Viewing archive of Monday, 23 September 2019

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2019 Sep 23 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 23 Sep 2019 until 25 Sep 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
23 Sep 2019068014
24 Sep 2019067021
25 Sep 2019067013

Bulletin

Solar X-ray flux remained below B class levels throughout the period. The Solar disk is spotless and X-ray flux is expected to remain at or below background levels.

There are currently no SoHO-LASCO coronagraph observations available, HAO- kCOR ground-based coronagraph observations (around 18:00 UT on 22-Sep-2019) combined with STEREO-A COR coronagraph and SDO-AIA EUV observations indicate no Earth-directed CMEs (Coronal Mass Ejection) were produced. Without LASCO data to corroborate the absence of a CME, these observations should be treated with caution, with the small possibility of an unobserved Earth directed CME having been produced.

Proton levels were at background values and are expected to remain so.

The solar wind speed has been slowly decreasing from around 350 to 300 km/s over the past 24 hours. The total magnetic field strength has fluctuated around 5 nT. The Bz component has been largely positive, fluctuating between -2 and 5 nT. Geomagnetic conditions ranged between Kp index 0-1 (NOAA) and local K index 0-3 (Dourbes) over the past 24 hours.

Solar wind conditions are expected to increase at the end of the day, and then become enhanced over the following 24 hours due to a high speed stream (HSS) from a recurrent equatorial coronal hole. The solar wind speed is anticipated to reach speeds exceeding 500 km/s.

Geomagnetic conditions are expected to become unsettled around the end of the day, with some active periods due to HSS solar wind enhancements.

Today's estimated international sunspot number (ISN): 000, based on 19 stations.

Solar indices for 22 Sep 2019

Wolf number Catania///
10cm solar flux068
AK Chambon La Forêt005
AK Wingst004
Estimated Ap003
Estimated international sunspot number000 - Based on 22 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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G3 - Strong geomagnetic storm

Observed Kp: 7
Threshold reached: 19:32 UTC

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

Kuopio
Arkhangelsk

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

Aalborg
Tallinn
Helsinki, Tampere, Turku
Petrozavodsk, Saint Petersburg, Surgut, Syktyvkar
Stockholm
The strength of the interplanetary magnetic field is moderate (14.44nT), the direction is North (13.76nT).
The Disturbance Storm Time index predicts strong storm conditions right now (-149nT)

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