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SLR-Mail No.1634

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Date:2007-12-26 12:22:00
Sender:Mark Davis, NRL <slrmail@dgfi.badw.de>
Subject:[SLR-Mail] No. 1634: URGENT
Author:Mark Davis, NRL
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SLR Electronic Mail 2007-12-26 12:22:00 UTC Message No. 1634
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Author: Mark Davis, NRL
Subject: URGENT

Atmospheric Neutral Density Experiment MAA Spacecraft Re-Enters

The Atmospheric Neutral Density Experiment (ANDE) Risk Reduction
flight was launched on Dec. 9, 2006 and deployed into orbit by the
Space Shuttle Discovery on Dec. 21, 2006. On Dec. 25, 2007 the MAA
(ANDERRA) spacecraft re-entered the atmosphere; the FCal (ANDERRP)
spacecraft is not expected to decay until April 2008. Thanks to the
international laser ranging service (ILRS) and amateur HAM radio
enthusiasts the ANDERR data set is extensive. The Naval Research
Laboratory would like to that all of the sites that participated in
data collection on the ANDERR MAA satellite and encourage continued
efforts for the remainder of the ANDERR FCAL orbital lifetime (~April
2008). The primary mission objective is to test the deployment
mechanism from the Shuttle for the ANDE flight in mid 2009 The
follow-on ANDE mission scheduled for launch in 2009 will consist of
two spherical spacecraft also fitted with retro-reflectors for SLR.
One of these spacecraft will also carry instrumentation to measure
the in-situ atmospheric density, composition and winds. Scientific
objectives of the ANDE risk reduction flight include; monitor total
neutral density along the orbit for improved orbit determination of
resident space objects, monitor the spin rate and orientation of the
spacecraft, provide a test object for the space surveillance network
(SSN) sensors, both radar and optical.

Each of the two ANDE missions consists of two spherical spacecraft
fitted with retro-reflectors for satellite laser ranging (SLR). The
constant and well-determined cross section and surface properties of
the ANDERR spacecraft provide an ideal set of objects for monitoring
atmospheric drag and the calibration of SSN assets. The ANDE risk
reduction mission spacecraft each contain a small lightweight payload
designed to determine the spin rate and orientation of the spacecraft
from on-orbit measurements and from ground based observations.

The 20th Space Control Squadron, USAF in Dahlgren, VA, processes US
Space Surveillance Network (SSN) radar observation data of the two
ANDERR spacecraft. The product is a set of vectors that is provided
to NRL, along with the radar observations, up to three times a day.
These state vectors merged with the SLR data and processed by
NRL’s OCEAN orbit determination software to produce a set of
ephemeredes. As a backup the radar data are processed at NLR using
Special-K orbit determination software. These ephemeris files are
reformatted into the consolidated prediction format used by the ILRS
tracking stations. This format consists of minute satellite state
vector (x, y, and z positions and velocities at a given time plus
other parameters) over the several day prediction period. These
predictions are distributed via the NASA CDDIS data center and the
European Data Center. Onboard sun sensor data and thermal data are
telemetered to the ground via HAM radio frequencies. These data are
collected worldwide by amateur HAM radio enthusiast and stored in a
database at NRL.

The spin rate of the MAA spacecraft was estimated by several
different methods; video from the STS-116 deployment, on-board
telemetry from the MAA spacecraft, observations from the AEOS
telescope on Maui, and satellite laser ranging (SLR) observations.
The four independent measures of the MAA spin rate were plotted
versus mission elapsed time in days and fit with an exponential
function. The results is a decay constant of -0.189.

It is clear that the ANDERR spacecraft are useful calibration targets
due to their well-characterized size and shape. The SLR observations
performed by the members of the ILRS have been used to augment the
radar data to constrain the accuracy and stability of the estimated
ballistic coefficient and to assess the accuracy of the predictions
with absolute confidence. The data show a consistent over estimation
of the density by the atmospheric models, NRLMSISE 2000 as well as
J70. The average in-track time bias at the 24-hour mark improved by
15.2% with a 39.9% improvement in standard deviation. While the
average fitted CD for J70 was closer to the analytic value, the MSIS
CD values have considerably less variation. The over specification of
total density is in agreement with the findings of Emmert and Picone
(JGR, 2004), who have shown a consistent decrease in thermospheric
density of the past three decades. The models are having a difficult
time properly capturing the effect of geomagnetic forcing (especially
at low end of the solar/geomagnetic forcing range), as correlations
are evident in the fitted CD values with the geomagnetic ap index.
The data set from the ANDERR mission will aide researchers in
improving the current atmospheric density an wind models.


Best Regards,
Andrew Nicholas

ANDE PI: Andrew Nicholas, NRL 7669, andrew.nicholas@nrl.navy.mil
SLR POC: Mark Davis, NRL 8123, mark.davis@nr.navy.mil
HAM POC: Bob Bruninga, USNA, bruninga@usna.edu

From: slrmail@dgfi.badw.de

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