Välja antud: 2019 Apr 09 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
09 Apr 2019 | 080 | 013 |
10 Apr 2019 | 081 | 008 |
11 Apr 2019 | 082 | 007 |
Over the past 24 hours solar activity has been low. The largest flare was a B5.6 class flare. Active Region (AR) 2738 (Mcintosh class:Hhx; Mag. type:Alpha) has been most active, producing several B-class flares, including the B5.6 class flare, which peaked at 14:00 UT (08-Apr-2019). Former AR 2737 is near the west solar limb, and has shown little activity. No significant filament channels have been seen on the solar disk. No Earth directed Coronal Mass Ejections (CMEs) have been detected. There are no significant low latitude coronal holes on the solar disk. The greater than 10MeV proton flux remained at background levels over the past 24 hours. Solar activity is expected to remain low over the next 24 hours with a reasonable chance of a C-class flare from AR 2738.
The solar wind speed has fluctuated between 380 and 480 km/s over the past 24 hours. The total magnetic field strength has fluctuated around 5.0 nT. The Bz component has been mainly negative, ranging between -7 and +5 nT. Geomagnetic conditions ranged between Kp index 2-4 (NOAA) and local K index 2-3 (Dourbes) over the past 24 hours. Geomagnetic conditions are expected to be quiet to unsettled.
Today's estimated international sunspot number (ISN): 012, based on 19 stations.
Wolf number Catania | 013 |
10cm solar flux | 079 |
AK Chambon La Forêt | 022 |
AK Wingst | 014 |
Estimated Ap | 015 |
Estimated international sunspot number | 013 - Based on 25 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
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