Results 161 to 170 of about 1,446 (180)
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Coronal Holes and the High-Speed Solar Wind
Space Science Reviews, 2002Coronal holes are the lowest density plasma components of the Sun's outer atmosphere, and are associated with rapidly expanding magnetic fields and the acceleration of the high-speed solar wind. Spectroscopic and polarimetric observations of the extended corona, coupled with interplanetary particle and radio sounding measurements going back several ...
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Coronal mass ejections: Relationship with solar flares and coronal holes
2002Abstract The Coronal Mass Ejections (CMEs) observed by the LASCO coronagraph and associated solar activity phenomena whose locations were identified by EIT and solar Hα flare observations during year 2000 indicate that about 40%, 26% and 30% of CMEs were observed when there were coronal holes (CHs) within 1–10, 11–20 and 21–40 degrees, respectively
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Population of Bright Plume Threads in Solar Polar Coronal Holes
Solar Physics, 2021Zhenghua Huang +2 more
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The Evolution of Coronal Holes over Three Solar Cycles Using the McIntosh Archive
Solar Physics, 2020Ian M Hewins +2 more
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Rotating solar coronal holes and periodic modulation of the upper atmosphere
Geophysical Research Letters, 2008Jiuhou Lei +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, 2011A H Gabriel, W H Matthaeus, G Poletto
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Interplanetary and solar surface properties of coronal holes observed during solar maximum
Journal of Geophysical Research, 2003J Woch, S K Solanki, R Von Steiger
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Polar coronal holes during the past solar cycle: Ulysses observations
Journal of Geophysical Research, 2011R Von Steiger, T H Zurbuchen
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Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976
Solar Physics, 1976J W Harvey, Sheeley N R, Harvey J W
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