To: | "Thomas Giella KN4LF" <kn4lf@tampabay.rr.com> |
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Subject: | [Propagation] KN4LF Prop Comments/SIDC Belgium Daily Solar & GeoReport |
From: | "Thomas Giella KN4LF" <kn4lf@tampabay.rr.com> |
Date: | Sat, 1 Jan 2005 11:18:32 -0500 |
List-post: | <mailto:propagation@contesting.com> |
Per my forecast outlook #2005-001 issued on Friday 12/31/04 sunspot group
number 10175 is now producing huge X class solar flares. It has also
produced 4 large M class solar flares and 5 coronal mass ejections.
Fortunately so far none of the CME's are totally geoeffective (Earth Facing)
but could still cause active Kp-4 to minor Kp-5 geomagnetic storming in 2-3
days. This group should make for some interesting solar, space weather and geomagnetic conditions this first week of 2005! 73, Thomas Giella, KN4LF Plant City, FL ----- :Issued: 2005 Jan 01 1224 UTC :Product: documentation at http://sidc.oma.be/products/meu #------------------------------------------------------------------------------# # DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC (RWC-Belgium) # #------------------------------------------------------------------------------# SIDC URSIGRAM 50101 SIDC SOLAR BULLETIN 01 Jan 2005, 1143UT SIDC FORECAST (valid from 1230UT, 01 Jan 2005 until 03 Jan 2005) SOLAR FLARES : Active (M-class flares expected, probability >= 50%) GEOMAGNETISM : Active conditions expected (A>=20 or K=4) SOLAR PROTONS : Quiet PREDICTIONS FOR 01 Jan 2005 10CM FLUX: 101 / AP: 014 PREDICTIONS FOR 02 Jan 2005 10CM FLUX: 101 / AP: 022 PREDICTIONS FOR 03 Jan 2005 10CM FLUX: 102 / AP: 034 COMMENT: Catania sunspot group 98 (NOAA 0715) again produced 2 major flares in the past 24 hours. Yesterday afternoon it was responsible for an M1.2 flare. Early in the UT day it generated an X1.7 flare, its largest event up till now and surprising in view of the relatively limited size of the sunspot group. No LASCO images are available so far, but EIT images clearly show that both of these major flares were accompanied by EIT waves and coronal dimmings. Thus, CMEs were generated, which are most likely at least partial halo events. Shock fronts from these CMEs may reach the earth during the next few days, but in the absence of reliable speed estimates we cannot provide estimates of the arrival times. We expect further M-class flares from Catania sunspot group 98, with a small chance for another X-flare. The group is also likely to generate more CMEs with an increasing probability of geo-effectiveness. SOLAR INDICES FOR 31 Dec 2004 SUNSPOT INDEX : 037 10CM SOLAR FLUX : 099 AK CHAMBON LA FORET : 017 AK WINGST : /// ESTIMATED AP : 011 NOTICEABLE EVENTS SUMMARY DAY BEGIN MAX END LOC XRAY OP 10CM RADIO BURST TYPES Catania NOAA NOTE 31 1438 1445 1448 N04E38 M1.2 36 III/2 98 0715 SXI-derived location 01 0001 0031 0039 N06E34 X1.7 760 CTM/1,II/2,IV/2,III/2 98 0715 SXI-derived location ----- Joint USAF/NOAA Report of Solar and Geophysical Activity SDF Number 366 Issued at 2200Z on 31 Dec 2004 IA. Analysis of Solar Active Regions and Activity from 30/2100Z to 31/2100Z: Solar activity was at moderate levels today. Region 715 (N04E34) produced an M4/2n event that occurred at 30/2218Z along with an associated Tenflare (230 sfu), a Type IV spectral radio sweep, and a Type II spectral radio sweep with an estimated shock velocity of 1378 km/s. A related CME was observed on LASCO imagery which appears to have a slight Earth directed component. A more recent M1 x-ray flare occurred at 31/1445Z from this region, and due to insufficient data, it is uncertain whether this flare produced a CME. White light analysis has shown a decay in sunspot area over the period although a small delta magnetic structure can be seen in the southern most cluster of the penumbral spots. The remainder of the disk/limbs were quiescent today. A new region was numbered today as Region 717 (N07W56). IB. Solar Activity Forecast: Solar activity is expected to be at low to moderate levels. Region 715 remains capable of producing M-class flare activity. IIA. Geophysical Activity Summary 30/2100Z to 31/2100Z: The geomagnetic field was at quiet to unsettled levels today. IIB. Geophysical Activity Forecast: The geomagnetic field is expected to be at quiet to unsettled levels through day one (1 Jan) of the period. A recurrent high speed coronal hole stream and the CME's that occurred yesterday in response to the M2/Sf event and the M4/2n event that occurred today should induce active to minor storm conditions on days two and three (2-3 Jan). III. Event Probabilities 01 Jan-03 Jan Class M 60/50/50 Class X 10/10/10 Proton 05/05/05 PCAF green IV. Penticton 10.7 cm Flux Observed 31 Dec 099 Predicted 01 Jan-03 Jan 100/100/095 90 Day Mean 31 Dec 105 V. Geomagnetic A Indices Observed Afr/Ap 30 Dec 012/015 Estimated Afr/Ap 31 Dec 008/009 Predicted Afr/Ap 01 Jan-03 Jan 008/012-015/020-015/015 VI. Geomagnetic Activity Probabilities 01 Jan-03 Jan A. Middle Latitudes Active 20/35/35 Minor storm 01/15/15 Major-severe storm 01/05/05 B. High Latitudes Active 25/40/35 Minor storm 05/20/15 Major-severe storm 01/10/05 73, 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 Propagation eReflector: http://lists.contesting.com/mailman/listinfo/propagation KN4LF Daily Solar Space Weather & Geomagnetic Data Archive: http://www.kn4lf.com/kn4lf5.htm KN4LF Daily LF/MF/HF Radio Propagation Outlook: http://www.kn4lf.com/kn4lf6.htm KN4LF HF/MF Radio Propagation Theory Notes: http://www.kn4lf.com/kn4lf8.htm KN4LF Amateur & SWL Radio History: http://www.kn4lf.com/index.htm
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