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Solar activity report

Report of Solar-Geophysical Activity 2025 May 31 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 151 Issued at 2200Z on 31 May 2025

IA. Analysis of Solar Active Regions and Activity from 30-2100Z to 31-2100Z

Solar activity has been at high levels for the past 24 hours. There are currently 5 numbered sunspot regions on the disk.
IB. Solar Activity Forecast
Solar activity is likely to be moderate with a chance for X-class flares on days one, two, and three (01 Jun, 02 Jun, 03 Jun).
IIA. Geophysical Activity Summary 30-2100Z to 31-2100Z
The geomagnetic field has been at quiet to active levels for the past 24 hours. Solar wind speed reached a peak of 822 km/s at 31/0518Z. Total IMF reached 7 nT at 31/0045Z. The maximum southward component of Bz reached -6 nT at 30/2248Z. Protons greater than 10 MeV at geosynchronous orbit reached a peak level of 25 pfu at 31/2045Z. Electrons greater than 2 MeV at geosynchronous orbit reached a peak level of 9162 pfu.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at active to severe storm levels on day one (01 Jun), minor storm to severe storm levels on day two (02 Jun) and active to major storm levels on day three (03 Jun). Protons are expected to cross threshold on days one, two, and three (01 Jun, 02 Jun, 03 Jun).
III. Event Probabilities 01 Jun to 03 Jun
Class M65%65%65%
Class X25%25%25%
Proton75%75%75%
PCAFyellow
IV. Penticton 10.7 cm Flux
  Observed       31 May 164
  Predicted   01 Jun-03 Jun 165/160/150
  90 Day Mean        31 May 154

V. Geomagnetic A Indices
  Observed Afr/Ap 30 May  018/016
  Estimated     Afr/Ap 31 May  014/018
  Predicted    Afr/Ap 01 Jun-03 Jun  052/096-055/100-031/044

VI. Geomagnetic Activity Probabilities 01 Jun to 03 Jun
A. Middle Latitudes
Active05%15%30%
Minor storm40%35%35%
Major-severe storm55%55%25%
B. High Latitudes
Active01%01%05%
Minor storm05%05%15%
Major-severe storm95%95%80%

All times in UTC

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