Results 81 to 90 of about 4,088,052 (157)
Automated detection of solar eruptions
Observation of the solar atmosphere reveals a wide range of motions, from small scale jets and spicules to global-scale coronal mass ejections (CMEs).
Hurlburt N.
doaj +1 more source
Characteristics of coronal mass ejections in the near Sun interplanetary space [PDF]
Based on the observations from the Large Angle and Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory (SOHO) spacecraft we studied coronal mass ejections (CME) parameters between 6 and 10 solar radii from the Sun.
Nat Gopalswamy +2 more
doaj
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
core +3 more sources
The Internal Magnetic Field Structure of Interplanetary Coronal Mass Ejections in the Heliosphere
Interplanetary coronal mass ejections (ICMEs) are major drivers of heliospheric disturbances and space-weather effects. Here, we present a multispacecraft study of 96 magnetic clouds (MCs) distributed over a broad range of heliocentric distances and ...
Ziwei Huang +9 more
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Modeling observations of solar coronal mass ejections with heliospheric imagers verified with the Heliophysics System Observatory. [PDF]
Möstl C +21 more
europepmc +1 more source
While the amount of solar coronal energy flux leaving the “quiet” Sun, coronal holes, and active regions has been estimated by many, similar calculations for transients like coronal mass ejections (CMEs) based on observations are few. Using spectroscopic
R. Ramesh +5 more
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Coronal mass ejections (CMEs) release between ≈10 ^30 and 10 ^33 erg of energy into the corona; however, their detailed energy budget is difficult to constrain.
E. M. Wraback +3 more
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Simultaneous in situ measurements of coronal mass ejections (CMEs), including both plasma and magnetic field, by two spacecraft in radial alignment have been extremely rare.
F. Regnault +6 more
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Driving Dynamical Inner‐Heliosphere Models With In Situ Solar Wind Observations
Accurately reconstructing the solar wind throughout the inner heliosphere is essential for understanding solar–terrestrial interactions and improving space‐weather forecasts.
M. J. Owens +10 more
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This study examines the statistical properties of coronal mass ejections (CMEs) over two and a half solar cycles (1996–2025) using coronal observations from the SOHO LASCO CDAW and CACTus catalogs, supplemented by sunspot number records and in situ ...
Olga Khabarova +4 more
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