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Ministry of Land, Infrastructure, Transport and Tourism Geospatial Information Authority of Japan Status Report of GSI Masafumi Ishigaki (Geospatial Information Authority of Japan; GSI) 9 Nov. 2018

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Page 1: Status Report of GSI - auscope.phys.utas.edu.au

Ministry of Land, Infrastructure, Transport and TourismGeospatial Information Authority of Japan

Status Report of GSI

Masafumi Ishigaki(Geospatial Information Authority of Japan;

GSI)9 Nov. 2018

Page 2: Status Report of GSI - auscope.phys.utas.edu.au

Location of GSI and Ishioka

Tsukuba (GSI)

Ishioka

KashimaTokyo

Page 3: Status Report of GSI - auscope.phys.utas.edu.au

Diameter 13.2 m

Optics Ring Focus

Surface Accuracy < 0.1 mm RMS

Slew Rate

Az 12 deg/sec

El 6 deg/sec

Equipment for VLBI observation

Observation building

Ishioka Geodetic Observing Station

Page 4: Status Report of GSI - auscope.phys.utas.edu.au

Ishioka Geodetic Observing Station

Gravity measurement facility

GNSS observation stations

Observation building

Page 5: Status Report of GSI - auscope.phys.utas.edu.au

Observational Status in 2018

Triband

QRFH

• Legacy S/X observation R1(26) R4(24) INT (81) AOV (7) T2 (3) APSG (1)

• Broadband observation VGOS Test (7) AOV broadband experiment Broadband observation with NICT

Page 6: Status Report of GSI - auscope.phys.utas.edu.au

Legacy Observation: INT2

UT1-UTC w.r.t. IERS EOPC04.08

[use

c]

Year/Month

2016/1

finals2000A.alleopc04.62-now

2016/7 2017/1 2017/7 2018/72018/1

others

Page 7: Status Report of GSI - auscope.phys.utas.edu.au

Baseline AnalysisB

asel

ine

Year

Tsukuba-Kokee

Ishioka-Kokee

6cm/year

Tohoku earthquake(64cm)

Page 8: Status Report of GSI - auscope.phys.utas.edu.au

• Involved in almost all AOV sessions so far• GSI also

1. makes schedules2. carries out correlation3. provides feedback to participating stations

AOV Sessions in 2018

Session Date Stations Sked. Corr.

AOV019 23-JanHoIsKbKeKmShT6UrWwYg

SHAO SHAO

AOV020 27-Feb IsKeKgK1SyWwYg GSI GSI AOV021 20-Mar HoIsKeKmShUrWwYg SHAO SHAO

AOV022 1-MayBdHoIsKeKmShSvWwYgZc

UTAS SHAO

AOV023 21-May HoIsK1KgVmWwYg UTAS GSI AOV024 19-Jun HoKeK1KvSyWwYg GSI GSI

AOV025 24-JulHoKeKmShT6UrWwYg

SHAO SHAO

AOV026 7-AugHoKeKgK1KvUrVmWwYg

UTAS SHAO

AOV027 18-Sep HoIsKeKmWwYg SHAO SHAO

AOV028 16-OctHoIsKbKeKvVmWwYg

GSI GSI

AOV029 22-NovHoIsKbKeKmShT6UrWwYg

SHAO SHAO

AOV030 11-Dec HoIsKeKvUrWwYg UTAS GSI

Page 9: Status Report of GSI - auscope.phys.utas.edu.au

Correlation & Analysis of AOV

• GSI provides correlation results alternately with SHAO

• It takes ~1 month from the end of observation to release of correlation report

2014 2015 2016 2017 2018 2019-150

-100

-50

0

50

100

150 KUNMING-YARRA12M

All

AOV

Year

Bas

elin

e [m

m]

2014 2015 2016 2017 2018 2019-150

-100

-50

0

50

100

150 SEJONG-WARK12M

All

AOV

Year

Bas

elin

e [m

m]

Page 10: Status Report of GSI - auscope.phys.utas.edu.au

Feedback to stations in AOV

• GSI provides feedback to AOV participating stations as a correlator in order to

share the problems among correlator, schedulerand stations

improve the data quality of following sessions

• The feedback is focusing on

SNR of each band

Data recording time

Phase cal etc.

Page 11: Status Report of GSI - auscope.phys.utas.edu.au

• Ishioka and Hobart succeeded in broadband experiment in August to September 2018

• Performance test of VGOS stations before joining VGOS Test of IVS

① 2018/8/8 UT4:30-5:00 (f18220)

② 2018/9/4 UT2:30-4:00 (f18247)

③ 2018/9/10 UT2:30-4:10 (f18253)

AOV Broadband experiment with Hobart

Page 12: Status Report of GSI - auscope.phys.utas.edu.au

• The data were correlated in UTAS• Detect fringes in each band

3GHz 5GHz

6GHz 10GHz

SNR 169.3 SNR 124.2

SNR 145.3 SNR 58.5

AOV Broadband experiment with Hb

Page 13: Status Report of GSI - auscope.phys.utas.edu.au

• Wakasugi visited UTAS and Mt. Pleasant Observatory from March 7 to 8, 2018

• Discussed several AOV topics

AOV Retreat

Page 14: Status Report of GSI - auscope.phys.utas.edu.au

Local Tie Works in Ishioka

• Need to derive the reference point of VLBI• Trying two kinds of method

Pillar

Pillar Pillar

Pillar

Reference Point

GNSS

Page 15: Status Report of GSI - auscope.phys.utas.edu.au

August 2018• Set TS in the vicinity of reference point of VLBI• Track the trajectory of targets from inside

1. Measurement from Inside

El axis

Az axis

Az cabin Az axisTarget

El axis

Az cabin

Page 16: Status Report of GSI - auscope.phys.utas.edu.au

Comparison result is coming soon

Spherical Surface

Reference Point

Target

1. Measurement from Outside

November 2018 (Now measuring!)• Set TS on the pillars• Track the trajectory of targets from outside

Page 17: Status Report of GSI - auscope.phys.utas.edu.au

Open Observatory of Ishioka

Saturday, October 27, 2018

Page 18: Status Report of GSI - auscope.phys.utas.edu.au

• Continue legacy S/X-band observations

AOV, R1, R4, T2, APSG and Intensives

 • Also participate in VGOS Test of IVS and other

broadband observations

→ Broadband experiment with other stations is welcomed!

Future Plan

Page 19: Status Report of GSI - auscope.phys.utas.edu.au

Summary

• Ishioka station has performed international

observations since 2015.

• GSI is involved in AOV as a station, scheduler, and

correlator.

• Ishioka station succeeded in the AOV broadband

experiment with Hobart.

• Local tie of VLBI-GNSS is now measured in Ishioka.

• GSI will continue to be involved in the AOV sessions

as both legacy and VGOS station.

Page 20: Status Report of GSI - auscope.phys.utas.edu.au

Thank you so much for your kind

attention.