Radiovibrations.com - > Software - > Shortwave Browser

This site is about the simple offline version of the Shortwave Browser.
If you have internet access please use FMSCAN with better prediction, layout and more options.



Shortwave Database Browser 3.4

updated January 2010

Freeware: Complete Short Wave Frequency Database Tool with



The software will create a time- and day-specific bandscan of any shortwave segment including a signal strength prediction (the dB column):

For example for North Germany, 31.7.2005, no Threshold, 100 sunspots looking like this
(the real application has colours, I just didn't manage to get a coloured screenshot):



with frequency analysis over 24 hours

How to make it work

System requirements

Not much. This should even work on PCs from the early 90ies as it is written in ancient Pascal, still using MSDOS. It runs under Win 3.1, Win98 and WinXP, but has not yet been tested with Windows 7 and Vista. For the graphics, a EGA/VGA-card is required (standard).

Colums:

Some background information about the propagation analysis:
I searched the whole internet for a more-or-less simple algorhythm that calculates the signal strength on shortwave. Unfortunalety there was no free source code. The only thing available were 2 old Basic and Fortran files: Micromuf and Minimuf. They only calculate the lowest and highest usable frequencies. Micromuf even has a bug calculating the LUF - the code I found on various sites was faulty. I tried to solve that problem, after all Minimuf worked better. That was the algorhythm used in the earlier versions of the Shortwave Browser. But it wasn't good enough. So had to develop something on my own.

The propagation analysis works as follows: The initial signal strength is detemined by the transmitter power and the direction into which the transmitter antenna is beaming. Then signal travels in many hops to the receiver. On each hop, the intensity of the E- and F-layer of the ionosphere are determined by the position of the sun and the sunspot number. Each time the distance from signal to sun-in-zenith-point is being taken. This gives a value for the light and darkness. The lighter it is, the higher are the E- and F-MUF (all this can be roughly traced in the details mode). The F-Layer has a 2 hour delay effect because the high bands stay open long after dusk, whereas before dawn they can't be used. Around the equator the F-MUF stays very high until midnight, then it drops fast till sunrise. Around the pole, the F-layer is minimized.

So the length of each hop is determined by the F-intensity, the attenuation by the total number of hops, the frequency and the intensity of the E-layer. If the F-intensity isn't strong enough (F-MUF too low), no reception is possible. If the hop distance is too long and there is only one hop, it will give out the message 'SKP', whereas in the graph the signal is attenuated. Often you can pick up these signals by so-called backscatters, sometimes even quite strong, but usually with echoes becuase of the multi-path reception.

If you like you can adjust the city data (coordinates) in the DAT-file.

This tiny piece of MSDOS software was the basis for the shortwave section of FMSCAN. The online resource has improved algorithms for the prediction and is based on a combination of HFCC, EiBi, TBL and our own AMLIST data. Soon there will be an export function to generate a swdata file out of AMLIST/SWLIST.


Software (c) by Peer-Axel Kroeske DL2LBP.
Freeware and ready to run at any PC with DOS support.

Questions? Corrections? Ideas? Comments?
Mail me: PeerAxel@aol.com

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