Results 131 to 140 of about 235 (149)
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Solar Physics, 1983
The spatial and temporal behavior of excess and depleted density regions of the coronal transient accompanying the west limb solar flare of 18:21 UT on June 29, 1980, is modeled mathematically on the basis of SMM-X-ray-polychrometer data, and the results are compared to observations made with the radio spectrograph at Harvard Radio Astronomy Station at
S. T. Wu +7 more
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The spatial and temporal behavior of excess and depleted density regions of the coronal transient accompanying the west limb solar flare of 18:21 UT on June 29, 1980, is modeled mathematically on the basis of SMM-X-ray-polychrometer data, and the results are compared to observations made with the radio spectrograph at Harvard Radio Astronomy Station at
S. T. Wu +7 more
openaire +1 more source
Search for transient coronal holes by SOLAR-A soft X-ray telescope
2005We propose to perform a systematic search for new coronal holes which are expected to be formed in association with solar-filament disappearances, because, some disappearing-filament associated solar wind shock waves are seemed to be driven by transient high-speed streams.
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2005
Numerical simulation is made of the transient heat conduction during local heating in a model coronal magnetic loop with an applied axial electric current.
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Numerical simulation is made of the transient heat conduction during local heating in a model coronal magnetic loop with an applied axial electric current.
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Interchange reconnection as the source of the fast solar wind within coronal holes
Nature, 2023Stuart D Bale +2 more
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2019
A subset at least of the slow solar wind is released in the form of transients ejected continually along streamer rays. The physical mechanisms responsible for these transient releases of dense material are not yet fully understood. We exploit a period when the NASA Solar-TErrestrial RElations Observatory-A (STEREO-A) was in orbital quadrature with ...
Rouillard, A. P. +25 more
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A subset at least of the slow solar wind is released in the form of transients ejected continually along streamer rays. The physical mechanisms responsible for these transient releases of dense material are not yet fully understood. We exploit a period when the NASA Solar-TErrestrial RElations Observatory-A (STEREO-A) was in orbital quadrature with ...
Rouillard, A. P. +25 more
openaire +1 more source
Picoflare jets power the solar wind emerging from a coronal hole on the Sun
Science, 2023Lakshmi Pradeep Chitta +2 more
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Exploiting Electrical Transients to Quantify Charge Loss in Solar Cells
Joule, 2020Dongmei Li, Qingbo Meng
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Highly structured slow solar wind emerging from an equatorial coronal hole
Nature, 2019Stuart D Bale +2 more
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Morphology, dynamics and plasma parameters of plumes and inter-plume regions in solar coronal holes
Astronomy and Astrophysics Review, 2011William H Matthaeus, Yi-ming Wang
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