Issued: 2020 Apr 17 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
17 Apr 2020 | 069 | 007 |
18 Apr 2020 | 068 | 009 |
19 Apr 2020 | 069 | 008 |
The Sun was spotless again. Solar activity was at very low levels and is expected to remain so.
The greater than 10 MeV proton flux and the greater than 2 MeV electron flux were at nominal values and are expected to remain so.
No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery.
Solar wind speed was on a mostly declining trend, varying between 370 and 300 km/s and ending the period with low values around 310 km/s (DSCOVR). Bz varied between -4 and +3 nT, being mostly negative since 06UT. The direction of the interplanetary magnetic field (phi angle) was in a predominantly sunward orientation (negative sector).
Geomagnetic activity was at quiet levels, with an isolated unsettled episode recorded by Dourbes during the 15-18UT interval. Geomagnetic conditions are expected to be quiet to unsettled during the next few days.
Today's estimated international sunspot number (ISN): 000, based on 27 stations.
Wolf number Catania | /// |
10cm solar flux | 069 |
AK Chambon La Forêt | 007 |
AK Wingst | 006 |
Estimated Ap | 004 |
Estimated international sunspot number | 000 - Based on 34 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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