Viewing archive of Saturday, 22 February 2014

Solar activity report

Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Report of Solar-Geophysical Activity 2014 Feb 22 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 53 Issued at 2200Z on 22 Feb 2014

IA. Analysis of Solar Active Regions and Activity from 21-2100Z to 22-2100Z

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C7 event observed at 22/1550Z. There are currently 8 numbered sunspot regions on the disk.
IB. Solar Activity Forecast
Solar activity is expected to be low with a chance for M-class flares on days one, two, and three (23 Feb, 24 Feb, 25 Feb).
IIA. Geophysical Activity Summary 21-2100Z to 22-2100Z
The geomagnetic field has been at quiet to active levels for the past 24 hours. Solar wind speed, as measured by the ACE spacecraft, reached a peak speed of 504 km/s at 22/0120Z. Total IMF reached 6 nT at 21/2304Z. The maximum southward component of Bz reached -5 nT at 21/2319Z. Electrons greater than 2 MeV at geosynchronous orbit reached a peak level of 1760 pfu.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at quiet to active levels on day one (23 Feb) and quiet to unsettled levels on days two and three (24 Feb, 25 Feb). Protons greater than 10 MeV have a slight chance of crossing threshold on day one (23 Feb).
III. Event Probabilities 23 Feb to 25 Feb
Class M50%50%50%
Class X05%05%05%
Proton10%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       22 Feb 163
  Predicted   23 Feb-25 Feb 170/175/175
  90 Day Mean        22 Feb 155

V. Geomagnetic A Indices
  Observed Afr/Ap 21 Feb  009/010
  Estimated     Afr/Ap 22 Feb  014/019
  Predicted    Afr/Ap 23 Feb-25 Feb  016/020-009/010-009/008

VI. Geomagnetic Activity Probabilities 23 Feb to 25 Feb
A. Middle Latitudes
Active35%10%10%
Minor storm20%01%01%
Major-severe storm05%01%01%
B. High Latitudes
Active10%15%15%
Minor storm30%25%20%
Major-severe storm50%20%20%

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

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

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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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