DATA_SET_DESCRIPTION |
Data Set Overview
=================
All ALTITUDE data are packaged by periapsis number for each
aerobraking orbit. ALTITUDE data are provided in a table labeled
Pyyyy.tab where 'yyyy' is the four digit periapsis number.
Parameters
==========
Altitude: Units = km
Latitude: Units = degrees
Longitude: Units = degrees
Local Solar Time: Units = N/A
Longitude of the Sun: Units = degrees
Solar Zenith Angle: Units = degrees
Density: Units = kg/km**3
Sigma Density: Units = kg/km**3
Scale Height: Units = km
Sigma Scale Height: Units = km
Data
====
For each orbit, ALTITUDE data consist of an 11 by 10 array in the
file folder Pyyyy. Each row gives atmospheric characteristics at a
constant altitude. When applicable, inbound and outbound legs are
in separate rows. The altitude levels going from row 1 to row 11
are: periapsis, 1.26 nbar inbound, 1.26 nbar outbound, 130 km
inbound, 130 km outbound, 140 km inbound, 140 km outbound, 150 km
inbound, 150 km outbound, 160 km inbound, 160 km outbound. The
columns from one to ten are separated as follows: altitude,
latitude, longitude, local solar time, longitude of the sun, solar
zenith angle, density, sigma density, scale height, and sigma scale
height.
Processing
==========
Density and density scale heights are provided at reference
altitudes of periapsis, 1.26 nbar, 130, 140, 150, and 160 km. The
latter 4 are obtained by a least squares fit to the 40 point running
mean data sets that span 5 km on either side of a reference altitude
for both the inbound and outbound portions of the orbit. The values
at periapsis are obtained by a similar fit to all data within 10km
of the periapsis altitude. See [TOLSONETAL1999B].
Coordinate System
=================
Latitude and longitude are in the IAU Mars Centered Mars Equatorial
System. Altitude is above the IAU reference ellipsoid, with
a=3393.4 km and f=0.0052083 and including corrections for (4,4)
gravitational potential.
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CONFIDENCE_LEVEL_NOTE |
Confidence Level Overview
=========================
Standard deviations on density and scale height are based on the
formal covariance matrix for the linear regression of log density
and altitude. Data noise is assumed to be the standard deviation of
the fit.
Review
======
Comparisons were made with operational data sets. Deviations were
within expectations founded on archiving analysis that is based on
(4,4) gravitational potential and numerically integrated precision
trajectories that were not included in operational software.
Data Coverage and Quality
=========================
Data coverage during an aerobraking pass has varied throughout the
mission. Early in the mission, data were received for 500 seconds on
either side of periapsis. Later, the data started between 200 and
250 seconds before periapsis. This change was made to reduce
propulsion usage. Though this change somewhat reduced the accuracy
of determining the accelerometer bias, it had the advantage of
reducing the corruption of the data set with thruster firings while
still inside the detectable atmosphere. Not all orbits have yet
been included in current archiving data sets. Omitted orbits
include orbits where automatic data processing procedures did not
produce realistic answers. If required, many of these orbits can be
recovered by manual manipulation of data and data analysis
procedures.
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