Results 51 to 60 of about 1,134 (135)
Some Coronal Mass Ejections are Caused by Shock Waves in Other Regions of the Sun
, 2000 This press release examines evidence of a possible new triggering mechanism for coronal mass ejections (CMEs) from the Sun. Scientists using data from the Yohkoh and SOHO satellites noticed that interconnecting X-ray loops, as they disappeared, were ...
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Stealth Coronal Mass Ejections from Active Regions [PDF]
, 2019 Stealth coronal mass ejections (CMEs) are eruptions from the Sun that have no obvious low coronal signature. These CMEs are characteristically slower events but can still be geoeffective and affect space weather at Earth.
Green, L, O'Kane, J, Reid, H, Long, DM
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Differences between CME-driven storms and CIR-driven storms [PDF]
, 2006 Twenty one differences between CME-driven geomagnetic storms and CIR-driven geomagnetic storms are tabulated. (CME-driven includes driving by CME sheaths, by magnetic clouds, and by ejecta; CIR-driven includes driving by the associated recurring high ...
Borovsky, Joseph E., Denton, Michael H.
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ON SUN-TO-EARTH PROPAGATION OF CORONAL MASS EJECTIONS: II. SLOW EVENTS AND COMPARISON WITH OTHERS
, 2015 As a follow-up study on Sun-to-Earth propagation of fast coronal mass ejections (CMEs), we examine the Sun-to-Earth characteristics of slow CMEs combining heliospheric imaging and in situ observations.
Richardson, John D. +6 more
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Dynamics of filaments, flares and coronal mass ejections (CMEs)
, 2005 The objective of this dissertation is to investigate the connection between the dynamics of solar surface phenomena such as filament eruptions, flares, the coronal mass ejections (CMEs), the core of so-called solar activity, and the properties of the ...
Jing, Ju
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Tuning the Exospace Weather Radio for Stellar Coronal Mass Ejections
, 2020 Coronal mass ejections (CMEs) on stars other than the Sun have proven very difficult to detect. One promising pathway lies in the detection of type II radio bursts.
Poppenhäger, Katja +9 more
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Interplanetary Coronal Mass Ejections During 1996 - 2007
, 2007 Interplanetary coronal mass ejections, the interplanetary counterparts of coronal mass ejections at the Sun, are the major drivers of interplanetary shocks in the heliosphere, and are associated with modulations of the galactic cosmic ray intensity, both
Richardson, I. G., Cane, H. V.
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Coronal mass ejections are not coherent magnetohydrodynamic structures
, 2017 Coronal mass ejections (CMEs) are episodic eruptions of solar plasma and magnetic flux that travel out through the solar system, driving extreme space weather. Interpretation of CME observations and their interaction with the solar wind typically assumes
Owens, M. J. +5 more
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