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Space Weather Guide


   What is space weather?
    Most of the time space, weather is of little concern in our everyday lives. However, when the space environment is disturbed by the variable output of particles and radiation from the Sun, technologies that we depend on in our daily life, in space orbit as well as on the ground, can be affected. Some of the most dramatic space weather effects occur in association with eruptions of material from the solar atmosphere into interplanetary space. Thus, our space weather is a consequence of the behavior of the Sun, the nature of Earth's magnetic field and atmosphere, and our location in the solar system. The increasing deployment of radiation -current- and field sensitive technological systems over the last few decades and the increasing presence of complex systems in space combine to make society more vulnerable to solar-terrestrial disturbances. This has been emphasized by the large number of problems associated with the severe magnetic storms between 1989 and 1991 as the 11 year solar activity cycle peaked.

SOHO Real-time View of the Sun

  Space Weather Outlook

    
     Summary For January 25-31
    No space weather storms were observed.
     
     
    Outlook For February 3-9
    No space weather storms are expected.
     
     
     
     For current space weather conditions see: 
    Space Weather Now, 
    Today's Space Weather and 
    Space Weather Alerts  
    
    
    
  Joint USAF/NOAA Report of Solar and Geophysical Activity 8 Feb 2010
    :Product: Report of Solar-Geophysical Activity
    :Issued: 2010 Feb 08 2208 UTC
    # Prepared jointly by the U.S. Dept. of Commerce, NOAA,
    # Space Weather Prediction Center and the U.S. Air Force.
    #
    Joint USAF/NOAA Report of Solar and Geophysical Activity
    :::::::::: CORRECTED COPY ::::::::::
    SDF Number 039 Issued at 2200Z on 08 Feb 2010
    IA. Analysis of Solar Active Regions and Activity from 07/2100Z
    to 08/2100Z: Solar activity was moderate. Region 1045 (N23W17)
    produced three M-class events in the last 24 hours. STEREO and
    SOHO/LASCO imagery observed CME activity with each of the three
    events. The largest event was a M4 at 08/0743Z with an associated
    Tenflare of 150 sfu. This region has continued to grow in both
    white light area coverage and sunspot count and is a magnetic
    beta-gamma-delta configuration. There were two additional Tenflares
    observed during the period (both associated with Region 1045
    events), a C7/Sf at 08/0415Z with a 100 sfu Tenflare, and a C8/1f at
    08/0523Z with a 100 sfu Tenflare. A new region was numbered today
    as Region 1047 (S15E70).
    IB. Solar Activity Forecast: Solar activity is expected to be
    moderate with M-class flares likely. There is a slight chance for a
    X-class event from Region 1045.
    IIA. Geophysical Activity Summary 07/2100Z to 08/2100Z:
    The geomagnetic field was quiet. One unsettled period at
    mid-latitudes was reported at 08/1600Z.
    IIB. Geophysical Activity Forecast: The geomagnetic field is
    expected to be predominantly unsettled with isolated active
    conditions for the next three days (09-11 February). These
    conditions are forecast due to the recent CME activity.
    III. Event Probabilities 09 Feb-11 Feb
    Class M 70/70/70
    Class X 15/15/15
    Proton 05/05/05
    PCAF green
    IV. Penticton 10.7 cm Flux
    Observed 08 Feb 094
    Predicted 09 Feb-11 Feb 096/096/094
    90 Day Mean 08 Feb 078
    V. Geomagnetic A Indices
    Observed Afr/Ap 07 Feb 002/003
    Estimated Afr/Ap 08 Feb 003/005
    Predicted Afr/Ap 09 Feb-11 Feb 008/008-008/009-010/010
    VI. Geomagnetic Activity Probabilities 09 Feb-11 Feb
    A. Middle Latitudes
    Active 25/25/25
    Minor storm 05/05/05
    Major-severe storm 01/01/01
    B. High Latitudes
    Active 30/30/35
    Minor storm 05/05/10
    Major-severe storm 02/01/05
NOAA/SEC Satellite Environment
GOES X-Ray Flux

Dst Geomagnetic Index Estimate
Auroral Activity Extrapolated from NOAA POES

Low: Dst > -20 nT
Medium: -20 nT > Dst > -50 nT
High: High: -50 nT > Dst > -100 nT
Extreme: Dst < -100 nT

SOHO CELIAS/MTOF Proton Monitor
ACE Solar Wind Real-Time Data



Note: Images and text on this page are provided by NASA/ESA SOHO website. Space Weather Today from NOAA's Space Environment Center.


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