Viewing archive of Friday, 29 May 2020

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2020 May 29 1234 UTC

SIDC Forecast

Valid from 1230 UTC, 29 May 2020 until 31 May 2020
Solar flares

C-class flares expected, (probability >=50%)

Geomagnetism

Active conditions expected (A>=20 or K=4)

Solar protons

Quiet

10cm fluxAp
29 May 2020069011
30 May 2020070018
31 May 2020070010

Bulletin

The active region that is still in the process of rotating to the visible side of the Sun was source of several B-class flares during last 30 hours. The same region was this morning also the source of C 9.3 GOES flare (peaked at 10:46 UT) and M 1.1 flare (peak at 07:24 UT). We can expect more C-class flares and possibly also isolated M-class flares in the coming hours. The coronagraph observation of the CMEs possibly associated with the C-class and M-class flares are not yet available. However, as the source region is still partially on the back side of the Sun, the possibly associated CMEs will not be Earth directed. During last 24 hours proton flux levels were at background values and are expected to remain so.

The Earth is still inside the slow solar wind with the speed of about 290 km/s. The interplanetary magnetic field magnitude is rather stable and it amounts about 4 nT. The solar wind originating from the extension of the southern polar coronal hole that crossed central meridian on May 25 might be expected later today or tomorrow morning. It might be closely followed by the solar wind originating from the small and patchy equatorial coronal hole (negative polarity) that reached central meridian on the midday of May 27. On May 30 we can also expect the arrival of the CME-driven shock wave associated with rather faint CME (observed above the west solar limb early on May 26). The geomagnetic conditions are quiet and we expect quiet to possibly active geomagnetic conditions in the next 24 hours.

Today's estimated international sunspot number (ISN): 000, based on 31 stations.

Solar indices for 28 May 2020

Wolf number Catania///
10cm solar flux068
AK Chambon La Forêt007
AK Wingst004
Estimated Ap003
Estimated international sunspot number000 - Based on 38 stations

Noticeable events summary

DayBeginMaxEndLocStrengthOP10cmCatania/NOAARadio burst types
29071307240728----M1.1--/----III/2

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

All times in UTC

<< Go to daily overview page

Active geomagnetic conditions

Observed Kp: 4
Threshold reached: 23:02 UTC

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

Reykjavik

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

Monday, 14 April 2025
23:15 UTC - Geomagnetic activity

Active geomagnetic conditions (Kp4) Threshold Reached: 23:01 UTC

alert


07:09 UTC - Solar flare

Moderate M4.28 flare from sunspot region 4055

alert


06:48 UTC - Radio Blackout

Minor R1 radio blackout in progress (≥M1 - current: M1.53)


06:24 UTC - Solar flare

Moderate M1.49 flare from sunspot region 4055

alert


06:06 UTC - Radio Blackout

Minor R1 radio blackout in progress (≥M1 - current: M1.16)


Get instant alerts!

Space weather facts

Last X-flare2025/03/28X1.1
Last M-flare2025/04/14M4.2
Last geomagnetic storm2025/04/06Kp5 (G1)
Spotless days
Last spotless day2022/06/08
Monthly mean Sunspot Number
March 2025134.2 -20.4
April 2025132.1 -2.1
Last 30 days130.6 -13.6

This day in history*

Solar flares
12001X20.6
22000M6.14
32002M5.32
42024M4.02
52000M3.24
DstG
11971-143G3
21961-118G4
31989-95G1
41990-80G1
51973-71
*since 1994

Social networks