Limitation of VLBI angular resolution

Details Limitation of VLBI angular resolution Limitation of VLBI angular resolution

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.213..119m&link_type=abstract

In ESA QUASAT: A VLBI Obs. in Space p 119-121 (SEE N85-16700 07-88)

Physics

2

Angular Resolution, Radar Resolution, Very Long Base Interferometry, Atmospheric Scattering, Interplanetary Medium, Interstellar Matter, Radar Scattering, Spectral Sensitivity

Scientific paper

The effects of scattering and interferometer sensitivity on VLBI angular resolution are summarized. Atmospheric, interplanetary, and interstellar scattering, and scattering due to the envelope of the object limit the baseline maximum length for 1 cm waves to 1 million km; for metric waves it is several thousand km. For centimeter waves, sensitivity limits baselines to 100,000 km, with approximately 40 microarcsec angular resolution.

Affiliated with

Also associated with

No associations

Rating

Limitation of VLBI angular resolution does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Limitation of VLBI angular resolution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Limitation of VLBI angular resolution will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1393635