Viewing archive of Saturday, 26 October 2019

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2019 Oct 26 1247 UTC

SIDC Forecast

Valid from 1230 UTC, 26 Oct 2019 until 28 Oct 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
26 Oct 2019067023
27 Oct 2019067013
28 Oct 2019067007

Bulletin

Solar X ray flux remained below B level throughout the period. There are no active regions on disk and X-ray flux is expected to remain at background levels.

Form around 9:24UT yesterday October 25 onwards a faint slow CME front is visible along the southern Solar limb in SoHO/LASCO C2 coronagraph images. It is not believed to be related to the filament eruption reported yesterday and its origin remains unclear. In STEREO A COR2 data a corresponding CME is visible from around 6:54 UT onward, directed straight West as seen from STEREO location. Combining these data it seems likely that the CME is Earthbound with an expected arrival time around midnight October 29/30. No other Earth-directed CME's were detected in coronagraph images.

Solar high energy proton fluxes were at background levels and are expected to remain so.

Solar wind speed increased at the start of the period to around 670 km/s before starting a slow gradual decline to current values of 600 km/s. Total magnetic field was mostly in the 4-6nT range but recently increased to around 10nT. Bz was variable over the period but tended to be negative this morning with values down to -6nT and -8.5nT more recently. The phi angle was firmly in the positive sector. Solar wind is expected to slowly decline over the next 24-48 hours as the high speed stream subsides.

Geomagnetic conditions were quiet to active (NOAA Kp 3-4, local K Dourbes 2-4) with just recently a minor storming episode (NOAA Kp 5 for the 9-12UT period). Active geomagnetic conditions are likely over the next 24-48 hours before returning to unsettled conditions. Initially, isolated periods of minor geomagnetic storms are still possible.

Today's estimated international sunspot number (ISN): 000, based on 22 stations.

Solar indices for 25 Oct 2019

Wolf number Catania///
10cm solar flux069
AK Chambon La Forêt031
AK Wingst021
Estimated Ap026
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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G1 - Minor geomagnetic storm

Observed Kp: 5
Threshold reached: 04:05 UTC

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

Gillam, MB, Yellowknife, NT

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

Edmonton, AB, Iqaluit, NU, Saskatoon, SK, Whitehorse, YT
Anchorage, AK, Juneau, AK
The solar wind speed is currently moderately high (652.2 km/sec.)
The Disturbance Storm Time index predicts moderate storm conditions right now (-59nT)

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