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[Propagation+Space Weather] Weekly Propagation Summary - 2015 Sep 07 16:

To: propagation@contesting.com
Subject: [Propagation+Space Weather] Weekly Propagation Summary - 2015 Sep 07 16:10 UTC
From: nw7us@sunspotwatch.com
Reply-to: Practical radio-wave propagation and space weather <propagation@contesting.com>
Date: Mon, 7 Sep 2015 16:10:14 +0000
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Here is this week's space weather and geophysical report, issued 2015 Sep 07 0436 UTC.

Highlights of Solar and Geomagnetic Activity 31 August - 06 September 2015

Solar activity was at very low to low levels over the period. An isolated C2 flare was observed at 31/0522 UTC from Region 2403 (S15, L=193, class/area Fki/1190 on 25 Aug) and a C1 flare occurred at 03/1137 UTC from Region 2407 (N16, L=145, class/area Cso/050 on 01 Sep). No further notable flaring occurred during the period. On 04 September, an approximate 15 degree filament eruption, centered near S17E10, was observed lifting off in SDO/AIA 304 imagery between 04/1709-1854 UTC. A partial-halo coronal mass ejection (CME) was observed in SOHO/LASCO C2 imagery beginning at 04/1948 UTC with most of the ejecta directed off the SE limb. WSA/ENLIL analysis of the CME determined that an Earth-directed component was not likely.

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was at high levels from 31 August through 02 September and again from 05-06 September reaching a maximum flux value over the period of 3,188 pfu at 05/1840 UTC. Moderate levels occurred on 03-04 September.

Geomagnetic field activity began the period at quiet levels under a nominal solar wind regime. At 02/1522 UTC, a solar sector boundary crossing was observed in ACE solar wind data accompanied by a slow increase in solar wind speed. By late on 03 September, total field increased to around 12-14 nT with the Bz component deflecting southward to -10 nT. Quiet to unsettled levels were observed on 02-03 September. By 04 September, solar wind increased to around 450-550 km/s range as a co-rotating interaction region (CIR) followed by a positive polarity coronal hole high speed stream (CH HSS) became geoeffective. Solar wind speeds remained in the 400-500 km/s range through the rest of the period. The geomagnetic field responded with active to minor storm (G1-Minor) levels through midday on 04 September followed by quiet to active levels on 05-06 September.

Forecast of Solar and Geomagnetic Activity 07 September - 03 October 2015

Solar activity is expected to be at very low to low levels with M-class flares (R1-R2, Minor-Moderate) likely from 11-24 September with the return of old Region 2403 (S15, L=192).

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 from 13-18 September, 20-21 September, 26-28 September and again from 02-03 October due to CH HSS effects.

Geomagnetic field activity is expected to be at unsettled levels from 07-08, 11-16, 18-20, 24-25, and 30 September-03 October. Active periods are expected on 07, 12, 19, 24 September-03 October with minor storm periods (G1-Minor) possible on 19 September and 01 October, all due to recurrent CH HSS effects.

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Weekly Propagation Summary - 2015 Sep 07 16:10 UTC

Live data and images: SunSpotWatch.com

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