Results 141 to 150 of about 243 (164)
Update of the Photometric Calibration of the LASCO-C2 Coronagraph Using Stars. [PDF]
Colaninno RC, Howard RA.
europepmc +1 more source
Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab
Santos Ld +13 more
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Stellar activity and coronal heating: an overview of recent results. [PDF]
Testa P, Saar SH, Drake JJ.
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Magnetism, dynamo action and the solar-stellar connection. [PDF]
Brun AS, Browning MK.
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From Starspots to Stellar Coronal Mass Ejections—Revisiting Empirical Stellar Relations [PDF]
Abstract Upcoming missions, including the James Webb Space Telescope, will soon characterize the atmospheres of terrestrial-type exoplanets in habitable zones around cool K- and M-type stars by searching for atmospheric biosignatures.
Konstantin Herbst +2 more
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Indications of stellar coronal mass ejections through coronal dimmings [PDF]
Coronal mass ejections (CMEs) are huge expulsions of magnetized matter from the Sun and stars, traversing space with speeds of millions of kilometers per hour. Solar CMEs can cause severe space weather disturbances and consumer power outages on Earth, whereas stellar CMEs may even pose a hazard to the habitability of exoplanets.
Karin Dissauer +2 more
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The quest for stellar coronal mass ejections in late-type stars [PDF]
International ...
Lidia Van Driel-Gesztelyi +2 more
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Stellar coronal mass ejections – I. Estimating occurrence frequencies and mass-loss rates [PDF]
18 pages, 8 figures, 1 table, accepted to ...
Helmut Lammer +2 more
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The Search for Stellar Coronal Mass Ejections
2017Coronal mass ejections (CMEs) may dramatically impact habitability and atmospheric composition of planets around magnetically active stars, including young solar analogs and many M dwarfs. Theoretical predictions of such effects are limited by the lack of observations of stellar CMEs. This thesis addresses this gap through a search for the spectral and
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Observations and simulations of stellar coronal mass ejections
SCIENTIA SINICA Technologica, 2023Hui TIAN +7 more
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