Comment:	Digi VHF Biala Podl (WIDE,SP,XL,BP)
Location:	52°01.86' N 23°05.88' E - lokaator KO12NA17SK - show map 1.3 km Läände peiling 263° from Biała Podlaska, Biała Podlaska, Lublin Voivodeship, Poland [?] 15.1 km Põhja peiling 339° from Łomazy, Powiat bialski, Lublin Voivodeship, Poland 41.0 km Läände peiling 260° from Brest, Brestskaya Voblastsʼ, Belarus 94.2 km Kirdesse peiling 23° from Lublin, Lublin Voivodeship, Poland
Last position:	2025-09-04 04:58:05 UTC (14m29s ago) 2025-09-04 06:58:05 CEST local time at Biała Podlaska, Poland [?]
Last telemetry:	2025-09-04 04:59:00 UTC (13m34s ago) – show telemetry Ch 1: 20, Ch 2: 0, Ch 3: 70, Ch 4: 0, Ch 5: 0  1     2     3     4     5     6     7     8
Device:	Microsat: WX3in1
Last path:	SP8XXT-2>APMI01 via TCPIP*,qAS,SP8XXT
Positions stored:	2
Other SSIDs:	SP8XXT-5 SP8XXT-11 SP8XXT-9
APRS igate – Statistics for 2025-09:
Stations heard directly:	4 on radio path – show map
Last heard a station directly:	2025-09-04 04:58:24 UTC (14m10s ago)
Position packets heard directly:	17 on radio path
Position packets sent to APRS-IS:	46 – show map

Only stations from which a position packet has been heard are shown here. The range statistics show some extra long hops, because some digipeaters do not correctly add themselves to the digipeater path. Please check the raw packets.

This page shows real-time information collected from the Automatic Position Reporting System Internet network (APRS-IS). APRS is used by amateur (ham) radio operators to transmit real-time position information, weather data, telemetry and messages over the radio. A vehicle equipped with a GPS receiver, a VHF transmitter or HF transceiver and a small computer device called a tracker transmits it's location, speed and course in a small data packet, which is then received by a nearby iGate receiving site which forwards the packet on the Internet. Systems connected to the Internet can send information on the APRS-IS without a radio transmitter, or collect and display information transmitted anywhere in the world.