Name:
F0KZ5651
Station ID:
346696
Source:
Symbol:
Latest Packet:
Position Packet
Receive Time:
1750431363
Age:
1750431363
Path:
APN100,TCPIP*,qAS,UT8IBK
Equipment:
Unknown Equipment
Latest Position:
50.43783, 30.68817
Receive Time:
(Received in latest packet)
Packet frequency:
calculating ...
Packets stored:
retrieving ...
Nearby stations/objects:
Last Received
Distance
UT3ULJ
1750443188
8.99 km
UT4UTI-1
1750444412
11.47 km
UT4UGW-13
1750444315
16.11 km
UT3USD
1750443388
16.37 km
UR4URA
1750443925
18.3 km
UT6UO-1
1750444592
20.68 km
EL-UR3CNO
1750444357
20.76 km
KYIV-1
1750444618
22.07 km
UT6UW-1
1750444504
32.78 km
ER-UR0UUK
1750444275
32.95 km
- The specified "Station ID" is the ID that this station has on this website, this ID is useful when creating a link to this website. Read more in the About/FAQ.
- To get a better understanding of the APRS path I recommend reading the explanation written by wa8lmf.
- If this packet has the "Posambiguity"-mark it means that the sent position is ambiguous (a configured number of digits has been truncated from the end of the position).
- PHG stands for Power-Height-Gain (and directivity). The height is not the height above sea-level, it is the height above average terrain (HAAT = Height Above Average Terrain). PHG is used to calculate the relative RF range of a station. If this station has reported several positions or symbols the PHG data will only be used for the position and symbol used in the PHG-packet.
- RNG is the "pre-calculated omni-directional radio range" of the station (reported by the station itself). If this station has reported several positions or symbols the RNG data will only be used for the position and symbol used in the RNG-packet. It seems like many D-STAR station use the RNG value to specifify D-STAR range.
- One object may be sent by several different senders. On the map they may share the same path, but they all have their own "Station information" modal.
- If station has more than 15 related stations we will only show the 10 closest related stations.
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