Viewing archive of Tuesday, 16 April 2024 - Sunspot regions

Sunspot regions

Courtesy of SDO, SOHO (NASA) and the [MDI, AIA, EVE, and/or HMI] consortium.
Sunspot number New regionsBackground fluxMaximum fluxCM
176 -171 -1C1.67M1.1441

Sunspot regions

Region 13628

Number of
sunspots
Size Class Magn. Class Spot Location
1 60 HSX N05W0*
HMIIF
HMIBC

Region 13633

Number of
sunspots
Size Class Magn. Class Spot Location
3 2 80 CSO S10W65
HMIIF
HMIBC

Region 13634

Number of
sunspots
Size Class Magn. Class Spot Location
9 -14 310 10 DHI N25W56
HMIIF
HMIBC

Region 13635

Number of
sunspots
Size Class Magn. Class Spot Location
3 10 AXX N22W28
HMIIF
HMIBC

Region 13636

Number of
sunspots
Size Class Magn. Class Spot Location
3 90 CSO S18E06
HMIIF
HMIBC

Region 13637

Number of
sunspots
Size Class Magn. Class Spot Location
2 20 10 DRO S12E25
HMIIF
HMIBC

Region 13638

Number of
sunspots
Size Class Magn. Class Spot Location
8 4 80 CAI S17E30
HMIIF
HMIBC

Region 13639

Number of
sunspots
Size Class Magn. Class Spot Location
19 5 310 70 EKI N30E34
HMIIF
HMIBC

Solar flares on this day

C2.7 C4.8 C5.3

Region 13641

Number of
sunspots
Size Class Magn. Class Spot Location
6 -13 110 20 DAO N11W15
HMIIF
HMIBC

Region 13642

Number of
sunspots
Size Class Magn. Class Spot Location
5 10 BXO N18W25
HMIIF
HMIBC

Region 13643

Number of
sunspots
Size Class Magn. Class Spot Location
6 -2 100 DAI S10E49
HMIIF
HMIBC

Solar flares on this day

C3.9

Region 13644

Number of
sunspots
Size Class Magn. Class Spot Location
2 80 DSO N12E72
HMIIF
HMIBC

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

Oulu, Rovaniemi, Sodankylä, Utsjoki
Reykjavik
Kirkenes, Tromsø
Murmansk
Kiruna, Luleå
A transequatorial coronal hole was detected in an earth-facing position on Monday, 24 March 2025

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Latest alerts

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. 

alert

Read more
13:55 UTC - Coronal hole

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

alert


02:45 UTC - Geomagnetic activity

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

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Saturday, 22 March 2025
23:45 UTC - Geomagnetic activity

Minor G1 geomagnetic storm (Kp5) Threshold Reached: 23:37 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 days138.7 -14.7

This day in history*

Solar flares
12000X2.61
22000M4.09
32000M3.71
42024M2.7
52001M2.43
DstG
11991-281G4
21969-228G4
32023-163G4
42024-128G4
52002-100G2
*since 1994

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