VLBI (Very Long Baseline Interferometry)
GPTKB entity
Statements (50)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
astronomical technique
|
| gptkbp:baselineLength |
thousands of kilometers
|
| gptkbp:correlates |
data from different telescopes
|
| gptkbp:developedBy |
1960s
|
| gptkbp:enables |
spacecraft tracking
study of active galactic nuclei study of quasars study of solar system objects study of cosmic microwave background study of star-forming regions deep space navigation study of interstellar medium measurement of Earth's rotation measurement of continental drift measurement of nutation measurement of precession measurement of tectonic plate motion study of supernova remnants high angular resolution imaging of black holes measurement of universal time planetary radar observations precise position measurements study of cosmic jets study of extragalactic radio sources study of gravitational lenses study of masers study of pulsars sub-milliarcsecond resolution |
| https://www.w3.org/2000/01/rdf-schema#label |
VLBI (Very Long Baseline Interferometry)
|
| gptkbp:measures |
gptkb:radio_waves
|
| gptkbp:recordedAt |
signals independently at each telescope
|
| gptkbp:relatedTo |
gptkb:European_VLBI_Network_(EVN)
gptkb:Very_Long_Baseline_Array_(VLBA) gptkb:Square_Kilometre_Array_(SKA) gptkb:Very_Large_Array_(VLA) gptkb:space_VLBI interferometry radio telescope arrays |
| gptkbp:usedBy |
gptkb:Event_Horizon_Telescope
gptkb:International_VLBI_Service_for_Geodesy_and_Astrometry |
| gptkbp:usedFor |
geodesy
radio astronomy |
| gptkbp:uses |
gptkb:atomic_clocks
hydrogen masers multiple radio telescopes data correlation software very large data storage |
| gptkbp:bfsParent |
gptkb:Effelsberg_100-m_Radio_Telescope
|
| gptkbp:bfsLayer |
4
|