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Identifications of Emission Lines in the EUV Solar Spectrum

Published online by Cambridge University Press:  12 April 2016

Carole Jordan
Carole Jordan*
Affiliation:
Astrophysics Research Unit, Culham Laboratory, Abingdon, Berks., England

Extract

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In this brief review of solar line identifications the progress made since the previous conference in this series, which was held in Maryland in 1968, will be discussed.

Only lines which appear in emission when seen in the solar disk will be included, thus excluding lines from low stages of ionization at wavelengths of above about 2000Å which can appear in emission at the limb.

It is convenient to divide the solar spectrum between about 1.5 Å and 2300 Å into wavelength regions, since the various types of transitions which will be discussed tend to appear over restricted wavelength ranges.

Type
Section III / Stellar and Solar UV Radiation
Information
International Astronomical Union Colloquium , Volume 14: Special Issue: Ultraviolet and X-Ray Spectroscopy of Astrophysical and Laboratory Plasmas , November 1972 , pp. 595 - 605
Copyright
Copyright © Reidel 1972

References

Batstone, R. M., Evans, K., Parkinson, J. H., and Pounds, K. A.: 1970, Solar Phys. 13, 389.Google Scholar
Bely, O. and Blaha, M.: 1968, Solar Phys. 3, 563.Google Scholar
Blake, R. L., Chubb, T. H., Friedman, H., and Unzicker, A. E., 1965, Astrophys. J. 142, 1.Google Scholar
Burton, W. M. and Ridgeley, A.: 1970, Solar Phys. 14, 3.CrossRefGoogle Scholar
Burton, W. M., Ridgeley, A., and Wilson, R., 1967, Monthly Notices Roy. Astron. Soc. 135, 207.CrossRefGoogle Scholar
Doschek, G. A. and Meekins, J. F.: 1970, Solar Phys. 13, 220.Google Scholar
Doschek, G. A., Meekins, J. F., Kreplin, R. W., Chubb, T. A., and Friedman, H.: 1971, Astrophys. J. 170, 573.Google Scholar
Dupree, A. K. and Reeves, E. M.: 1971, Astrophys. J. 165, 599.CrossRefGoogle Scholar
Edlén, B.: 1972, Solar Phys., in press.Google Scholar
Edlén, B., Palenius, H. P., Bockasten, K., Hallin, R., and Bromander, J.: 1969, Solar Phys. 9, 432.Google Scholar
Engelhardt, W. and Sommer, J.: 1971, Astrophys. J. 167, 201.Google Scholar
Fawcett, B. C.: 1970a, J. Phys. B. 3, 1152.Google Scholar
Fawcett, B. C.: 1970b, J. Phys. B. 3, 1732.Google Scholar
Fawcett, B. C.: 1971a, J. Phys. B. 4, 981.CrossRefGoogle Scholar
Fawcett, B. C.: 1971b, J. Phys. B. 4, 1577.Google Scholar
Fawcett, B. C.: 1971c, Astrophysics Research Unit Report-R2., H. M. Stationery Office.Google Scholar
Fawcett, B. C. and Hayes, R. W.: 1971, J. Phys. B., in press.Google Scholar
Fawcett, B. C., Peacock, N. J. and Cowan, R. D.: 1968, J. Phys. B. 1, 295.Google Scholar
Fawcett, B. C., Gabriel, A. H., and Paget, T. W.: 1971, J. Phys. B. 4, 986.Google Scholar
Feldman, U. and Cohen, L.: 1968, Astrophys. J. 151, 55.Google Scholar
Feldman, U., Behring, W., and Cohen, L.: 1972, this issue, p. 608.CrossRefGoogle Scholar
Flower, D. R.: 1971, J. Phys. B. 4, 697.CrossRefGoogle Scholar
Flower, D. R. and Jordan, C.: 1971, Astron. Astrophys. 14, 473.Google Scholar
Freeman, F. F. and Jones, B. B.: 1970, Solar Phys. 15, 288.Google Scholar
Gabriel, A. H. and Jordan, C.: 1969a, Nature 221, 947.CrossRefGoogle Scholar
Gabriel, A. H. and Jordan, C.: 1969b, Monthly Notices Roy. Astron. Soc. 145, 241.Google Scholar
Gabriel, A. H., Garton, W. R. S., Goldberg, L., Jones, T. J. L., Jordan, C., Morgan, F. J., Nicholls, R. W., Parkinson, W. H., Paxton, H. J. B., Reeves, E. M., Shenton, D. B., Speer, R. J., and Wilson, R.: 1971, Astrophys. J. 169, 595.Google Scholar
Grineva, Yu. I., Karev, V. I., Korneev, V. V., Krutov, V. V., Mandel’stam, S. L., Vainstein, L. A., Vasiljev, B. N. and Zitnik, I. A.: 1971, paper presented at COSPAR, Seattle and to be published in Kosmich. Issled. USSR.Google Scholar
Hall, L. A. and Hinteregger, H. E.: 1970, J. Geophys. Res. 75, 6959.CrossRefGoogle Scholar
Hall, L. A., Damon, K. R., and Hinteregger, H. E.: 1963, Space Res. 3, 745.Google Scholar
Jefferies, J. T.: 1969, Mem. Soc. Roy. Sci. Liege, 17, 213.Google Scholar
Jordan, C.: 1968, J. Phys. B. 1, 1004.Google Scholar
Jordan, C.: 1971, Solar Phys. 21, 381.Google Scholar
Meekins, J. F., Doschek, G. A., Friedman, H., Chubb, T. A., and Kreplin, R. W.: 1970, Solar Phys. 13, 198.Google Scholar
Neupert, W. M.: 1971, Solar Phys. 18, 474.Google Scholar
Neupert, W. M. and Swartz, M.: 1970, Astrophys. J. 160, L189.Google Scholar
Neupert, W. M., Gates, W., Swartz, M., and Young, R., 1967, Astrophys. J. 149, 79.Google Scholar
Parkinson, J. H.: 1971, Nature, (Physical Science) 233, 44.Google Scholar
Speer, R. J., Garton, W. R. S., Goldberg, L., Parkinson, W. H., Reeves, E. M., Morgan, J. F., Nicholls, R. W., Jones, T. J. L., Paxton, H. J. B., Shenton, D. B., and Wilson, R.: 1970, Nature 226, 249.Google Scholar
Svensson, L. A.: 1971, Solar Phys. 18, 232.CrossRefGoogle Scholar
Svensson, L. A. and Eckberg, J. O.: 1968, Arkiv. Fysik 37, 65.Google Scholar
Wagner, W. J. and House, L. L.: 1969, Astrophys. J. 155, 677.Google Scholar
Wagner, W. J. and House, L. L.: 1971, Astrophys. J. 166, 683.CrossRefGoogle Scholar
Walker, A. B. C. and Rugge, H. R.: 1970, Astron. Astrophys. 5, 4.Google Scholar
Walker, A. B. C. and Rugge, H. R.: 1971, Astrophys. J. 164, 181.Google Scholar
Widing, K. G. and Sandlin, G. D.: 1968, Astrophys. J. 152, 545.Google Scholar
Widing, K. G., Sandlin, G. D., and Cowan, R.: 1971, Astrophys. J. 169, 405.Google Scholar