Collection Information
IDENTIFIER urn:nasa:pds:magellan_bsr_calibrated:srf::1.0
NAME Magellan Bistatic Radar Calibrated: Srf Collection
TYPE Calibration
DESCRIPTION The srf collection contains power spectra for the RCP and LCP channels which were used to 'equalize' (flatten) the spectral response of the filters in the receiving system. Since the filtering is entirely digital, there is no reason to believe that the RCP and LCP noise power spectra would differ; but separate srf files have been derived for the two channels. Standard deviation of individual frequency bins is about 1.3 percent of the mean.
SEARCH/ACCESS DATA Magellan Bistatic Radar Calibrated Online
   
Citation
DIGITAL OBJECT IDENTIFIER (DOI) 10.17189/c7sf-7t57 (from parent bundle)
AUTHORS
EDITORS
PUBLICATION YEAR 2024
DESCRIPTION The srf collection contains power spectra for the RCP and LCP channels which were used to 'equalize' (flatten) the spectral response of the filters in the receiving system. Since the filtering is entirely digital, there is no reason to believe that the RCP and LCP noise power spectra would differ; but separate srf files have been derived for the two channels. Standard deviation of individual frequency bins is about 1.3 percent of the mean.
   
Context
START DATE TIME 1994-06-05T01:41:31.000Z
STOP DATE TIME 1994-06-05T01:48:11.000Z
LOCAL MEAN SOLAR TIME
LOCAL TRUE SOLAR TIME
SOLAR LONGITUDE
PRIMARY RESULT PURPOSE Science
PRIMARY RESULT PROCESSING LEVEL Calibrated
PRIMARY RESULT DESCRIPTION
PRIMARY RESULT WAVELENGTH RANGE
PRIMARY RESULT DOMAIN Surface
PRIMARY RESULT DISCIPLINE NAME Geosciences
INVESTIGATION Magellan
OBSERVING SYSTEM
OBSERVING SYSTEM COMPONENT Magellan
Radio Science Subsystem
TARGET Venus
REFERENCES