Accurate Intensity – Velocity Phase Difference in the Potassium Resonance Line Obtained with VAMOS

Author:

Magrì M.,Oliviero M.,Severino G.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference18 articles.

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2. Ermolli, I., Fofi, M., Bernacchia, C., Berrilli, F., Caccin, B., Egidi, A., Florio, A.: 1998, Solar Phys. 177, 1.

3. Georgobiani, D., Stein, R.F., Nordlund, Å: 2003, Astrophys. J. 596, 698.

4. Hill, F., Deubner, F.-L., Isaak, G.: 1991, In: Cox, A.N., Livingston, W.C., Matthews, M.S. (eds.) Solar Interior and Atmosphere, University of Arizona, Tucson, 329.

5. Jiménez, A., Roca Cortés, T., Severino, G., Marmolino, C.: 1999, Astrophys. J. 525, 1042.

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