Viewing archive of Friday, 2 October 2020

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2020 Oct 02 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 02 Oct 2020 until 04 Oct 2020
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
02 Oct 2020073006
03 Oct 2020072004
04 Oct 2020072004

Bulletin

The solar activity was at very low levels with no significant flares recorded. The solar disk remains spotless and no significant flares are expected over the next 24 hours.

No Earth-directed Coronal Mass Ejections (CMEs) were observed in the available coronagraph imagery.

The greater than 10 MeV proton flux was at nominal levels in the past 24 hours, and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux was continuously recorded above the 10^3 pfu threshold over the past 24 hours, remaining greater than 10^4 pfu. The electron flux is expected to remain elevated over the next 24 hours.

Over the past 24 hours the solar wind conditions remained under the waning influence of the high-speed stream related to the positive-polarity coronal hole (CH82). The total interplanetary magnetic field, as recorded by ACE and DSCOVR, varied between 2 nT and 4 nT with a weak north-south component fluctuating in the range of -3 nT and 3 nT. In the past 24 hours the solar wind speed continued to decline varying between 580 km/s and 490 km/s. The solar wind conditions are expected to continue returning to background levels over the next 24 hours.

The geomagnetic conditions over the past 24 hours were mostly quiet to unsettled with maximum recorded Kp and K Dourbes indices equal to 3. Quiet to unsettled conditions are expected to continue over the next 24 hours. A new small-area negative-polarity coronal hole (CH83) has now formed on the western hemisphere close to the central meridian. As a result we might observe unsettled to active conditions after 2.5-3 days.

Today's estimated international sunspot number (ISN): 000, based on 11 stations.

Solar indices for 01 Oct 2020

Wolf number Catania000
10cm solar flux073
AK Chambon La Forêt021
AK Wingst012
Estimated Ap012
Estimated international sunspot number000 - Based on 26 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

Whitehorse, YT
Fairbanks, AK

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

Thursday, 10 April 2025
23:00 UTC - Geomagnetic activity

Active geomagnetic conditions (Kp4) Threshold Reached: 22:47 UTC

alert


20:45 UTC - Hemispheric Power Index

The OVATION model predicts the Hemispheric Power Index to reach 50GW at 21:37 UTC


01:45 UTC - Geomagnetic activity

Active geomagnetic conditions (Kp4) Threshold Reached: 01:41 UTC

alert


Get instant alerts!

Space weather facts

Last X-flare2025/03/28X1.1
Last M-flare2025/04/08M1.5
Last geomagnetic storm2025/04/06Kp5 (G1)
Spotless days
Last spotless day2022/06/08
Monthly mean Sunspot Number
March 2025134.2 -20.4
April 2025141.4 +7.2
Last 30 days137.9 +0.4

This day in history*

Solar flares
12013M9.34
22024M5.47
32001M3.41
42000M1.63
52000M1.5
DstG
12001-271G4
21990-190G3
31978-114G4
41982-110G2
51959-88G1
*since 1994

Social networks