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Magellan Bistatic Radar (BSR)

The Magellan Bistatic Radar (BSR) Raw Data Archive is a time-ordered collection of raw and partially processed data from bistatic radar experiments conducted using the Magellan spacecraft while it orbited Venus.

The Bistatic Radar Calibrated Data Archive contains time-ordered amplitude- and frequency-calibrated data, power spectra and voltage cross spectra, along with ancillary data.

In the tables below, click on the volume ID to get to the volume's top-level directory, from which you may access all the files. For an introduction to the volume, read the aareadme file in the top-level directory. To find the location of a specific data product, look in the cumulative index on the last volume.

Magellan Bistatic Radar Calibrated Data Archive

Volume Index Errors and Anomalies
mg_2501 Index table and label errata.txt
mg_2502 Index table and label errata.txt
mg_2503 Index table and label errata.txt

Magellan Bistatic Radar Raw Data Archive

Volume Index Errors and Anomalies
mg_2301 Index table and label errata.txt
mg_2302 Index table and label errata.txt
mg_2303 Index table and label errata.txt
mg_2304 Index table and label errata.txt
mg_2305 Index table and label errata.txt
mg_2306 Index table and label errata.txt
mg_2307 Index table and label errata.txt
mg_2308 Index table and label errata.txt
mg_2309 Index table and label errata.txt
mg_2310 Index table and label errata.txt
mg_2311 Index table and label errata.txt
mg_2312 Index table and label errata.txt
mg_2313 Index table and label errata.txt

Data Set Producer

The person most directly responsible for construction and release of these data sets is Dick Simpson, Experiment Engineer for the Mars Global Surveyor Radio Science Team and Radio Science Advisor to the Planetary Data System. Although many people contributed to the volume set, any faults in the product are his alone. The Team Leader for the Mars Global Surveyor Radio Science Team and Principal Investigator for this archiving activity is G. Leonard Tyler. The persons most directly involved with analysis of the data were Gordon Pettengill, Peter Ford, and Dick Simpson. Please direct any questions and comments to the PDS Geosciences Node, geosci@wunder.wustl.edu.

 

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