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VERY LONG BASELINE ARRAY OBSERVATIONAL STATUS SUMMARY J.M. Wrobel 1994 June 23Contents 1INTRODUCTION2ANTENNA SITES63ANTENNAS64FREQUENCIES5VLBA SIGNAL PATH 5.1 Antenna and Subreflector 5.2 Feed ............
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01
Determine the purpose of the very long baseline array (VLBA)
02
Choose the appropriate equipment for the VLBA, such as telescopes and receivers
03
Set up the telescopes at the desired locations and align them properly
04
Connect the telescopes to the receivers and make sure they are functioning correctly
05
Collect data from the VLBA and process it accordingly

Who needs very long baseline array?

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Astronomers studying distant objects in space
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Researchers monitoring geological activity over large distances
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Scientists studying atmospheric phenomena
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The Very Long Baseline Array (VLBA) is a radio observatory consisting of ten antennas located in the United States that work together to create high-resolution images of astronomical objects.
Researchers and institutions using the VLBA for astronomical research are required to file reports or proposals related to their observations and findings.
To fill out a VLBA proposal, researchers must provide detailed information about their intended observations, including the scientific goals, target objects, and technical requirements, according to the specific guidelines issued by the observatory.
The purpose of the VLBA is to provide high-resolution imaging of celestial objects, allowing astronomers to study their properties and behaviors more accurately than with single-dish telescopes.
Reports must include details such as the observation dates, target objects, data analysis methods, and results from experiments conducted using the VLBA.
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