The Chromosphere and Spicules

Author:

Aschwanden Markus J.

Publisher

Springer International Publishing

Reference211 articles.

1. Alissandrakis, C.E., Patsourakos, S., Nindos, A., et al. 2017, Center-to-limb observations of the Sun with ALMA. Implications for solar atmospheric models, A&A 605, A78, [2 c, 2 c/y].

2. Avrett, E.H. and Loeser, R. 2008, Models of the solar chromosphere and transition region from SUMER and HRTS observations: Formation of the EUV spectrum of hydrogen, carbon, and oxygen, ApJS 175, 229, [150 c, 16 c/y].

3. Avrett, E.H., Tian, H., Landi, E., et al. 2015, Modeling the chromosphere of a sunspot and the Quiet Sun, ApJ 811, 87, [4 c, 2 c/y].

4. Carlsson, M. and Stein, R.E. 1995, Does a nonmagnetic solar chromosphere exist? ApJ 440, L29, [268 c, 12 c/y].

5. Carlsson, M. 2007, Modeling the solar chromosphere, in ASP Conf. Ser. 368, The physics of chromospheric plasmas, (ed. P. Heinzel, R. Dorotovic, and R.J. Rutten), (San Francisco: ASP), 49, [15 c, 1 c/y].

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