Viewing archive of Saturday, 15 May 2021

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2021 May 15 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 15 May 2021 until 17 May 2021
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
15 May 2021076009
16 May 2021075007
17 May 2021076017

Bulletin

Solar activity was very low over the past 24 hours. NOAA Active Region (AR) 2822 (Catania sunspot group 93, mag. configuration Beta) has decayed during the past 24 hours and produced only B-class flares. NOAA AR 2823 (Catania sunspot group 94, mag. configuration Alpha) did not produce significant flare activity and continued to decay in the last 24 hours. Solar activity is expect to remain very low over the next 24 hours with a small chance of C-class events.

A partial halo Coronal Mass Ejection (CME) was detected in SoHO/LASCO C2 and STEREO-A/COR2 coronagraph images at around 12:00 UT March 13. The projected speed is 190 km/s and it is expected to arrive around the 18 May.

The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu in the past 24 hours and is expected to remain so. The 24-hour electron fluence was at nominal levels in the past 24 hours and is expected to remain so.

A negative polarity Coronal Hole (CH) with a latitudinal extension form -30 degrees to +30 degrees has reached the central meridian.

The Earth is under the influence of the slow solar wind. The solar wind speed ranged between 380 and 490 km/s over the past 24 hours. The Bz component of the magnetic field fluctuated between -7 and +9 nT. The interplanetary magnetic field angle was predominantly negative (towards the Sun). The solar wind conditions are expected to continue to reflect the slow solar wind regime for the next 24 hours.

Geomagnetic conditions were quiet to unsettled (NOAA Kp and local K Dourbes: 1-3). They are expected to remain quiet to unsettled for the next 24 hours.

Today's estimated international sunspot number (ISN): 028, based on 08 stations.

Solar indices for 14 May 2021

Wolf number Catania026
10cm solar flux071
AK Chambon La Forêt011
AK Wingst005
Estimated Ap004
Estimated international sunspot number025 - Based on 28 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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Current data suggests there is a moderate possibility for aurora to appear at the following high latitude regions in the near future

Gillam, MB, Yellowknife, NT

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

Edmonton, AB, Iqaluit, NU, Saskatoon, SK, Whitehorse, YT
Anchorage, AK, Juneau, AK

Type II Radio Emission

Begin time: Tuesday, 8 April 2025 05:53 UTC
Velocity: 456km/sec
A southern hemisphere coronal hole was detected in an earth-facing position on Tuesday, 8 April 2025

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