Viewing archive of Thursday, 16 February 2017

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2017 Feb 16 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 16 Feb 2017 until 18 Feb 2017
Solar flares

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

Geomagnetism

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

Solar protons

Quiet

10cm fluxAp
16 Feb 2017075011
17 Feb 2017075025
18 Feb 2017075012

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 was around 310 km/s until 6:25 UT on February 16, when it jumped to around 370 km/s, probably marking the arrival of a high speed stream from a positive coronal hole. Since then, solar wind speed has fluctuated between 370 and 430 km/s. The magnitude of the Interplanetary Magnetic Field (IMF) was around 3 nT until about 1:45 UT on February 16, when it started rising to values around 10 nT. Quiet geomagnetic conditions (K Dourbes between 0 and 2; NOAA Kp between 1 and 2) were registered in the past 24 hours. Due to the arrival of the high speed stream, quiet to active geomagnetic levels (K Dourbes < 5) are expected on February 16, 17 and 18, with possible minor storm episodes (K Dourbes = 5).

Today's estimated international sunspot number (ISN): 014, based on 21 stations.

Solar indices for 15 Feb 2017

Wolf number Catania///
10cm solar flux075
AK Chambon La Forêt006
AK Wingst002
Estimated Ap002
Estimated international sunspot number023 - Based on 26 stations

Noticeable events summary

DayBeginMaxEndLocStrengthOP10cmCatania/NOAARadio burst types
None

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

All times in UTC

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G2 - Moderate geomagnetic storm

Observed Kp: 6
Threshold reached: 16:44 UTC

Current data suggests there is a moderate possibility for aurora to appear at the following middle latitude regions in the near future

Surgut, Syktyvkar

Current data suggests there is a slight possibility for aurora to appear at the following middle latitude regions in the near future

Kazan, Moscow, Perm, Yaroslavl
The strength of the interplanetary magnetic field is moderate (16.16nT), the direction is moderately South (-14.28nT).
The Disturbance Storm Time index predicts strong storm conditions right now (-150nT)

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