Viewing archive of Wednesday, 27 June 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 Jun 27 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 179 Issued at 2200Z on 27 Jun 2012

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

Solar activity was low. Regions 1512 (S15E11) and 1513 (S15E58) each produced low-level C-class flares as well as occasional optical subflares. Region 1512 showed spot and penumbral growth in its intermediate portion along with an increase in magnetic complexity and was classified as a Dki/beta-gamma. Region 1513 showed a minor increase in spot count during the period and was classified as a Cso/beta. New Regions 1514 (S16E55) and 1515 (S16E70) were numbered and were classified as a Bxo/beta and Cso/beta, respectively. Region 1515 produced occasional optical subflares during the latter half of the period. No Earth-directed coronal mass ejections were observed during the period.
IB. Solar Activity Forecast
Solar activity is expected to be low through the period (28 - 30 June) with a chance for an M-class flare.
IIA. Geophysical Activity Summary 26-2100Z to 27-2100Z
The geomagnetic field was quiet with unsettled to active periods detected at high latitudes.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be quiet on day 1 (28 June). Field activity is expected to increase to quiet to unsettled levels on day 2 (29 June) with a chance for active levels due to the arrival of a co-rotating interaction region in advance of a coronal hole high-speed stream (CH HSS). A further increase to unsettled to active levels is expected on day 3 (29 June) with a chance for minor storm levels due to CH HSS effects.
III. Event Probabilities 28 Jun to 30 Jun
Class M25%25%25%
Class X01%01%01%
Proton01%01%01%
PCAFGreen
IV. Penticton 10.7 cm Flux
  Observed       27 Jun 106
  Predicted   28 Jun-30 Jun  110/115/115
  90 Day Mean        27 Jun 118
V. Geomagnetic A Indices
  Observed Afr/Ap 26 Jun  007/009
  Estimated     Afr/Ap 27 Jun  004/005
  Predicted    Afr/Ap 28 Jun-30 Jun  006/007-009/010-015/018
VI. Geomagnetic Activity Probabilities 28 Jun to 30 Jun
A. Middle Latitudes
Active10%15%25%
Minor storm01%01%10%
Major-severe storm01%01%01%
B. High Latitudes
Active20%20%15%
Minor storm20%25%30%
Major-severe storm10%20%40%

All times in UTC

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Current data suggests there is a moderate possibility for aurora to appear at the following high latitude regions in the near future

Gillam, MB, Whitehorse, YT, Yellowknife, NT
Fairbanks, AK

Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future

Edmonton, AB, Iqaluit, NU, Saskatoon, SK
Anchorage, AK, Juneau, AK

Current data suggests there is a slight possibility for aurora to appear at the following middle latitude regions in the near future

Calgary, AB, Winnipeg, MB
The strength of the interplanetary magnetic field is moderate (10.08nT), the direction is slightly South (-5.69nT).
The Disturbance Storm Time index predicts moderate storm conditions right now (-51nT)

S1 - Minor solar radiation storm

Minor impacts on HF radio through polar regions

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