Välja antud: 2021 Sep 14 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
14 Sep 2021 | 084 | 007 |
15 Sep 2021 | 083 | 004 |
16 Sep 2021 | 080 | 001 |
The solar activity was at low levels with a single C-class flare over the past 24 hours. NOAA Active Region (AR) 2866 (Catania group 40) produced the C-class flare today 06:53 UT, but its magnetic progress cannot be easily estimated as it is close to the disk's edge. NOAA AR 2868 (Catania group 39) will rotate out of Earth's view in the next 24 hours hence the chances of detectable activity are reduced. An isolated C-class flare is possible in the next 24 hours, but not most likely.
A Coronal Mass Ejection (CME) that was observed by LASCO-C2/SOHO and COR2/STEREO in Sep 13 12:00 UT is likely to be geo-effective. Based on COR2 observations, its speed is estimated to be 300 km/s and it is expected to reach Earth around the Sep 18. A smaller CME detected by LASCO-C2/SOHO in Sep 14 around 06:00 UT, is also expected to reach Earth, possibly in the same day (Sep 18).
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2MeV electron flux was below the 1000 pfu threshold and is expected to remain so in the next 24 hours. The 24h fluence for the greater than 2MeV electron flux was at nominal levels and is expected to remain so in the next 24 hours.
The Solar Wind (SW) parameters measured by ACE and DSCOVR show that the Earth's environment is still under the influence of the ICME that arrived in Sep 13. The solar wind speed varied between 430 and 520 km/s in the past 24 hours. The total magnetic field varied between 3.7 and 9.2 nT and the Bz magnetic field component between -6.5 and 5.7 nT during the last 24 hours. The interplanetary magnetic field remained positive (directed away from the Sun) throughout the last 24 hours. The solar wind parameters are expected to remain at this level for a large part of the next 24 hours and then change to a typical slow solar wind regime.
The geomagnetic conditions over the past 24 hours were both globally and locally quiet to unsettled (NOAA Kp and K Dourbes 0-3). They are expected to maintain the same variety in values in the next 24 hours, as the solar wind conditions are not expected to change.
Today's estimated international sunspot number (ISN): 023, based on 21 stations.
Wolf number Catania | 036 |
10cm solar flux | 083 |
AK Chambon La Forêt | 019 |
AK Wingst | 010 |
Estimated Ap | 011 |
Estimated international sunspot number | 032 - Based on 28 stations |
Day | Begin | Max | Lõpp | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Puuduvad |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
Kõik ajad UTC-s
<< Mine igapäevase ülevaate lehele
Paljud inimesed külastavad SpaceWeatherLive lehte selleks, et jälgida, mis toimub Päikesel või, kas on oodata virmalisi. Suurema liiklusega on serveri koormus ning maksumus kõrgem. Kui sulle meeldib see, mida me sinu heaks teeme, siis saad sa sellele ka ise natukene kaasa aidata, annetades selle lehe käigus hoidmise ja arendamise heaks. Ette tänades SpeaceWeatherLive meeskond!
Viimane X-loide | 28/03/2025 | X1.1 |
Viimane M-loide | 01/04/2025 | M5.6 |
Viimane geomagnetiline torm | 27/03/2025 | Kp5 (G1) |
Plekivabasid päevi | |
---|---|
Viimane päikese plekivaba päev | 08/06/2022 |
Kuu keskmine päikeseplekkide arv | |
---|---|
veebruar 2025 | 154.6 +17.6 |
Viimased 30 päeva | 128.5 -22.7 |