Results 91 to 100 of about 3,198,119 (194)
Modelling electron beams in flux-rope coronal mass ejections
Astronomy & AstrophysicsContext. Counterstreaming suprathermal electron beams are frequently observed within interplanetary coronal mass ejections (CMEs) and are commonly interpreted as signatures of particle trapping along closed magnetic flux ropes.
Flossie M., Wijsen N., Poedts S.
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Solar energetic particle events: phenomenology and prediction
, 2002 Solar energetic particle events can cause major disruptions to the operation of spacecraft in earth orbit and outside the earth's magnetosphere and have to be considered for EVA and other manned activities. They may also have an effect on radiation doses
Patrick, G.J. +4 more
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Corotating interaction regions as seen by the STEREO Heliospheric Imagers 2007 – 2010 [PDF]
, 2015 T.M. Conlon and A.O. Williams were supported by an STFC, UK studentship and S.E. Milan was supported by STFC grant ST/K001000/1. Date of Acceptance: 08/08/2015NASA’s Solar Terrestrial Relations Observatory (STEREO) mission has coincided with a pronounced
J. A. Davies +7 more
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The Astrophysical JournalStudies for inferring the global characteristics of coronal mass ejections (CMEs) from multipoint local in situ observations have been undertaken previously, but limited studies have utilized measurements from multiple spacecraft with sufficiently small ...
Anjali Agarwal, Wageesh Mishra
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The Astrophysical JournalThe radial and lateral dimensions of coronal mass ejections (CMEs) influence their duration and probability of encounter at Earth. These properties are linked to the expansion speeds of CMEs in different radial and lateral directions; however, most ...
Anjali Agarwal +4 more
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Regarding the detectability and measurement of coronal mass ejections
Journal of Space Weather and Space Climate, 2015 In this review I discuss the problems associated with the detection and measurement of coronal mass ejections (CMEs). CMEs are important phenomena both scientifically, as they play a crucial role in the evolution of the solar corona, and technologically,
Howard Timothy A.
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Evolution of Coronal Mass Ejection Properties through Superposed Epoch Analysis from 0.2 to 2.2 au
The Astrophysical JournalCoronal mass ejections (CMEs) are explosive and energetic events consisting of strong magnetic structures erupting from the solar corona. We use superposed epoch analysis (SEA) to investigate the general properties of CMEs as measured in situ from 0.2 to
Yakub Olufadi +8 more
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Observing Solar Coronal Mass Ejections from Space [PDF]
In this contribution to the panel discussion of the IAU Symposium 388 Solar and Stellar Coronal Mass Ejections , I concentrate on white-light observations of solar coronal mass ejections (CMEs) from space and specifically address the following aspects ...
Lamy, Philippe
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Detecting Stellar Coronal Mass Ejections via Coronal Dimming in the Extreme Ultraviolet
The Astrophysical JournalStellar flares and coronal mass ejections (CMEs) can strip planetary atmospheres, reducing the potential habitability of terrestrial planets. While flares have been observed for decades, stellar CMEs remain elusive.
James Paul Mason +4 more
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Journal of Space Weather and Space Climate, 2012 In past studies, we classified the near-Earth solar wind into three basic flow types based on inspection of solar wind plasma and magnetic field parameters in the OMNI database and additional data (e.g., geomagnetic indices, energetic particle, and ...
Richardson Ian G., Cane Hilary V.
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