Viewing archive of Wednesday, 26 August 2020

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2020 Aug 26 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 26 Aug 2020 until 28 Aug 2020
Solar flares

Quiet conditions (<50% probability of C-class flares)

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
26 Aug 2020071013
27 Aug 2020071012
28 Aug 2020071013

Bulletin

Solar X-ray flux has been below background (B) level throughout the period. There are no spotted regions on disc and X-ray flux is expected to remain at or below background (B) values.

There were no Earth directed coronal mass ejections observed in coronagraph data.

The greater than 10 MeV proton flux was at background levels over the past 24 hours. It is expected to stay at background levels for the next 24 hours. The greater than 2 MeV electron flux was at nominal levels over the past 24 hours and is expected to remain so over the next 24 hours.

Another coronal hole of positive polarity seems to be forming around disc centre and adds to the likelihood of Solar wind perturbations later in the week.

Solar wind conditions showed the expected enhancements. Solar wind speed rose from under 350 km/s to currently just under 450 km/s. The magnetic field phi angle switched into the away sector early in the period. The total magnetic field reached a peak of 8.5 nT this morning and remains at levels around 6nT, while Bz was overall variable. As other coronal holes are lining up, these moderate Solar wind enhancements are expected to last on and off over the next days.

Quiet to unsettled geomagnetic conditions have been recorded (NOAA Kp 1-2 while local K Dourbes reaching 3 just recently). Geomagnetic conditions are expected to be mostly quiet to unsettled, with some isolated active periods not excluded depending on the evolution of the Solar wind enhancements.

Today's estimated international sunspot number (ISN): 000, based on 14 stations.

Solar indices for 25 Aug 2020

Wolf number Catania///
10cm solar flux071
AK Chambon La Forêt009
AK Wingst004
Estimated Ap003
Estimated international sunspot number000 - Based on 23 stations

Noticeable events summary

DayBeginMaxEndLocStrengthOP10cmCatania/NOAARadio burst types
None

Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive

All times in UTC

<< Go to daily overview page

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

Fairbanks, AK
The direction of the interplanetary magnetic field is slightly South (-6.55nT).

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!

Donate SpaceWeatherLive Pro
Support SpaceWeatherLive with our merchandise
Check out our merchandise

Latest alerts

Wednesday, 2 April 2025
04:03 UTC - Hemispheric Power Index

The OVATION model predicts the Hemispheric Power Index to reach 50GW at 04:56 UTC


01:45 UTC - Geomagnetic activity

Active geomagnetic conditions (Kp4) Threshold Reached: 01:32 UTC

alert


Tuesday, 1 April 2025
22:51 UTC - Solar flare

Moderate M2.5 flare

alert


22:30 UTC - Radio Blackout

Minor R1 radio blackout in progress (≥M1 - current: M1.45)


Get instant alerts!

Space weather facts

Last X-flare2025/03/28X1.1
Last M-flare2025/04/01M2.5
Last geomagnetic storm2025/03/27Kp5 (G1)
Spotless days
Last spotless day2022/06/08
Monthly mean Sunspot Number
February 2025154.6 +17.6
April 2025152.5 -2.1
Last 30 days130.7 -17.9

This day in history*

Solar flares
12001X1.77
22017M8.35
31999M6.2
42001M3.57
52017M1.81
DstG
11979-168G4
21960-151G3
31992-105G2
42004-104G2
51994-103G3
*since 1994

Social networks