Difference between revisions of "Solar cycle"
Jump to navigation
Jump to search
(Created page with "Variation of the solar activity between two extremes with a cycle time of approximately 11 years. The solar activity can be described by the number of observed sunspots. (IC...") |
|||
Line 1: | Line 1: | ||
Variation of the solar activity between two extremes with a cycle time of approximately 11 years. The solar activity can be described by the number of observed sunspots. ([[ICRP Publication 123]], 2013) | Variation of the solar activity between two extremes with a cycle time of approximately 11 years. The solar activity can be described by the number of observed sunspots. ([[ICRP Publication 123]], 2013) | ||
+ | ''ICRP Glossary entry - May 2019'' | ||
− | ''[[ICRP Glossary]] | + | |
+ | '''Return to [[ICRP Glossary|Glossary]]''' |
Latest revision as of 14:01, 13 September 2019
Variation of the solar activity between two extremes with a cycle time of approximately 11 years. The solar activity can be described by the number of observed sunspots. (ICRP Publication 123, 2013)
ICRP Glossary entry - May 2019
Return to Glossary