Derivation of the Major Properties of Prominences Using NLTE Modelling

Author:

Labrosse Nicolas

Publisher

Springer International Publishing

Reference62 articles.

1. Anzer, U., & Heinzel, P. (1999). The energy balance in solar prominences. Astronomy and Astrophysics, 349, 974–984.

2. Auer, L., Bendicho, P. F., & Trujillo Bueno, J. (1994). Multidimensional radiative transfer with multilevel atoms. 1: ALI method with preconditioning of the rate equations. Astronomy and Astrophysics, 292, 599–615.

3. Ballester, J. L. (2014). Magnetism and dynamics of prominences: MHD waves. In J.-C. Vial, & O. Engvold (Eds.), Solar Prominences, ASSL (Vol. 415, pp. 257–296). Springer.

4. Bommier, V., Landi Degl’Innocenti, E., Leroy, J.L., & Sahal-Brechot, S. (1994). Complete determination of the magnetic field vector and of the electron density in 14 prominences from linear polarization measurements in the HeI D3 and H-alpha lines. Solar Physics, 154, 231–260. doi:10.1007/BF00681098.

5. Engvold, O. (2014). Description and classification of prominences. In J.-C. Vial, & O. Engvold (Eds.), Solar prominences, ASSL (Vol. 415, pp. 31–60). Springer.

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