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The Magellan Mission
to Venus
The Magellan spacecraft, named after the
sixteenth-century Portuguese explorer whose expedition
first circumnavigated the Earth, was launched May 4,
1989, and arrived at Venus on August 10, 1990. During
the first 8-month mapping cycle around Venus, Magellan
collected radar images of 84 percent of the planet's
surface, with resolution 10 times better than that of
the earlier Soviet Venera 15 and 16 missions. Altimetry
and radiometry data also measured the surface topography
and electrical characteristics. During the extended
mission, two further mapping cycles from May 15, 1991 to
September 14, 1992 brought mapping coverage to 98% of
the planet, with a resolution of approximately 100m.
Precision radio tracking of the spacecraft measured
Venus' gravitational field to show the planet's internal
mass distribution and the forces that have created the
surface features. Magellan's data permitted the first
global geological understanding of Venus, the planet
most like Earth in our solar system.
Read more about this mission on the
NASA Mission Page.
All Magellan data sets are now available online.
The
Venus Orbital Data Explorer (ODE)
here at the Geosciences Node provides search
capabilities for Magellan data sets.
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Post-Mission Derived Data Sets |
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Full-Resolution Radar Mosaics (FMAPs) at the PDS
Imaging Node
- This archive was produced by the U.S. Geological
Survey after the Magellan mission ended. It contains
full-resolution mosaicked images covering about 92%
of the planet. Images were generated from the F-BIDR
products. This link leads to the PDS Imaging Node
web site.
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Stereo-Derived
Topography
(PDS4)
- This archive contains a map of stereo-derived
topography produced from the Magellan FMAPs.
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| Magellan Data Sets |
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MIDR: Mosaicked Image
Data Record (PDS4)
- The Magellan MIDR PDS4 archive bundle contains
products restored from the original PDS dataset
generated by the Magellan project in the 1990's.
Each MIDR have been reformatted into a single mosaic
from the original tiled products. Browse products
are also included and are stored as JPEG images. The
bundle includes all F-MIDRS (Full resolution) and
C1, 2, 3-MIDRs (Compressed resolution) products.
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GXDR: Global Topography
and Surface Property Data
(PDS4)
- The GxDR data set consists of MIT Altimetric
and Radiometric Global Data Records: the Global
Topography Data Record (GTDR), Global Emissivity
Data Record (GEDR), Global Slope Data Record
(GSDR), and Global Reflectivity Data Record
(GREDR).
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ARCDR: Processed
Altimetry and Radiometry Composite Data Record
(PDS4)
- Along track estimates of elevation, Fresnel
reflectivity, surface roughness, brightness
temperature, emissivity derived from Magellan
altimeter and radiometer data.
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Spherical Harmonic, Topography, and Gravity Data
(PDS4)
- This archive contains Magellan
spherical harmonic models of the
Venusian gravity and topography field,
and digital maps of Bouguer anomalies,
free-air gravity accelerations and
errors, geoid anomalies and errors, and
topography.
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F-BIDR: Full Resolution
Basic Image Data Record
- F-BIDRs are long, narrow, almost pole-to-pole
image swaths that form the basic Magellan image
data product. They are pieced together to form
mosaics (F-MIDRs) for selected areas of the
planet.
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C-BIDR: Compressed Basic
Image Data Record
- C-BIDRs are compressed image swaths that are
pieced together to form the compressed mosaics
(C1, C2, and C3-MIDRs).
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SCVDR: Surface
Characteristics Vector Data Record
(PDS4)
- The Surface Characteristics Vector Data Record
(SCVDR) is an orbit-by-orbit reduction of Magellan
scattering and emission measurements carried out
at Stanford University. The SCVDR includes
near-nadir scattering functions obtained by
numerical inversion from altimetry (ALT) echoes,
results (e.g., rms surface slopes and Fresnel
reflectivity) from fitting analytic functions to
those inversions, scattering function segments at
oblique incidence angles derived from synthetic
aperture radar (SAR) echoes, and estimates of
surface emissivity derived from thermal microwave
radiometry (RAD) measurements. The SCVDR is one of
several inputs to the Global Vector Data Record
(GVDR), a gridded summary of scattering results,
also produced at Stanford.
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GVDR: Global Vector Data
Record
(PDS4)
- The Global Vector Data Record (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.
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BSR: Bistatic Radar
(PDS4)
- The Magellan Bistatic Radar 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.
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ALT-EDR: Altimetry
Experiment Data RecordALT-EDR: Altimetry
Experiment Data Record
- The ALTEDR volumes contain Magellan ALT-EDR
(Altimeter Experiment Data Record) archive
products. They also contain documentation files
which describe the ALT-EDRs. Each ALT-EDR data
directory contains the raw altimeter data returned
from one orbit and the ancillary files necessary
to understand the data.
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LOSAPDR: Line Of Sight
Acceleration Profile Data Record (PDS4)
- This archive contains Magellan Cycle 4, 5 and
6 LOSAPDR (Line of Sight Acceleration Profile Data
Record) products. It also contains documentation
which describes the LOSAPDRs. Each LOSAPDR product
contains the results from processing of radio
tracking data of the Magellan spacecraft.
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Radio Tracking
Data
- This archive contains Magellan radio tracking
data in the form of ODF and TDF files.
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