Issued: 2020 May 15 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 15 May 2020 | 068 | 006 |
| 16 May 2020 | 070 | 005 |
| 17 May 2020 | 070 | 004 |
The Sun was spotless. Solar activity was at very low levels and is expected to remain so. A small active region may round the northeast limb on 16 May.
The greater than 10 MeV proton flux and the greater than 2 MeV electron flux were at nominal levels during the last 24 hours and are expected to remain so.
No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery.
Solar wind speed varied between 280 and 320 km/s, with Bz varying between -3 and +5 nT (DSCOVR). The direction of the interplanetary magnetic field (phi angle) was mostly oriented away from the Sun (positive sector), being in a negative sector during the 00-03UT interval and briefly around 21UT and 08UT.
Geomagnetic activity was at quiet levels, with unsettled conditions recorded by Dourbes during the 09-12UT interval. Geomagnetic conditions are expected to be mostly quiet with an occasional unsettled episode possible.
Today's estimated international sunspot number (ISN): 000, based on 22 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 068 |
| AK Chambon La Forêt | 007 |
| AK Wingst | 004 |
| Estimated Ap | 002 |
| Estimated international sunspot number | 000 - Based on 31 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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