.: 1970b, Solar Phys. 11, 208.
Withbroe, G. L. and Gurman, J. B.: 1973, Astrophys. J. 183, 279.
Wolff, R. S.: 1974, Solar Phys. 34, 163.
Zirker, J. B.: 1971, in C. J. Macris (ed.), Physics of the Solar Corona, D. Reidel Publ. Co., Dordrecht, Holland, p. 140.
Author information
Authors and Affiliations
Additional information
Now at: Observatorio Astronomico Nacional, APTO, Postal 877, Ensenada, B. C., Mexico
Rights and permissions
About this article
Cite this article
Billings, D.E., Alvarez, M. Coronal information from EUV disk spectral line intensities. Sol Phys 40, 23–38 (1975). https://doi.org/10.1007/BF00183149
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00183149