Here is the current forecast discussion on space weather and geophysical activity, issued 2016 Jan 30 1230 UTC.
Solar Activity
24 hr Summary: Solar activity remained at low levels. Region 2488 (N04W76, Cao/beta) produced an impulsive C1/Sf flare at 29/1641 UTC. The region continued to show signs of decay and magnetic simplification as it approached the west limb. Region 2489 (N10W08, Dho/beta) indicated some penumbral decay within its trailer spots and was quiet during the period.
An eruption along a filament channel, located near the SW limb, occurred at approximately 29/2100 UTC as viewed in SDO/AIA 193 and 304 imagery.
Associated with this eruption was a long duration C2 x-ray event which began at 29/2048 UTC, reached a maximum at 29/2146 UTC and ended at 29/2257 UTC. SOHO/LASCO C2 and C3 imagery observed a coronal mass ejection (CME) off the SW limb, first visible at 29/2117 UTC and 29/2154 UTC, respectively. Initial analysis, and subsequent WSA-Enlil model output, suggests the CME does not have an Earth-directed component.
However, further analysis will be conducted as additional coronagraph imagery becomes available. No other CMEs were visible in available coronagraph imagery.
Forecast: Solar activity is expected to be low with a slight chance for M-class (R1-R2 (Minor-Moderate) Radio Blackouts) over the next three days (30 Jan - 01 Feb).
Energetic Particle
24 hr Summary: The greater than 2 MeV electron flux was at normal levels and the greater than 10 MeV proton flux was at background levels throughout the period.
Forecast: The greater than 2 MeV electron flux is expected to be at normal to moderate levels over the next three days (30 Jan - 01 Feb) and the greater than 10 MeV proton flux is expected to remain at background levels throughout the forecast period.
Solar Wind
24 hr Summary: Solar wind parameters were at background levels throughout the period.
Solar wind speeds slowly decreased from initial values near 310 km/s to end-of-period values approaching 270 km/s. IMF total field strength (Bt) values ranged between 2-5 nT while the Bz component reached a maximum southward value of -3 nT between about 29/1600-1820 UTC. The phi angle remained steady in a positive (away) solar sector orientation.
Forecast: Solar wind parameters are expected to remain at background levels throughout the forecast period (30 Jan - 01 Feb) under a nominal solar wind regime.
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 over the next three days (30 Jan - 01 Feb) under a nominal solar wind regime.
Don't forget to visit our live space weather and radio propagation web site, at: http://SunSpotWatch.com/
Live Aurora mapping is at http://aurora.sunspotwatch.com/
If you are on Twitter, please follow these two users:
+ https://Twitter.com/NW7US
+ https://Twitter.com/hfradiospacewx
Get the space weather and radio propagation self-study course, today. Visit http://nw7us.us/swc for the latest sale and for more information!
Check out the stunning view of our Sun in action, as seen during the last five years with the Solar Dynamics Observatory (SDO): https://www.youtube.com/watch?v=zXN-MdoGM9g
We're on Facebook: http://NW7US.us/swhfr
Live data: SunSpotWatch.com
|