Here is the current forecast discussion on space weather and geophysical activity, issued 2017 Apr 11 1230 UTC.
Solar Activity
24 hr Summary: Solar activity was at very low levels. Region 2650 (N09E50, Cao/beta) produced a B5/Sf flare at 10/1821 UTC and a B3 flare at 11/0300 UTC. Otherwise flare activity was near background levels. Region 2648 (S03W55) remains a spotless plage region.
The filament eruption from the NE quadrant of the Sun (centered at approximately N16E35) mentioned in the previous discussion was associated with a CME first observed in SOHO/LASCO-C2 imagery at 10/0125 UTC. Forecaster analysis and WSA/Enlil modeling determined a possible glancing blow from the CME, with arrival on 15 April.
Forecast: Solar activity is expected to be very low with a slight chance for C-class activity through the forecast period (11-13 Apr).
Energetic Particle
24 hr Summary: The greater than 2 MeV electron flux was at moderate to high levels with a peak flux of 3,860 pfu observed at 10/1715 UTC. The greater than 10 MeV proton flux remained at background values.
Forecast: The greater than 2 MeV electron flux is expected to be at moderate to high levels all three days (11-13 Apr). No solar radiation storms are expected during the forecast period.
Solar Wind
24 hr Summary: Solar wind parameters were indicative of near background solar wind environment. Solar wind speeds were primarily around 425 km/s. Total field was steady around 5 to 7 nT. Bz was mostly northward for the first half of the period, then became more variable in the latter half, with a maximum southward deflection of -5 nT. Phi angle was negative until near 11/0000 UTC when it switched to a negative sector.
Forecast: A weak connection with an isolated, positive polarity CH HSS is possible during days one and two (11-12 Apr) of the forecast period.
Geospace
24 hr Summary: The geomagnetic field was at mostly quiet levels but reached active levels during the last synoptic period (11/09-12 UTC).
Forecast: Mostly quiet to unsettled conditions are expected for the next two days (11-12 Apr), with isolated active periods, due to the possibility of interfacing with an isolated, positive polarity CH HSS. Quiet conditions are expected to return on day three (13 Apr).
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