Galactic cosmic radiation - Revision history

Charlotte White at 14:27, 7 September 2021

2021-09-07T14:27:06Z

Karen Clement at 20:14, 12 September 2019

2019-09-12T20:14:42Z

Intern: Created page with "Charged particle radiation that enters the heliosphere continuously from outer space from all directions. The radiation contains electrons (approximately 2%) and a broad range..."

2019-06-04T19:02:33Z

Created page with "Charged particle radiation that enters the heliosphere continuously from outer space from all directions. The radiation contains electrons (approximately 2%) and a broad range..."

New page

Charged particle radiation that enters the heliosphere continuously from outer space from all directions. The radiation contains electrons (approximately 2%) and a broad range of charged particles from protons up to high Z particles with energies up to several hundreds of GeV and even higher. The fluence rate of GCR in the heliosphere is inversely correlated with the solar activity. It is caused by the solar magnetic field, which is coupled to the solar wind. ([[ICRP Publication 123]], 2013)

''[[ICRP Glossary]] entry - June 2019''

← Older revision		Revision as of 14:27, 7 September 2021
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−	Charged particle radiation that enters the heliosphere continuously from outer space from all directions. The radiation contains electrons (approximately 2%) and a broad range of charged particles from protons up to high Z particles with energies up to several hundreds of GeV and even higher. The fluence rate of GCR in the heliosphere is inversely correlated with the solar activity. It is caused by the solar magnetic field, which is coupled to the solar wind. ~~([[ICRP Publication 123]], 2013)~~	+	Charged particle radiation that enters the heliosphere continuously from outer space from all directions. The radiation contains electrons (approximately 2%) and a broad range of charged particles from protons up to high Z particles with energies up to several hundreds of GeV and even higher. The fluence rate of GCR in the heliosphere is inversely correlated with the solar activity. It is caused by the solar magnetic field, which is coupled to the solar wind.
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−	~~''ICRP Glossary entry - June 2019''~~

		+	(Adapted from [[ICRP Publication 123]], 2013)

	'''Return to [[ICRP Glossary\|Glossary]]'''		'''Return to [[ICRP Glossary\|Glossary]]'''

← Older revision		Revision as of 20:14, 12 September 2019
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	Charged particle radiation that enters the heliosphere continuously from outer space from all directions. The radiation contains electrons (approximately 2%) and a broad range of charged particles from protons up to high Z particles with energies up to several hundreds of GeV and even higher. The fluence rate of GCR in the heliosphere is inversely correlated with the solar activity. It is caused by the solar magnetic field, which is coupled to the solar wind. ([[ICRP Publication 123]], 2013)		Charged particle radiation that enters the heliosphere continuously from outer space from all directions. The radiation contains electrons (approximately 2%) and a broad range of charged particles from protons up to high Z particles with energies up to several hundreds of GeV and even higher. The fluence rate of GCR in the heliosphere is inversely correlated with the solar activity. It is caused by the solar magnetic field, which is coupled to the solar wind. ([[ICRP Publication 123]], 2013)

		+	''ICRP Glossary entry - June 2019''

−	''[[ICRP Glossary]] ~~entry - June 2019~~''	+
		+	'''Return to [[ICRP Glossary\|Glossary]]'''