Solar region summary

Below you'll find a daily report brought to you by the NOAA about the solar regions during the past day and the prediction for the coming days. This page is daily updated around midnight.

Solar region summary 2025 Mar 25 0030 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Solar Region Summary

SRS Number 84 Issued at 0030Z on 25 Mar 2025 This report is compiled from data received at SWO on 24 Mar
I. Regions with Sunspots
Locations Valid at 24/2400Z
NmbrLocationLoAreaZLLNNMag Type
4028S16W801440010Axx0204Alpha
4030S18W651290100Hsx0201Alpha
4035N15W220840010Bxo0906Beta
4036N07W651290260Dhi0909Beta-Gamma
4039N09E230410010Bxo0303Beta
4040S08E320320010Axx0102Alpha
IA. H-alpha plages without spots
Locations Valid at 24/2400Z Mar
NmbrLocationLo
4032N28W90154
4033N19W61125
4034S11W49113
4037N19W62126
4038S14E20044
4041N18E35029
4042S12E40024
II. Regions Due to Return 25 Mar to 27 Mar
NmbrLatLo
4012S14322
4024N05309

Active geomagnetic conditions

Observed Kp: 4
Threshold reached: 20:32 UTC

Current data suggests there is a moderate 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

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

Tórshavn
Kuopio
Bergen, Trondheim
Arkhangelsk, Vorkuta
Sundsvall, Umeå

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

Tampere
Petrozavodsk
The strength of the interplanetary magnetic field is moderate (10.15nT), the direction is slightly South (-6.66nT).

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Latest alerts

20:45 UTC - Geomagnetic activity

Active geomagnetic conditions (Kp4) Threshold Reached: 20:19 UTC

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13:00 UTC - Type II Radio Emission

Begin Time: 25/03/2025 12:36 UTC Estimated Velocity: 516km/sec.


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. 

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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