Flows along arch filaments observed in the GRIS ‘very fast spectroscopic mode’.

Autor: González Manrique, S. J.1,2 (AUTHOR) smanrique@aip.de, Denker, C.1 (AUTHOR), Kuckein, C.1 (AUTHOR), Yabar, A. Pastor3,4 (AUTHOR), Collados, M.3 (AUTHOR), Verma, M.1 (AUTHOR), Balthasar, H.1 (AUTHOR), Diercke, A.1,2 (AUTHOR), Fischer, C. E.5 (AUTHOR), Gömöry, P.6 (AUTHOR), Bello González, N.5 (AUTHOR), Schlichenmaier, R.5 (AUTHOR), Armas, M. Cubas3,4 (AUTHOR), Berkefeld, T.5 (AUTHOR), Feller, A.5 (AUTHOR), Hoch, S.7 (AUTHOR), Hofmann, A.1 (AUTHOR), Lagg, A.7 (AUTHOR), Nicklas, H.8 (AUTHOR), Orozco Suárez, D.3,4 (AUTHOR)
Zdroj: Proceedings of the International Astronomical Union. Oct2016 Supplement, Vol. 12 Issue S327, p28-33. 6p. 4 Graphs.
Databáze: Academic Search Ultimate