US Government security requirements no longer permit CDDIS to offer data via traditional unencrypted anonymous ftp; this service was discontinued on October 31, 2020. All data are still available, however access must be via HTTPS or ftp-ssl.

Instructions with examples and our FAQ can be found at: https://cddis.nasa.gov/Data_and_Derived_Products/CDDIS_Archive_Access.html.

If you still have difficulty after reading and attempting the examples on that page, please contact us at support-cddis@earthdata.nasa.gov.

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About the CDDIS VLBI data and products archive

VLBI is a geometric technique, measuring the time difference between the arrival at two Earth-based antennas of a radio wavefront emitted by a distant quasar. The simultaneous measurements are compared at correlators; the difference in the arrival times between antennas yields a determination of the distance between the antennas and thus the precise positions of the antennas themselves. The VLBI technique can also determine the inertial reference frame defined by these quasars as well as the orientation of the Earth in this frame.

The globally distributed networks of VLBI antennas participate in highly coordinated experiments in order to perform simultaneous measurements, which are compared and correlated, generating VLBI database files. As additional analysis is performed on the experiments (e.g., the application of meteorological information, theoretical quantities and models), new versions of the database files are generated and archived. All versions are retained at the CDDIS and other IVS data centers for documentation purposes. The VLBI experiment data consist of the observing site parameters, source information, correlated delay and delay rate between the observing antennas as a function of time, along with meteorological data and system parameters that must be applied to the correlated measurements.

The CDDIS is one of the primary data centers supporting the International VLBI Service for Geodesy and Astrometry (IVS). Network stations forward raw observations to correlators who then submit the experiment databases to the IVS data centers.

VLBI determines the relative positions of the antennas to a few millimeters and the quasar positions to fractions of a milliarcsecond. Since the antennas are fixed to the Earth, their locations track the instantaneous orientation of the Earth in the inertial reference frame.