UTC | Freq | Call | DXCC | Comment | Spotter |
---|---|---|---|---|---|
00:20 | 3573.0 | SP9TBT | ![]() |
FT8 -14dB from JO90 2742Hz | SP3VSC |
00:16 | 3573.0 | F5RRS | ![]() |
FT8 +01dB from JN36 2254Hz | SP3VSC |
00:14 | 3830.0 | YH1AU | ![]() |
ORARI 2025 | YB1APR |
23:58 | 3573.0 | C31KC | ![]() |
ft8 tnx 73 | CT7AUT |
23:25 | 3574.2 | J88BTI | ![]() |
QRV | J88BTI |
22:38 | 3840.0 | YH5NL | ![]() |
SSB ORARI 2025 | YB1APR |
22:23 | 3573.0 | EG25FDC | ![]() |
ft8 Fiesta del Cielo 73s | EB4GRT |
22:19 | 3705.0 | EG25FDC | ![]() |
Fiesta del cielo de Gijon 2025 | EA2XG |
22:19 | 3840.0 | YH5NL | ![]() |
ORARI 2025 ssb | YB1APR |
22:16 | 3573.0 | EG25FDC | ![]() |
ft8 tnx 73 | CT7AUT |
22:11 | 3705.0 | EG25FDC | ![]() |
Fiesta Del Cielo De Gijon 2025 | EA7XJ |
22:08 | 3705.0 | EG25FDC | ![]() |
SPECIAL EVENT QRZ.COM | EA1BXK |
21:59 | 3573.0 | CR5Q | ![]() |
IN63IN<>IM67 | EA1FCH |
21:50 | 3855.0 | YH8AW | ![]() |
ssb ORARI 2025 | YB1APR |
21:48 | 3573.0 | CR5Q | ![]() |
43 ANIV MCF | CT7AUT |
21:46 | 3733.0 | EJ3VP | ![]() |
new freq | EI5JDB |
21:28 | 3720.0 | EJ3VP | ![]() |
EI5JDB | |
21:27 | 3573.0 | DO4RK | ![]() |
FT8 -14dB from JO62 2028Hz | SP3VSC |
21:15 | 3573.0 | YC2KME | ![]() |
FT8 -20 dB 1307 Hz | UT7UA |
21:14 | 3720.0 | EJ3VP | ![]() |
G3PXT |
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.