Data provided by National Oceanic and Atmospheric Administration
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.
About this Dataset
Updated: 2024-02-22
Metadata Last Updated:
2025-11-19T16:45:23.106Z
Date Created:
N/A
Data Provided by:
Dataset Owner:
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| Title | Sunspot Drawings Photosphere Observed from McMath-Hulbert Observatory |
|---|---|
| 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. |
| Modified | 2025-11-19T16:45:23.106Z |
| Publisher Name | N/A |
| Contact | N/A |
| Keywords | 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 , climatologyMeteorologyAtmosphere |
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