Viewing archive of Sunday, 13 October 2019

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2019 Oct 13 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 13 Oct 2019 until 15 Oct 2019
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
13 Oct 2019068005
14 Oct 2019068007
15 Oct 2019067005

Bulletin

Solar activity was at very low levels, no significant flares have been recorded. The Sun remained spotless. 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.

Solar activity is expected to remain at very low levels.

The solar wind speed gradually decreased from 400 km/s to 340 km/s (ACE). The total magnetic field varied between 1 and 5 nT. The direction of the interplanetary magnetic field (phi angle) was predominantly directed away from the Sun (positive sector), with a prolonged interval in the negative sector from 05:00 to 09:30 UT Oct 13. Bz varied between -3 and +4 nT. Geomagnetic activity quiet, with the Kp index (NOAA) and the local k index (Dourbes) recording values of 0-2.

Quiet conditions are expected, with possible unsettled intervals due to the influence of a negative polarity coronal hole which began to traverse the central meridian on Oct 10.

Today's estimated international sunspot number (ISN): 000, based on 20 stations.

Solar indices for 12 Oct 2019

Wolf number Catania///
10cm solar flux068
AK Chambon La Forêt006
AK Wingst006
Estimated Ap004
Estimated international sunspot number000 - Based on 20 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

Nuuk
The solar wind speed is currently moderately high (500.1 km/sec.)
A southern hemisphere coronal hole was detected in an earth-facing position on Tuesday, 8 April 2025

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