A type II solar radio burst without a coronal mass ejection
D. E. Morosan +4 more
openalex +1 more source
An Extreme Stellar Prominence Eruption Observed by LAMOST Time-domain Spectroscopy
We report the detection of an extreme stellar prominence eruption on the M dwarf Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) J044431.62+235627.9, observed through time-domain H α spectroscopy with the LAMOST.
Hong-Peng Lu +8 more
doaj +1 more source
Multiple magnetic reconnection sites associated with a coronal mass ejection in the solar wind [PDF]
J. T. Gosling +4 more
openalex +1 more source
Anticorrelated temperature-density profiles in the quiet solar corona and coronal mass ejections: Approach based on the spin-type Hamiltonians [PDF]
Yurii V. Dumin
openalex +2 more sources
How Does the Critical Torus Instability Height Vary with the Solar Cycle?
The ideal magnetohydrodynamic torus instability can drive the eruption of coronal mass ejections. The critical threshold of magnetic field strength decay for the onset of the torus instability occurs at different heights in different solar active regions,
Alexander W. James +4 more
doaj +1 more source
Statistical Analysis of the Relation between Coronal Mass Ejections and Solar Energetic Particles
Kosuke Kihara +6 more
openalex +1 more source
CONSTRAINING THE MASSES AND THE NON-RADIAL DRAG COEFFICIENT OF A SOLAR CORONAL MASS EJECTION [PDF]
C. Kay, L. F. G. dos Santos, M. Opher
openalex +1 more source
Observations of solar energetic particle events during multiple coronal mass ejections [PDF]
S. Pohjolainen +2 more
openalex +1 more source
Nonlinear Force‐free Field Modeling of a Solar Active Region around the Time of a Major Flare and Coronal Mass Ejection [PDF]
C. J. Schrijver +16 more
openalex +1 more source

