Существующий: 2016 Oct 02 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 02 Oct 2016 | 079 | 018 |
| 03 Oct 2016 | 078 | 010 |
| 04 Oct 2016 | 076 | 010 |
There are presently no active regions on the visible side of the Sun, and accordingly solar activity is low (without C-class flares reported). We expect low solar activity to persist in the coming hours. The CME, first seen in the SOHO/LASCO C2 field of view at about 14:24 UT on October 1, was associated with the EUV wave and coronal dimming. The bulk of the CME mass was in the north-east direction, and the CME had angular width of about 90 degrees and projected speed of 400 km/s (as reported by the CACTus software package). This CME will not arrive at the Earth.
The solar wind speed is slowly decreasing and it is presently about 500 km/s. The interplanetary magnetic field magnitude is stable having value of about 5 nT. Due to the long interval of the negative value of the Bz component of the interplanetary magnetic field and the fast solar wind, active geomagnetic conditions were reported (around 23:40 UT) on October 1. The local station at Dourbes reported K=4, and NOAA reported Kp=4. We expect quiet to unsettled geomagnetic conditions in the coming hours.
Today's estimated international sunspot number (ISN): 008, based on 17 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 081 |
| AK Chambon La Forêt | 037 |
| AK Wingst | 023 |
| Estimated Ap | 025 |
| Estimated international sunspot number | 000 - Based on 23 stations |
| Day | Begin | Max | Конец | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
|---|---|---|---|---|---|---|---|---|---|---|
| Нет | ||||||||||
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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