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Autor:
J. C. Noens, R. T. Salakhutdinov, A. Bucher, I. S. Kim, V. I. Skomorovsky, F. I. Guetman, A. A. Semenikin, C. A. Druzhinin
Publikováno v:
International Astronomical Union Colloquium. 144:575-578
The red coronal line of Fe X (6374 Å) seems to be extremely suitable for filter observations due to reduced sky scattering in this spectral interval and absence of blending by Fraunhofer lines. Comparative analysis of location of Hαstructures in co