Välja antud: 2019 Feb 24 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
24 Feb 2019 | 070 | 003 |
25 Feb 2019 | 070 | 002 |
26 Feb 2019 | 069 | 016 |
Solar activity was at very low levels. The dynamic, 20-degrees long filament located near N15W40 erupted between 20:00UT (23 February) and 01:00UT (24 February), ejecting mostly to the north and west. No x-ray flare was associated with this event, but some coronal dimming to the northeast of the filament was observed in extreme ultraviolet imagery (SDO/AIA 193). LASCO/C2 coronagraphic imagery showed a coronal mass ejection (CME) becoming first visible at 01:48UT. Preliminary analysis of currently available CACTus imagery gives a plane-of-the-sky speed of about 310 km/s, with no obvious earth-directed component. The greater than 10 MeV proton flux was at nominal values. A negative polarity equatorial coronal hole (CH) is transiting the central meridian.
Solar activity is expected to remain at very low levels.
Solar wind speed declined further from 375 to 325 km/s (DSCOVR). Bz varied between -3 and +3 nT. The interplanetary magnetic field was directed away from the Sun (positive sector). Geomagnetic activity was at quiet levels, with unsettled episodes at Dourbes during the 12-15UT interval and near the end of the period.
Mostly quiet geomagnetic conditions are expected until the arrival of the co-rotating interaction region and high speed stream from the negative polarity CH, currently expected for 26 February. This may result in minor geomagnetic storming.
Today's estimated international sunspot number (ISN): 000, based on 22 stations.
Wolf number Catania | /// |
10cm solar flux | 071 |
AK Chambon La Forêt | 004 |
AK Wingst | 002 |
Estimated Ap | 001 |
Estimated international sunspot number | 000 - Based on 30 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 | M2.5 |
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 |
aprill 2025 | 152.5 -2.1 |
Viimased 30 päeva | 130.7 -17.9 |