Viewing archive of Tuesday, 21 May 2019

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2019 May 21 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 21 May 2019 until 23 May 2019
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
21 May 2019069007
22 May 2019068007
23 May 2019068004

Bulletin

Over the past 24 hours solar activity has been low. The visible solar disc was spotless and the X-ray flux remained below B-class level. No Earth directed Coronal Mass Ejections (CMEs) have been detected. The greater than 10MeV proton flux remained at background levels over the past 24 hours. Solar activity is expected to remain low over the next 24 hours.

The solar wind speed has fluctuated between 355 and 450 km/s over the past 24 hours. The total magnetic field strength fluctuated around 5 nT for much of the period, with a minimum of 0.6 nT and a maximum of 7.1 nT recorded. The Bz component was predominantly positive and ranged between -4.8 and +7.1 nT.

Geomagnetic conditions have been quiet to unsettled over the past 24 hours, with Kp index (NOAA) and local K index (Dourbes) ranging between 1-2 and 1-3, respectively. Quiet to unsettled geomagnetic conditions are expected to continue over the next 24 hours, due to the weak solar wind stream associated with the patchy negative polarity equatorial coronal hole which began to traverse the central meridian on 18 May.

Today's estimated international sunspot number (ISN): 000, based on 21 stations.

Solar indices for 20 May 2019

Wolf number Catania///
10cm solar flux069
AK Chambon La Forêt008
AK Wingst008
Estimated Ap007
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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