Magellan Radar System (RDRS)
ODE: Venus
Mission: Magellan
Instrument: Magellan Web Page
PDS Geosciences Node: PDS Source Information
RDRS Derived Data Products that use the PDS4 standard:
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Type |
Description |
PDS4 Bundle |
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Full-Resolution Mosaicked Data Image Record (F-MIDR) are mosaics of full-resolution image swaths (F-BIDRs) covering selected areas of the planet. |
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The C1-MIDRs are Compressed resolution MIDRs made from CBIDRs and have a pixel size of 225 m. |
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The C2-MIDRs were reduced in pixel size by a factor of three relative to C1-MIDRs. |
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The C3-MIDRs were reduced by another factor of three relative to that of C2-MIDRs. |
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Polar MIDRs. |
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Altimeter and Radiometry Composite Data Records (ARCDRs) Altimetry data (ADF) |
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Altimeter and Radiometry Composite Data Records (ARCDRs) Radiometry data (RDF) |
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The ANF contains the results of inverting the time and frequency spectra of a single orbit of Magellan altimetry, from the ALT-EDR product, by means of the accompanying Geometry Matrix File (GMF). The ANF contains a CCSD header, a keyword and value SFDU, a binary header record SFDU, and one or more binary data record SFDUs, sandwiched between starting and ending marker SFDUs. |
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The EDF contains measurements of the microwave emissivity of the Venus surface, obtained from the radiometer mode of the Magellan radar sensor. The EDF contains a CCSD header, a keyword and value SFDU, a binary header record SFDU, and one or more binary data record SFDUs, sandwiched between starting and ending marker SFDUs. |
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The NFF contains the results of fitting the radar scattering cross sections contained in the accompanying Altimetry Inversion Data File to one or more theoretical models. The NFF contains a CCSD header, a keyword and value SFDU, a binary header record SFDU, and one or more binary data record SFDUs, sandwiched between starting and ending marker SFDUs. |
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The OHF identifies the orbit number, time frame, and orbital geometry for one Magellan orbit. The OHF contains only a CCSD header, a keyword and value SFDU, and a binary header record SFDU. |
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The OIF contains the results of fitting the radar backscatter cross-section measurements of a single Magellan orbit, from the oblique sinusoidal (polar) image file of the C-BIDR or F-BIDR product, to a quadratic function, along with a histogram of pixel values used in the fit. The OIF contains a CCSD header, a keyword and value SFDU, a binary header record SFDU, and one or more binary data record SFDUs, sandwiched between starting and ending marker SFDUs. |
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The SIF contains the results of fitting the radar backscatter cross-section measurements of a single Magellan orbit, from the sinusoidal image file of the C-BIDR or F-BIDR product, to a quadratic function, along with a histogram of pixel values used in the fit. The SIF contains a CCSD header, a keyword and value SFDU, a binary header record SFDU, and one or more binary data record SFDUs, sandwiched between starting and ending marker SFDUs. |
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Global Emissivity Data Record from Global Topography and Surface Property Set (GXDR) More Information: |
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Global Reflectivity Data Record from Global Topography and Surface Property Set (GXDR) More Information: |
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Global Slope Data Record from Global Topography and Surface Property Set (GXDR) More Information: |
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Global Topography Data Record - Global Topography and Surface Property Set (GXDR) This is an ODE Logical Product. NOTE: These products were initially distributed on tape and then CDs. The documentation terminology still reflects this form of distribution. More Information: |
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Global Vector Data Record (GVDR) - The GVDR is a sorted collection of scattering and emission measurements. The sorting is into a grid of equal area 'pixels' distributed regularly about the planet. For data acquired from the same pixel but in different observing geometries, there is a second level of sorting to accommodate the different geometrical conditions. The 'pixel' dimension is 18.225 km. The GVDR is presented in Sinusoidal Equal Area (equatorial), Mercator (equatorial), and Polar Stereographic (polar) projections. This is an ODE Logical Product. NOTE: These products were initially distributed on tape and then CDs. The documentation terminology still reflects this form of distribution. More Information: |
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Using a fully automated process, the left-left stereo data collected by Magellan were used to generate topography for ~20% of the planet. The map was generated by Robert R. Herrick at the University of Alaska, Fairbanks. Please see the document for more information. |
RDRS Derived Data Products that use the PDS3 standard:
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Type |
Description |
PDS3 Data Set |
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Full-Resolution Basic Image Data Record - The F-BIDRs are full-resolution images in the form of long, narrow, almost pole-to-pole swaths. These swaths are pieced together to generate the image mosaics (F-MIDRs, C1-, C2-, and C3-MIDRs) for easier viewing. This is an ODE Logical Product. NOTE: These products were initially distributed on tape and then CDs. The documentation terminology still reflects this form of distribution. More Information:
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Compressed-Resolution Basic Image Data Record - The C-BIDRs are compressed-resolution image swaths. These swaths are pieced together to generate the compressed image mosaics (C1-, C2-, and C3-MIDRs).. This is an ODE Logical Product. NOTE: These products were initially distributed on tape and then CDs. The documentation terminology still reflects this form of distribution. More Information: |
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Full Resolution Radar Mosaics More Information: |
MGN-V-RDRS-5-DIM-V1.0 |
More information about the Magellan mission can be found in:
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R. S. Saunders, A. J. Spear, P. C. Allin, R. S. Austin, A. L. Berman, R. C. Chandlee, J. Clark, A. V. Decharon, E. M. De Jong, D. G. Griffith, J. M. Gunn, S. Hensley, W. T. K. Johnson, C. E. Kirby, K. S. Leung, D. T. Lyons, G. A. Michaels, J. Miller, R. B. Morris, A. D. Morrison, R. G. Piereson, J. F. Scott, S. J. Shaffer, J. P. Slonski, E. R. Stofan, T. W. Thompson, and S. D. Wall, Magellan Mission Summary, Journal of Geophysical Research, Vol. 97, NO. E8, PP. 13,067-13,090, 1992, doi:10.1029/92JE01397.