ARLA/CLUSTER: Fwd: Space Weather

ARLA - Associação de Radioamadores do Litoral Alentejano cs1rla.arla gmail.com
Quarta-Feira, 9 de Janeiro de 2008 - 12:30:23 WET


---------- Forwarded message ----------
From: Salomao Fresco <sal.fresco  gmail.com>
Date: 08/01/2008 21:12
Subject: Space Weather
To: ARLA <cs1rla.arla  gmail.com>

Ler com atenção!

Para quem está nas latitudes médias e elevadas tem sido um festival!
O DXrobot está a emitir avisos diários.

Cumprimentos

Salomão
CT2IRJ


SPACE WEATHER
Current conditions  *Solar wind*
speed: *631.3 *km/sec
density: *0.4 *protons/cm3
explanation <http://spaceweather.com/glossary/solarwinddata.html> | more
data <http://www.sec.noaa.gov/ace/MAG_SWEPAM_24h.html>
Updated: Today at 2055 UT   *X-ray Solar Flares*
6-hr max: *A0 *1910 UT Jan08
24-hr: *A0 *1910 UT Jan08
explanation <http://spaceweather.com/glossary/flareclasses.html> |
more data<http://www.sec.noaa.gov/rt_plots/xray_5m.html>
Updated: Today at: 2055 UT     Daily Sun: 08 Jan 08
<http://www.spaceweather.com/images2008/08jan08/midi512_blank.gif?PHPSESSID=jneoqaqtbvriimcg193k32svj1>
 Decaying
and tiny sunspot 980 is a surprising source of C-class flares. Credit:
SOHO/MDI    *Sunspot number: 14 *
What is the sunspot number?
<http://spaceweather.com/glossary/sunspotnumber.html>Updated 05 Jan 2008
<http://spaceweather.com/glossary/sunspotnumber.html>    Far side of the
Sun:
<http://www.spaceweather.com/images2008/06jan07/midi_farside_blank.gif?PHPSESSID=jneoqaqtbvriimcg193k32svj1>
 This
holographic image <http://spaceweather.com/glossary/farside.html> reveals no
large sunspots on the far side of the sun. Image credit: SOHO/MDI    *Planetary
K-index*
Now: *Kp= 4 *unsettled
24-hr max: *Kp= 4 *unsettled
explanation <http://www.spaceweather.com/glossary/kp.html> | more data
<http://www.sec.noaa.gov/rt_plots/kp_3d.html>    Current Auroral Oval:
<http://www.sec.noaa.gov/pmap/gif/pmapN.gif>
  Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
Updated:
What is the auroral
oval?<http://www.northern-lights.no/english/what/oval.shtml>
*Interplanetary Mag. Field*
Btotal: *4.9 *nT
Bz: *4.4 *nT *south *
explanation <http://spaceweather.com/glossary/imf.html> | more
data<http://www.sec.noaa.gov/ace/MAG_24h.html>
Updated: Today at 2056 UT   Coronal Holes:
<http://www.spaceweather.com/images2008/08jan08/coronalhole_hinode_blank.jpg?PHPSESSID=jneoqaqtbvriimcg193k32svj1>
 Earth
is inside a solar wind stream flowing from the indicated coronal hole.
Credit: SOHO Extreme UV Telescope      SPACE WEATHER
NOAA Forecasts
    Updated at: 2008 Jan 07 2203 UTC     FLARE
 0-24 hr
 24-48 hr
 CLASS M
 05 %
 05 %
 CLASS X
 01 %
 01 %
    Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are
given for three activity levels:
active<http://spaceweather.com/glossary/geostorm.html>,
minor storm <http://spaceweather.com/glossary/geostorm.html>, severe
storm<http://spaceweather.com/glossary/geostorm.html>  Updated
at: 2008 Jan 07 2203 UTC   Mid-latitudes
 0-24 hr
 24-48 hr
 ACTIVE
 30 %
 25 %
 MINOR
 15 %
 10 %
 SEVERE
 01 %
 01 %
  High latitudes
 0-24 hr
 24-48 hr
 ACTIVE
 35 %
 25 %
 MINOR
 15 %
 10 %
 SEVERE
 10 %
 05 %

-- 
Cumprimentos

Salomão Fresco
CT2IRJ

_________________________________________________________
If it works... dont fix it!


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