Download presentation
Presentation is loading. Please wait.
Published byProsper Clarke Modified over 9 years ago
1
ASTRO-G Ground Tracking Station Plan Y.Murata (JAXA) Start from HALCA design Functions –Uplink reference signal –Data demodulation –Data recording –Telemetry Data Extraction –Doppler measurement
2
Signal from Astronomical Objects Orbit Prediction VSOP tracking station H maser Uplink Freq. Cntl. Downlink Freq. Cntl. D/C LNAANT A/D MOD TX HGA RX LOCAL VLBI data SYNC (4byte) DEMOD 2way phase residual 2way Doppler TLM Header (8byte) VLBI data 32M clock 1PPS gen. 1 PPS VLBI Recording TLM ground 15.3 GH z+ Doppler Correction CW 14.2 GH z QPSK 1 Frame (10,000 byte / 5 ms)
4
Difference from HALCA tracking station Frequencies – Up: 40 GHz + Doppler Compensation(?) –Down: 37 – 38 GHz Data demodulation –1 Gbps QPSK Data recording –Giga-bit recording, VSI (VERA, Mark 5, K5/VSI, …) Telemetry Data Extraction –Realtime / near realtime Doppler measurement No Phase cal pulse
5
Number of Tracking stations
6
Tracking time (%)
7
FAKESAT for VSOP-2 D.W.Murphy Linux/Cygwin ○ Kaj Wiik,R.Dodson
9
Visibility of HALCA from tracking stations (ah=21,000km, i=31) ω= 270 ω= 0 ω= 90 ω= 180 SANT MALI HART USUD TIDB MADR GOLD GBANK North Apogee South Apogee
10
Visibility of ASTRO-G from tracking stations (ah=25,000km) ω= 270 ω= 0 ω= 90 ω= 180 SANT MALI HART USUD TIDB MADR GOLD GBANK
11
Visibility of ASTRO-G from tracking stations (ah=36,000km, i=28) ω= 270 ω= 0 ω= 90 ω= 180 SANT MALI HART USUD TIDB MADR GOLD GBANK
12
Tracking station coverage requirements 3-4 tracking stations Uniform Longitude coverage Low Latitude is better
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.