Viewing archive of Thursday, 1 November 2018

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2018 Nov 01 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 01 Nov 2018 until 03 Nov 2018
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
01 Nov 2018068008
02 Nov 2018068003
03 Nov 2018068024

Bulletin

Solar activity was at very low levels. No sunspot regions were observed on the visible solar disk. No earth-directed coronal mass ejections (CMEs) were observed over the last 24 hours. The greater than 10 MeV proton flux was at nominal values. A positive polarity equatorial coronal hole is transiting the Central Meridian.

Solar activity is expected to remain at very low levels.

Solar wind speed showed a slightly increasing trend and varied between 320 and 360 km/s (DSCOVR). Bz ranged between -5 and +4 nT, with a mostly negative stretch near -4 nT from 04-07UT. The direction of the interplanetary magnetic field (phi angle) was mostly away from the Sun (positive sector), with negative sectors from 00:30-04:30UT and from 06-08UT, and variable after 08UT. Quiet geomagnetic conditions were observed with an unsettled episode in K Dourbes during the 06-11UT interval.

Quiet to unsettled geomagnetic conditions are expected until the arrival of the co-rotating interaction region and the high speed wind stream associated with the positive polarity CH. Based on STEREO-A data, this arrival is expected for 3 November, with wind speeds possibly up to 650 km/s and Bz around -10 nT. Geomagnetic conditions may then reach minor storm levels, a moderate storming episode not excluded.

Today's estimated international sunspot number (ISN): 000, based on 10 stations.

Solar indices for 31 Oct 2018

Wolf number Catania///
10cm solar flux068
AK Chambon La Forêt009
AK Wingst005
Estimated Ap004
Estimated international sunspot number/// - Based on /// 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 high possibility for aurora to appear at the following high latitude regions in the near future

Sodankylä, Utsjoki
Tromsø
Murmansk
Kiruna

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

Tórshavn
Oulu, Rovaniemi
Kirkenes, Trondheim
Arkhangelsk
Luleå, Umeå

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

Kuopio
Bergen
Sundsvall

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

Helsinki, Tampere, Turku
Petrozavodsk, Syktyvkar
The solar wind speed is currently moderately high (538.6 km/sec.)
The strength of the interplanetary magnetic field is moderate (11.19nT), the direction is slightly South (-9.98nT).
The Disturbance Storm Time index predicts moderate storm conditions right now (-90nT)

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