CCSD3ZF0000100000001NJPL3IF0PDS200000001 = SFDU_LABEL /* Detached PDS label for the Pioneer Venus ORAD database file */ RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 186 FILE_RECORDS = 144129 ^TABLE = "PVEN001S.DAT" OBJECT = TABLE INTERCHANGE_FORMAT = ASCII ROWS = 144129 COLUMNS = 25 /* Dataset descriptive parameters */ DATA_SET_ID = "P12-V-ORAD-4-ALT/RAD-V1.0" TARGET_NAME = VENUS EVENT_START_TIME = 1978-12-05 EVENT_STOP_TIME = 1981-03-23 SPACECRAFT_NAME = "PIONEER VENUS ORBITER" INSTRUMENT_NAME = "ORBITING RADAR" TRANSMITTED_POLARIZATION = "LINEAR" RECEIVED_POLARIZATION = "SAME SENSE LINEAR" WAVELENGTH = 17. PRODUCER_FULL_NAME = "GORDON H. PETTENGILL" NOTE = "This data set consists of measurements made by the Radar Mapper Experiment on the Pioneer Venus Orbiter spacecraft. The measurements were made during each 12-second spacecraft rotation period for a period of 32 minutes either side of periapsis, when the range to the surface was less that about 4500 km. This data set contains results from the altimetry and radiometry measurements. Each record describes the data collected during a single 12-second roll period. If multiple altimetry measurements were made at that time, the individual results have been averaged. This data set includes corrections for timing errors, orbit determination errors, and for atmospheric delay and attenuation. There remain severe systematic errors in the planetary radius and Fresnel reflectivity parameters, the former due to a combination of spacecraft timing and orbit determination errors, the latter to spacecraft timing errors alone. All fields are separated by commas. For reference, see Pettengill, G.H., E. Eliason, P.G. Ford, G.B. Loriot, H. Masursky, and G.E. McGill, Pioneer Venus radar results: Altimetry and surface properties, J. Geophys. Res., 85, 8261-8270, 1980." /* Descriptions of each column in the file */ OBJECT = COLUMN NAME = DATE DATA_TYPE = INTEGER UNIT = DAYS START_BYTE = 1 BYTES = 8 FORMAT = 'I8' DESCRIPTION = "The year and day-of-year of the observation, as supplied by the Pioneer project. The year occupies the first 5 bytes, the day the remaining 3 bytes. This field may be used to correlate this radar observation record with data from other Pioneer Venus instruments, but the RADAR_DATE field should be used for radar mapping purposes. A value of 0 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = TIME DATA_TYPE = INTEGER UNIT = MILLISECONDS START_BYTE = 10 BYTES = 9 FORMAT = 'I9' DESCRIPTION = "The time of the observation, in milliseconds from midnight UT, as supplied by the Pioneer project. As with the Date field, this should only be used for comparison purposes. The accurate radar observation time is contained in the RADAR_TIME field. A value of 0 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = ORBIT_NUMBER DATA_TYPE = INTEGER UNIT = "N/A" START_BYTE = 20 BYTES = 5 FORMAT = 'I5' DESCRIPTION = "The Pioneer Venus orbit number. The spacecraft maintained a nearly 24-hour orbit. Radar data was taken from orbit 3 on December 7, 1978 through orbit 834 on March 19, 1981. A value of 0 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = ROLL_TIME DATA_TYPE = INTEGER UNIT = SECONDS START_BYTE = 26 BYTES = 6 FORMAT = 'I6' DESCRIPTION = "The time from periapsis, in seconds, supplied by the Pioneer project. Negative values represent pre-periapsis measurements. This time field is specified in precisely 12 second intervals from the periapsis time derived from spacecraft doppler tracking. The 12-second interval was chosen to closely approximate the spacecraft spin period. Radar data were taken once per spacecraft rotation, and therefore not at exactly 12-second intervals. In addition, the radar altimeter was able to refine the measurement of UT of periapsis. Each radar observation was therefore assigned to a particular 12-second interval by counting spacecraft revolutions before or after the true periapsis, assigning the last radar measurement before periapsis to the Roll field with value 0. A value of 0 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RADAR_DATE DATA_TYPE = INTEGER UNITS = DAYS START_BYTE = 33 BYTES = 8 FORMAT = 'I8' DESCRIPTION = "The year and day-of-year of the observation. The year occupies the first 5 bytes, the day the remaining 3 bytes. A value of 99999999 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RADAR_TIME DATA_TYPE = INTEGER UNITS = MILLISECONDS START_BYTE = 42 BYTES = 9 FORMAT = 'I9' DESCRIPTION = "The time that the first altimeter pulse left the transmitter, measured in milliseconds from midnight UT. A value of 999999999 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RADIOMETER_LATITUDE DATA_TYPE = REAL UNITS = DEGREES START_BYTE = 52 BYTES = 7 FORMAT = 'F7.3' DESCRIPTION = "The latitude of the radiometric brightness measurement. Latitudes are expressed in degrees, positive in the northern hemisphere, negative in the southern. The body-fixed 1985 IAU coordinate system (VBF85) is used. A value of 999.999 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RADIOMETER_LONGITUDE DATA_TYPE = REAL UNITS = DEGREES START_BYTE = 60 BYTES = 7 FORMAT = 'F7.3' DESCRIPTION = "The longitude of the radiometric brightness measurement. Longitudes are expressed in degrees, in the range 0 through 360. Longitudes increase eastward of the prime meridian, and the (retrograde) planetary rotation is from east to west. The body-fixed 1985 IAU coordinate system (VBF85) is used. A value of 999.999 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = PLANET_RADIANCE DATA_TYPE = REAL UNITS = CENTIVOLTS START_BYTE = 68 BYTES = 6 FORMAT = 'F6.1' DESCRIPTION = "The voltage reading from the radar receiver during the radiometry period, when the transmitter was turned off and the antenna pointed within about 5 degrees of the plane defined by the spacecraft spin-axis and the nadir. A value of 9999.9 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPACE_RADIANCE DATA_TYPE = REAL UNITS = CENTIVOLTS START_BYTE = 75 BYTES = 6 FORMAT = 'F6.1' DESCRIPTION = "The voltage reading from the radar receiver during the radiometry-background period, when the transmitter was turned off and the antenna pointed within about 5 degrees of the plane defined by the spacecraft spin-axis and the zenith. A value of 9999.9 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = BRIGHTNESS_TEMPERATURE DATA_TYPE = REAL UNITS = "DEGREES KELVIN" START_BYTE = 82 BYTES = 6 FORMAT = 'F6.1' DESCRIPTION = "The microwave brightness temperature of the planet, in degrees Kelvin, derived from the PLANET_RADIANCE (PC) and SPACE_RADIANCE (SC) measurements, as follows: the data set was divided into 1 degree latitude intervals. For each interval, the average SC reading was taken to represent a measurement of the 3K cold sky. The average PC values from lowland regions were interpreted as measuring an average temperature of 735K with an emissivity of 88%. BRIGHTNESS_TEMPERATURE is therefore obtained by (735*0.88*(PC-)+3*(-PC))/(-). This formula may occasionally predict a negative brightness temperature value, a result of the large random noise component in PC and SC along with the assumption of linear temperature response. A value of 9999.9 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RADAR_LATITUDE DATA_TYPE = REAL UNITS = DEGREES START_BYTE = 89 BYTES = 7 FORMAT = 'F7.3' DESCRIPTION = "The latitude of the average radar altimeter footprint for this observation. Because of the delay and doppler filtering applied by the on-board data processing electronics, the footprint is not necessarily centered about the sub-spacecraft point, nor is it symmetric with respect to the antenna axis. In addition, some observations are, in fact, averaged over up to 4 measurements taken at varying doppler frequency offsets, corresponding to 4 separated footprints spaced along the spacecraft ground track. Latitudes are expressed in degrees, positive in the northern hemisphere, negative in the southern. The body-fixed 1985 IAU coordinate system (VBF85) is used. A value of 999.999 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RADAR_LONGITUDE DATA_TYPE = REAL UNITS = DEGREES START_BYTE = 97 BYTES = 7 FORMAT = 'F7.3' DESCRIPTION = "The longitude of the average radar altimeter footprint. Longitudes are expressed in degrees, in the range 0 through 360. Longitudes increase eastward of the prime meridian, and the (retrograde) planetary rotation is from east to west. The body-fixed 1985 IAU coordinate system (VBF85) is used. A value of 999.999 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = CROSS_TRACK_FOOTPRINT_SIZE DATA_TYPE = REAL UNITS = KILOMETERS START_BYTE = 105 BYTES = 5 FORMAT = 'F5.1' DESCRIPTION = "The average cross-track dimension of the altimeter footprint. This is determined by the delay-resolution of the radar receiver. A value of 9999. for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = ALONG_TRACK_FOOTPRINT_SIZE DATA_TYPE = REAL UNITS = KILOMETERS START_BYTE = 111 BYTES = 5 FORMAT = 'F5.1' DESCRIPTION = "The average along-track dimension of the altimeter footprint. For spacecraft altitudes above about 500 km, this is also determined by the delay-resolution of the radar receiver. Below this altitude, it is determined by the frequency resolution. The high altitude footprints are therefore circular, and the low altitude ones are approximately elliptical with ALONG_TRACK_FOOTPRINT_SIZE < CROSS_TRACK_FOOTPRINT_SIZE. A value of 9999. for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RADIUS DATA_TYPE = REAL UNITS = KILOMETERS START_BYTE = 117 BYTES = 8 FORMAT = 'F8.3' DESCRIPTION = "The planetary radius measured by the radar altimeter. A correction has been made for atmospheric delay, using the results of Kliore et al., 1985. A value of 9999.999 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RADIUS_ERROR DATA_TYPE = REAL UNITS = KILOMETERS START_BYTE = 126 BYTES = 7 FORMAT = 'F7.3' DESCRIPTION = "The formal error in planetary radius, derived from the statistics of the time-sampled altimetry echo-power profile. A value of 999.999 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RMS_SLOPE DATA_TYPE = REAL UNITS = DEGREES START_BYTE = 134 BYTES = 7 FORMAT = 'F7.3' DESCRIPTION = "The RMS average surface slope at meter scale, from the altimeter measurement. The slope is derived by analyzing the time-sampled profile according to Hagfors' Law of near-normal-incidence scattering from a quasi-specular surface, where the specific radar cross-section varies with the scattering angle t according to 0.5*R*C*(cos(t)**4+C*sin(t)**2)**(-1.5), where R is the FRESNEL_REFLECTIVITY and the Hagfors constant C is RMS_SLOPE**(-2) in radians. A value of 999.999 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SLOPE_ERROR DATA_TYPE = REAL UNITS = DEGREES START_BYTE = 142 BYTES = 7 FORMAT = 'F7.3' DESCRIPTION = "The formal error in surface slope, derived during the process of fitting the returned time-sampled radar echo to a set of Hagfors Law templates. A value of 999.999 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FRESNEL_REFLECTIVITY DATA_TYPE = REAL UNITS = "N/A" START_BYTE = 150 BYTES = 5 FORMAT = 'F5.2' DESCRIPTION = "The Fresnel reflectivity of the surface. This is related to the (complex) surface bulk dielectric constant E by ((sqrt(E)-1)/(sqrt(E)+1))**2. A value of 99.99 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FRESNEL_REFLECTIVITY_ERROR DATA_TYPE = REAL UNITS = "N/A" START_BYTE = 156 BYTES = 5 FORMAT = 'F5.2' DESCRIPTION = "The formal error in Fresnel reflectivity, derived during the process of fitting the returned time-sampled radar echo to a set of theoretical templates derived from Hagfors Law." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FRESNEL_REFLECTIVITY_CORRECTION DATA_TYPE = REAL UNITS = "N/A" START_BYTE = 162 BYTES = 5 FORMAT = 'F5.2' DESCRIPTION = "A correction to the Fresnel reflectivity to account for that fraction of the incident radar beam that is reflected by sub-wavelength-sized scatterers. This component was estimated, where possible, from the ORAD side looking radar imaging mode, and modeled by the phenomenological function g*a*Rf*cos(t)**1.5, where t is the scattering angle, g = 2.69 is a fitted geometrical factor, and a is the fraction of the surface covered by diffusely-scattering material. Rf is the true Fresnel reflectivity, and may be reconstructed from FRESNEL_REFLECTIVITY+FRESNEL_REFLECTIVITY_CORRECTION. This correction is only available for that portion of the altimetric data set that is also covered by side-looking imaging data, i.e. from about 15 degrees south to 45 degrees north latitude. A value of 99.99 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RADIUS_SLOPE_CORRELATION DATA_TYPE = REAL UNITS = "N/A" START_BYTE = 168 BYTES = 5 FORMAT = 'F5.2' DESCRIPTION = "The formal correlation coefficient between the planetary radius and the surface slope, derived while fitting the observed echo-power profile to Hagfors Law derived templates. A value of 99.99 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RADIUS_REFLECTIVITY_CORRELATION DATA_TYPE = REAL UNITS = "N/A" START_BYTE = 174 BYTES = 5 FORMAT = 'F5.2' DESCRIPTION = "The formal correlation coefficient between the planetary radius and the Fresnel reflectivity, derived while fitting the observed echo-power profile to Hagfors Law derived templates. A value of 99.99 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SLOPE_REFLECTIVITY_CORRELATION DATA_TYPE = REAL UNITS = "N/A" START_BYTE = 180 BYTES = 5 FORMAT = 'F5.2' DESCRIPTION = "The formal correlation coefficient between the surface slope and the Fresnel reflectivity, derived while fitting the observed echo-power profile to Hagfors Law derived templates. A value of 99.99 for this field means the field is undefined for this record and should be ignored." END_OBJECT = COLUMN END_OBJECT = PV_RADAR_TABLE END