Viewing archive of Tuesday, 14 March 2023

Solar activity report

Report of Solar-Geophysical Activity 2023 Mar 14 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 73 Issued at 2200Z on 14 Mar 2023

IA. Analysis of Solar Active Regions and Activity from 13-2100Z to 14-2100Z

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C3 event observed at 14/0605Z from Region 3250 (S18W22). There are currently 8 numbered sunspot regions on the disk.
IB. Solar Activity Forecast
Solar activity is expected to be very low with a chance for a C-class flares on days one and two (15 Mar, 16 Mar) and likely to be low with a slight chance for an M-class flare on day three (17 Mar).
IIA. Geophysical Activity Summary 13-2100Z to 14-2100Z
The geomagnetic field has been at quiet to active levels for the past 24 hours. Solar wind speed reached a peak of 445 km/s at 14/0837Z. Total IMF reached 16 nT at 14/0431Z. The maximum southward component of Bz reached -10 nT at 14/0814Z. Protons greater than 10 MeV at geosynchronous orbit reached a peak level of 16 pfu at 14/2035Z. Electrons greater than 2 MeV at geosynchronous orbit reached a peak level of 504 pfu.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at quiet to minor storm levels on days one and two (15 Mar, 16 Mar) and quiet to unsettled levels on day three (17 Mar). Protons greater than 10 Mev are expected to cross threshold on day one (15 Mar) and have a chance of crossing threshold on day two (16 Mar).
III. Event Probabilities 15 Mar to 17 Mar
Class M05%05%10%
Class X01%01%01%
Proton99%25%01%
PCAFin progress
IV. Penticton 10.7 cm Flux
  Observed       14 Mar 139
  Predicted   15 Mar-17 Mar 140/142/150
  90 Day Mean        14 Mar 172

V. Geomagnetic A Indices
  Observed Afr/Ap 13 Mar  002/003
  Estimated     Afr/Ap 14 Mar  013/018
  Predicted    Afr/Ap 15 Mar-17 Mar  020/025-021/025-007/010

VI. Geomagnetic Activity Probabilities 15 Mar to 17 Mar
A. Middle Latitudes
Active35%35%20%
Minor storm30%30%05%
Major-severe storm10%15%01%
B. High Latitudes
Active05%05%15%
Minor storm20%20%25%
Major-severe storm70%70%25%

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

Nuuk
Sodankylä
Reykjavik
Tromsø
Kiruna
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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