Viewing archive of Sunday, 8 July 2018

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2018 Jul 08 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 08 Jul 2018 until 10 Jul 2018
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
08 Jul 2018072004
09 Jul 2018073010
10 Jul 2018074009

Bulletin

Over the past 24 hours solar activity has been low. No significant flares have been recorded. A recurrent Active Region (AR) has just rotated onto the East limb, and has the potential to produce flaring activity. The greater than 10MeV proton flux remained at background levels over the past 24 hours. No Earth directed CMEs were detected. Solar activity is expected to remain low over the next 24 hours. The solar wind speed has fluctuated between 450 and 500 km/s over the past 24 hours. The total magnetic field strength has fluctuated around 5 nT. The Bz component has fluctuated between -2 and +2 nT. Geomagnetic conditions ranged between Kp index 0-2 (NOAA) and local K index 1-3 (Dourbes) over the past 24 hours. The small region of patchy coronal hole located at central latitudes has the potential to enhance solar wind speeds and geomagnetic activity marginally. Geomagnetic conditions are expected to be quiet.

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

Solar indices for 07 Jul 2018

Wolf number Catania///
10cm solar flux072
AK Chambon La Forêt010
AK Wingst008
Estimated Ap007
Estimated international sunspot number000 - Based on 32 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

Gillam, MB, Yellowknife, NT

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