Results 1 to 10 of about 22,877 (292)
Living Reviews in Solar Physics, 2018 Prominences are intriguing, but poorly understood, magnetic structures of the solar corona. The dynamics of solar prominences has been the subject of a large number of studies, and of particular interest is the study of prominence oscillations.
Iñigo Arregui +2 more
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Physics of Solar Prominences: II—Magnetic Structure and Dynamics
Space Science Reviews, 2010 Observations and models of solar prominences are reviewed. We focus on non-eruptive prominences, and describe recent progress in four areas of prominence research: (1) magnetic structure deduced from observations and models, (2) the dynamics of ...
Guillaume Aulanier
exaly +4 more sources
Earth and Space Science, 2020 Solar prominences are structures of importance because of their role in polar field reversal. We study the long‐term variation of the time latitude distribution of solar prominences in this article.
Subhamoy Chatterjee +2 more
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Causal relationships between eruptive prominences and coronal mass ejections [PDF]
Annales Geophysicae, 2008 A close association between eruptive prominences and CMEs, both slow and fast CMEs, was reported in many studies. Sometimes it was possible to follow the material motion starting from the prominence (filament) activation to the CME in the high corona.
B. Filippov, S. Koutchmy
doaj +6 more sources
Solar prominences: theory and models
Living Reviews in Solar Physics, 2018 Magnetic fields suspend the relatively cool material of solar prominences in an otherwise hot corona. A comprehensive understanding of solar prominences ultimately requires complex and dynamic models, constrained and validated by observations spanning ...
Sarah E Gibson
exaly +3 more sources
Solar Prominences: Observations
Living Reviews in Solar Physics, 2014 Solar prominences are one of the most common features of the solar atmosphere. They are found in the corona but they are one hundred times cooler and denser than the coronal material, indicating that they are thermally and pressure isolated from the ...
Susanna Parenti
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PROMINE, 2017 Characteristics of sediment Tras Nagreg as part of the volcanic process in the region provides anopportunity and potential to be utilized through mining activities. Mining activities, as a capitalintensive,labor-intensive and risk-filled industry, do not always have a negative impact on thesurrounding community, there is something to do with the ...
Dono Guntoro +4 more
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Downward and Upward Propagating Magneto-Acoustic Waves Over a Solar Limb Prominence [PDF]
Iranian Journal of Astronomy and Astrophysics, 2023 Prominences are cold and dense chromospheric material suspended in the solar atmosphere with the support of coronal magnetic fields. Oscillatory behavior of a limb core prominence is studied in the AIA 171, 193, 211, 335, and 94 \AA\ passbands of AIA ...
Neda Dadashi, Maryam Ghiassi
doaj +1 more source
Prominence observations with ALMA
Frontiers in Astronomy and Space Sciences, 2022 This review comes at the time when ALMA successfully obtained the first regular observations of both a prominence and a filament. These observations have a spatial resolution of 1-2 arcsec, far better than previous prominence observations in the mm/sub ...
Petr Heinzel +5 more
doaj +1 more source
Spectral Evolution of an Eruptive Polar Crown Prominence With IRIS Observations
Frontiers in Physics, 2021 Prominence eruption is closely related to coronal mass ejections and is an important topic in solar physics. Spectroscopic observation is an effective way to explore the plasma properties, but the spectral observations of eruptive prominences are rare ...
Jianchao Xue +4 more
doaj +1 more source