Telescope quadrant error
RESTRICTED
to the rate quadrant and for that reason would
arrive at the set actual range angle position of
the rate quadrant
too soon; (2) second,
because of
the acceleration of the rate of drive
of the tele-
scope quadrant, it wili be travelling
too fast
toward the
quadrant; that
sighting
angle changes more
angle chases e be slowliven at arnet 37°a 37%
sighting angle.
2.
The same
reasoning leading to
an opposite
conclusion is followed where the optics are to the
rear of vertical when the telescope guadrant is at
zero degrees.
3. When the
position of the transverse
hai r
is out of relationship to the position of the
telescope quadrant, it is obvious that the optics
will not be driven toward vertical at the
rate that the sighting angle changes. This is
because of the acceleration of the rate of drive
of the
telescope quadrant.
The quadrant will
drive at the
rate
the sighting
changes only when
it is set the same
angle
ing
angle. Therefore, this is another of the three
cases in
which
synchronization is impossibie,
it is
the most important
example.
The remaining
example is that of
erratic disc speed.
4. The transverse hair may be in the verti-
cal
with the
telescope
quadrant at zero, and yet
when
the optics
are being opened toward maximum
sighting angle,
the
transverse hair may get
out of
relationship to the telescope
quadrant.
This will
occur only when
of foreign matter is on
one of the sheaves and it begins to contact the
cable when the
optics are opened up to that
point,
or it will occur where there
a kink in the
cable and only
then when that kink begins to con-
tact one of
The transverse hair
should
always be at exactly the same setting
the telescope quadrant throughout the
entire
range
quadrant.
rate
is,
the
the
optics
are
being
driven
at
a
rate
for
a
the
sight-
and
a
piece
is
the
sheaves.
of
the
telescope
214