Issued: 2019 Apr 10 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 10 Apr 2019 | 079 | 019 |
| 11 Apr 2019 | 079 | 011 |
| 12 Apr 2019 | 078 | 011 |
Over the past 24 hours solar activity has been low. The largest flare was a B2.0 class flare. Active Region (AR) 2738 (Mcintosh class:Cho; Mag. type:Beta) has been most active, the region has shown some evidence of flux emergence and cancellation in HMI magnetogram observations, this may increase flaring activity. Former AR 2737 has moved over the west solar limb. 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 400 and 480 km/s over the past 24 hours, with a jump in speed experienced late on 09-Apr-2019. The total magnetic field strength has fluctuated between 4 and 8 nT. The Bz component has fluctuated around 0 nT, ranging between -8 and +7 nT. Geomagnetic conditions ranged between Kp index 2-4 (NOAA) and local K index 1-3 (Dourbes) over the past 24 hours. The Kp 4 was produced this morning due to a Bz of -8 nT and solar wind speeds reaching 480 km/s. Geomagnetic conditions are expected to be quiet with periods of unsettled-to-active conditions created by sporadic fluctuations in Bz and the solar wind speed.
Today's estimated international sunspot number (ISN): 014, based on 24 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 079 |
| AK Chambon La Forêt | 019 |
| AK Wingst | 010 |
| Estimated Ap | 010 |
| Estimated international sunspot number | 013 - Based on 26 stations |
| Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
|---|---|---|---|---|---|---|---|---|---|---|
| None | ||||||||||
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
All times in UTC
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