UTC | Freq | Call | DXCC | Comment | Spotter |
---|---|---|---|---|---|
22:19 | 10136.0 | MD0CCE | ![]() |
ft8 | CT1FIU |
22:15 | 10136.0 | LA5ITA | ![]() |
FT8 -12dB from JO59 1628Hz | EA2DYB |
22:11 | 10136.0 | VK2LAW | ![]() |
CCC VK2* | IT9STG |
22:10 | 10136.0 | LU7DUE | ![]() |
FT8 -17dB from GF05 852Hz | EA2DYB |
22:09 | 10136.0 | R6OP | ![]() |
FT8 -07dB from KN88 1028Hz | EA2DYB |
22:08 | 10136.0 | AO3100CCI | ![]() |
FT8 +00dB 1556Hz | EA2DYB |
22:05 | 10136.0 | S50XX | ![]() |
FT8 +01dB from JN65 2568Hz | EA2DYB |
22:03 | 10143.0 | ZS8W | ![]() |
811Hz -16db +0.6SEC CQ CQ | JH0BQX |
22:03 | 10136.0 | F4WEJ | ![]() |
FT8 +01dB from JN37 2568Hz | EA2DYB |
22:02 | 10120.0 | EH1DIO | ![]() |
Heavy Metal Music World Day | EA1DD |
22:02 | 10136.0 | G0LLE | ![]() |
FT8 -01dB from JO01 641Hz | EA2DYB |
22:01 | 10143.0 | ZS8W | ![]() |
811Hz 15db +0.6SEC CQ | JH0BQX |
21:54 | 10136.0 | VK3BVP | ![]() |
FT8 -18dB from QF31 1344Hz | EA2DYB |
21:52 | 10136.0 | DL4BG | ![]() |
FT8 -15dB from JO43 1171Hz | EA2DYB |
21:51 | 10116.0 | TM44REF | ![]() |
FY5KE | |
21:49 | 10136.0 | AN3100JT | ![]() |
FT8 +05dB 1723Hz | EA2DYB |
21:47 | 10136.0 | DL9GCW | ![]() |
FT8 +05dB from JN48 2568Hz | EA2DYB |
21:45 | 10116.0 | TM44REF | ![]() |
Merci 73 | F4FCC |
21:45 | 10136.0 | DF5KA | ![]() |
FT8 +04dB from JO33 1834Hz | EA2DYB |
21:43 | 10136.0 | DL6AZ | ![]() |
FT8 -15dB from JO42 2505Hz | EA2DYB |
The DX Cluster is a tool used by radio amateurs to share real-time information about radio links (DX) and active stations in frequency. It is a network of interconnected servers that allows radio operators to post and receive reports (called "spots") on active DX stations in the band, indicating frequency, callsign, mode and other useful information.
A DX Cluster node is a server or access point that offers service to other hams, allowing them to connect via specific software, via packet radio, or via telnet terminal.
Radio operators publish "spots" to report DX stations they have heard or connected to, specifying the frequency and other information.
The spots are shared in real time with all users connected to the DX Cluster's worldwide network.
Radio amateurs and SWLs can use this information to search for new DX stations to connect (or listen to), following the frequency and mode directions.