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Difference between revisions of "HF Propagation"

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** [https://www.swpc.noaa.gov/communities/radio-communications NOAA Radio Communications Dashboard]
 
** [https://www.swpc.noaa.gov/communities/radio-communications NOAA Radio Communications Dashboard]
 
** [https://www.swpc.noaa.gov/products/real-time-solar-wind NOAA Real Time Solar Wind]
 
** [https://www.swpc.noaa.gov/products/real-time-solar-wind NOAA Real Time Solar Wind]
 +
* [https://www.robkalmeijer.nl/techniek/electronica/radiotechniek/hambladen/qst/1992/11/page80/index.html  Rob's Web - Introduction to Grey Line DXing]
 
* [https://www.qrparci.org/resource/FDIM81.pdf Solar Activity and HF Propagation] '''Note:''' PDF file from QRPARCI
 
* [https://www.qrparci.org/resource/FDIM81.pdf Solar Activity and HF Propagation] '''Note:''' PDF file from QRPARCI
 
* [https://sdo.gsfc.nasa.gov/ Solar Dynamics Observatory]
 
* [https://sdo.gsfc.nasa.gov/ Solar Dynamics Observatory]

Revision as of 16:42, 21 July 2021

Radio and TV signals aren't always limited to traveling line of sight distances. On HF this is commonly caused by refraction (bending) of the signal at the upper layers of the atmosphere known as the ionosphere. On frequencies higher than this, while solar activity plays a role, Earth based weather events are the most common cause of propagation. These links explore several sites, and software, that can be used to help predict how a HF signal will propagate. For propagation topics above 30 Mhz, please see our DXing Above 30 Mhz article.


Links and Online Maps

Links
Online Maps

Software

Technical