Viewing archive of Saturday, 30 November 2019

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2019 Nov 30 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 30 Nov 2019 until 02 Dec 2019
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
30 Nov 2019070005
01 Dec 2019070004
02 Dec 2019070003

Bulletin

Solar activity was at very low levels. The visible solar disk was spotless. No earth-directed coronal mass ejections (CMEs) have been observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal values.

Solar activity is expected to remain at very low levels.

Solar wind speed gradually increased from initial values around 360 km/s to near 400 km/s at the end of the period (ACE). The interplanetary magnetic field (phi angle) was predominantly directed towards the Sun (negative sector). Bz varied between -6 and +5 nT, with a sustained negative stretch near -5 nT between 19-22UT that resulted in unsettled to active geomagnetic conditions during the 21-24UT interval (Kp = 3; K Dourbes = 4). For the remainder of the period, geomagnetic activity was mostly at quiet levels.

Geomagnetic activity is expected to remain at mostly quiet levels, an unsettled interval not excluded.

Today's estimated international sunspot number (ISN): 000, based on 28 stations.

Solar indices for 29 Nov 2019

Wolf number Catania000
10cm solar flux070
AK Chambon La Forêt011
AK Wingst007
Estimated Ap005
Estimated international sunspot number000 - Based on 24 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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Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future

Tórshavn
Oulu, Rovaniemi, Kuopio, Sodankylä
Trondheim
Arkhangelsk, Murmansk
Kiruna, Luleå, Sundsvall, Umeå

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

Tampere
The maximum X-ray flux of the past two hours is:
C8.08

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