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Observation Settings

Or select it on the map:
This Earth map fragment is intended to illustrate celestial motion across the sky, emphasizing both bearing and elevational perspectives. The map's center point corresponds to the transit, showcasing celestial objects at their highest point, while elevation gradually decreases towards the map edges. This dynamic representation offers insights into the changing positions of celestial bodies with a focus on their bearing and elevational trajectories.
Your location: Santa Clara, United States
Timezone:
Latitude:
37.3541
Longitude:
-121.955

Active Sunspots

Below is a list of all sunspot regions currently visible on the solar disk. Each sunspot is an area of intense magnetic activity, often associated with solar flares and coronal mass ejections.

Every entry includes the NOAA active region number, magnetic classification, estimated area in millionths of the solar hemisphere (MSH), number of distinct spots, and flare probabilities. The list is continuously updated with the latest data from solar observatories.

4492

Sunspot Region

Spot count:
3
Area:
230
Coordinates:
N15E73
Class:
Hax
Magnetic Class:
A
AR 4492 is an Hax-class sunspot group that emerged on 2026-07-18 22:12. It covers 230 millionths of the solar disk and contains 3 individual spots.
View detailed sunspot info

4489

Sunspot Region

Spot count:
10
Area:
170
Coordinates:
S07W12
Class:
Cso
Magnetic Class:
BG
AR 4489 is an Cso-class sunspot group that emerged on 2026-07-12 22:18. It covers 170 millionths of the solar disk and contains 10 individual spots.
View detailed sunspot info

4491

Sunspot Region

Spot count:
1
Area:
10
Coordinates:
S11E21
Class:
Axx
Magnetic Class:
A
AR 4491 is an Axx-class sunspot group that emerged on 2026-07-15 18:45. It covers 10 millionths of the solar disk and contains 1 spot.
View detailed sunspot info

Acknowledgements

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

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

Additional event data is provided by NASA’s DONKI (Database of Notifications, Knowledge, Information), which offers alerts and detailed records of solar flares, CMEs, and geomagnetic storms.