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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