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Sky-Tonight.com / Sun / Sunspots / Sunspot region 4549
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This Earth map lets you select the observer’s location used to calculate the bearing and elevation of celestial objects. The selected point determines how the sky, rise and set times, and object positions are shown.
Your location: Santa Clara, United States
Timezone:
Latitude:
37.3541
Longitude:
-121.955

Sunspot region AR 4549

Sunspot AR 4549 is a moderate-sized, magnetically complex active region visible on the Sun. It contains 20 spots and covers 180 millionths of the solar hemisphere. This region has produced no significant flares. Current flare probabilities are C 75%, M 35% and X 5%. Its heliographic latitude is N10°, Earth-facing longitude -13° and Carrington longitude 215°.

Sunspot location on the solar map

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Selected map type: AIA 171 Å

Sunspot properties

Region number4549
First observed5 October 2026 at 01:48
Sunspot typeDai
Magnetic classBGD
Area180 MSH
Spot count20
Heliographic extent8 degrees
Latitude10°
Longitude-13°
Carrington longitude215
Statusf

Flare activity

No flares detected.
Flare classBegin time (UTC)Peak time (UTC)End time (UTC)LocationDuration

Sunspot evolution

These graphs show how the region’s area and visible spot count changed over time.

Area

Area 0 0

Area is measured in millionths of the solar hemisphere (MSH); growth can indicate increasing magnetic complexity.

Spot count

Sunspots 0 0

The spot count records the visible spots in the region at each observation.

Detailed history

DateArea (MSH)Spot countClassificationflaresLocation

Acknowledgments

We thank the teams behind the Solar Dynamics Observatory (SDO), including the HMI, AIA and EVE teams, for continuous solar monitoring.

We also thank National Aeronautics and Space Administration (NASA), Goddard Space Flight Center (GSFC), National Oceanic and Atmospheric Administration (NOAA) for supporting solar science and public data access.

Additional event data are provided by NASA’s DONKI (Database of Notifications, Knowledge, Information), with records of flares, CMEs and geomagnetic storms.