Solar phenomena
id:
solar-phenomena-175-3603288
title:
Solar phenomena
text:
Solar phenomena are natural phenomena which occur within the atmosphere of the Sun. They take many forms, including solar wind, radio wave flux, solar flares, coronal mass ejections, coronal heating and sunspots. These phenomena are believed to be generated by a helical dynamo, located near the center of the Sun's mass, which generates strong magnetic fields, as well as a chaotic dynamo, located near the surface, which generates smaller magnetic field fluctuations. All solar fluctuations togethe
brand slug:
wiki
category slug:
encyclopedia
description:
Natural phenomena within the Sun's atmosphere
original url:
https://en.wikipedia.org/wiki/Solar_phenomena
date created:
2003-04-06T20:40:10Z
date modified:
2024-09-03T06:59:11Z
main entity:
{"identifier":"Q7297568","url":"https://www.wikidata.org/entity/Q7297568"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/7/74/Activity_Continues_On_the_Sun.jpg","width":1280,"height":960}
fields total:
13
integrity:
16