Results 141 to 150 of about 2,729 (231)
On the Origins of Coronal Alfvénic Waves
The Astrophysical Journal LettersAlfvénic waves are considered a key contributor to the energy flux that powers the Sun’s corona, with theoretical models demonstrating their potential to explain coronal EUV and X-ray emission and the acceleration of the solar wind.
Richard J. Morton, Roberto Soler
doaj +1 more source
Superposed epoch analysis of high-speed-stream effects at geosynchronous orbit: Hot plasma, cold plasma, and the solar wind [PDF]
, 2008 Superposed epoch analyses of magnetospheric plasma analyzer (MPA) data from Los Alamos National Laboratory (LANL) satellites are performed to reveal the density, temperature and flow velocity behavior of the hot ion plasma (0.1–45 keV), the hot electron ...
Borovsky, Joseph E., Denton, Michael H.
core
Source Materials and Heating of Alfvénic Slow and Hot Solar Wind Revealed by Heavy Ions
The Astrophysical JournalThis work quantitatively studies the differences of heavy ions among non-Alfvénic slow wind (N-ASSW), classical fast wind (FSW), and Alfvénic slow and hot wind (ASSW and AHSW) by effect size and Kolmogorov–Smirnov statistic.
Shuyi Meng, Shuo Yao
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Differences between CME-driven storms and CIR-driven storms [PDF]
, 2006 Twenty one differences between CME-driven geomagnetic storms and CIR-driven geomagnetic storms are tabulated. (CME-driven includes driving by CME sheaths, by magnetic clouds, and by ejecta; CIR-driven includes driving by the associated recurring high ...
Borovsky, Joseph E., Denton, Michael H.
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Magnetohydrodynamic Waves in Solar Coronal Arcades
The Astrophysical Journal, 1996 R. Oliver, A. W. Hood, E. R. Priest
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The Astrophysical JournalDuring solar cycle minimum, polar coronal holes show a prominent radio brightening cap. The analysis of polar microwave enhanced radiation in polar coronal holes is helpful for understanding the magnetic field characteristics and the origin of the solar ...
Jing Huang +6 more
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Waves and Oscillations in Solar Coronal Loops
, 2010 Basic Sun characteristic, solar corona mainly. Introducing spacecrafts SoHO and TRACE as fundamental instruments of observing solar corona activities and close description this activities in therms of MHD theory. Recherche reflects the current trends in
BEDNÁŘ, Vít
core
Signatures of Nonlinear Waves in Coronal Plumes and Holes
, 1999 In recent Ultraviolet Coronagraph Spectrometer/Solar and Heliospheric Observatory (UVCS/SOHO) White Light Channel (WLC) observations we found quasi-periodic variations in the polarized brightness (pB) in the polar coronal holes at heliocentric distances ...
Ofman, Leon
core
Multiwavelength Multipoint Observations of the October 28, 2021 Type III Radio Burst. [PDF]
Sol PhysMartinez Oliveros JC +8 more
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The Sun as a driver of the inner heliosphere: Modern investigations of fundamental plasma processes. [PDF]
Nat CommunErvin T, Nakhleh AJ, Bharati Das S.
europepmc +1 more source