space VLBI

E499557

Space VLBI is a radio astronomy technique that extends very long baseline interferometry by placing one or more antennas in space to achieve extremely high angular resolution beyond the limits of Earth-based arrays.

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Predicate Object
instanceOf radio astronomy technique
very long baseline interferometry extension
aimsFor extremely high angular resolution
appliesTo active galactic nuclei
compact radio sources
masers
pulsars
quasars
comparedTo ground VLBI
dataProcessing VLBI correlator
fringe fitting
imaging and deconvolution
enables baselines longer than Earth’s diameter
microarcsecond-scale imaging
extends Earth-based VLBI baselines into space
very long baseline interferometry
field radio astronomy
goal resolve structure of the most compact radio sources in the universe
hasChallenge complex correlation processing
limited downlink bandwidth
onboard data recording constraints
spacecraft pointing accuracy
isLimitedBy available observing frequencies on spacecraft
launch and mission cost
spacecraft mission lifetime
observes centimeter wavelengths
decimeter wavelengths
millimeter wavelengths
offers higher angular resolution than ground VLBI
requires accurate time synchronization
correlation of space and ground data
global networks of ground radio telescopes
high-stability frequency standards
international collaboration
precise orbit determination
supports astrometry of compact radio sources
measurements of brightness temperature limits
studies of jet formation in active galactic nuclei
tests of general relativity near compact objects
uses antennas in space
ground-based radio telescopes
radio interferometry
usesBaselineLengthsUpTo hundreds of thousands of kilometers
wasDemonstratedBy HALCA satellite NERFINISHED
RadioAstron mission NERFINISHED
TDRSS Orbital VLBI experiment
VSOP mission NERFINISHED

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