lunedì 14 gennaio 2019

Propagation outlook from Boulder

Space Weather Prediction Center
National Oceanic and Atmospheric Administration

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:Product: Weekly Highlights and Forecasts
:Issued: 2019 Jan 14 0403 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact on the Web
# https://www.swpc.noaa.gov/content/subscription-services
#
#                Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity
07 - 13 January 2019

Solar activity was very low. The solar disk was spotless during the
reporting period. No Earth-directed CMEs were observed.

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit reached
high levels on 07-10 Jan and moderate levels on 11-13 Jan. The peak
flux was 2,970 pfu observed at 07/2040 UTC.

Geomagnetic field activity ranged from quiet to active levels. Solar
wind parameters began the period under waning negative polarity
coronal hole high speed stream (CH HSS) effects. Solar wind speed
began the period near 535 km/s, but diminished to near 345 km/s by
10/0720 UTC. Total field remained at 6 nT or less during this time.
The geomagnetic field responded with quiet to unsettled levels on 07
Jan followed by quiet levels on 08-10 Jan. By late on 10 Jan, solar
wind speed once again increased to near 515 km/s by 11/0435 UTC
while total field only increased briefly to a maximum of 8 nT at
11/0635 UTC. The Bz component deflected southward for approximately
3 hours to near -6 nT. The geomagnetic field responded with an
isolated active period on 11 Jan. By 12 and 13 Jan, solar wind speed
had decreased to below 400 km/s. The geomagnetic field was once
again quiet on 12-13 Jan.

Forecast of Solar and Geomagnetic Activity
14 January - 09 February 2019

Solar activity is expected to be at very low levels on 14-19 Jan and
03-09 Feb. A slight chance for C-class flares is expected on 20
Jan-02 Feb due to the return of old Region 2732 (N09, L=215).

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is
expected to reach high levels on 25-27 Jan and 02-06 Feb due to
recurrent CH HSS influence.

Geomagnetic field activity is expected to be at unsettled levels on
15-16 Jan. Unsettled to active levels are expected on 24-26 Jan and
31 Jan - 03 Feb with G1 (Minor) storm levels likely on 24 Jan due to
recurrent CH HSS effects.

:Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2019 Jan 14 0403 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact on the Web
# https://www.swpc.noaa.gov/content/subscription-services
#
#      27-day Space Weather Outlook Table
#                Issued 2019-01-14
#
#   UTC      Radio Flux   Planetary   Largest
#  Date       10.7 cm      A Index    Kp Index
2019 Jan 14      69           5          2
2019 Jan 15      69           8          3
2019 Jan 16      69           8          3
2019 Jan 17      69           5          2
2019 Jan 18      70           5          2
2019 Jan 19      70           5          2
2019 Jan 20      71           5          2
2019 Jan 21      71           5          2
2019 Jan 22      71           5          2
2019 Jan 23      71           5          2
2019 Jan 24      71          20          5
2019 Jan 25      71          12          4
2019 Jan 26      71           8          3
2019 Jan 27      71           5          2
2019 Jan 28      71           5          2
2019 Jan 29      71           5          2
2019 Jan 30      71           5          2
2019 Jan 31      71          10          3
2019 Feb 01      71          15          4
2019 Feb 02      70          12          4
2019 Feb 03      70           8          3
2019 Feb 04      70           5          2
2019 Feb 05      69           5          2
2019 Feb 06      69           5          2
2019 Feb 07      69           5          2
2019 Feb 08      69           5          2
2019 Feb 09      69           5          2
(SWPC via DXLD)