Viewing archive of Thursday, 12 July 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 Jul 12 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 194 Issued at 2200Z on 12 Jul 2012

IA. Analysis of Solar Active Regions and Activity from 11-2100Z to 12-2100Z

Solar activity was high. At 12/1649Z, a long-duration X1/2b flare was observed from Region 1520 (S16W09). The event was visible in GONG H-alpha imagery as a bright ribbon flare that erupted along the region?s long E/W oriented inversion line. Associated with this event were Type II (1268 km/s) and Type IV radio emissions along with an 800 sfu Tenflare. Limited satellite imagery indicated a CME was associated with this event. STEREO Behind COR2 imagery observed a CME lifting off the west limb, first visible at 12/1710Z. Further analysis of this CME is ongoing. During the past 24 hours, Region 1520 grew in both area and spot count and maintained a complex beta-gamma-delta magnetic configuration. Region 1521 (S21W21) also grew in area and spot count and remained a beta-gamma magnetic classification. New Regions 1522 (N13W21) and 1523 (S27E31) emerged on the disk as simple bi-polar spot groups.
IB. Solar Activity Forecast
Solar activity is expected to be moderate with a chance for X-class events for the next three days (13 - 15 July).
IIA. Geophysical Activity Summary 11-2100Z to 12-2100Z
The geomagnetic field was at quiet to active levels with isolated high latitude major storm intervals from 11/0600 - 1200Z. ACE solar data indicated wind velocities decreased steadily through the period from 500 km/s to near 400 km/s while the Bz component of the interplanetary magnetic field did not vary much beyond +/- 5 nT. The greater than 10 MeV proton flux at geosynchronous orbit exceeded the 10 pfu event threshold at 12/1835Z. At the time of this report, flux levels were at 35 pfu and rising. The greater than 100 MeV flux at geosynchronous orbit was enhanced, but below event threshold levels of 1 pfu. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels during the period.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at mostly quiet to unsettled levels for day one (13 July). Unsettled to active levels, with isolated minor storm intervals, are expected on days two and three (14 - 15 July) as effects from the 12 July CME are expected to become geoeffective.
III. Event Probabilities 13 Jul to 15 Jul
Class M80%80%80%
Class X35%35%35%
Proton99%99%50%
PCAFred
IV. Penticton 10.7 cm Flux
  Observed       12 Jul 165
  Predicted   13 Jul-15 Jul  165/165/165
  90 Day Mean        12 Jul 127
V. Geomagnetic A Indices
  Observed Afr/Ap 11 Jul  010/012
  Estimated     Afr/Ap 12 Jul  009/011
  Predicted    Afr/Ap 13 Jul-15 Jul  006/008-015/018-013/015
VI. Geomagnetic Activity Probabilities 13 Jul to 15 Jul
A. Middle Latitudes
Active20%40%35%
Minor storm05%15%10%
Major-severe storm01%01%01%
B. High Latitudes
Active20%10%15%
Minor storm25%30%30%
Major-severe storm25%55%45%

All times in UTC

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