Alpha–Proton Differential Flow of a Coronal Mass Ejection at 15 Solar Radii
Xuechao Zhang +6 more
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Future opportunities in solar system plasma science through ESA's exploration programme. [PDF]
Holmstrom M, Lester M, Sanchez-Cano B.
europepmc +1 more source
Mapping the Sun's coronal magnetic field using the Zeeman effect. [PDF]
Schad TA +11 more
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Europa Clipper Magnetometer Boom Deployment: A First Look at the Magnetometer Observations of the Spacecraft and the Interplanetary Magnetic Field. [PDF]
Cochrane CJ +21 more
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Revealing an unexpectedly low electron injection threshold via reinforced shock acceleration. [PDF]
Raptis S +5 more
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Influence of geomagnetic disturbances on myocardial infarctions in women and men from Brazil. [PDF]
Rezende LFC +6 more
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Solar Wind Magnetosphere Ionosphere Link Explorer (SMILE): Science and Mission Overview. [PDF]
Wang C +3 more
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The launch of solar coronal mass ejections: Results from the coronal mass ejection onset program
Journal of Geophysical Research: Space Physics, 1990We describe a set of solar coronal mass ejection (CME) events where coincident data sets from both X ray and white light instruments have been made available through deliberate planning. Using these we have been able to put tight limits on possible descriptions of the typical sequence of events, and these we relate to interpretations of models ...
R. A. Harrison +4 more
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The Hydromagnetic Nature of Solar Coronal Mass Ejections
Annual Review of Astronomy and Astrophysics, 2005▪ Abstract Solar coronal mass ejections (CMEs) are a major form of activity on the Sun. A CME takes 1015-16g of plasma from the low corona into the solar wind, to disturb the near-Earth space if the CME direction is favorable. We summarize current observations and ideas of CME physics to provide a hydromagnetic view of the CMEs as the products of ...
Mei Zhang, Boon Chye Low
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