Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q127948> ?p ?o }
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- Q127948 subject Q7217154.
- Q127948 subject Q8266666.
- Q127948 abstract "Coronal holes are part of the Sun's corona and are constantly changing and reshaping because the corona is not uniform. Coronal holes are areas where the Sun's corona is darker, and colder, and has lower-density plasma than average because there is lower energy and gas levels. The sun contains magnetic fields that arch away from areas in the corona that are very thin due to the lower levels of energy and gas, which cause coronal holes to appear when they do not fall back. Thus, solar particles or solar wind escape and create a lower density and lower temperature in that area. The aurora borealis that is seen at the northern and southern poles are the result of solar wind entering the Earth’s atmosphere.".
- Q127948 thumbnail Coronal_Hole_Magnetic_Field_Lines.svg?width=300.
- Q127948 wikiPageWikiLink Q10251.
- Q127948 wikiPageWikiLink Q11408.
- Q127948 wikiPageWikiLink Q1369318.
- Q127948 wikiPageWikiLink Q1445154.
- Q127948 wikiPageWikiLink Q170754.
- Q127948 wikiPageWikiLink Q190776.
- Q127948 wikiPageWikiLink Q2314257.
- Q127948 wikiPageWikiLink Q34777.
- Q127948 wikiPageWikiLink Q49385.
- Q127948 wikiPageWikiLink Q544.
- Q127948 wikiPageWikiLink Q7217154.
- Q127948 wikiPageWikiLink Q79833.
- Q127948 wikiPageWikiLink Q8266666.
- Q127948 wikiPageWikiLink Q912887.
- Q127948 comment "Coronal holes are part of the Sun's corona and are constantly changing and reshaping because the corona is not uniform. Coronal holes are areas where the Sun's corona is darker, and colder, and has lower-density plasma than average because there is lower energy and gas levels. The sun contains magnetic fields that arch away from areas in the corona that are very thin due to the lower levels of energy and gas, which cause coronal holes to appear when they do not fall back.".
- Q127948 label "Coronal hole".
- Q127948 depiction Coronal_Hole_Magnetic_Field_Lines.svg.