Services |
|
Geosciences Node Data |
|
Help |
|
Scheduled Maintenance |
This site may be down on Thursdays
between 7:00 and 9:30 pm Central Time for maintenance.
|
|
2001 Mars Odyssey:
Radio Science
Odyssey Radio Science data
sets are produced by Richard Simpson, PDS Radio Science Subnode at Stanford
University, and archived by the Geosciences Node.
These volumes contain archival raw, partially processed, and
ancillary/supporting radio science data acquired during the Mars Mapping phase
of the 2001 Mars Odyssey mission. The radio observations were carried out using
the Odyssey spacecraft and Earth-based receiving stations of the NASA Deep Space
Network (DSN). The observations were designed to provide information for the
Odyssey Navigation Team to reconstruct and predict the spacecraft trajectory.
They may also have value in improving the model of the gravity field of Mars.
Each volume contains data from part of the mapping period. The Mapping phase
began in February 2002 and was scheduled to run for one Mars year. Data are
organized in approximate chronological order; receipt of data at Stanford was
generally more important in determining placement than strict order of
generation or applicability. An index table is included with each volume,
listing each file in the volume; a separate cumulative index table shows all
files within the set of volumes.
Radio Science Data |
Data acquired in |
2016 |
Data acquired in |
2015 |
Data acquired in |
2014 |
Data acquired in |
2013 |
Data acquired in |
2012 |
Data acquired in |
2011 |
Data acquired in |
2010 |
Data acquired in |
2009 |
Data acquired in |
2008 |
Data acquired in |
2007 |
Data acquired in |
2006 |
Data
acquired in |
2005 |
Data acquired in |
2004 |
Data acquired in |
2003 |
Data acquired in |
2002 |
Note
The Odyssey Project has no formal Radio Science team; therefore there has
been no formal scientific review of these data. These data are being archived by
the PDS Radio Science Subnode to make the data equally available to all who
might be interested. These data will be put into the public domain as quickly as
possible in order to make it most useful to the largest number of people.
If you note omissions and/or errors, please make notes and send them to Dick
Simpson (rsimpson@magellan.stanford.edu)
and we will either try to make the repairs and/or ensure that the deficiencies
are not repeated on future volumes. This will constitute the PDS "peer review"
by which the suitability of the volumes for long-term archive is judged.
|