Viewing archive of Monday, 27 October 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 Oct 27 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 300 Issued at 2200Z on 27 Oct 2014

IA. Analysis of Solar Active Regions and Activity from 26-2100Z to 27-2100Z

Solar activity has been at high levels for the past 24 hours. The largest solar event of the period was a X2 event observed at 27/1447Z from Region 2192 (S12W59). There are currently 5 numbered sunspot regions on the disk.
IB. Solar Activity Forecast
Solar activity is likely to be high on days one, two, and three (28 Oct, 29 Oct, 30 Oct).
IIA. Geophysical Activity Summary 26-2100Z to 27-2100Z
The geomagnetic field has been at quiet to unsettled levels for the past 24 hours. Solar wind speed, as measured by the ACE spacecraft, reached a peak speed of 476 km/s at 27/0417Z. Total IMF reached 8 nT at 27/1649Z. The maximum southward component of Bz reached -7 nT at 27/1735Z. Electrons greater than 2 MeV at geosynchronous orbit reached a peak level of 758 pfu.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at quiet to unsettled levels on days one, two, and three (28 Oct, 29 Oct, 30 Oct). Protons have a chance of crossing threshold on days one, two, and three (28 Oct, 29 Oct, 30 Oct).
III. Event Probabilities 28 Oct to 30 Oct
Class M85%85%85%
Class X55%55%55%
Proton45%45%45%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       27 Oct 188
  Predicted   28 Oct-30 Oct 165/150/140
  90 Day Mean        27 Oct 142

V. Geomagnetic A Indices
  Observed Afr/Ap 26 Oct  011/010
  Estimated     Afr/Ap 27 Oct  011/012
  Predicted    Afr/Ap 28 Oct-30 Oct  008/012-008/010-007/010

VI. Geomagnetic Activity Probabilities 28 Oct to 30 Oct
A. Middle Latitudes
Active20%15%10%
Minor storm05%05%01%
Major-severe storm01%01%01%
B. High Latitudes
Active20%15%15%
Minor storm30%25%25%
Major-severe storm25%25%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

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

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