90 SURVEY NAVIGATION, AUTHOR'S PRESENTATION
Author's Presentation of the Paper
This Congress period celebrates the cente-
nary of aerial survey. In this one hundred years
important developments have taken place, and
a review of the present survey of navigation
shows some fascinating possibilities. The two
aspects of this paper are survey navigation as
such, and determination of camera orientation
elements in flight.
A variety of methods and instruments is
available for these processes, some of the older
existing methods can supply near-perfect photo
coverage or high accuracy camera orientation
data. On the other hand, some new systems
developed for supersonic speed navigation, for
space navigation and for automatic guidance
can now perform with an accuracy in flight
which is of the same order as the photogram-
metrist has always required for his orientation
elements. Time limitations do not permit elabo-
ration on any particular method now. You can
find the most important characteristics in my
paper, together with a comprehensive reference
literature.
At this moment, we shall restrict ourselves
to the most important conclusions.
I have put these conclusions together in a
few groups and I propose for them to be dis-
cussed in a few groups because we are dealing
with about fifteen or twenty different methods.
First of all, these conclusions are that in-
strumental navigation methods are in rapid
development to extremely high accuracies.
Many of them can provide for near-perfect sur-
vey navigation, and some of them even reach a
degree of accuracy which enables the determi-
nation of camera orientation elements at each
exposure station.
Now, about survey navigation. Of the various
possibilities, a line-of-sight navigation method
executed by a completely competent crew ac-
cording to sound principles has been shown to
supply near-perfect results. For instance, for
photographic surveys, IGN’s deviations in side
lap are not more than 5% side lap. Longitudinal
overlaps shall be kept to a minimum with only
a few per cent tolerance. This is in favour of an
appreciable reduction in the number of photo-
graphs. A longitudinal overlap can be reduced
by using overlap regulators, either of the visual
type or of the photo-electric automatic type. The
use of an intervalometertimer is economical on-
ly in small-scale photography. Once it is possi-
ble, or has proved to be possible, to keep over-
lap longitudinal and lateral within 5% , we come
to a possibility which I have called “bloc photog-
raphy”. Bloc photography, having all the nadir
points within 5% of each ideal position, should
in many cases be preferred to the normal strip
photography. It provides for points common to
six photographs, which is the optimum econo-
my of minor control. This can be obtained in
three ways: either by taking 90% overlap and
rejecting three-quarters of the photographs; or
it is obtained by individual pin-pointing of each
photograph; or it may be made possible by
coupling the exposure it commands to some
automatic guidance such as Doppler, Aerodist
or some other navigational computer.
Doppler navigation is reported to provide
appreciable saving in flight time, for instance
twenty-five per cent and forty per cent savings
are reported, and a great improvement in flight
line positioning as compared with coventional
operations.
In the near future, further improvements
may be expected from the combined use of the
Doppler with Inertial systems or Startracking,
and also from the use of Aerodist.
Now about camera orientation methods: for
elevation control we use statoscopes which give
flying height differences, mean error of the or-
der of 13 to 2 metres, and the radar altimeter
which provides for ground clearance, mean er-
ror of the order of 1 metre plus some metres
terrain influence. Both have proven their value
and a combination of the two is called A P R.
This provides for terrain elevations and profi-
les, spot heights, mean errors of the order of
3 to 3 metres at well-defined hard points. This
combination is recommended.
Regarding planimetric control, that can, as
we all know, be obtained by means of Shoran
and Hiran and Decca; a promising new devel-
opment is Aerodist. Its performance is expected
to have a mean error of the order of one metre
plus 1 : 100,000 of the distance. Verticality in-
formation can be obtained by means of solar
periscopes. Mean errors of the order of three
sexagesimal degrees are possible. The horizon
camera in its new version may prove to be of
great importance. It gives a verticality indication
which is expected to be of mean error of the or-
der of three sexagesimal degrees.
Another development of great potential in-
terest is the new automatic inertial vertical
which is now under trial. It gives vertical photo-
graphs with an expected mean error of three
sexagesimal minutes. Gyro verticals cannot be
and will not be sufficiently accurate for photo-
grammetric stereoscopic orientation, but they
can be
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