Full text: Commissions I and II (Part 4)

  
  
  
  
  
  
  
  
184 RECENT DEVELOPMENT OF APPROXIMATE INSTRUMENTS, DISCUSSION 
g. Stereometer instruments with other correction devices. 
(Stereographometro Nistri, Stereomicrometer Santoni). 
I myself have many objections against this classification. I should like to have amend- 
ments. A classification on precision, I think is not very practical. 
3. Evaluation of instruments of this nature relative to *exact" restitution instruments. 
Prof. Gotthardt's publications may be a starting point in this discussion. Related to 
this discussion we may deal with the question of the future of approximate instru- 
ments. Those who cannot see any future are reminded of the fact that about the 
whole U.S.S.R. for instance, was mapped with instruments of this nature. 
4. What is the opinion of the panel about using (approximately) rectified photographs 
in instruments of this type? 
Will it be possible to use also superwide-angle lenses then? 
(Question suggested by Mr. E. Santoni.) 
Discussion 
Mr H. C. ZorN: May 1 first introduce the 
members of this panel to you. On my right we 
have Mr Baboz; on the left is Mr McMillen 
from the United States; and at the end is Mr 
Santoni from Italy. 
The members of this panel have agreed to 
pool the available time for their lectures and 1 
will thus give a short review of the contents. I 
will try to list out of those papers the main 
points of interest about which a discussion may 
be necessary. 
The papers offered for discussion are, first, 
one by Mr Santoni; second, that of Mr Baboz; 
then one from Mr McMillen; and another one 
has been added, somewhat late, from Mr 
Makarovic from Jugoslavia. Is Mr Makarovic 
present at this moment? (Mr Makarovic then 
joined the members of the panel on the plat- 
form.) 
My own publication, as it appears in Photo- 
grammetria, B, will be integrated in my present 
talk. First of all, I would like to say a few words 
about Mr Santoni’s paper called, “Le domaine 
d’emploi des appareils de restitution non fondés 
sur une reconstruction rigoureuse des faisceaux 
perspectifs”. In my opinion, this paper belongs 
mainly, in fact, to Commission IV because it 
deals with the application of instruments more 
than with the instruments themselves. However, 
there are some points of interest in it. The main 
conclusions of Mr Santoni are that instruments 
of third order will be used for map revision, not 
only of small-scale but also of large-scale maps. 
It follows that those instruments will be used 
for new map-making, and it may be an idea in 
that respect to use rectified photographs. If we 
use rectified photographs, then it may also be 
possible to use superwide-angle photography, 
in those instruments which will not take them 
normally, for example the stereomicrometer of 
Mr Santoni. 
This raises the point that we must have a 
rectifier. I think we must have a 1 : 1 rectifier. 
Maybe, the big ones can also be used. I do not 
know much about the application of that. After 
my talk, I should like to put to Mr Santoni the 
following question: which rectifier do you 
suggest, a telescopic one or the normal one 
which we all know? 
Mr Santoni wants to use for his rectification 
data, given either by solar periscope or aerial 
triangulation, so that the ¢ and the c can be 
introduced into the rectifier. 
Mr Baboz’s paper deals with the Stéréoflex, 
and the first statement in his paper is that for 
small-scale maps the interpretation of the ter- 
rain forms is more important than the metric 
value of it. That is a very acceptable statement. 
It may be somewhat indefinite, and if there is 
time available maybe some of you will want to 
comment on this statement. I had hoped to be 
able to use a slide of this instrument just to show 
you what we are talking about, but apparently 
we failed in getting the slide here in time, so I 
am afraid you will have to use your imagination. 
However, I think the majority of you know the 
instrument. The negatives are in a vertical posi- 
tion and you have two semi-transparent mirrors 
in front of you. You look through and against 
those mirrors, so that you see the two photo- 
graphs stereoscopically, and at the same time 
you see the floating mark on the table just over 
the pencil or the connecting point of the pan- 
tograph. The main thing you will notice is that 
we are using here an affine model, so that means 
we have not introduced a proper principal dis- 
tance but another distance of about 300 metres, 
and that makes that model deformed. 
This proportion between the horizontal and 
vertical scale can easily be computed, so in 
practice this is not a disadvantage, only we 
understand that in this instrument also there are 
model deformations. At the Institut Géogra- 
phique National in Paris this instrument has 
  
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