Visualizzazione archivio di sabato, 10 marzo AM

Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2018 Mar 10 1232 UTC

SIDC Forecast

Valid from 1230 UTC, 10 Mar 2018 until 12 Mar 2018
Brillamenti solari

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

Geomagnetism

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

Protoni solari

Quiet

10cm fluxAp
10 Mar 2018068031
11 Mar 2018068031
12 Mar 2018068011

Bulletin

Solar X ray flux remained below B level and with no spotted regions on the visible disk chances for any flare occurrences remain very low.

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

Proton flux levels were at background values and are expected to remain so.

A recurrent large elongated negative polarity coronal hole just north of the equator is about to transit the central meridian.

Solar wind conditions became enhanced with an increase in density, speed and magnetic field from around 17:20UT. By 23:00 UT speed reached around 450 km/s and total magnetic field reached 15nT. The total magnetic field remained around 15 nT since then, while speed recovered to under 400 km/s. The Bz component of the magnetic field was consistently negative for a significant amount of time (down to -12nT, but currently -2 to -3 nT). The rotation of the magnetic field as also visible in a gradual shift of the magnetic field phi angle is indicative of the fact that this perturbation marks the passage of the ejecta of March 6 or 7. The timing of the event suggests that the ejecta of March 7 may still arrive later on and cause further perturbations later today or tomorrow. Afterwards, Solar wind conditions should slowly return to nominal with later the influence of the high speed stream of the elongated coronal hole expected from March 14 onwards.

Geomagnetic conditions were quiet to active (NOAA Kp 1-4), with the active periods related to the consistently negative values of Bz. Geomagnetic conditions are expected to remain quiet to active, but should recover to quiet to unsettled on March 12.

Today's estimated international sunspot number (ISN): 000, based on 11 stations.

Solar indices for 09 Mar 2018

Wolf number Catania///
10cm solar flux068
AK Chambon La Forêt023
AK Wingst014
Estimated Ap013
Estimated international sunspot number000 - Based on 25 stations

Noticeable events summary

DayBeginMaxFineLocStrengthOP10cmCatania/NOAARadio burst types
Nessuna

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

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Notizie sul meteo spaziale

Ultimo brillamento X2026/03/30X1.5
Ultimo brillamento M2026/04/03M1.3
Ultima tempesta geomagnetica2026/04/02Kp6- (G2)
Giorni senza macchie
Ultimi 365 giorni3 giorni
20263 giorni (3%)
Ultimo giorno senza macchie2026/02/24
Media mensile Numero di Macchie Solari
febbraio 202678.2 -34.3
aprile 2026141 +62.8
Ultimi 30 giorni94.6 +27

Questo giorno nella storia*

Brillamenti solari
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31999M6.2
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DstG
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51994-103G3
*dal 1994

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