Fundamental Technologies

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A12.3 Location and Content of UDS Files

A12.3.1 Overview

This section provides detailed information about the location and content of each of the data sets currently accessible through the UDS, which include the following instruments:

Data from the unified and radio plasma wave (URAP) and the solar X-ray and cosmic gamma-ray burst (GRB) investigations will be made available at a later date.

The UDS is in principle a distributed system with individual data sets residing on storage media managed at nominated institutes within each PI team. In cases where this is not possible, for reasons such as inadequate network connections or mass storage limitations, a temporary alternative location will be used for on-line storage. Magnetic field data are currently stored at Imperial College, London; solar wind data are kept at JPL; and COSPIN data are located at ESTEC. The remaining particle data sets (SWICS, EPAC, and HISCALE) are temporarily located at ESTEC.

Each sub-section of this section contains information for a single instrument, sub-system, or group of selected measurements. The information provided includes:

1If a VAX machine is not configured to recognize a node name, it is necessary to use the node number as an alternative.

This information is duplicated in the README.TXT files which can be found in the appropriate UDS sub-directory.

Next: A12.3.2 VHM/FGM, A12.3.3 SWICS, and A12.3.4 EPAC

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Updated 11/19/02, T. Hunt-Ward