Electron Densities in the Solar Polar Coronal Holes from Density-Sensitive Line Ratios of Si VIII and S X
暂无分享,去创建一个
H. Warren | U. Schühle | G. Doschek | J. Mariska | J. Laming | K. Wilhelm | P. Lemaire | T. G. Moran
[1] J. Raymond,et al. Electron-ion Equilibration in Nonradiative Shocks Associated With SN 1006 , 1996 .
[2] Madhulika Guhathakurta,et al. Physical Properties of Polar Coronal Rays and Holes as Observed with the Spartan 201-01 Coronagraph , 1995 .
[3] S. Habbal,et al. How reliable are coronal hole temperatures deduced from observations , 1993 .
[4] G. Rottman,et al. Coronal Density and Temperature Structure from Coordinated Observations Associated with the Total Solar Eclipse of 1988 March 18 , 1992 .
[5] G. Doschek,et al. Solar coronal Ar/Fe and Ne/Mg abundance ratios derived from ultraviolet forbidden line spectra , 1990 .
[6] H. Mason,et al. Electron densities in the solar corona from density-sensitive line ratios in the N I isoelectronic sequence , 1978 .
[7] U. Feldman,et al. The dynamical properties of the solar corona from intensities and line widths of EUV forbidden lines of Si VIII, Fe XI, and Fe XII , 1978 .
[8] J. Harvey,et al. A comparison of He ii 304 Å and He i 10 830 Å spectroheliograms , 1977 .
[9] U. Feldman,et al. The coronal temperature and nonthermal motions in a coronal hole compared with other solar regions , 1977 .
[10] J. Mariska. Extreme Ultraviolet Observations of a Polar Coronal Hole , 1976 .
[11] H. F. Allen. Atlas of Strabismus , 1973 .
[12] R. Wilson,et al. The Ultraviolet Emission Spectrum of the Solar Chromosphere and Corona , 1967 .
[13] J. G. Timothy,et al. FIRST RESULTS OF THE SUMER TELESCOPE AND SPECTROMETER ON SOHO – II. Imagery and Data Management , 1997 .
[14] Donald M. Hassler,et al. First results of the SUMER telescope and spectrometer-solar ultraviolet measurements of emitted radiation-on SOHO, I. Spectra and Spectroradiometry , 1997 .
[15] C. Jordan. The identification of new forbidden coronal lines in the solar EUV spectrum , 1971 .
[16] J. V. Vleck,et al. Multiplet Intensities for the Nebular Lines ^{4}S - _{2}D of ο II. , 1949 .