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
Documents 1 The search for signatures of ion cyclotron resonance in the low corona Laurent Dolla Jacques Solomon Philippe Lemaire Institut d'Astrophysique Spatiale

221 views

Capabilities of UV Coronagraphic Spectroscopy for Studying the Source Regions of SEPs & the Solar Wind John Kohl, Steven Cranmer, Larry Gardner, Jun Lin,
Documents Capabilities of UV Coronagraphic Spectroscopy for Studying the Source Regions of SEPs & the Solar Wind John Kohl, Steven Cranmer, Larry Gardner, Jun Lin,

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Hybrid simulations of parallel and oblique electromagnetic alpha/proton instabilities in the solar wind Q. M. Lu School of Earth and Space Science, Univ
Documents 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
Documents 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

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Spectroscopic Diagnostics of Solar Wind, CME, and SEP Source Regions Imaging Workshop, NSSTC, Huntsville, AL, 9-10 November 2004 Spectroscopic Diagnostics
Documents Spectroscopic Diagnostics of Solar Wind, CME, and SEP Source Regions Imaging Workshop, NSSTC, Huntsville, AL, 9-10 November 2004 Spectroscopic Diagnostics

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General Properties Internal Structure Solar Atmosphere Photosphere, chromosphere, and corona
Documents General Properties Internal Structure Solar Atmosphere Photosphere, chromosphere, and corona

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Boundaries, shocks, and discontinuities. How discontinuities form Often due to “wave steepening” Example in ordinary fluid: –V s 2 = dP/d m –P
Documents Boundaries, shocks, and discontinuities. How discontinuities form Often due to “wave steepening” Example in ordinary fluid: –V s 2 = dP/d m –P

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Quelques développements récents sur la physique du chauffage coronal. T. Passot UNS, CNRS, OCA Hinode/XRT Thanks to: E. Buchlin, S. Galtier. Some viewgraphs
Documents 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……
Documents SUMER Analysis: That was 1999……

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Q. M. Lu
Documents Q. M. Lu

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Self Consistent Solar Wind ModelsS. R. Cranmer, 25 January 2010, ISSI, Bern, Switzerland Self Consistent Solar Wind Models Steven R. Cranmer Harvard-Smithsonian
Documents 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
Documents Ingolf E. Dammasch ROB/SIDC Brussels, Belgium

47 views