Viewing archive of Thursday, 5 July 2018

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 2018 Jul 05 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 186 Issued at 2200Z on 05 Jul 2018

IA. Analysis of Solar Active Regions and Activity from 04-2100Z to 05-2100Z

Solar activity has been at very low levels for the past 24 hours. There are currently 0 numbered sunspot regions on the disk.
IB. Solar Activity Forecast
Solar activity is expected to be very low on days one, two, and three (06 Jul, 07 Jul, 08 Jul).
IIA. Geophysical Activity Summary 04-2100Z to 05-2100Z
The geomagnetic field has been at quiet to minor storm levels for the past 24 hours. Solar wind speed reached a peak of 465 km/s at 05/1945Z. Total IMF reached 12 nT at 05/1945Z. The maximum southward component of Bz reached -8 nT at 05/1111Z. Electrons greater than 2 MeV at geosynchronous orbit reached a peak level of 1221 pfu.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at quiet to active levels on day one (06 Jul) and quiet levels on days two and three (07 Jul, 08 Jul).
III. Event Probabilities 06 Jul to 08 Jul
Class M01%01%01%
Class X01%01%01%
Proton01%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       05 Jul 068
  Predicted   06 Jul-08 Jul 068/068/070
  90 Day Mean        05 Jul 071

V. Geomagnetic A Indices
  Observed Afr/Ap 04 Jul  004/004
  Estimated     Afr/Ap 05 Jul  012/016
  Predicted    Afr/Ap 06 Jul-08 Jul  011/005-005/005-006/005

VI. Geomagnetic Activity Probabilities 06 Jul to 08 Jul
A. Middle Latitudes
Active30%15%10%
Minor storm10%05%01%
Major-severe storm01%01%01%
B. High Latitudes
Active15%15%15%
Minor storm25%20%20%
Major-severe storm40%20%15%

All times in UTC

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

Sodankylä, Utsjoki
Reykjavik
Tromsø
Kiruna
A transequatorial coronal hole was detected in an earth-facing position on Monday, 24 March 2025

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Coronal hole faces Earth

The anticipated strong G3 geomagnetic storm watch never materialized as the coronal mass ejection that was supposed to arrive early yesterday didn't arrive until today just past midnight UTC. The impact was very lackluster with the Bt (total strength of the IMF) increasing to a moderate 15nT at best and the solar wind speed reaching just 420km/s. A far cry from the anticipated 700 to 800km/s. That once again goes to show how hard it is to forecast space weather events and any resulting geomagnetic conditions. We remain under the influence of the CME and high latitude sky watchers should remain alert for some nice aurora displays but middle latitude sky watchers will probably have to wait for the next opportunity. 

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