Viewing archive of Thursday, 13 October 2011

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 2011 Oct 13 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 286 Issued at 2200Z on 13 Oct 2011

IA. Analysis of Solar Active Regions and Activity from 12-2100Z to 13-2100Z

Solar activity was low. A new spot group emerged and was numbered Region 1320 (S22W39). There are currently ten numbered regions, several producing C-class events.
IB. Solar Activity Forecast
Solar activity is expected to be low with a chance for an M-class event over the next 3 days (14-16 October).
IIA. Geophysical Activity Summary 12-2100Z to 13-2100Z
The geomagnetic field was quiet.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be mostly quiet on day 1 (14 October). Conditions are forecast to increase to quiet to unsettled conditions with the chance for active periods on days 2 and 3 (15-16 October) from anticipated CH HSS effects.
III. Event Probabilities 14 Oct to 16 Oct
Class M30%30%30%
Class X01%01%01%
Proton01%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       13 Oct 138
  Predicted   14 Oct-16 Oct  135/135/135
  90 Day Mean        13 Oct 116
V. Geomagnetic A Indices
  Observed Afr/Ap 12 Oct  004/006
  Estimated     Afr/Ap 13 Oct  005/005
  Predicted    Afr/Ap 14 Oct-16 Oct  005/005-008/008-008/008
VI. Geomagnetic Activity Probabilities 14 Oct to 16 Oct
A. Middle Latitudes
Active10%30%30%
Minor storm01%10%10%
Major-severe storm01%01%01%
B. High Latitudes
Active10%40%40%
Minor storm01%20%20%
Major-severe storm01%05%05%

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

Iqaluit, NU
Nuuk
Reykjavik
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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13:55 UTC - Coronal hole

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

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02:45 UTC - Geomagnetic activity

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

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