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The top documents tagged [fast solar wind]

1 The search for signatures of ion cyclotron resonance in the low corona Laurent Dolla Jacques Solomon Philippe Lemaire Institut d'Astrophysique Spatiale
1 The search for signatures of ion cyclotron resonance in the low corona Laurent Dolla Jacques Solomon Philippe Lemaire Institut d'Astrophysique Spatiale
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Capabilities of UV Coronagraphic Spectroscopy for Studying the Source Regions of SEPs & the Solar Wind John Kohl, Steven Cranmer, Larry Gardner, Jun Lin,
Capabilities of UV Coronagraphic Spectroscopy for Studying the Source Regions of SEPs & the Solar Wind John Kohl, Steven Cranmer, Larry Gardner, Jun Lin,
217 views
Hybrid simulations of parallel and oblique electromagnetic alpha/proton instabilities in the solar wind Q. M. Lu School of Earth and Space Science, Univ
Hybrid simulations of parallel and oblique electromagnetic alpha/proton instabilities in the solar wind Q. M. Lu School of Earth and Space Science, Univ
217 views
Solar activity over the last 1150 years: does it correlate with climate? S.K. Solanki 1, I. Usoskin 2, M. Schüssler 1, K. Mursula 2 1: Max-Planck-Institut
Solar activity over the last 1150 years: does it correlate with climate? S.K. Solanki 1, I. Usoskin 2, M. Schüssler 1, K. Mursula 2 1: Max-Planck-Institut
214 views
Spectroscopic Diagnostics of Solar Wind, CME, and SEP Source Regions Imaging Workshop, NSSTC, Huntsville, AL, 9-10 November 2004 Spectroscopic Diagnostics
Spectroscopic Diagnostics of Solar Wind, CME, and SEP Source Regions Imaging Workshop, NSSTC, Huntsville, AL, 9-10 November 2004 Spectroscopic Diagnostics
221 views
General Properties Internal Structure Solar Atmosphere Photosphere, chromosphere, and corona
General Properties Internal Structure Solar Atmosphere Photosphere, chromosphere, and corona
53 views
Boundaries, shocks, and discontinuities. How discontinuities form Often due to “wave steepening” Example in ordinary fluid: –V s 2 = dP/d m –P
Boundaries, shocks, and discontinuities. How discontinuities form Often due to “wave steepening” Example in ordinary fluid: –V s 2 = dP/d m –P
218 views
Quelques développements récents sur la physique du chauffage coronal. T. Passot UNS, CNRS, OCA Hinode/XRT Thanks to: E. Buchlin, S. Galtier. Some viewgraphs
Quelques développements récents sur la physique du chauffage coronal. T. Passot UNS, CNRS, OCA Hinode/XRT Thanks to: E. Buchlin, S. Galtier. Some viewgraphs
213 views
SUMER Analysis: That was 1999……
SUMER Analysis: That was 1999……
21 views
Q. M. Lu
Q. M. Lu
26 views
Self Consistent Solar Wind ModelsS. R. Cranmer, 25 January 2010, ISSI, Bern, Switzerland Self Consistent Solar Wind Models Steven R. Cranmer Harvard-Smithsonian
Self Consistent Solar Wind ModelsS. R. Cranmer, 25 January 2010, ISSI, Bern, Switzerland Self Consistent Solar Wind Models Steven R. Cranmer Harvard-Smithsonian
222 views
Ingolf E. Dammasch ROB/SIDC Brussels, Belgium
Ingolf E. Dammasch ROB/SIDC Brussels, Belgium
47 views