Dual chromospheric flows in the surroundings of a solar pore

Author:

Leiko U.M., ,Kondrashova N.N.,

Publisher

National Academy of Sciences of Ukraine (Co. LTD Ukrinformnauka)

Subject

General Medicine

Reference41 articles.

1. 1.U. M. Leiko and N. N. Kondrashova, "The chromospheric line-of-sight velocity variations in a solar microflare," Izv. Krym. Astrofiz. Obs. 109 (3), 72-77 (2013).

2. 2.R. Aznar Cuadrado, S. K. Solanki, and A. Lagg, "Supersonic downflows in the solar chromosphere are very common," in Proc. Int. Sci. Conf. on Chromospheric and Coronal Magnetic Fields, Katlenburg-Lindau, Germany, Aug. 30-Sept. 2, 2005, Ed. by D. E. Innes, A. Lagg, S. K. Solanki, and D. Danesy (ESA, Noordwijk, 2005), paper id. 49.1.

3. 3.R. Aznar Cuadrado, S. K. Solanki, and A. Lagg, "Velocity distribution of chromospheric downflows," in Proc. Workshop Modern Solar Facilities - Advanced Solar Science, Göttingen, Germany, Sept. 27-29, 2006, Ed. by F. Kneer, K. G. Puschmann, and A. D. Wittmann (Universitatsverlag Göttingen, Göttingen, 2007), pp. 173-176.

4. 4.P. Brekke, N. Brynildsen, O. Kjeldseth-Moe, et al., "Multiple flow velocities in the transition region," Adv. Space Res. 11 (5), 251-254 (1991).

5. 5.P. Brekke, O. Kjeldseth-Moe, and G. E. Brueckner, "Multiple downflow velocities above sunspots," Astrophys. Space Sci. 170, 135-140 (1990).

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