Viewing archive of Wednesday, 10 February 2010

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 2010 Feb 10 2201 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 041 Issued at 2200Z on 10 Feb 2010

IA. Analysis of Solar Active Regions and Activity from 09-2100Z to 10-2100Z

Solar activity was low. Todays activity consisted of 3 C-class events, as well as numerous B-class events. Region 1045 (N22W39) produced the largest event of the day, a C3.7 flare at 10/1514Z, but is beginning to show signs of decay. Region 1046 (N24E28) and Region 1047 (S18E43) remain stable and quiet. There is a recurrent, southern hemisphere coronal hole near the center disk.
IB. Solar Activity Forecast
Solar activity is expected to be predominately low. However, there is a chance for an isolated M-class flare for the next 3 days (11-13 February).
IIA. Geophysical Activity Summary 09-2100Z to 10-2100Z
The geomagnetic field has been quiet.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be unsettled on day 1 (11 February). An increase to unsettled with a slight chance for active conditions is expected on day 2 (12 February), and unsettled conditions are expected on day 3 (13 February). The activity is forecast as a response to CME activity on 6 February.
III. Event Probabilities 11 Feb to 13 Feb
Class M30%20%20%
Class X05%05%05%
Proton01%01%01%
PCAFGreen
IV. Penticton 10.7 cm Flux
  Observed       10 Feb 091
  Predicted   11 Feb-13 Feb  090/090/092
  90 Day Mean        10 Feb 078
V. Geomagnetic A Indices
  Observed Afr/Ap 09 Feb  001/003
  Estimated     Afr/Ap 10 Feb  003/004
  Predicted    Afr/Ap 11 Feb-13 Feb  010/010-012/012-008/010
VI. Geomagnetic Activity Probabilities 11 Feb to 13 Feb
A. Middle Latitudes
Active30%35%30%
Minor storm05%10%05%
Major-severe storm01%05%01%
B. High Latitudes
Active35%40%35%
Minor storm10%15%10%
Major-severe storm01%05%01%

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

Oulu, Rovaniemi, Sodankylä, Utsjoki
Reykjavik
Kirkenes, Tromsø
Murmansk
Kiruna, Luleå

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

Tórshavn
Kuopio
Bergen, Trondheim
Arkhangelsk, Vorkuta
Sundsvall, Umeå

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

Tampere
The solar wind speed is currently moderately high (513 km/sec.)
The strength of the interplanetary magnetic field is high (20.09nT), the direction is slightly South (-9.06nT).

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