Viewing archive of Sunday, 3 December 2017

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2017 Dec 03 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 03 Dec 2017 until 05 Dec 2017
Solar flares

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

Geomagnetism

Moderate (ISES: Major) magstorm expected (A>=50 or K=6)

Solar protons

Quiet

10cm fluxAp
03 Dec 2017071004
04 Dec 2017070054
05 Dec 2017070045

Bulletin

Solar activity was at very low levels. The Sun is spotless. No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels.

Quiet flaring conditions are expected.

ACE data indicated solar wind speed decreased further from initial values near 400 km/s to about 350 km/s by the end of the period. Bz varied between +3 nT and -4 nT. The interplanetary magnetic field was mostly directed towards the Sun. The extension of a positive northern polar CH is transiting the central meridian.

The geomagnetic field was quiet to unsettled levels throughout the period, and is expected to remain so until the arrival of the high speed stream from the northern polar coronal hole (CH) extension and its associated preceding co-rotating interaction region. Based on observations from the previous solar rotation and from STEREO-A, their influence may start affecting the earth environment late on 03 December or on 04 December, with minor to moderate geomagnetic storming possible.

Today's estimated international sunspot number (ISN): 000, based on 09 stations.

Solar indices for 02 Dec 2017

Wolf number Catania///
10cm solar flux072
AK Chambon La Forêt006
AK Wingst003
Estimated Ap003
Estimated international sunspot number000 - Based on 13 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

Gillam, MB, Iqaluit, NU
Nuuk
The direction of the interplanetary magnetic field is slightly South (-6.84nT).
The maximum X-ray flux of the past two hours is:
C6.12

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