UTC | Freq | Call | DXCC | Comment | Spotter |
---|---|---|---|---|---|
22:10 | 10136.0 | LU7DUE | ![]() |
FT8 -17dB from GF05 852Hz | EA2DYB |
22:10 | 3573.0 | RX6AOB | ![]() |
FT8 IM99sm -> KN94ws | EB5BZM |
22:10 | 50313.0 | PY5XT | ![]() |
FT8 -13 dB 1820Hz 2nd | WW1L |
22:09 | 10136.0 | R6OP | ![]() |
FT8 -07dB from KN88 1028Hz | EA2DYB |
22:08 | 10136.0 | AO3100CCI | ![]() |
FT8 +00dB 1556Hz | EA2DYB |
22:07 | 50313.0 | VA2WA | ![]() |
FT8 -10 dB 1664 Hz | PY5CC |
22:05 | 10136.0 | S50XX | ![]() |
FT8 +01dB from JN65 2568Hz | EA2DYB |
22:03 | 50313.0 | HI4T | ![]() |
FT8 -14 dB 1715Hz 2nd | WW1L |
22:03 | 10136.0 | F4WEJ | ![]() |
FT8 +01dB from JN37 2568Hz | EA2DYB |
22:02 | 50313.0 | PY2JF | ![]() |
FT8 -21 dB 1871Hz 1st | WW1L |
22:02 | 3573.0 | F8ATS | ![]() |
FT8 IM99sm -> JN18dp | EB5BZM |
22:02 | 10136.0 | G0LLE | ![]() |
FT8 -01dB from JO01 641Hz | EA2DYB |
22:01 | 3573.0 | OK1UKC | ![]() |
FT8 IM99sm -> JO60pj | EB5BZM |
22:00 | 21074.0 | W2CG | ![]() |
FT8 | LU1EEP |
22:00 | 21074.0 | CO7MS | ![]() |
FT8 -10 dB 1612 Hz | K4CUP |
21:58 | 50313.0 | PY5JO | ![]() |
FT8 -23 dB 2022Hz 2nd | WW1L |
21:57 | 14084.0 | Z68ZZ | ![]() |
FT8 GUD SIG SP | JH0NOS |
21:57 | 3573.0 | F1GTU | ![]() |
FT8 IM99sm -> JN05ie | EB5BZM |
21:56 | 3573.0 | EA7BHO | ![]() |
FT8 IM99sm -> IM87dd | EB5BZM |
21:54 | 10136.0 | VK3BVP | ![]() |
FT8 -18dB from QF31 1344Hz | 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.