Välja antud: 2021 Oct 27 1232 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10 cm vool | Ap | |
---|---|---|
27 Oct 2021 | 110 | 003 |
28 Oct 2021 | 100 | 004 |
29 Oct 2021 | 090 | 007 |
Solar flaring activity was moderate during the last 24 hours, with an M1 flare detected on 16 Oct 15:57 UT at N13E89 (possibly NOAA returning active region 2885). Several C-class flares were detected from NOAA Active Region (AR) 2887 (Beta magnetic configuration) and from the two returning ARs, while NOAA 2889 (Beta magnetic configuration) produced one C-class flare. The ARs 2886, 2888 (both with Alpha magnetic configuration) and 2890 (Beta magnetic configuration) did not produced any significant activity. Several C-class flares are expected for the next 24 hours (mostly from the NOAA AR 2887 and the two returning ARs), and there is a good chance of one or more M-class flares.
No Earth directed CMEs have been detected in the available coronagraph imagery. A few CMEs and outward flows were detected by CACTUS from SOHO/LASCO-C2 data during the last 24 hours, however those events took place at the east of the solar limb and they are not expected to be geo- effective.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold and is expected to remain below this threshold during the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so.
The solar wind speed (as measured by DSCOVR) increased from 310 to 420 km/s during the last 24 hours. The total magnetic field ranged from 1 nT to around 7 nT, while the Bz varied between -4 and +5 nT in the last 24 hours. The interplanetary magnetic field phi angle was predominantly in the negative sector (directed towards the Sun) during the last 24 hours. The solar wind conditions are expected to remain in the slow solar wind regime for the next 24 hours.
Geomagnetic conditions were globally and locally quiet (NOAA Kp and K Dourbes indices 1-2). Geomagnetic conditions are expected to remain quiet for the next 24 hours.
Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 101, põhineb 17 jaamadel.
Catania Wolfi number | /// |
10cm päikesevoog | 109 |
AK Chambon La Forêt | 008 |
AK Wingst | 005 |
Hinnanguline Ap | 004 |
Hinnanguline rahvusvaheline päikeselaikude arv | 086 - Põhineb 29 jaamal |
Päev | Algus | Maks | Lõpp | Lokatsioon | Tugevus | OP | 10cm | Catania/NOAA | Raadiosignaalipursete tüübid |
---|---|---|---|---|---|---|---|---|---|
26 | 1542 | 1557 | 1602 | ---- | M1.0 | --/2891 |
Andmed on esitanud Päikeseinfektide Andmeanalüüsi Keskus (Solar Influences Data Analysis Center)© - SIDC - Töötleb 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 | 30/04/2025 | M2.03 |
Viimane geomagnetiline torm | 03/05/2025 | Kp5 (G1) |
Plekivabasid päevi | |
---|---|
Viimane päikese plekivaba päev | 08/06/2022 |
Kuu keskmine päikeseplekkide arv | |
---|---|
aprill 2025 | 140.6 +6.4 |
mai 2025 | 79 -61.6 |
Viimased 30 päeva | 105.3 -31.1 |