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Home - Indirect solar x-ray Flare Monitoring (InFlaMo)Space Weather ionosphere disturbance monitor physics
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Space Weather ionosphere disturbance monitor physics
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Home - Indirect solar x-ray Flare Monitoring (InFlaMo) | src.danielides.eu Reviews
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Space Weather ionosphere disturbance monitor physics
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Scientific Background - Indirect solar x-ray Flare Monitoring (InFlaMo)
http://src.danielides.eu/scientific-background.html
When a solar flare. Occurs on Sun (picture beside is taken by the GOES 14 satellite on October 8th, 2012 around noon UTC) a blast of intense ultraviolet. Hits the dayside of the Earth after a propagation time of about 8 minutes. This high energy radiation is absorbed by atmospheric particles. Raising them to excited states and knocking electrons free in the process of photoionization. The low altitude ionospheric layers. Are recorded and indicate when solar x-ray flares. And can disturb ionosphere (.
Technical Background - Indirect solar x-ray Flare Monitoring (InFlaMo)
http://src.danielides.eu/technical-background.html
To monitor effects of the lower ionosphere a simple single frequency. And a suitable antenna is needed. Such a set-up is suitable for especially K-12 projects to demonstrate basic effects. A more complex VLF radio receiver. Is recording a broader spectrum. And can be utilized for advanced studies of the lower ionosphere. For both systems a (passiv) loop antenna or an active antenna system can be utilized. Sinlge frequency (narrow band) VLF receiver. At the InFlaMo project we call this receiver type a.
Home - Indirect solar x-ray Flare Monitoring (InFlaMo)
http://src.danielides.eu/home.html
Welcome to the InFlaMo Network Portal. Project monitors the space weather situation. Via ground based and satellite measurements. From ground it is possible to detect sudden ionospheric disturbances (SID). Which are also called. Mögel–Dellinger effect. SID is caused by solar x-ray radiation at ionospheric hights and coinside with the appearance of solar x-ray flares. Around 1935 and also described by the German physicist. Non-statistacally) one can detect solar x-ray flares. View onto Sun. This is ar...
Products - Indirect solar x-ray Flare Monitoring (InFlaMo)
http://src.danielides.eu/inflamo-products.html
SID and GOES x-ray plots and data. The InFlaMo project is currently in its start-up phase. So far there is no ready archive or data search function available. Each SID station may link to an own website for representing of their own data. Some SID stations are not yet operating own websites and data are only on demand available. For hourly updated VLF data from Station. SID monitor at 24.00 kHz from Station SWMS DE17139a. Is available on demand. A SuperSID monitor at Moscow / Russian Federation.
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Home - Indirect solar x-ray Flare Monitoring (InFlaMo)
Welcome to the InFlaMo Network Portal. Project monitors the space weather situation. Via ground based and satellite measurements. From ground it is possible to detect sudden ionospheric disturbances (SID). Which are also called. Mögel–Dellinger effect. SID is caused by solar x-ray radiation at ionospheric hights and coinside with the appearance of solar x-ray flares. Around 1935 and also described by the German physicist. Non-statistacally) one can detect solar x-ray flares. View onto Sun. This is ar...
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