Astrophysics (Index)About

interferometry

(analysis of superimposed EMR waves)

Interferometry is the use and analysis of superimposed electromagnetic radiation (EMR) waves. The patterns produced by waves from different directions and/or wavelengths (wave interference) include information about relative directions and wavelengths. A device carrying out this function is called an interferometer, which offers data for analysis on the differences found in waves gathered by pairs of data sources, such as the EMR waves gathered by two telescopes that are some distance apart.

Radio astronomy makes much use of interferometry (radio interferometry), using multiple radio telescopes (dishes) to achieve a higher angular resolution. Keck Observatory and other twin/multiple telescopes can be used for interferometry of visible light (optical interferometry). A type of imaging spectrograph, the imaging Fourier transform spectroscopy makes use of a type of interferometry.

Gravitational-wave detectors such as LIGO also use interferometry (with Michelson interferometers) to measure extremely small distance-differences.


(science,astronomy,measurement)
Further reading:
https://en.wikipedia.org/wiki/Interferometry
https://en.wikipedia.org/wiki/Astronomical_optical_interferometry
https://www.eso.org/sci/meetings/2015/eris2015/L1_Jackson_Interferometry.pdf
https://science.nrao.edu/opportunities/courses/casa-caltech-winter2012/Isella_Radio_Interferometry_Basics_Caltech2012.pdf
https://kiss.caltech.edu/workshops/black_hole/Presentations/Johnson.pdf

Referenced by pages:
angular resolution
aperture masking interferometry (AMI)
baseline
CLEAN
convolution
correlator
DECIGO
dirty image
DSA-2000
electronic very-long-baseline interferometry (e-VLBI)
European Southern Observatory Very Large Telescope (ESO VLT)
Fourier space
high-resolution imaging
infrared (IR)
intensity interferometer
LISA
MeerKLASS
millimeter astronomy
New Gravitational Wave Observatory (NGO)
optical interferometer
Parkes Observatory
pipeline
point source
Queen's University Radio Observatory (QRO)
radio astronomy
Radio Camera Initiative (RCI)
speckle imaging
speckle masking
speckle suppression
speckles
spectral correlator
stellar parameter determination
stellar radius determination
Submillimeter Array (SMA)
submillimeter astronomy
synthetic aperture radar (SAR)
TianQin
tomography
TripleSpec (TSpec)
Very Large Array (VLA)
very-long-baseline interferometry (VLBI)
visibility

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