Viewing archive of Sunday, 14 April 2002 - Sunspot regions

Sunspot regions

Courtesy of SDO, SOHO (NASA) and the [MDI, AIA, EVE, and/or HMI] consortium.
Sunspot number New regionsBackground fluxMaximum fluxCM
236 -211 1C3.43M2.0764

Sunspot regions

Region 9893

Number of
sunspots
Size Class Magn. Class Spot Location
17 -14 400 10 FKI N18W53

Solar flares on this day

M2.07 M1.38 C9.84 M1.03

Region 9896

Number of
sunspots
Size Class Magn. Class Spot Location
1 -4 100 20 HAX S10W33

Region 9899

Number of
sunspots
Size Class Magn. Class Spot Location
3 -6 160 -20 HAX N18W19

Region 9900

Number of
sunspots
Size Class Magn. Class Spot Location
10 -4 100 -40 CSO S29W68

Region 9901

Number of
sunspots
Size Class Magn. Class Spot Location
20 3 250 60 DAI N20W39

Region 9902

Number of
sunspots
Size Class Magn. Class Spot Location
7 -1 90 -30 EAO N13E03

Region 9904

Number of
sunspots
Size Class Magn. Class Spot Location
8 3 30 BXO S14W56

Region 9905

Number of
sunspots
Size Class Magn. Class Spot Location
6 -6 60 10 DAO S15W41

Region 9906

Number of
sunspots
Size Class Magn. Class Spot Location
38 18 470 280 DKC S15E13

Solar flares on this day

C5.56

Region 9907

Number of
sunspots
Size Class Magn. Class Spot Location
30 16 440 60 DAC S04E46

Solar flares on this day

C7.95 M1.24 C7.63 C6.3

Region 9908

Number of
sunspots
Size Class Magn. Class Spot Location
7 3 60 40 DSO N04W40

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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Latest alerts

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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Space weather facts

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 2025140.6 -14
Last 30 days138 -16.1

This day in history*

Solar flares
12024M4.4
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32001M3.57
42004M3.43
52008M2.47
DstG
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*since 1994

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