Sunspot Drawings Photosphere Observed from McMath-Hulbert Observatory
The photosphere of the Sun has a temperature of around 6, 000 degreesK and is the region in which sunspot activity is located. Sunspots appear dark against the surface of the sun due to the sunspots lower temperatures. Sunspots are solar active regions having stron magnectic fields and propensity for erupting in the form of solar flares. They typically form near the solar equator. This dataset shows drawings done at the McMath Observatory.
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Photosphere_Sunspot Drawings_McMathHulbert Directory
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Global Change Master Directory (GCMD) Keywords
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Complete Metadata
| @type | dcat:Dataset |
|---|---|
| accessLevel | non-public |
| contactPoint |
{
"fn": "DOC/NOAA/NESDIS/NCEI > National Centers for Environmental Information, NESDIS, NOAA, U.S. Department of Commerce",
"@type": "vcard:Contact",
"hasEmail": "mailto:solar.ngdc@noaa.gov"
}
|
| describedByType | application/octet-steam |
| description | The photosphere of the Sun has a temperature of around 6, 000 degreesK and is the region in which sunspot activity is located. Sunspots appear dark against the surface of the sun due to the sunspots lower temperatures. Sunspots are solar active regions having stron magnectic fields and propensity for erupting in the form of solar flares. They typically form near the solar equator. This dataset shows drawings done at the McMath Observatory. |
| distribution |
[
{
"@type": "dcat:Distribution",
"title": "Photosphere_Sunspot Drawings_McMathHulbert Directory",
"accessURL": "https://www.ngdc.noaa.gov/stp/space-weather/solar-data/solar-imagery/photosphere/sunspot-drawings/mcmath/",
"mediaType": "text/html",
"description": "All images and related documentation.",
"describedByType": "application/octet-stream"
},
{
"@type": "dcat:Distribution",
"title": "Global Change Master Directory (GCMD) Keywords",
"accessURL": "https://www.earthdata.nasa.gov/learn/find-data/idn/gcmd-keywords",
"mediaType": "text/html",
"description": "The information provided on this page seeks to define how the GCMD Keywords are structured, used and accessed. It also provides information on how users can participate in the further development of the keywords.",
"describedByType": "application/octet-stream"
}
]
|
| identifier | https://data.noaa.gov/waf/NOAA/NESDIS/NGDC/STP/Solar_Imagery/iso/xml/Photosphere_SunspotDrawings_McMathHulbert_stp.xml |
| issued | 1942-06-24T00:00:00.000+00:00 |
| keyword |
[
"Sun-Earth Interactions > Solar Activity > Solar Active Regions",
"Sun-Earth Interactions > Solar Activity > Solar Imagery",
"Sun-Earth Interactions > Solar Activity > Sunspots",
"Sun-Earth Interactions > Solar Activity > Corona",
"Sun-Earth Interactions > Solar Activity > Solar Synoptic Maps",
"Space > Solar Region > Photosphere",
"Solar Telescopes",
"Solar Observatory Stations",
"DOC/NOAA/NESDIS/NCEI > National Centers for Environmental Information, NESDIS, NOAA, U.S. Department of Commerce",
"DOC/NOAA/NESDIS/NGDC > National Geophysical Data Center, NESDIS, NOAA, U.S. Department of Commerce",
"NOAA > Space Weather Program",
"WDS > World Data Service for Geophysics, Boulder"
]
|
| language |
[]
|
| license | https://creativecommons.org/publicdomain/zero/1.0/ |
| modified | 1942-06-24T00:00:00.000+00:00 |
| publisher |
{
"name": "DOC/NOAA/NESDIS/NGDC > National Geophysical Data Center, NESDIS,
NOAA, U.S. Department of Commerce",
"@type": "org:Organization"
}
|
| rights | otherRestrictions |
| temporal | 1942-06-24T00:00:00+00:00/1960-12-31T00:00:00+00:00 |
| title | Sunspot Drawings Photosphere Observed from McMath-Hulbert Observatory |
