Results 171 to 180 of about 16,696 (216)

Future opportunities in solar system plasma science through ESA's exploration programme. [PDF]

NPJ Microgravity
Holmstrom M, Lester M, Sanchez-Cano B.
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The delayed arrival of faster solar energetic particles as a probe into the shock acceleration process. [PDF]

Natl Sci Rev
Li Y, Guo J, Pacheco D, Wang Y, Temmer M, Ding Z, Wimmer-Schweingruber RF.   +6 more
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Multispacecraft Observations of the 2024 September 9 Backside Solar Eruption That Resulted in a Sustained Gamma Ray Emission Event. [PDF]

Sol Phys
Gopalswamy N, Mäkelä P, Akiyama S, Xie H, Yashiro S, Bale SD, Wimmer-Schweingruber RF, Kühl P, Krucker S.   +8 more
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Science development study for the Atacama Large Aperture Submillimeter Telescope (AtLAST): Solar and stellar observations. [PDF]

Open Res Eur
Wedemeyer S, Barta M, Brajša R, Chai Y, Costa J, Gary D, Gimenez de Castro G, Gunar S, Fleishman G, Hales A, Hudson H, Kirkaune M, Mohan A, Motorina G, Pellizzoni A, Saberi M, Selhorst CL, Simoes PJA, Shimojo M, Skokić I, Sudar D, Menezes F, White SM, Booth M, Klaassen P, Cicone C, Mroczkowski T, Cordiner MA, Di Mascolo L, Johnstone D, van Kampen E, Lee M, Liu D, Maccarone T, Orlowski-Scherer J, Saintonge A, Smith M, Thelen AE.   +37 more
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Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab

Santos Ld, Owen J, Duvvuri G, Loyd ROP, Vidotto A, Presa A, Bourrier V, King G, Airapetian V, Ehrenreich D, France K, Lendl M, Lothringer J, Nielsen L.   +13 more
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Coronal Mass Ejections

Space Science Reviews, 2006
A Brief History of CME Science.- Coronal Mass Ejections: Overview of Observations.- In-Situ Solar Wind and Magnetic Field Signatures of Interplanetary Coronal Mass Ejections.- An Introduction to CMEs and Energetic Particles.- An Introduction to Theory and Models of CMEs, Shocks, and Solar Energetic Particles.- An Introduction to the pre-CME Corona ...
H. Kunow, N. U. Crooker, J. A. Linker, R. Schwenn, R. Von Steiger   +4 more
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Coronal Mass Ejections

Annual Review of Astronomy and Astrophysics, 1984
Sudden expulsions of dense clouds of plasma from the outer atmosphere of the Sun, termed "coronal mass ejections" (CMEs), are the focus of intense observational and theoretical efforts. CMEs are a type of coronal transient, the general name given the disruption of coronal structure.
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Coronal mass ejections

AIP Conference Proceedings, 2000
The most dramatic changes in the solar corona occur during coronal mass ejections, or CMEs, during which solar material is propelled outward into the heliosphere from regions in the corona not previously participating in the solar wind expansion. These ejections often produce major solar wind disturbances, large geomagnetic storms, enhancements of ...
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Radio Signatures of Coronal Mass Ejection Interaction: Coronal Mass Ejection Cannibalism?

The Astrophysical Journal, 2001
We report the first detection at long radio wavelengths of interaction between coronal mass ejections (CMEs) in the interplanetary medium. The radio signature is in the form of intense continuum-like radio emission following an interplanetary type II burst. At the time of the radio enhancement, coronagraphic images show a fast CME overtaking a slow CME.
N. Gopalswamy, S. Yashiro, M. L. Kaiser, R. A. Howard, J.-L. Bougeret   +4 more
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Coronal mass ejections

Reviews of Geophysics, 1987
While the first coronal mass ejections (CMEs) were observed with the OSO‐7 white light coronagraph (Tousey, 1973), it was the Skylab coronagraph observations that clearly established CMEs as an important component of solar coronal physics. CMEs have been defined by Hundhausen et al.
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