Viewing archive of Saturday, 17 September 2011

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 2011 Sep 17 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 260 Issued at 2200Z on 17 Sep 2011

IA. Analysis of Solar Active Regions and Activity from 16-2100Z to 17-2100Z

Solar activity was low during the past 24 hours. Regions 1289 (N22W67) and 1290 (S13W84) each produced C-class events, the largest a long duration C2 event from Region 1289 at 16/2351Z. An associated CME first became visible on LASCO C2 imagery at 16/2348Z and had an estimated plane-of-sky speed of 575 km/s. Further analysis will be conducted to determine geoeffectiveness.
IB. Solar Activity Forecast
Solar activity is expected to be low with a chance for isolated M-class flares for the next three days (18-20 September).
IIA. Geophysical Activity Summary 16-2100Z to 17-2100Z
The geomagnetic field was quiet until approximately 17/0400Z when effects from the 14 September CME arrived at Earth. A shock was observed at ACE at 17/0256Z which was followed by a sudden impulse of 21 nT observed by the Boulder magnetometer. Solar wind speeds increased from approximately 350 km/s to 450 km/s along with a noticeable increase in temperature and density. The interplanetary magnetic field Bt reached +14 nT and there were several extended periods of southward Bz with a maximum deviation of -12 nT. Conditions at Earth increased to active levels following shock arrival with an isolated minor storm period at 17/1800Z. Solar wind speeds peaked at 550 km/s around 17/1115Z but have since decreased to approximately 450 km/s. 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 quiet to unsettled with a slight chance for isolated active periods on day one (18 September) as effects from the 14 September CME subside. Mostly quiet conditions are expected for days two and three (19-20 September).
III. Event Probabilities 18 Sep to 20 Sep
Class M30%35%35%
Class X01%01%01%
Proton01%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       17 Sep 145
  Predicted   18 Sep-20 Sep  145/145/145
  90 Day Mean        17 Sep 102
V. Geomagnetic A Indices
  Observed Afr/Ap 16 Sep  002/002
  Estimated     Afr/Ap 17 Sep  023/032
  Predicted    Afr/Ap 18 Sep-20 Sep  010/010-005/005-005/005
VI. Geomagnetic Activity Probabilities 18 Sep to 20 Sep
A. Middle Latitudes
Active20%10%05%
Minor storm10%01%01%
Major-severe storm01%01%01%
B. High Latitudes
Active25%15%05%
Minor storm15%05%01%
Major-severe storm01%01%01%

All times in UTC

<< Go to daily overview page

Latest news

Support SpaceWeatherLive.com!

A lot of people come to SpaceWeatherLive to follow the Sun's activity or if there is aurora to be seen, but with more traffic comes higher server costs. Consider a donation if you enjoy SpaceWeatherLive so we can keep the website online!

SpaceWeatherLive Pro
Support SpaceWeatherLive with our merchandise
Check out our merchandise

Latest alerts

Get instant alerts!

Space weather facts

Last X-flare2024/12/08X2.2
Last M-flare2024/12/22M1.0
Last geomagnetic storm2024/12/17Kp5+ (G1)
Spotless days
Last spotless day2022/06/08
Monthly mean Sunspot Number
November 2024152.5 -13.9
December 2024103.3 -49.2
Last 30 days115.4 -40.8

This day in history*

Solar flares
11999M7.71
22013M4.82
32023M3.33
42013M2.8
51999M2.61
DstG
11982-101G3
22014-71G1
32001-59
41987-59
51989-58G1
*since 1994

Social networks