The need for large numbers of sensor platforms to fulfill the
total coverage of the Federation Sensor Network has led to the
development of mass produced sensor platforms, as opposed to the early
days of the federation where each platform was unique.
The
movement to a mass produced sensor platform system meant that a standard
reliable product could be distributed, which would behave in known ways,
as it would be tried and tested. Also these platforms are now made to
accept plug-in replacements or upgrades, which greatly extends a
platforms lifetime, as improved instruments could be easily installed
without expert knowledge, this also means that the maintenance times on
these platforms is also much reduced.
Despite
the mass production of sensor platforms, there is no one ubiquitous
design, there are in fact many different designs which are mass
produced, these roughly fall into three different categories, these are
system sensors, close system sensors, and specialized platforms. Each of
these categories occupies a different placement within a system, and
have different sensors accordingly.
The
most powerful and most numerous are the system sensor platforms (SSPs),
this type of platform lies well outside of the systems sun usually on
the boundary of the Oort cloud. Each system has at least six of these
platforms, this minimum number provides very good coverage (when
arranged 90°
apart from each other, the points of an octahedron), but the addition of
further sensors greatly improves resolution as sensors can cooperate
together.
This
type of sensor platform is dominated by the large mass sensors, that
allow it to very accurately detect spatial curvature, so much so that a
single platform can detect the normal above light drive of a small craft
over half a light year away. The mass sensors are divided into two
different types, the most sensitive are the stacked mass sensors, which
are the most powerful and sensitive types, though there field of view is
very limited, these sensors are responsible for the large spires on
these deep space platforms. The other type which are in effect simpler,
are radial mass sensors, these project outwards from the platform, and
the whole structure spun. Though the resolution of these sensors is not
as good over distance as a stacked mass sensor, they give an
omnidirectional coverage, and in certain respects are better for
determining small objects. Both of these large mass sensors are affected
by heat, and perform much better in deep space, which is why they have
come to dominate the system sensor platforms.
This
type of platform also has a standard range of other instruments,
generally including, radio, infrared and optical telescopes, and
infrared, visible and ultraviolet spectrometers. Most system sensor
platforms do not carry highly sophisticated magnetometers or particle
analyzers, though they carry powerful radar sounding equipment. These
other instruments are second to the mass sensors but increase the
versatility of the platform.
The
second type of platform are the close system sensor platforms (CSSPs),
these platforms unlike the deep space SSPs are place usually in the
ecliptic and usually not further than 20 AU from the systems star. These
sensors are unsurprisingly designed to monitor the planets of the system
and the sun, and where there mass sensors are cruder than the SSP’s
the other instruments are much more advanced. The most powerful tools
that the CSSP’s have are the range of telescopes that they carry,
which enable them to spy on the entire spectrum, however these powerful
telescopes rely on bending space to gather light, and the coils that
generate this curvature sorely interfere with mass sensors. For this
reason CSSPs have their mass sensors on long booms well away from the
platform, these sensors do not have the resolution of the SSP’s but as
most of the system’s objects lie with a few light hours of these
stations they are more than sufficient to provide high detail of
planets.
The
CSSP’s strength is in the electromagnetic spectrum, which makes it
ideal for monitoring the changing chemistry and weather of planets, and
also the behaviour of the central sun. There is no general number on the
amount of these type of platforms required per system, but even a
planetary blank system should have three to observe the systems sun, if
there are planets then more sensors stations would provide better
information, in very complex systems there can be upwards of twenty
CSSPs which not only have orbits around the sun but also around resident
planets.
The
last major category, the specialized sensor platforms cover the atypical
varieties that don’t fit into SSPs and CSSPs. There are many types of
specialized sensors platforms, some are specifically designed to monitor
stars, these are generally used if the sun’s behaviour is complex and
therefore under study. Another major type is the Planetary Mass Sensor
Platforms (PMSP), which take the powerful mass sensing instruments of
the SSPs are shield them for close system use, these types of platforms
are used to monitor tidal forces, or to observe subsurface volcanism and
water flow.
This
category also includes the fairly unique sensor platforms that buck the
mass produced trend, these are generally created because an object needs
particularly special observation, these are generally described as
Scientific Observation Platforms (SOPs).
Together
these three major types of platforms form the principle dedicated units
of the FSN, and contribute a permanent service, where as ship coverage
is used as and when. The maintenance time of the sensor platforms used
to be performed by contracted craft who would be refit with the relevant
manufacturing ability, but after 2155 these went into decline as the
Orca fleet began to assume this function, as their designs included the
necessary workshops. Most large sensor stations have supra-c propulsion
units, which means they deploy from the construction, and return for
reclamation, this means that the touring ships needs only perform
maintenance and refueling (CSSP’s may be solar powered but like other
platforms have fusion drives). It is estimated that sensor platforms
consume less than one ten thousandth of total fleet task forcing, and as
most of these runs are to check the health, and not to make repairs this
can be reduced greatly in times of crisis. |