Viewing archive of Wednesday, 22 January 2003 - Sunspot regions

Sunspot regions

Courtesy of SDO, SOHO (NASA) and the [MDI, AIA, EVE, and/or HMI] consortium.
Sunspot number New regionsBackground fluxMaximum fluxCM
152 -150 -2B4.86M1.7621

Sunspot regions

Region 10254

Number of
sunspots
Size Class Magn. Class Spot Location
1 100 10 HSX S14W77

Region 10257

Number of
sunspots
Size Class Magn. Class Spot Location
2 -3 80 -30 DAO N16W88

Region 10258

Number of
sunspots
Size Class Magn. Class Spot Location
1 -1 50 -20 HSX N07W41

Region 10259

Number of
sunspots
Size Class Magn. Class Spot Location
4 -6 20 -30 CRO N10W28

Region 10260

Number of
sunspots
Size Class Magn. Class Spot Location
10 70 DAO N14W00

Region 10261

Number of
sunspots
Size Class Magn. Class Spot Location
3 -1 40 DAO N26W73

Region 10262

Number of
sunspots
Size Class Magn. Class Spot Location
1 10 AXX S05W73

Region 10263

Number of
sunspots
Size Class Magn. Class Spot Location
4 1 50 40 CAO S13W40

Region 10266

Number of
sunspots
Size Class Magn. Class Spot Location
9 7 100 70 DAO S23E43

Region 10267

Number of
sunspots
Size Class Magn. Class Spot Location
5 4 120 70 CAO S20E64

Region 10268

Number of
sunspots
Size Class Magn. Class Spot Location
3 70 CAO N12E23

Region 10269

Number of
sunspots
Size Class Magn. Class Spot Location
4 60 HAX S09E76

All times in UTC

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Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future

Gillam, MB, Yellowknife, NT
A transequatorial coronal hole was detected in an earth-facing position on Monday, 24 March 2025

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Monday, 24 March 2025
Coronal hole faces Earth

The anticipated strong G3 geomagnetic storm watch never materialized as the coronal mass ejection that was supposed to arrive early yesterday didn't arrive until today just past midnight UTC. The impact was very lackluster with the Bt (total strength of the IMF) increasing to a moderate 15nT at best and the solar wind speed reaching just 420km/s. A far cry from the anticipated 700 to 800km/s. That once again goes to show how hard it is to forecast space weather events and any resulting geomagnetic conditions. We remain under the influence of the CME and high latitude sky watchers should remain alert for some nice aurora displays but middle latitude sky watchers will probably have to wait for the next opportunity. 

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13:55 UTC - Coronal hole

A transequatorial coronal hole is facing Earth. Enhanced solar wind could arrive in ~3 days

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02:45 UTC - Geomagnetic activity

Active geomagnetic conditions (Kp4) Threshold Reached: 02:33 UTC

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Last X-flare2025/02/23X2.0
Last M-flare2025/03/21M1.2
Last geomagnetic storm2025/03/22Kp6- (G2)
Spotless days
Last spotless day2022/06/08
Monthly mean Sunspot Number
February 2025154.6 +17.6
March 2025138.3 -16.4
Last 30 days136.1 -18.1

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