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Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab
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Auroral flares and solar flares
Space Science Reviews, 1975The morphology of development of auroral flares (magnetospheric substorms) for both electron and proton auroras is summarized, based on ground-based as well as rocket-borne and satellite-borne data with specific reference to the morphology of solar flares.
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2012
Science fiction produced in the 1970s has long been undervalued, dismissed by Bruce Sterling as “confused, self-involved, and stale.” The New Wave was all but over and Cyberpunk had yet to arrive. The decade polarised sf – on the one hand it aspired to be a serious form, addressing issues such as race, Vietnam, feminism, ecology and sexuality, on the ...
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Science fiction produced in the 1970s has long been undervalued, dismissed by Bruce Sterling as “confused, self-involved, and stale.” The New Wave was all but over and Cyberpunk had yet to arrive. The decade polarised sf – on the one hand it aspired to be a serious form, addressing issues such as race, Vietnam, feminism, ecology and sexuality, on the ...
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2020
Abstract A solar flare is a transient increase in solar brightness powered by the release of magnetic energy stored in the Sun’s corona. Flares are observed in all wavelengths of the electromagnetic spectrum. The released magnetic energy heats coronal plasma to temperatures exceeding ten million Kelvins, leading to a significant ...
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Abstract A solar flare is a transient increase in solar brightness powered by the release of magnetic energy stored in the Sun’s corona. Flares are observed in all wavelengths of the electromagnetic spectrum. The released magnetic energy heats coronal plasma to temperatures exceeding ten million Kelvins, leading to a significant ...
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Is FLARE for Neutrino Solar Flare?
2005The Fermi Lab Liquid ARgon experiment, FLARE, a huge neutrino argon-liquid project detector of 50 kt mass, might in a near future enlarge the neutrino telescope accuracy revealing in detail solar, supernova, atmospheric as well as largest solar flares neutrino.
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1999
In this paper, the dynamics, the magnetohydrodynamics and the energetics of flaring magnetic loops are reviwed. It is also emphasized that the presented model is in no way a unique one. The most commonly occurring type is labelled as B type flares. This paper reviews the general features of a B type flare.
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In this paper, the dynamics, the magnetohydrodynamics and the energetics of flaring magnetic loops are reviwed. It is also emphasized that the presented model is in no way a unique one. The most commonly occurring type is labelled as B type flares. This paper reviews the general features of a B type flare.
openaire +1 more source