Visualizzazione archivio di venerdì, 2 luglio AM

Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2021 Jul 02 1240 UTC

SIDC Forecast

Valid from 1230 UTC, 02 Jul 2021 until 04 Jul 2021
Brillamenti solari

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

Geomagnetism

Quiet (A<20 and K<4)

Protoni solari

Quiet

10cm fluxAp
02 Jul 2021093007
03 Jul 2021091016
04 Jul 2021089010

Bulletin

X-ray flux remained below C level with only some B level flares. The largest region on disc, NOAA region 2835 (Catania group 9), has simplified in magnetic complexity (now classified beta-gamma) but remains the most likely source for flaring at above C level. NOAA region 2836 (Catania group 10) has lost its trailing spot while region 2837 (Catania group 11) has developed leading spots. Some C class flare activity remains likely, primarily from region 2835, with also still a chance for flaring at M class level.

No new Earth directed CMEs have been recorded in coronagraph data.

A small negative polarity coronal hole started transiting the central meridian around midnight. Although it is seen to fade as it is transiting the central meridian, some influence on Solar wind conditions near Earth could still be possible starting around noon July 5.

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 was below the 1000 pfu event threshold. The 24h electron fluence was at normal levels and electron fluence is expected to remain at normal levels over the next days.

Solar wind conditions displayed a decline towards slow Solar wind conditions. The Solar wind speed decreased from over 500 km/s to around 420 km/s. The interplanetary magnetic field decreased from 8.6nT to around 5nT with a variable Bz component. The magnetic field phi angle indicated that the interplanetary magnetic field is pointing away from the Sun. A further return towards slow Solar wind conditions is expected with tomorrow July 3 some possible perturbations related to the possible arrival of the CME from June 29. From July 5 onwards some increase is possible related to the negative polarity coronal hole that is currently transiting the central meridian.

Geomagnetic conditions were quiet to unsettled (local K Dourbes 1-3 and NOAA Kp 1-2). Geomagnetic conditions are expected to be quiet with tomorrow also unsettled and some active periods possible in case the CME arrives.

Today's estimated international sunspot number (ISN): 053, based on 21 stations.

Solar indices for 01 Jul 2021

Wolf number Catania055
10cm solar flux094
AK Chambon La Forêt008
AK Wingst008
Estimated Ap007
Estimated international sunspot number053 - Based on 28 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!

Molte persone vengono su SpaceWeatherLive per seguire l'attività del Sole o sapere se ci sia la possibilità di vedere l'aurora, ma a maggior traffico corrispondono costi maggiori. Considerate una donazione se vi piace SpaceWeatherLive così che possiamo mantenere online il sito web!

Dona SpaceWeatherLive Pro
Supporta SpaceWeatherLive con il nostro merchandise
Dai un'occhiata al nostro merchandise

Notizie sul meteo spaziale

Ultimo brillamento X2025/03/28X1.1
Ultimo brillamento M2025/04/01M2.5
Ultima tempesta geomagnetica2025/03/27Kp5 (G1)
Giorni senza macchie
Ultimo giorno senza macchie2022/06/08
Media mensile Numero di Macchie Solari
marzo 2025134.2 -20.4
aprile 2025143 +8.8
Ultimi 30 giorni129.8 -16.3

Questo giorno nella storia*

Brillamenti solari
12001X1.21
22001M7.3
32001M4.52
42013M3.28
52004M2.47
DstG
11993-165G3
21968-112G3
31978-109G1
41984-108G2
51989-101G2
*dal 1994

Social networks