Response of the low ionosphere to X-ray and Lyman-α solar flare emissions

Author:

Raulin Jean-Pierre1,Trottet Gérard2,Kretzschmar Matthieu34,Macotela Edith L.5,Pacini Alessandra6,Bertoni Fernando C. P.1,Dammasch Ingolf E.7

Affiliation:

1. Centro de Radio Astronomia e Astrofísica Mackenzie, CRAAM; Universidade Presbiteriana Mackenzie; São Paulo SP Brazil

2. Observatoire de Paris, LESIA-CNRS UMR 8109; Univ. P & M Curie and Paris-Diderot; Observatoire de Meudon Meudon France

3. Solar Terrestrial Center of Excellence; Royal Observatory of Belgium; Brussels Belgium

4. LPC2E, UMR 6116 CNRS & University of Orléans; Orléans France

5. Comisión Nacional de Investigación y Desarrollo Aeroespacial (CONIDA); Lima Peru

6. Universidade do Vale do Paraíba (UNIVAP); São José dos Campos SP Brazil

7. Solar Influence Data Analysis Center/Royal Observatory of Belgium; Brussels Belgium

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference33 articles.

1. The study of solar flares by means of very long radio waves;Bracewell;Mon. Not. R. Astron. Soc.,1949

2. Analysis of daytime ionosphere behavior between 2004 and 2008 in Antarctica;Correia;J. Atmos. Sol. Terr. Phys.,2011

3. VLF phase perturbation associated with meteor shower ionization;Chilton;J. Geophys. Res.,1961

4. The LYRA instrument onboard PROBA2: Description and in-flight performance;Dominique;Solar Physics,2012

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