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Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2018 Mar 17 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 17 Mar 2018 until 19 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
17 Mar 2018068024
18 Mar 2018068029
19 Mar 2018068012

Bulletin

Solar X ray flux remained below B level. NOAA active region 2701 decayed shortly after emerging but meanwhile a new, yet unnumbered, bipolar region is forming around N20W33. Solar X-ray flux is still expected to remain below C level.

No Earth directed CMEs have been observed in coronagraph data.

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

Solar wind remained enhanced with solar wind speed first declining to around 420km/s before increasing again to around 500 km/s currently. Total magnetic field reached a maximum of 13nT in the afternoon of March 16 but meanwhile declined to nominal values of around 5nT. The magnetic field phi angle was steady in the negative sector. Enhanced solar wind conditions are expected to continue at least today and into tomorrow under the influence of the negative polarity coronal hole in the northern hemisphere.

Geomagnetic conditions were quiet to active (local K Dourbes 1-4, NOAA Kp 3-4). Active geomagnetic conditions are still to be expected today and tomorrow.

Today's estimated international sunspot number (ISN): 000, based on 04 stations.

Solar indices for 16 Mar 2018

Wolf number Catania000
10cm solar flux069
AK Chambon La Forêt037
AK Wingst022
Estimated Ap024
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 X2025/12/08X1.1
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