Here is the current forecast discussion on space weather and geophysical activity, issued 2017 Apr 29 1230 UTC.
Solar Activity
24 hr Summary: Solar activity was at very low levels. Region 2654 (N11E45, Axx/alpha) exhibited minor decay while Regions 2651 (N12W67, Hsx/alpha) and 2653 (S09W26, Hsx/alpha) were stable throughout the period. No Earth-directed CMEs were observed in available coronagraph imagery.
Forecast: Solar activity is expected to remain at very low levels throughout the forecast period (29 Apr-01 May).
Energetic Particle
24 hr Summary: The greater than 2 MeV electron flux reached very high levels this period with a peak flux of 56,297 pfu observed at 28/1645 UTC. The greater than 10 MeV proton flux was steady at background levels.
Forecast: The greater than 2 MeV electron flux is expected to continue at high to very high levels on day one (29 Apr) with high levels likely on days two and three (30 Apr-01 May). The greater than 10 MeV proton flux is expected to continue at background levels throughout the forecast period.
Solar Wind
24 hr Summary: Solar wind parameters reflected a nominal solar wind environment. Solar wind speeds were steady between 375-400 km/s with a period of anomalous, non-physical values reported between 28/1725-1900 UTC. Total field strength values were between 5-7 nT and the southward component of the magnetic field ranged between +4/-6 nT. The phi angle was steady in a negative (toward) solar sector orientation.
Forecast: Solar wind parameters are expected to remain at nominal levels on day one through the majority of day two (29-30 Apr). By late on day two, a solar sector boundary crossing (SSBC) into a positive (away) sector is expected followed by the weak influence of a positive polarity CH HSS. Enhanced solar wind parameters are expected to persist into day three (01 May).
Geospace
24 hr Summary: The geomagnetic field was quiet throughout the period under a background solar wind environment.
Forecast: The geomagnetic field is expected to continue at quiet levels on day one (29 Apr). Isolated unsettled activity is likely on day two (30 Apr) due to a solar sector boundary crossing (negative to positive) and isolated active conditions are likely on day three (01 May) due to the weak influence of a positive polarity CH HSS.
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