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It may seem, at first, a bit surprising that a section on Space Weather is included on a weather site. However, weather is not limited to planetary bodies. A star's corona is constantly being lost to space, creating what is essentially a very thin atmosphere throughout the Solar System. The movement of mass ejected from the Sun is known as the solar wind. Inconsistencies in this wind and larger events on the surface of the star, such as coronal mass ejections, form a system that has features analogous to conventional weather systems (such as pressure and wind) and is generally known as space weather. Coronal mass ejections have been tracked as far out in the solar system as Saturn. The activity of this system can affect planetary atmospheres and occasionally surfaces. The interaction of the solar wind with the terrestrial atmosphere can produce spectacular aurorae and can play havoc with electrically sensitive systems such as electricity grids and radio signals. Recently I watched a rather scary documentary titled "Cosmic Fire" which described, among other things, the effects that a massive solar storm can have on the earth, its technology and the weather. I invite you to look up the "Carrington Effect" |
Solar Activity Forecast:
Solar activity is expected to be low.
Geophysical Activity Forecast:
The geomagnetic field is expected to be quiet for the next 36 hours. An increase to unsettled levels is expected mid-day on 23 February and continuing through 24 February due to a coronal hole high speed stream.
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SOHO EIT 304 |
SOHO EIT 284 |
Mauna Loa Solar Image |
The sun is constantly monitored for sun spots and coronal mass ejections. EIT (Extreme ultraviolet Imaging Telescope) images the solar atmosphere at several wavelengths, and therefore, shows solar material at different temperatures. In the images taken at 304 Angstrom the bright material is at 60,000 to 80,000 degrees Kelvin. In those taken at 171 Angstrom, at 1 million degrees. 195 Angstrom images correspond to about 1.5 million Kelvin, 284 Angstrom to 2 million degrees. The hotter the temperature, the higher you look in the solar atmosphere.
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Solar Cycle Progression Solar Cycle chart updated using the latest ISES predictions. |
Real-Time Solar Wind Real-Time Solar Wind data broadcast from NASA's ACE satellite. |
The Solar Cycle is observed by counting the frequency and placement of sunspots visible on the Sun. Solar minimum occurred in December, 2008. Solar maximum is expected to occur in May, 2013.
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Solar X-ray Flux This plot shows 3-days of 5-minute solar x-ray flux values measured on the SWPC primary and secondary GOES satellites. |
Satellite Environment Plot The Satellite Environment Plot combines satellite and ground-based data to provide an overview of the current geosynchronous satellite environment. |
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Northern Hemi Auroral Map |
Southern Hemi Auroral Map |
Instruments on board the NOAA Polar-orbiting Operational Environmental Satellite (POES) continually monitor the power flux carried by the protons and electrons that produce aurora in the atmosphere. SWPC has developed a technique that uses the power flux observations obtained during a single pass of the satellite over a polar region (which takes about 25 minutes) to estimate the total power deposited in an entire polar region by these auroral particles. The power input estimate is converted to an auroral activity index that ranges from 1 to 10.
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