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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
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Space Weather Outlook
Joint USAF/NOAA Solar Geophysical Activity Report and Forecast 22 February 2017
Joint USAF/NOAA Solar Geophysical Activity Report and Forecast
SDF Number 53 Issued at 2200Z on 22 Feb 2017
IA. Analysis of Solar Active Regions and Activity from 21/2100Z to 22/2100Z: Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C4 event observed at 22/1327Z from Region 2638 (N19E35). There are currently 1 numbered sunspot regions on the disk.
IB. Solar Activity Forecast: Solar activity is expected to be very low with a chance for a C-class flares on days one, two, and three (23 Feb, 24 Feb, 25 Feb).
IIA. Geophysical Activity Summary 21/2100Z to 22/2100Z: The geomagnetic field has been at quiet to active levels for the past 24 hours. Solar wind speed reached a peak of 469 km/s at 22/0441Z. Total IMF reached 9 nT at 22/1302Z. The maximum southward component of Bz reached -6 nT at 22/1451Z. Electrons greater than 2 MeV at geosynchronous orbit reached a peak level of 719 pfu.
IIB. Geophysical Activity Forecast: The geomagnetic field is expected to be at quiet to minor storm levels on day one (23 Feb), quiet to active levels on day two (24 Feb) and quiet to unsettled levels on day three (25 Feb).
III. Event probabilities 23 Feb-25 Feb
Class M 05/05/05
Class X 01/01/01
Proton 01/01/01
PCAF green
IV. Penticton 10.7 cm Flux
Observed 22 Feb 083
Predicted 23 Feb-25 Feb 084/084/083
90 Day Mean 22 Feb 077
V. Geomagnetic A Indices
Observed Afr/Ap 21 Feb 004/004
Estimated Afr/Ap 22 Feb 010/013
Predicted Afr/Ap 23 Feb-25 Feb 014/020-010/012-007/008
VI. Geomagnetic Activity Probabilities 23 Feb-25 Feb
A. Middle Latitudes
Active 35/30/20
Minor Storm 25/10/05
Major-severe storm 05/01/01
B. High Latitudes
Active 10/15/15
Minor Storm 20/25/25
Major-severe storm 60/40/30
NOAA/SEC Satellite Environment |
GOES X-Ray Flux |
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Dst Geomagnetic Index Estimate |
Auroral Activity Extrapolated from NOAA POES |
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Low: Dst > -20 nTMedium: -20 nT > Dst > -50 nTHigh: High: -50 nT > Dst > -100 nTExtreme: Dst < -100 nT |
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SOHO CELIAS/MTOF Proton Monitor |
ACE Solar Wind Real-Time Data |
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Note: Images and text on this page are provided by NASA/ESA SOHO website.
Space Weather Today from
NOAA's Space Environment Center.