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[Propagation] Fw: SIDC Weekly Bulletin

To: "a Propagation Reflector" <propagation@contesting.com>
Subject: [Propagation] Fw: SIDC Weekly Bulletin
From: "Thomas Giella KN4LF" <kn4lf@tampabay.rr.com>
Date: Mon, 11 Apr 2005 12:54:24 -0400
List-post: <mailto:propagation@contesting.com>
> :Issued: 2005 Apr 11 1649 UTC
> :Product: documentation at http://sidc.oma.be/products/bul
> #--------------------------------------------------------------------#
> # SIDC Weekly bulletin on Solar and Geomagnetic activity             #
> #--------------------------------------------------------------------#
> WEEK 223 from 2005 Apr 04
>
> SOLAR ACTIVITY
> --------------
>
> In the beginning of the week the most of solar activity was produced by 
> the NOAA AR 0747, Catania sunspot group 49. It produced 3 C-flares on 
> April 5 and 6, the strongest one being the C1.6 flare on April 6. On April 
> 9 a new active region (NOAA AR 0751, Catania number 52) has quickly 
> emerged and started to grow rapidly. It produced several strong B-flares, 
> including two B8.2 flares on April 9 and 10.
>
> Two large low-latitude coronal holes were observed in the northern 
> hemisphere. On April 4 the first of them was already approaching the 
> western limb. The western edge of the second coronal hole reached the 
> central meridian on April 8.
>
> GEOMAGNETIC ACTIVITY
> --------------------
>
> On April 4 the interaction region between the fast flow from the first 
> low-latitude coronal hole in the northern hemisphere and slower solar wind 
> stream has arrived. It contained predominantly southward interplanetary 
> magnetic field and thus produced a minor geomagnetic storm. The Kp index 
> from Dourbes reached 5 on April 4, IZMIRAN gives the maximal value of 6 
> (on April 4) and NOAA SEC - 7 (early on April 5). Until April 7 the Earth 
> was situated inside this fast flow. However, the interplanetary magnetic 
> field was quite weak (less than 5 nT) and oscillated around zero. The 
> disturbed geomagnetic conditions were thus finished on April 6. The 
> magnetic field remained weak during the following period of the slow wind 
> flow. The rest of the week was thus quiet as the fast flow from the second 
> coronal hole did not arrive yet.
>
> ---------------------------------------------------------------------------
> DAILY INDICES
> DATE           RC   10CM   Ak   BKG    M   X
> 2005 Apr 04   ///   85   ///   A6.6   0   0
> 2005 Apr 05   ///   88   ///   A7.1   0   0
> 2005 Apr 06   ///   88   ///   A7.8   0   0
> 2005 Apr 07   045   88   ///   A6.9   0   0
> 2005 Apr 08   053   88   ///   A6.1   0   0
> 2005 Apr 09   046   88   ///   A8.5   0   0
> 2005 Apr 10   ///   88   ///   B1.0   0   0
> # RC  : Sunspot index from Catania Observatory (Italy)
> # 10cm: 10.7 cm  radioflux (DRAO, Canada)
> # Ak  : Ak Index Wingst (Germany)
> # BKG : Background GOES X-ray level (NOAA, USA)
> # M,X : Number of X-ray flares in M and X class, see below (NOAA, USA)
> ---------------------------------------------------------------------------
> NOTICEABLE EVENTS
> DAY BEGIN MAX  END  LOC    XRAY OP TENCM TYPE                       Cat 
> NOAA NOTE
>
>
> #--------------------------------------------------------------------#
> # Solar Influences Data analysis Center - RWC Belgium                #
> # Royal Observatory of Belgium                                       #
> # Fax : 32 (0) 2 373 0 224                                           #
> # Tel.: 32 (0) 2 373 0 491                                           #
> #                                                                    #
> # For more information, see http://sidc.oma.be.  Please do not reply #
> # directly to this message, but send comments and suggestions to     #
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> #--------------------------------------------------------------------#

73 & GUD DX,
Thomas F. Giella, KN4LF
Retired Space & Atmospheric Weather Forecaster
Plant City, FL, USA
Grid Square EL87WX
Lat & Long 27 58 33.6397 N 82 09 52.4052 W
kn4lf@arrl.net

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