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Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2019 May 10 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 10 May 2019 until 12 May 2019
Brillamenti solari

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

Geomagnetism

Minor storm expected (A>=30 or K=5)

Protoni solari

Quiet

10cm fluxAp
10 May 2019075025
11 May 2019074047
12 May 2019073010

Bulletin

X-ray flux remained below C level with Catania groups 16 and 17 (NOAA AR 2740 and 2741) remaining inactive. X-ray flux is expected to remain below C level.

No new Earth directed CME's have been observed in coronagaph data.

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

Solar wind saw the expected weak solar wind increase. Solar wind speed reached just over 390 km/s before coming down again to current levels around 325 km/s. Total magnetic field was around 8nT at the start of the period but quickly recovered to nominal values around 4nT with Bz variable and the phi angle in the negative sector. Solar wind is expected to become disturbed from this afternoon onwards by the arrival of the May 6 CME though solar wind speed should not become too much increased.

Geomagnetic conditions were quiet to unsettled (NOAA Kp 1-2, local K Dourbes 0-3). Geomagnetic conditions may reach minor storm levels due to the expected CME arrival.

Today's estimated international sunspot number (ISN): 028, based on 20 stations.

Solar indices for 09 May 2019

Wolf number Catania028
10cm solar flux076
AK Chambon La Forêt014
AK Wingst///
Estimated Ap010
Estimated international sunspot number026 - Based on 20 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
Ultimo brillamento M2025/12/21M1.3
Ultima tempesta geomagnetica2025/12/22Kp5 (G1)
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