Viewing archive of Sunday, 15 April 2001

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 2001 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 105 Issued at 2200Z on 15 Apr 2001

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

Solar activity was high. Region 9415 (S12W87) produced an X14/2b flare at 15/1350 UTC. This event had an associated Type II, with a speed of 1000 km/s, and Type IV radio sweeps. It was also accompanied by a tenflare of 48000 sfu. A 12 degree filament located at S23W02 disappeared between 14/2054 UTC and 15/1135 UTC.
IB. Solar Activity Forecast
Solar activity is expected to be low to moderate. Region 9415 is still capable of producing a major flare before it rotates over the western limb.
IIA. Geophysical Activity Summary 14-2100Z to 15-2100Z
The geomagnetic field was unsettled to active. The X-class event described in Part IA produced proton events at greater than 10 and 100 MeV flux at geosynchronous orbit which are still in progress. The greater than 100 MeV crossed event threshold at 15/1405 UTC, and so far have reached a peak flux of 146 pfu at 15/1525 UTC. The greater than 10 MeV crossed event threshold at 15/1410 UTC and has reached a peak flux of 951 pfu at 15/1920 UTC. A ground level event was measured on the Thule riometer at 15/1505 UTC, and a polar cap absorption (PCA) event began at 15/1950 UTC.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be quiet to active for April 16 and 17. Active to minor storm conditions are expected on April 18 as a result of the X14 mentioned in Part IA above. Effects from a high speed coronal stream may also be expected on April 18. The greater than 10 MeV proton event is expected to continue for most of the period, and the greater than 100 MeV proton event is expected to go below threshold by sometime on April 16.
III. Event Probabilities 16 Apr to 18 Apr
Class M80%70%60%
Class X25%10%10%
Proton90%10%10%
PCAFin progress
IV. Penticton 10.7 cm Flux
  Observed       15 Apr 134
  Predicted   16 Apr-18 Apr  145/150/160
  90 Day Mean        15 Apr 166
V. Geomagnetic A Indices
  Observed Afr/Ap 14 Apr  013/015
  Estimated     Afr/Ap 15 Apr  015/015
  Predicted    Afr/Ap 16 Apr-18 Apr  015/015-015/020-020/035
VI. Geomagnetic Activity Probabilities 16 Apr to 18 Apr
A. Middle Latitudes
Active25%25%50%
Minor storm05%05%10%
Major-severe storm01%01%05%
B. High Latitudes
Active30%35%60%
Minor storm10%10%15%
Major-severe storm05%05%10%

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!

100%
Support SpaceWeatherLive with our merchandise
Check out our merchandise

Latest alerts

Get instant alerts!

Space weather facts

Last X-flare2024/11/06X2.39
Last M-flare2024/11/11M1.3
Last geomagnetic storm2024/11/10Kp5+ (G1)
Spotless days
Last spotless day2022/06/08
Monthly mean Sunspot Number
October 2024166.4 +25
November 2024175.7 +9.3
Last 30 days166.1 +21.7

This day in history*

Solar flares
12012M8.59
22012M4.14
32005M3.59
42012M3.56
52003M2.36
DstG
11960-339G5
21998-131G2
31989-121G1
41999-106G2
51979-92G1
*since 1994

Social networks