Vydáno: 2019 Feb 04 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
04 Feb 2019 | 071 | 003 |
05 Feb 2019 | 070 | 004 |
06 Feb 2019 | 069 | 004 |
The solar activity has been quiet over the past 24 hours. The visible solar disc was spotless, and the X-ray flux remained below B-level. Flaring conditions is expected to remain at low levels.
No Earth directed coronal mass ejection has been observed. The greater than 10 MeV solar protons flux remained at nominal levels over the past 24 hours and is expected to remain so.
The Earth is still inside the influence of the speed stream associated with negative polarity coronal hole that had reached the central meridian last week. The solar wind speed decreased from about 568 km/s to 410 km/s over the past 24 hours, and the interplanetary magnetic fields remained below 5 nT. The solar wind parameters are expected to globally return towards an ambient background and slow solar wind speed regime.
The geomagnetic conditions were mostly quiet and ranged between Kp index 0-3 (NOAA) and local K index 0-2 (Dourbes) over the past 24 hours. They are expected to remain mostly quiet, unsettled conditions periods remain likely to happen as the solar wind speed is still elevated (due to the extended and patchy shape of the coronal hole).
Today's estimated international sunspot number (ISN): 000, based on 13 stations.
Wolf number Catania | /// |
10cm solar flux | 071 |
AK Chambon La Forêt | 013 |
AK Wingst | 012 |
Estimated Ap | 011 |
Estimated international sunspot number | 000 - Based on 27 stations |
Day | Begin | Max | Konec | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Žádný |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
Všechny časy v UTC
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