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ASTRO-G Ground Tracking Station Plan Y.Murata (JAXA) Start from HALCA design Functions –Uplink reference signal –Data demodulation –Data recording –Telemetry.

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Presentation on theme: "ASTRO-G Ground Tracking Station Plan Y.Murata (JAXA) Start from HALCA design Functions –Uplink reference signal –Data demodulation –Data recording –Telemetry."— Presentation transcript:

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)

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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

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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


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