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Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2018 Sep 14 1249 UTC

SIDC Forecast

Brillamenti solari

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

Geomagnetism

Active conditions expected (A>=20 or K=4)

Protoni solari

Quiet

	10cm flux	Ap
14 Sep 2018	070	021
15 Sep 2018	071	013
16 Sep 2018	072	012

Bulletin

Over the past 24 hours solar activity has been quiet. No significant flares have been recorded. No Earth directed Coronal Mass Ejections (CMEs) have been detected. There are no significant filaments. Solar activity is expected to remain low over the next 24 hours with a low probability of C-class flares. The solar wind speed has fluctuated between 510 and 580 km/s over the past 24 hours. The total magnetic field strength has fluctuated around 5 nT. The Bz component has fluctuated around 0 nT, between -6.3 and +5.3 nT. Mostly unsettled to active geomagnetic conditions have been observed, with Kp recording an isolated minor storm episode during the 00-03UT interval this morning (14 September). Mostly unsettled geomagnetic conditions are expected for the next two days due to possible intremittent Earth interaction with the eleveated solar wind sterams coming from the positive polarity coronal hole. Active conditions can be expected as well on the day three (16 September) due to the influence of another neagtive polarity coronal hole.

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

Solar indices for 13 Sep 2018

Wolf number Catania	///
10cm solar flux	070
AK Chambon La Forêt	024
AK Wingst	022
Estimated Ap	021
Estimated international sunspot number	000 - Based on 30 stations

Noticeable events summary

Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive

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