martedì 27 febbraio 2018

Propagation outlook from Boulder

:Product: Weekly Highlights and Forecasts
:Issued: 2018 Feb 26 0308 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact on the Web
# http://www.swpc.noaa.gov/weekly.html
#
#                Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity 19 - 25 February 2018

Solar activity was very low throughout the summary period. No active
regions were observed on the visible disk. No Earth-directed CMEs
were observed in available coronagraph imagery.

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit reached
high levels from 19-26 Feb. A peak flux of 13,500 pfu was observed
on 19/2030 UTC.

Geomagnetic field activity ranged from quiet to G1 (Minor) storm
levels due to multiple negative coronal hole onsets. Quiet to G1
(Minor) storm levels on 19 Feb were associated with peak wind speeds
of just about 550 km/s from a negative polarity CH HSS. The
geomagnetic response declined along with solar wind speeds with
quiet to unsettled conditions observed on 20 Feb and quiet levels on
21 Feb . A subsequent enhancement in solar wind speeds from another
negative polarity CH HSS increased geomagnetic field activity to
quiet to active levels on 22 Feb, and further to quiet to G1 (minor)
storm levels on 23 Feb, which were also associated with peak wind
speeds around 550 km/s. Activity dropped to quiet to unsettled on 24
Feb and completely quiet by 25 Feb as effects from the CH HSS waned.

FORECAST OF SOLAR AND GEOMAGNETIC ACTIVITY 26 FEBRUARY - 24 MARCH 2018

Solar activity is expected to be very low throughout 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 high levels on 26-28 Feb and 18-24 Mar due to
elevated wind speeds from multiple coronal holes. Moderate levels
are anticipated on 15 Mar and the remainder of the forecast period
is expected to be at normal levels.

Geomagnetic field activity is expected to reach G1 (Minor)
geomagnetic storm levels on 26 Feb and 18 Mar. Active levels are
expected on 14 Mar, 16-17 Mar, 21 Mar and 22 Mar. Unsettled levels
are expected on 27 Feb, 15 Mar, and 23-24 Mar. Quiet conditions are
expected for the remainder of the forecast period. All elevations in
geomagnetic activity are anticipated due to multiple, recurrent CH
HSSs.

:Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2018 Feb 26 0308 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact on the Web
# http://www.swpc.noaa.gov/wwire.html
#
#      27-day Space Weather Outlook Table
#                Issued 2018-02-26
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2018 Feb 26      68          24          5
2018 Feb 27      68          12          3
2018 Feb 28      70           5          2
2018 Mar 01      75           5          2
2018 Mar 02      78           5          2
2018 Mar 03      78           5          2
2018 Mar 04      78           5          2
2018 Mar 05      78           5          2
2018 Mar 06      78           5          2
2018 Mar 07      78           5          2
2018 Mar 08      78           5          2
2018 Mar 09      78           5          2
2018 Mar 10      78           5          2
2018 Mar 11      78           5          2
2018 Mar 12      78           5          2
2018 Mar 13      75           5          2
2018 Mar 14      72          10          4
2018 Mar 15      70           8          3
2018 Mar 16      68          12          4
2018 Mar 17      68          15          4
2018 Mar 18      68          18          5
2018 Mar 19      68           5          2
2018 Mar 20      68           5          2
2018 Mar 21      68          12          4
2018 Mar 22      68          15          4
2018 Mar 23      68          10          3
2018 Mar 24      68           8          3
(SWPC via DXLD)