Випущено: 2018 Nov 01 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
01 Nov 2018 | 068 | 008 |
02 Nov 2018 | 068 | 003 |
03 Nov 2018 | 068 | 024 |
Solar activity was at very low levels. No sunspot regions were observed on the visible solar disk. No earth-directed coronal mass ejections (CMEs) were observed over the last 24 hours. The greater than 10 MeV proton flux was at nominal values. A positive polarity equatorial coronal hole is transiting the Central Meridian.
Solar activity is expected to remain at very low levels.
Solar wind speed showed a slightly increasing trend and varied between 320 and 360 km/s (DSCOVR). Bz ranged between -5 and +4 nT, with a mostly negative stretch near -4 nT from 04-07UT. The direction of the interplanetary magnetic field (phi angle) was mostly away from the Sun (positive sector), with negative sectors from 00:30-04:30UT and from 06-08UT, and variable after 08UT. Quiet geomagnetic conditions were observed with an unsettled episode in K Dourbes during the 06-11UT interval.
Quiet to unsettled geomagnetic conditions are expected until the arrival of the co-rotating interaction region and the high speed wind stream associated with the positive polarity CH. Based on STEREO-A data, this arrival is expected for 3 November, with wind speeds possibly up to 650 km/s and Bz around -10 nT. Geomagnetic conditions may then reach minor storm levels, a moderate storming episode not excluded.
Today's estimated international sunspot number (ISN): 000, based on 10 stations.
Wolf number Catania | /// |
10cm solar flux | 068 |
AK Chambon La Forêt | 009 |
AK Wingst | 005 |
Estimated Ap | 004 |
Estimated international sunspot number | /// - Based on /// stations |
Day | Begin | Max | Кінець | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Немає |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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