Coronal holes - Open Access .click

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Publications of the Astronomical Society of Australia, 1982
A coronal hole is a region of the solar corona characterised by diverging magnetic fields of single polarity and lower-than-average densities (and probably temperatures). It is now generally accepted that coronal holes are the source of high-speed streams in the solar wind (Munro and Withbroe 1972, Kopp and Holzer 1976, Steinolfson and Tandberg-Hanssen
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Waves in Polar Coronal Holes

2009
The fast solar wind originates from polar coronal holes. Recent observations from SoHO suggest that the solar wind is flowing from funnel-shaped magnetic fields anchored in the lanes of the magnetic network at the solar surface. Using the spectroscopic diagnostic capability of SUMER on SoHO and of EIS on HINODE, we study waves in polar coronal holes ...
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Activity Complexes and Coronal Holes on the Sun: Relationship Phenomenology

Astronomy Reports, 2023
Yazev S A, S A Yazev
exaly

Statistical Approach on Differential Emission Measure of Coronal Holes using the CATCH Catalog

Solar Physics, 2021
Stefan Hofmeister, Stephan G Heinemann, Astrid Veronig +2 more
exaly

The Evolution of Coronal Holes over Three Solar Cycles Using the McIntosh Archive

Solar Physics, 2020
Ian Hewins, Sarah Gibson, S W Mcintosh
exaly

Population of Bright Plume Threads in Solar Polar Coronal Holes

Solar Physics, 2021
Lidong Xia, Zhenghua Huang, Hui Fu
exaly

MHD Waves and Heating in Coronal Holes

Space Science Reviews, 2005
Leon Ofman
exaly

Evolution of Coronal Holes and Implications for High-Speed Solar Wind During the Minimum Between Cycles 23 and 24

Solar Physics, 2010
G De Toma
exaly