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.
About this Dataset
| Title | Sunspot Drawings Photosphere Observed from Kalocsa Solar 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. |
| Modified | 2025-11-19T16:45:22.869Z |
| 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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