Here is this week's space weather and geophysical report, issued 2016 Jun 20 0550 UTC.
Highlights of Solar and Geomagnetic Activity
13 - 19 June 2016
Solar activity was at very low levels the majority of the period
with low levels observed on 13 and 19 June due to a C3 flare at
13/0552 UTC from Region 2552 (N15, L=359, class/area Dao/150 on 11
June) and a C1 flare at 19/1158 UTC from Region 2558 (N13, L=215,
class/area Cso/030 on 19 June). The majority of the B-class activity
was caused by Region 2555 (S09, L=274, class/area Cao/080 on 17
June). No Earth-directed coronal mass ejections were observed during
the period.
No proton events were observed at geosynchronous orbit.
The greater than 2 MeV electron flux at geosynchronous orbit was at
normal to moderate levels throughout the period and briefly reached
high levels on 19 June with a maximum flux of 1,030 pfu at 19/1640
UTC.
The geomagnetic field ranged from quiet to G2-Moderate storm levels.
Solar wind conditions began the period under a waning positive
polarity coronal hole high speed stream (CH HSS). Solar wind speeds
decreased from approximately 620 km/s to around 420 km/s by midday
on 14 June. Total field decreased from 8 nT to 4 nT. By late on 14
June, total field increased to 15 nT with the Bz component mostly
southward near -14 nT while solar wind increased to a maximum of 772
km/s at 15/0410 UTC, indicative of a co-rotating interaction region
followed by another positive polarity CH HSS. The geomagnetic field
responded with quiet to active levels on 13 June, quiet to
G2-Moderate storm levels on 14 June and quiet to G1-Minor storm
levels on 15 June. By early on 16 June, total field decreased to
around 6 nT with solar wind speeds in the 500-600 km/s range. These
conditions continued until 19 June when solar wind speeds decreased
to nominal levels. Quiet conditions were observed on 16 and 19 June
with quiet to unsettled levels on 17-18 June.
Forecast of Solar and Geomagnetic Activity
20 June - 16 July 2016
Solar activity is expected to be at very low to low levels for the
forecast period.
No proton events are expected at geosynchronous orbit.
The greater than 2 MeV electron flux at geosynchronous orbit is
expected to be at normal to moderate levels with high levels likely
on 20-22 June, 26 June-01 July, 04-07 July and again on 16 July due
to CH HSS activity.
Geomagnetic field activity is expected to be at unsettled to active
levels from 23-27 June, 02-03 July, 07-12 July and 14-15 July.
G1-Minor storm levels are likely on 02-03 July and 11 July due to
recurrent CH HSS activity.
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 and images: SunSpotWatch.com
|