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Release No. 95-98
STS-74 Photogrammetric Appendage Structural
Dynamics Experiment (PASDE)
Understanding How Solar Arrays Move in Space
What Is PASDE?
The Photogrammetric Appendage Structural Dynamics Experiment (PASDE)
was developed to study vibrations in a solar array attached to the
Russian space station Mir. The structural stability of solar arrays
is crucial for the International Space Station and future spacecraft.
PASDE data will help engineers understand how solar panels move
in space and how to improve future solar panel designs.
Video Camera Portion of the STS-74 Photogrammetric Appendage
Structural Dynamics Experiment (PASDE)
What Is Photogrammetry?
Photogrammetry involves photographing an object with one or more
cameras, from two or more locations. Since the object is viewed
from many different angles, three-dimensional coordinates can be
determined from the two-dimensional measurements on the film. This
is done by a process known as optical triangulation. Photogrammetry
provides a cheap, accurate and versatile means of measuring the
dynamic motions of an object. This technique, used by PASDE, will
enable engineers to discern movements as small as 1/10 inch in the
tips of the Mir solar arrays.
Why Fly PASDE Aboard The Space Shuttle?
The objective of PASDE is to develop and demonstrate advanced
photogrammetric techniques to monitor on-orbit movements. The use
of photogrammetric techniques for these on-orbit measurements can
be a low-cost alternative to standard instrumentation, such as accelerometers,
that need to be directly attached to the object being studied.
How Does PASDE Work?
Photographic images of two panels on a solar array on
the Mir Kvant-2 module will be recorded by six 8-mm video recorders,
along with a timing signal provided by the space shuttle. The timing
signal will allow the images of the solar arrays to be correlated
with planned test activities. Since these images are viewed from
different angles, three-dimensional position data can be obtained
from the film by optical analysis. The images and time histories
will be processed for different points on the solar array to determine
array vibrations and movements during the various on-orbit tests.
What Components Make Up PASDE?
PASDE is made up of three Get-Away-Special (GAS) canisters mounted
in the payload bay of the Space Shuttle Atlantis (STS-74). The six
PASDE video cameras, two per GAS can, will focus on two sections
of the Mir Kvant-2 solar arrays, photographing their movements during
docking, thermal expansion and other planned on-orbit events. In
the illustration below, the Kvant-2 module and its solar arrays
are to the right, near the tail of the orbiter, and the three PASDE
GAS canisters are shown in their positions in the payload bay.
How Will The PASDE Data Be Used?
The data returned by PASDE can be used to help eliminate unacceptable
vibrations on the solar arrays of the International Space Station
and other space structures. Additionally, analysis of PASDE data
may provide considerable cost savings by assisting spacecraft designers
in the development of the optimum weight and stiffness of future
solar arrays.
Who Funds PASDE?
The PASDE project is part of the International Space Station's
Phase-1 flight program to the Russian Space Station Mir.
A color photo of a PASDE camera array in a GAS can structure
(L-95-3413) and a color or B/W copy of the illustration shown above
are available upon request. For more information on the PASDE project,
please contact the NASA Langley Office of Public Affairs at (804)
864-6124.
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