Просмотр архива за среда, 17 мая 2017

Daily bulletin on solar and geomagnetic activity from the SIDC

Существующий: 2017 May 17 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 17 May 2017 until 19 May 2017
Солнечные вспышки

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

Geomagnetism

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

Солнечные протоны

Quiet

10cm fluxAp
17 May 2017074017
18 May 2017074024
19 May 2017074010

Bulletin

In the past 24 hours, no C flares were observed. Very low solar activity (no C flares) is expected in the next 24 hours. Solar wind speed measured by DSCOVR decreased from about 550 to 470 km/s in the past 24 hours. The magnitude of the Interplanetary Magnetic Field (IMF) varied between about 2 and 6 nT. Solar wind speed is expected to decrease further within the next 24 hours. On May 17 or early on May 18, a glancing blow from the partial halo CME of May 13 may enhance solar wind conditions again. Quiet to unsettled geomagnetic conditions (K Dourbes between 1 and 3; NOAA Kp between 1 and 3) were registered in the past 24 hours. Quiet to unsettled levels are expected on May 17, 18 and the first half of May 19, with a chance for active geomagnetic levels (K Dourbes = 4) and a slight chance for minor geomagnetic storm intervals (K Dourbes = 5) on May 17 and 18. Active to minor storm conditions are possible late on May 19, as the high speed stream of a negative equatorial coronal hole is expected to arrive at Earth.

Today's estimated international sunspot number (ISN): 012, based on 22 stations.

Solar indices for 16 May 2017

Wolf number Catania027
10cm solar flux072
AK Chambon La Forêt013
AK Wingst010
Estimated Ap010
Estimated international sunspot number024 - Based on 26 stations

Noticeable events summary

DayBeginMaxКонецLocStrengthOP10cmCatania/NOAARadio burst types
Нет

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

Все время в UTC

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