Visualizzazione archivio di martedì, 18 maggio AM

Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2021 May 18 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 18 May 2021 until 20 May 2021
Brillamenti solari

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

Geomagnetism

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

Protoni solari

Quiet

10cm fluxAp
18 May 2021075007
19 May 2021077016
20 May 2021079007

Bulletin

Two active regions (ARs) visible on the disk, NOAA AR 2822 (inactive) and the AR rotating into view from the eastern limb. The latter produced a C1.1 flare at 02:09 UT. It was associated with an EUI wave and small eruption (that will not affect the Earth). More C-class flares can be expected, with a small chance of M-class flares.

No Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraphic imagery in the last 24 hours.

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 normal levels in the past 24 hours and is expected to remain so.

In the last 24 hours, the solar wind speed varied between 320 and 400 km/s. The interplanetary magnetic field polarity was mostly negative (towards the Sun). A weak shock was detected in DSCOVR data, the magnetic field jumped from 5 to 8 nT and the solar wind speed from 320 to 350 km/s, at 15:45 UT on 17 May. This could mark the arrival of the CME from May 13 (with the bulk of the ICME passing north of the Earth). After the shock, the interplanetary magnetic field reached 10 nT (with Bz up to -9 nT). The high speed solar wind from the coronal hole that crossed central meridian on 15 May is expected to arrive to the Earth in about 24 hours.

Geomagnetic conditions ranged from quiet to unsettled locally (KDourbes 0-3) and quiet to active (after the shock) at planetary levels (Kp 2-4). More active to minor storm conditions can be expected when the high speed solar wind stream arrives to the Earth in about 24 hours.

Today's estimated international sunspot number (ISN): 028, based on 25 stations.

Solar indices for 17 May 2021

Wolf number Catania011
10cm solar flux075
AK Chambon La Forêt018
AK Wingst008
Estimated Ap008
Estimated international sunspot number012 - Based on 29 stations

Noticeable events summary

DayBeginMaxFineLocStrengthOP10cmCatania/NOAARadio burst types
Nessuna

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

Tutti gli orari in UTC

<< Vai alla pagina della panoramica giornaliera

Ultime notizie

Supporta SpaceWeatherLive.com!

A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!

No Ads on SWL Pro!
No Ads on SWL Pro! Abbonamenti
Donations
Supporta SpaceWeatherLive.com! Dona
Supporta SpaceWeatherLive con il nostro merchandise
Dai un'occhiata al nostro merchandise

Notizie sul meteo spaziale

Ultimo brillamento X2025/12/08X1.1
Ultimo brillamento M2026/01/14M1.6
Ultima tempesta geomagnetica2026/01/11Kp5+ (G1)
Giorni senza macchie
Ultimo giorno senza macchie2022/06/08
Media mensile Numero di Macchie Solari
dicembre 2025124 +32.2
gennaio 202693.1 -30.9
Ultimi 30 giorni98.3 -7.4

Questo giorno nella storia*

Brillamenti solari
12005X3.79
22005X1.79
32005X1.24
42005X1.21
52023M6.03
DstG
11988-134G3
21960-104G2
31989-99G2
42022-73G1
51972-70G1
*dal 1994

Social networks