Components
Correlators
Functions of Correlators in the IVS Terms of Reference
|
Country
|
IVS Component Name (link to recent Annual/Biennial Report)
|
Primary Contact
|
Sponsoring Organization
|
Programs Supported
|
S
|
T
|
%
|
|
Austria
|
Vienna Correlator
|
Johannes Boehm
|
Vienna Center for VLBI
|
AUS-AST, VGOS-OPS
|
1.0
|
10
|
100%
|
|
China
|
Shanghai Correlator
|
Fengchun Shu
|
Shanghai Astronomical Observatory
|
CVN, AOV, APSG, AUS-AST, CRF, VGOS-OPS
|
0.8
|
4
|
50%
|
|
Germany
|
Astro/Geo Correlator at MPIfR
|
Simone Bernhart
|
MPIfR
,
BKG
,
Reichert GmbH
|
IVS-R1, IVS-T2, OHIG, IVS-INT-3, VGOS-OPS
|
2.8
|
10
|
50%
|
|
Japan
|
Tsukuba VLBI Center
|
Yu Takagi
|
Geospatial Information Authority of Japan
|
AOV, IVS-INT-2
|
0.5
|
10
|
100%
|
|
Russia
|
Institute of Applied Astronomy
|
Igor Surkis
|
Institute of Applied Astronomy
|
RU-I, RU-E
|
1
|
10
|
50%
|
|
USA
|
Washington Correlator
|
David Hall
|
NEOS
|
IVS-R4, CRF, TRF, IVS-INT-1, VGOS-OPS, VGOS-INT-A
|
1.0
|
10
|
100%
|
|
USA
|
MIT Haystack Correlator
|
Pedro Elosegui
|
NASA Goddard Space Flight Center
|
R&D, VGOS-OPS, VGOS-RD
|
0.5
|
20
|
12%
|
Key: S = storage capacity [PB], T = e-transfer speed [Gbps], % = %use
for geodesy
|
