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DSX

ResourceID
spase://SMWG/Observatory/DSX

Description

Demonstration and Science Experiments(DSX) Satellite When launched in 2008, the Demonstration
and Science Experiments (DSX) spacecraft will conduct basic research designed to significantly advance
Dept. of Defense capability to operate in the harsh radiation environment of medium earth orbit (MEO).
The ability to operate effectively in the MEO environment significantly increases the DOD capability to
field space systems that provide persistent global targeting grade space surveillance, high speed,
satellite based communication, lower cost global positioning system navigation and protection from
space weather on a responsive satellite platform. The three DSX experiments areas are: (1) Wave
Particle Interaction Experiment (WPIx), which will research the physics of very low frequency (VLF)
transmissions in the magnetosphere and characterize the capability of natural and man made VLF waves
to reduce space radiation (2) Space Weather Experiment (SWx), which will characterize and model the
space radiation environment in MEO, an orbital regime attractive for future DOD and commercial missions
(3) Space Environmental Effects (SEE), which will investigate and characterize the space weather effects
on spacecraft electronics and materials DSX uses a modular structure design that allows for launch either
as a primary satellite on a conventional launcher like the Minotaur, or as a secondary payload on a
larger rocket such as the evolved expendable launch vehicle (EELV). For the EELV launch scenario, the
EELV secondary payload adapter (ESPA) ring is upgraded to provide host spacecraft functions with the
addition of a host spacecraft bus (HSB). The experiment payloads are located in a payload module attached
to the ring opposite the HSB. Unlike the traditional ESPA approach, where individual satellites
separate from the ESPA ring to become free flyers, DSX's HSB and payload module remain attached to the
ring and are deployed as a single integrated spacecraft. For launch on a dedicated rocket, the HSB
and payload module are removed from the ESPA and are directly attached to one another in a stacked
configuration. DSX is baselined to be ready for launch in October 2008 and is seeking an elliptical
orbit of 6,000 by 12,000 kilometers with a mid inclination. In addition, the spacecraft is designed
for one year of orbital operations. The WPIx will transmit and receive VLF waves in the 10 to 50
kilohertz range, and quantify their effect on the trapped electron populations in the magnetosphere.
In addition, DSX will use ground transmitters and other space receivers to measure critical parameters
such as VLF injection across the ionosphere and the far field radiated patterns. The SWx will characterize
the high and low energy electron and proton fluence, radiation dose rates, local magnetic fields and pitch
angle distribution in the ''slot region'' orbit located near an altitude of 10,000 kilometers, between the
inner and outer Van Allen radiation belts. It is an attractive orbit for future communications and
surveillance satellites because it has a low radiation dose rate and sufficient altitude to allow
for global coverage, but yet is four times closer than geostationary (GEO) satellites, which increases
communications speed by a factor of eight. This attractive orbit has remained largely unexplored,
with most commercial, military, and science satellites opting for low earth orbit (LEO) or GEO orbits.
The SEE consists of NASA's Space Environment Testbed (SET) and several AFRL developed photometers and
radiometers. SET features four smaller experiments designed to investigate radiation effects on
electronics such as field programmable gate arrays and linear devices. The AFRL instruments will
directly measure the radiation induced degradation of the optical and thermal properties for several
spacecraft materials of interest. DSX will benefit the warfighter by significantly enhancing understanding
of the MEO environment, with particular emphasis on the ''slot region,'' which is attractive for future
space surveillance and high speed communication. In addition, DSX will perform the basic research
needed to assess the DOD's ability to actively regulate agitations to the space weather environment
that currently cause accelerated degradation of critical space assets.

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Details

Version:2.2.2

Observatory

ResourceID
spase://SMWG/Observatory/DSX
ResourceHeader
ResourceName
DSX
AlternateName
Demonstrations and Science Experiment
ReleaseDate
2019-05-05 12:34:56Z
Description

Demonstration and Science Experiments(DSX) Satellite When launched in 2008, the Demonstration
and Science Experiments (DSX) spacecraft will conduct basic research designed to significantly advance
Dept. of Defense capability to operate in the harsh radiation environment of medium earth orbit (MEO).
The ability to operate effectively in the MEO environment significantly increases the DOD capability to
field space systems that provide persistent global targeting grade space surveillance, high speed,
satellite based communication, lower cost global positioning system navigation and protection from
space weather on a responsive satellite platform. The three DSX experiments areas are: (1) Wave
Particle Interaction Experiment (WPIx), which will research the physics of very low frequency (VLF)
transmissions in the magnetosphere and characterize the capability of natural and man made VLF waves
to reduce space radiation (2) Space Weather Experiment (SWx), which will characterize and model the
space radiation environment in MEO, an orbital regime attractive for future DOD and commercial missions
(3) Space Environmental Effects (SEE), which will investigate and characterize the space weather effects
on spacecraft electronics and materials DSX uses a modular structure design that allows for launch either
as a primary satellite on a conventional launcher like the Minotaur, or as a secondary payload on a
larger rocket such as the evolved expendable launch vehicle (EELV). For the EELV launch scenario, the
EELV secondary payload adapter (ESPA) ring is upgraded to provide host spacecraft functions with the
addition of a host spacecraft bus (HSB). The experiment payloads are located in a payload module attached
to the ring opposite the HSB. Unlike the traditional ESPA approach, where individual satellites
separate from the ESPA ring to become free flyers, DSX's HSB and payload module remain attached to the
ring and are deployed as a single integrated spacecraft. For launch on a dedicated rocket, the HSB
and payload module are removed from the ESPA and are directly attached to one another in a stacked
configuration. DSX is baselined to be ready for launch in October 2008 and is seeking an elliptical
orbit of 6,000 by 12,000 kilometers with a mid inclination. In addition, the spacecraft is designed
for one year of orbital operations. The WPIx will transmit and receive VLF waves in the 10 to 50
kilohertz range, and quantify their effect on the trapped electron populations in the magnetosphere.
In addition, DSX will use ground transmitters and other space receivers to measure critical parameters
such as VLF injection across the ionosphere and the far field radiated patterns. The SWx will characterize
the high and low energy electron and proton fluence, radiation dose rates, local magnetic fields and pitch
angle distribution in the ''slot region'' orbit located near an altitude of 10,000 kilometers, between the
inner and outer Van Allen radiation belts. It is an attractive orbit for future communications and
surveillance satellites because it has a low radiation dose rate and sufficient altitude to allow
for global coverage, but yet is four times closer than geostationary (GEO) satellites, which increases
communications speed by a factor of eight. This attractive orbit has remained largely unexplored,
with most commercial, military, and science satellites opting for low earth orbit (LEO) or GEO orbits.
The SEE consists of NASA's Space Environment Testbed (SET) and several AFRL developed photometers and
radiometers. SET features four smaller experiments designed to investigate radiation effects on
electronics such as field programmable gate arrays and linear devices. The AFRL instruments will
directly measure the radiation induced degradation of the optical and thermal properties for several
spacecraft materials of interest. DSX will benefit the warfighter by significantly enhancing understanding
of the MEO environment, with particular emphasis on the ''slot region,'' which is attractive for future
space surveillance and high speed communication. In addition, DSX will perform the basic research
needed to assess the DOD's ability to actively regulate agitations to the space weather environment
that currently cause accelerated degradation of critical space assets.

Contacts
RolePersonStartDateStopDateNote
1.GeneralContactspase://SMWG/Person/Gregory.P.Ginet
2.GeneralContactspase://SMWG/Person/Michael.A.Xapsos
3.GeneralContactspase://SMWG/Person/Jon.Schoenberg
4.GeneralContactspase://SMWG/Person/Aaron.L.Adler
5.GeneralContactspase://SMWG/Person/Mark.R.Scherbarth
6.GeneralContactspase://SMWG/Person/Durand.Smith
InformationURL
Name
Proceedings of Society of Photographic Instrumentation Engineers Article
URL
Description

Detailed information on AFRL's Demonstration and Science Experiments (DSX) mission.

Location
ObservatoryRegion
Earth.Magnetosphere.RadiationBelt
ObservatoryRegion
Earth.Magnetosphere