Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q6582994> ?p ?o }
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- Q6582994 subject Q7060964.
- Q6582994 subject Q8175306.
- Q6582994 subject Q8266666.
- Q6582994 abstract "Sunspots are temporary phenomena on the photosphere of the Sun that appear visibly as dark spots compared to surrounding regions. They correspond to concentrations of magnetic field flux that inhibit convection and result in reduced surface temperature compared to the surrounding photosphere. Sunspots usually appear in pairs, with pair members of opposite magnetic polarity. The number of sunspots varies according to the approximately 11-year solar cycle.Individual sunspots may endure anywhere from a few days to a few months, but eventually decay. Sunspots expand and contract as they move across the surface of the Sun with a size ranging from 16 kilometers (10 mi) to 160,000 kilometers (100,000 mi) in diameter. The larger variety are visible from Earth without the aid of a telescope. They may travel at relative speeds, or proper motions of a few hundred meters per second when they first emerge.Indicating intense magnetic activity, sunspots accompany secondary phenomena such as coronal loops (prominences) and reconnection events. Most solar flares and coronal mass ejections originate in magnetically active regions around visible sunspot groupings. Similar phenomena indirectly observed on stars other than the sun are commonly called starspots and both light and dark spots have been measured.".
- Q6582994 thumbnail Solar_eclipse_of_October_23_2014_start_of_partial.jpg?width=300.
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- Q6582994 wikiPageExternalLink Metadata.do?Portal=GCMD&KeywordPath=%5BParameters%3ACategory%3D%27EARTH+SCIENCE%27%2CTopic%3D%27SUN-EARTH+INTERACTIONS%27%2CTerm%3D%27SOLAR+ACTIVITY%27%2CVariable%3D%27SUNSPOTS%27%5D&OrigMetadataNode=GCMD&EntryId=NOAA_NCDC_PALEO_2005-015&MetadataView=Brief&MetadataType=0&lbnode=gcmd3b.
- Q6582994 wikiPageExternalLink solanki2004.
- Q6582994 wikiPageExternalLink www.spaceweather.com.
- Q6582994 wikiPageExternalLink photosphere.
- Q6582994 wikiPageExternalLink sunspot_swedish_c1.jpg.
- Q6582994 wikiPageExternalLink fenyi.solarobs.unideb.hu.
- Q6582994 wikiPageExternalLink index.php3.
- Q6582994 wikiPageExternalLink www.lmsal.com.
- Q6582994 wikiPageExternalLink Ham_Radio_Toolbar.htm.
- Q6582994 wikiPageExternalLink Propfire.htm.
- Q6582994 wikiPageExternalLink Astro-Solar-Sunspots.htm.
- Q6582994 wikiPageExternalLink SolarCycle.
- Q6582994 wikiPageExternalLink www.solarcycle24.com.
- Q6582994 wikiPageExternalLink www.suntrek.org.
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- Q6582994 type Thing.
- Q6582994 comment "Sunspots are temporary phenomena on the photosphere of the Sun that appear visibly as dark spots compared to surrounding regions. They correspond to concentrations of magnetic field flux that inhibit convection and result in reduced surface temperature compared to the surrounding photosphere. Sunspots usually appear in pairs, with pair members of opposite magnetic polarity.".
- Q6582994 label "Sunspot".
- Q6582994 depiction Solar_eclipse_of_October_23_2014_start_of_partial.jpg.