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Sky-Tonight.com / Sun / Sunspots / Sunspot Region 4405
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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

Sunspot AR 4405

Sunspot AR 4405 is a moderate-sized, magnetically simple active region currently visible on the Sun’s surface. It contains 1 visible spot and spans an area of 100 millionths of the solar hemisphere. This region has produced 1 M-class flare, 1 X-class flare so far and currently shows a 0% probability of C-class, 0% of M-class, and 0% of X-class flares. It is located at heliographic latitude S28°, Earth-facing longitude -99°, and Carrington longitude 174°.

Sunspot Location on Map

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Selected map type: AIA 171 Å

Sunspot Properties

Region Number4405
First Observed2026-03-26 23:00
Sunspot TypeHsx
Magnetic ClassA
Area100 MSH
Number of Spots1
Extent17 heliographic degrees
Latitude-28°
Longitude-99°
Carrington Longitude174
Statusd

Flare Activity

Flare Class Begin Time (UTC) Peak Time (UTC) End Time (UTC) Location Duration
X1.42026-03-29 17:472026-03-29 18:192026-03-29 18:44S27E4532 minutes
M1.32026-03-27 17:162026-03-27 19:182026-03-27 20:35S24E70122 minutes

Sunspot Evolution

The following graphs show how this sunspot region 4405 has changed over time. The first graph displays its total area on the solar surface, while the second shows the number of individual sunspots observed within the region.

Sunspot Area

Area 0 364

This graph illustrates the physical growth of the sunspot region, measured in millionths of the solar hemisphere (MSH). Increases in area typically indicate developing magnetic complexity and potential for solar activity.

Spot Count

Sunspots 0 17

This graph shows the number of visible sunspots within the region at each observation time. A higher spot count often corresponds with a more active or complex region.

Detailed History

Date Area (MSH) Spot Count Classification Flares Location
2026-04-091001Hsx-S28W99
2026-04-081001Hsx-S28W85
2026-04-071203Cso-S28W72
2026-04-061204Eso-S28W60
2026-04-0515010Eao-S28W46
2026-04-0420010Fao-S28W33
2026-04-0318012Eao-S27W20
2026-04-0222015Eai-S27W07
2026-04-0121011Eac-S27E05
2026-03-3120011Esi-S27E18
2026-03-3017011EaoX1.4, 17:47-18:44S27E32
2026-03-291808Eao-S27E44
2026-03-283308EhiX1.4, 17:47-18:44S26E55
2026-03-272709Eho-S25E66

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.