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| This site may be down on Thursdays 
between 7:00 and 9:30 pm Central Time for maintenance. |  | 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 Magellan Bistatic Radar Raw Data 
									Archive To download the entire data sets or parts of them with FTP, use these URLs:  
                          
                          ftp://pds-geosciences.wustl.edu/mgn/mgn-v-rss-1-bsr-v1 
							
							ftp://pds-geosciences.wustl.edu/mgn/mgn-v-rss-4-bsr-v1
							 Data Set ProducerThe 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.    |