Viewing archive of Sunday, 15 April 2012

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 2012 Apr 15 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 106 Issued at 2200Z on 15 Apr 2012

IA. Analysis of Solar Active Regions and Activity from 14-2100Z to 15-2100Z

Solar activity increased to low levels. Two low-level C-class flares occurred from a source beyond the northeast limb. Region 1459 (S16E64) produced occasional B-class flares while it rotated more fully into view as a Dai-type group with a beta magnetic classification. Region 1455 (N05W46) showed intermediate spot development during the period and was classified as a Dsi-type with a beta magnetic classification. Small Axx-type Region 1454 (S12W00) produced a B9 x-ray flare at 15/0908Z associated with a slow partial-halo CME, which is not expected to be geoeffective. No new regions were numbered.
IB. Solar Activity Forecast
Solar activity is expected to be low through the period (16 - 18 April).
IIA. Geophysical Activity Summary 14-2100Z to 15-2100Z
Geomagnetic field activity decreased to mostly quiet levels. The greater than 2 MeV electron flux at geosynchronous orbit was at high levels throughout the period.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at quiet levels during the period (16 - 18 April).
III. Event Probabilities 16 Apr to 18 Apr
Class M10%10%10%
Class X01%01%01%
Proton01%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       15 Apr 102
  Predicted   16 Apr-18 Apr  100/100/100
  90 Day Mean        15 Apr 113
V. Geomagnetic A Indices
  Observed Afr/Ap 14 Apr  007/011
  Estimated     Afr/Ap 15 Apr  006/005
  Predicted    Afr/Ap 16 Apr-18 Apr  004/005-004/005-004/005
VI. Geomagnetic Activity Probabilities 16 Apr to 18 Apr
A. Middle Latitudes
Active10%10%10%
Minor storm01%01%01%
Major-severe storm01%01%01%
B. High Latitudes
Active15%15%15%
Minor storm01%01%01%
Major-severe storm01%01%01%

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

Oulu, Rovaniemi, Sodankylä, Utsjoki
Kirkenes, Tromsø, Trondheim
Arkhangelsk, Murmansk, Vorkuta
Kiruna, Luleå
A transequatorial coronal hole was detected in an earth-facing position on Monday, 24 March 2025

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