Datum verslag: 2024 Jul 13 1243 UTC
M-class flares expected (probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
13 Jul 2024 | 208 | 007 |
14 Jul 2024 | 208 | 022 |
15 Jul 2024 | 208 | 010 |
Solar flaring activity over the past 24 hours was at moderate levels with background C-class flaring and an M1.4-flare, peak time 03:18 UTC on July 13, associated with the largest and most complex active region NOAA AR 3738 (beta-gamma). This region was responsible for most of the registered flaring activity. There are currently eight numbered active regions on the visible solar disc, including the newly numbered NOAA AR 3748 (beta). Two new regions (possibly returning regions NOAA AR 3719 and NOAA AR 3720) have rotated onto disc from behind the south-east limb. NOAA AR 3743 (beta) has slightly decreased its magnetic complexity and produced isolated high C-class flaring together with NOAA AR 3740 (beta), which is now rotating behind the west limb. The remaining active regions have remained mostly stable and quiet. The solar flaring activity is likely to be at moderate levels over the coming days with 60% chance for M-class flaring and 15% chances for isolated X-class flaring.
No Earth-directed coronal mass ejection (CMEs) have been detected in the available coronagraph imagery over the past 24 hours.
Over the past 24 hours the solar wind parameters (ACE and DSCOVR) were indicative of background slow solar wind conditions. The solar wind velocity weakly varied between 308 km/s and 390 km/s. The interplanetary magnetic field registered a maximum value of 5.9 nT and a minimum Bz of -5 nT. The B field phi angle was predominantly in the negative sector (directed towards the Sun). The solar wind conditions are expected to register moderate disturbances later on July 13 and July 14 with anticipated high speed stream arrival related to a positive polarity equatorial coronal hole which crossed the central meridian on July 10.
The geomagnetic conditions over the past 24 hours were globally quiet and locally mostly quiet with a couple of hours with unsettled periods registered over Belgium. Quiet to active conditions are anticipated for late July 13 and July 14 with possible isolated minor storms due to anticipated high speed stream arrival.
Over the past 24 hours the greater than 10 MeV GOES proton flux was at background levels and is expected to remain so over the next days.
The greater than 2 MeV electron flux as measured by GOES 16 and GOES 18 was below the 1000 pfu threshold and is expected to remain so in the upcoming days. The 24h electron fluence was at nominal level and is expected to remain so in the next days.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 192, gebaseerd op 10 stations.
Wolfgetal Catania | 235 |
10cm zonneflux | 210 |
AK Chambon La Forêt | 008 |
AK Wingst | 007 |
Geschatte Ap | 006 |
Geschat internationaal zonnevlekkengetal | 172 - Gebaseerd op 13 stations |
Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen |
---|---|---|---|---|---|---|---|---|---|
13 | 0255 | 0318 | 0336 | ---- | M1.4 | 85/3738 |
Aangeboden door het Solar Influences Data Analysis Center© - SIDC - Verwerkt door SpaceWeatherLive
Alle tijden in UTC
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Matige M1.97 zonnevlam van zonnevlekkengebied 4079
Kleine R1 radio blackout gedetecteerd (≥M1 - momenteel: M1.89)
G1 - Kleine geomagnetische storm (Kp5) Drempel bereikt: 20:58 UTC
Het OVATION-model voorspelt dat het hemisferisch vermogen 50GW zal bereiken om 21:35 UTC
Actieve geomagnetische condities (Kp4) Drempel bereikt: 20:21 UTC
Laatste X-klasse uitbarsting | 28/03/2025 | X1.1 |
Laatste M-klasse uitbarsting | 12/05/2025 | M1.9 |
Laatste geomagnetische storm | 03/05/2025 | Kp5 (G1) |
Zonnevlekkenloze dagen | |
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Laatste zonnevlekkenloze dag | 08/06/2022 |
Maandelijks gemiddeld zonnevlekkengetal | |
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april 2025 | 140.6 +6.4 |
mei 2025 | 77.8 -62.8 |
Afgelopen 30 dagen | 101.4 -34 |