Hostname: page-component-76fb5796d-dfsvx Total loading time: 0 Render date: 2024-04-29T03:19:17.149Z Has data issue: false hasContentIssue false
  • English
  • Français

The VLB array: a new geophysical tool

Published online by Cambridge University Press:  03 August 2017

Edward B. Fomalont
Edward B. Fomalont*
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA 22903-2475

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The National Radio Astronomy Observatory is constructing a Very Long Baseline Array (VLBA) consisting of ten antennas across the USA, between Hawaii and the Virgin Islands. The array will be a dedicated instrument for producing milliarcsecond images of radio sources. However, exciting geophysical applications of the array are obvious and, furthermore, detailed geodetic, astrometric and environmental parameters are necessary for the VLBA to achieve its full sensitivity, resolution and positional capabilities.

Type
VII. Other Topics
Information
Symposium - International Astronomical Union , Volume 128: Earth's Rotation and Reference Frames for Geodesy and Geodynamics , 1988 , pp. 445 - 451
Copyright
Copyright © Reidel 1988 

References

Chikada, Y., et al., 1984, Indirect Imaging, edited by Roberts, J. A., Cambridge University Press, p. 387.Google Scholar
Kellermann, K. I. and Thompson, A. R., 1985, Science, 229, 123.CrossRefGoogle Scholar
Multidisciplinary Used of the Very Long Baseline Array, 1983, National Academy Press.Google Scholar
Readhead, A.C.S. and Wilkinson, P. N., 1978, Ap. J., 223, 25.Google Scholar