Very Long Baseline Interferometry (VLBI) array
GPTKB entity
Statements (42)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
astronomer
|
| gptkbp:baselineLength |
thousands of kilometers
|
| gptkbp:consistsOf |
multiple radio telescopes
|
| gptkbp:contributedTo |
gptkb:International_Celestial_Reference_Frame
gptkb:International_Terrestrial_Reference_Frame |
| gptkbp:dataCombinedBy |
correlator
|
| gptkbp:dataRecordedOn |
hard drives
magnetic tapes |
| gptkbp:dataTransferredBy |
physical shipment
high-speed networks |
| gptkbp:developedBy |
1960s
|
| gptkbp:enables |
gptkb:Event_Horizon_Telescope_observations
study of black holes study of active galactic nuclei study of quasars measurement of Earth's rotation measurement of gravitational lensing measurement of tectonic plate motion high angular resolution imaging of distant radio sources precise position measurements study of pulsars sub-milliarcsecond resolution |
| gptkbp:example |
gptkb:Very_Long_Baseline_Array
gptkb:European_VLBI_Network gptkb:East_Asian_VLBI_Network gptkb:Australian_Long_Baseline_Array |
| https://www.w3.org/2000/01/rdf-schema#label |
Very Long Baseline Interferometry (VLBI) array
|
| gptkbp:improves |
angular resolution with longer baselines
|
| gptkbp:mayInclude |
space-based radio telescopes
|
| gptkbp:measures |
gptkb:radio_waves
|
| gptkbp:operatesIn |
radio frequencies
|
| gptkbp:requires |
precise time synchronization
|
| gptkbp:technology |
interferometry
|
| gptkbp:usedBy |
astronomer
geodesists |
| gptkbp:usedFor |
astronomer
geodesy astrometry |
| gptkbp:uses |
gptkb:atomic_clocks
|
| gptkbp:bfsParent |
gptkb:VERA
|
| gptkbp:bfsLayer |
6
|