Introduction
Albatross is a computer program for interactive visualization
and analysis of the
UltraViolet Spectrometer
(UVS) and
TeleVision
Camera (TV) from the
Mariner
Mars 1971 (MM71) spacecraft.
The program (written in IDL) allows
the user to view any location of any size of the surface of Mars. The
surface can be one of topography (MGS MOLA), visual wavelength
photographic (Viking MDIM), thermal inertia (MGS TES), or geology
(USGS GEO).
On top of the surface, the footprints of the UVS are displayed. Moving
the mouse pointer near a footprint shows a plot of the reflectance as
a function of wavelength. Optionally, the ratio of one footprint to
another can be plotted.
Finally, the TV image associated with each UVS footprint can be
retrieved from the Internet and displayed.
Contact Ken Mankoff
(mankoff [at] lasp [dot] colorado [dot] edu)
with questions, comments, and bug reports
The
Mars Data Conglomerator may also be useful. It provides the same data
minus the UVS footprints, and no download is required.
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Documentation
Read the Albatross tutorial (HTML)
Read the IDL Documentation (ASCII text)
For information on the TV subsystem, read
JPL Technical Memorandum 33-585: Mariner Mars 1971 Television
Picture Catalog
Volume I (PDF, 180MB),
Volume I, Addendum I (PDF, 25MB)
Volume II (PDF, 110MB),
Volume II, Addendum I (PDF, 90MB)
Go to the Mars Data
Conglomerator website to view the surface of Mars with multiple
datasets, and learn more about the backgrounds used in Albatross
For information on the processing done to create this dataset, and how
to use the raw dataset without the Albatross software, read the
README, the
README.processing and the
README.usage (ASCII text) files.
For locations of surface features, consult:
International Astronomical Union (HTML)
Labeled MOLA map (PDF, 515K)
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