Datum verslag: 2019 Sep 21 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
21 Sep 2019 | 067 | 005 |
22 Sep 2019 | 067 | 007 |
23 Sep 2019 | 067 | 013 |
Solar X ray flux remained below B level throughout the period. The Solar disk is spotless and X-ray flux is expected to remain at or below background levels.
The filament eruption from the Southern hemisphere that was mentioned in yesterdays bulletin has been investigated further. While the STEREO/COR2 coronagraph data indicate a corresponding narrow CME that may be Earth directed its corresponding projected speed is below 300 km/s. SoHO/LASCO data do not show any clear signs of any (partial) halo CME but only some weak signatures of Eastward propagating material. It is hence assessed that the ejecta are possibly off the Sun-Earth line towards the East. Even if the ejecta would be towards the Earth, with such a slow speed it is unlikely to have any significant impact. Hence no specific arrival forecast is made. There were otherwise no Earth-directed CMEs observed in coronagraph data.
Proton levels were at background values and are expected to remain so.
Solar wind conditions were near nominal. Around 5:00UT Solar wind speed increased fairly suddenly from around 300 km/s to around 360 km/s along with total magnetic field going up from around 3nT to around 7nT. At that time the magnetic field phi angle started fluctuating between the positive and negative sector and Bz became pronounced negative. Solar wind conditions are expected to remain near nominal over the next 48 hours then followed towards the end of day 3 with the onset of a high speed stream related to the negative polarity equatorial coronal hole that passed the central meridian yesterday.
Geomagnetic conditions were quiet to unsettled (NOAA Kp 1-3 and local K Dourbes 0-3). Quiet to unsettled geomagnetic conditions are expected to continue the next 48 hours with later, towards the end of day 3, unsettled to active conditions expected under the high speed stream influence.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 000, gebaseerd op 23 stations.
Wolfgetal Catania | /// |
10cm zonneflux | 067 |
AK Chambon La Forêt | 008 |
AK Wingst | 003 |
Geschatte Ap | 002 |
Geschat internationaal zonnevlekkengetal | 000 - Gebaseerd op 30 stations |
Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen | |
---|---|---|---|---|---|---|---|---|---|---|
Geen |
Aangeboden door het Solar Influences Data Analysis Center© - SIDC - Verwerkt door SpaceWeatherLive
Alle tijden in UTC
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Actieve geomagnetische condities (Kp4) Drempel bereikt: 19:56 UTC
Het OVATION-model voorspelt dat het hemisferisch vermogen 50GW zal bereiken om 17:42 UTC
Actieve geomagnetische condities (Kp4) Drempel bereikt: 22:34 UTC
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