Viewing archive of Saturday, 16 November 2019

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2019 Nov 16 1235 UTC

SIDC Forecast

Valid from 1230 UTC, 16 Nov 2019 until 18 Nov 2019
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 Nov 2019070007
17 Nov 2019070018
18 Nov 2019070012

Bulletin

The solar activity has been at very low levels over the past 24 hours. The Sun is currently spotless and the X-ray flux remains below B-level. Solar activity is expected to remain at low levels for the next 24 hours.

No earth-directed coronal mass ejections (CMEs) have been observed in the available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal values.

The solar wind parameters were mostly at nominal values. On Nov 16, a minor enhancement of the solar wind environment was observed starting around 18:00 UT. This enhancement can be associated with the sector bordering crossing announcing the soon arrival of the expected coronal hole influence. The total magnetic field reached 7 nT around 19:30, the solar wind speed went up to 400 km/s, and the southern component of the magnetic filed fluctuated between -5.7 nT and 5 nT. The solar wind parameters are expected to return close to the nominal values for a short period of a few hours. Then we expect new enhancements of the solar wind parameters to start later today on Nov 16 or early 17 due to the influence of the negative polarity coronal hole high-speed streams, which has reached the central meridian on Nov 13.

Quiet geomagnetic conditions were observed over the past 24 hours. It is expected to remain so for a short period of a few hours until the arrival of influence due to the high-speed stream coming from the coronal hole later in Nov 16-17 were more active conditions are expected.

Today's estimated international sunspot number (ISN): 000, based on 14 stations.

Solar indices for 15 Nov 2019

Wolf number Catania000
10cm solar flux070
AK Chambon La Forêt007
AK Wingst///
Estimated Ap003
Estimated international sunspot number000 - Based on 12 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: 18:45 UTC

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

Arkhangelsk

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

Petrozavodsk, Surgut, Syktyvkar

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

Riga
Perm, Saint Petersburg, Yaroslavl
The strength of the interplanetary magnetic field is moderate (16.06nT), the direction is moderately South (-13.45nT).
The Disturbance Storm Time index predicts strong storm conditions right now (-143nT)

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