Viewing archive of Thursday, 2 June 2022

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2022 Jun 02 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 02 Jun 2022 until 04 Jun 2022
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
02 Jun 2022106007
03 Jun 2022108007
04 Jun 2022108007

Bulletin

Over the past 24 hours, solar flaring activity has been low. There was a C1.2 flare peaking at 06:20 UT, from the (unnumbered) active region rotating into view from the east limb. There are four active regions visible on the disk, NOAA AR 3025 rotated out of view over the west limb and 3026 and 3027 emerged, they have beta magnetic field configuration. The other two ARs are 3023 and 3024, with alpha magnetic field configuration. C-class flaring can be expected in the next 24 hours, mostly from the region that rotated into view over the east limb.

A wide CME (angular width around 100 degrees) was first seen at 06:12 UT by LASCO/C2, with a calculated 3D speed of 750 km/s. The CME originated from a filament eruption close to NOAA AR 3023 (S14W34). This CME has an Earth directed component with expected arrival around 01:00 UT on 5 June (with an error margin of 12 hours). Another filament erupted close to disk center around 01:00 UT on 1 June, but did not produce any relevant CME. Due to its location, a weak and narrow Earth directed CME can not be discarded, probably arriving together with the previous one, or close in time but with no significant impact expected.

The greater than 10 MeV proton flux was at nominal levels and is expected to remain so in the next 24 hours. The greater than 2MeV electron has been above the 1000 pfu threshold over the past 24 hours. Since the high speed solar wind stream is not affecting the Earth anymore, it can be expected to decrease. The 24h electron fluence is at moderate levels, and is expected to remain so in the next 24 hours.

The solar wind arriving to the Earth is slow, with speeds around 390 km/s and interplanetary magnetic field around 4 nT. Similar conditions are expected for the next 24 hours.

Over the past 24 hours, geomagnetic conditions were quiet (Kp=1, K_BEL=2). Over the next 24 hours, similar conditions are expected.

Today's estimated international sunspot number (ISN): 063, based on 20 stations.

Solar indices for 01 Jun 2022

Wolf number Catania081
10cm solar flux104
AK Chambon La Forêt008
AK Wingst015
Estimated Ap011
Estimated international sunspot number065 - Based on 29 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

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G1 - Minor geomagnetic storm

Observed Kp: 5
Threshold reached: 23:19 UTC

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

Tórshavn
Oulu, Rovaniemi, Sodankylä
Reykjavik
Tromsø
Kiruna, Luleå

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

Kuopio
Bergen, Trondheim
Arkhangelsk
Sundsvall, Umeå
The solar wind speed is currently moderately high (525.9 km/sec.)
The strength of the interplanetary magnetic field is moderate (11.36nT), the direction is North (3.6nT).
The Disturbance Storm Time index predicts moderate storm conditions right now (-85nT)
The maximum X-ray flux of the past two hours is:
C5.75

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