Improved computation of gravity-dependent signal path variation models for Cassegrainian VLBI telescopes with tapered illumination functions

Details Improved computation of gravity-dependent signal path variation models for Cassegrainian VLBI telescopes with tapered illumination functions Improved computation of gravity-dependent signal path variation models for Cassegrainian VLBI telescopes with tapered illumination functions

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010eguga..12.9042a&link_type=abstract

EGU General Assembly 2010, held 2-7 May, 2010 in Vienna, Austria, p.9042

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Improved computation of gravity-dependent signal path variation models
for Cassegrainian VLBI telescopes with tapered illumination functions

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