Tellina HF Path Propagation

Point-to-point HF path estimate using NOAA space-weather data, location path, mode, power, antenna and noise presets.
This is not the real VOACAP engine. It is a practical VOACAP-lite estimate for ham-radio use.

From location

City

Latitude

Longitude

To location

Leave To city empty for global / single-location forecast.

City

Latitude

Longitude

Station settings

Mode

Power

TX antenna

RX antenna

Noise

Path

Forecast time

Time is UTC. Changing date or hour updates the page automatically.

Path information

From location: Amsterdam, Netherlands — 52.4° N, 4.9° E
To location: Leave To city empty for global / single-location forecast.
Midpoint: 52.4° N, 4.9° E

Space-weather conditions

Solar flux F10.7 128.0

Kp 0.7

X-ray level B5.9

Solar wind 352 km/s

Estimated MUF 20.4 MHz

Bz: 0.5 nT

Kp forecast: 18:00–21:00 UTC

Hourly path/band forecast — 2026-06-22 UTC

Band	Frequency	00	01	02	03	04	05	06	07	08	09	10	11	12	13	14	15	16	17	18	19	20	21	22	23
160m	1.85 MHz	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	- 38%	- 38%	++ 88%	++ 88%	++ 88%	++ 88%
80m	3.65 MHz	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	- 38%	- 38%	++ 88%	++ 88%	++ 88%	++ 88%
60m	5.35 MHz	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	+ 75%	+ 75%	++ 90%	++ 90%	++ 90%	++ 90%
40m	7.10 MHz	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	+ 84%	+ 84%	++ 99%	++ 99%	++ 99%	++ 99%
30m	10.12 MHz	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	++ 94%	++ 94%	+ 79%	+ 79%	+ 79%	+ 79%
20m	14.20 MHz	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	++ 94%	++ 94%	+ 79%	+ 79%	+ 79%	+ 79%
17m	18.10 MHz	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	++ 92%	++ 92%	~ 49%	~ 49%	~ 49%	~ 49%
15m	21.20 MHz	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	~ 59%	~ 59%	! 16%	! 16%	! 16%	! 16%
12m	24.95 MHz	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	- 34%	- 34%	! 4%	! 4%	! 4%	! 4%
10m	28.40 MHz	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	-	! 0%	! 0%	! 0%	! 0%	! 0%	! 0%

Legend: ++ Excellent + Good ~ Fair - Poor ! Bad - No data

How to read this

This page estimates hourly HF path quality between two locations.
It uses distance, midpoint, day/night at the path midpoint, mode, power, antenna presets, receiver noise, Kp, solar flux and X-ray level.
Higher solar flux usually helps higher HF bands such as 15m, 12m and 10m.
High Kp can disturb polar and high-latitude paths.
Lower bands are usually better at night; higher bands usually need daylight and enough solar flux.
For a true VOACAP prediction, run the VOACAP engine with exact antennas, noise, SSN, power and circuit parameters.