Zobrazeno 1 - 6
of 6
pro vyhledávání: '"523.3"'
Autor:
Demidov, M. L.1 demid@iszf.irk.ru, Balthasar, H.2 hbalthasar@aip.de
Publikováno v:
Solar Physics. Dec2009, Vol. 260 Issue 2, p261-270. 10p. 1 Diagram, 1 Chart, 7 Graphs.
Autor:
Balthasar, H.1 hbalthasar@aip.de, Demidov, M.2 demid@iszf.irk.ru
Publikováno v:
Solar Physics. Oct2012, Vol. 280 Issue 2, p355-364. 10p.
Autor:
Demidov, M.1 demid@iszf.irk.ru, Balthasar, H.2 hbalthasar@aip.de
Publikováno v:
Solar Physics. Feb2012, Vol. 276 Issue 1/2, p43-59. 17p. 1 Diagram, 1 Chart, 18 Graphs.
Autor:
Demidov, M. L.1 demidov@iszf.irk.ru, Golubeva, E. M.1, Balthasar, H.2 hbalthasar@aip.de, Staude, J.2, Grigoryev, V. M.1
Publikováno v:
Solar Physics. Aug2008, Vol. 250 Issue 2, p279-301. 23p. 4 Diagrams, 3 Charts, 11 Graphs.
Autor:
Horst Balthasar, M. L. Demidov
Publikováno v:
Solar Physics. 260:261-270
Comparisons of solar magnetic-field measurements made in different spectral lines are very important, especially in those lines in which observations have a long history or(and) specific diagnostic significance. The spectral lines FeI 523.3 nm and Fe
Autor:
Bogdan, T.J.
Publikováno v:
Solar Physics; Mar2000, Vol. 192 Issue 1/2, p373-394, 22p