Terriers
Tomographic Experiment using Radiative Recombinative Ionospheric EUV and
Radio Sources, also called STEDI 2 and UNEX 02
After launch the satellite experienced attitude control problems causing the
battery to discharge.
Prime
contractor
|
Boston
University
|
Platform
|
Aeroastro
|
Mass
at launch
|
125
kg
|
Mass
in orbit
|
|
Dimension
|
|
Solar
array
|
|
Stabilization
|
spin
stabilized
|
DC
power
|
31
W
|
Design
lifetime
|
1
year
|
The satellite bus is being built by AeroAstro while the instrument package is
produced by the Center for Space Physics at Boston University and the
University of Illinois at Urbana-Champain (UIUC). Cleveland Heights High School
is also constructing a small experiment to go on the satellite.
Terriers primary goal is to, for the first time, demonstrate meridional 2D
(latitude-altitude) and global 3D imaging of the ionospheric electron density
and thermospheric photo-emission profiles using EUV emissions and tomographic
techniques. Secondary goals of Terriers focus on the study of several
ionospheric and thermospheric phenomena through the use of this novel
combination of techniques and observations. As a tertiary goal, Terriers will
test the utility of long term solar EUV irradiance measurements using a new
technique that we have recently proven on a sounding rocket. GISSMO measures
the solar EUV, one of the primary sources for the upper atmosphere.
Telemetry: 2.2729 GHz
Might also use 150/400 MHz