Installation Plan
This evolving document is a discussion of the
items that will be installed and the telescope / observatory
modifications needed for the new TCS.
Feb 21 2008: A decision has been made that the
conversion effort will be done in a non-reversible manner
(i.e. no going back) starting on the July 14th summer shutdown.
During this period the hour angle, declination, focus, mirror cover opener,
and dome azimuth will be installed and running before on-site observers are
allowed.
Slit operation and weather will follow at a later date.
Boxes
There will be five boxes, one tower, and one long conduit installed.
- Control Box - in the computer room
- West Box - on the telescope on the west side
- East Box - on the wall mounts Wall replacing the two dome control boxes
- North Box - small junction box in floor tunnel
- Slit Box - replacing slit controller on dome (installed later)
- Weather tower - at south west corner of building (installed later)
- Semi circular conduit - from east near slip ring to cable run
To follow this discussion print out a copy of the
Cable diagram.
The following discussion is roughly in the order of installation.
Control Box
The control box
has been mounted in the computer room.
on the wall adjacent to window.
Here is a drawing.
A cable with a line plug comes out of the box and will have
to be connected to the UPS.
A cable (C22) to the UPS for the "UPS GOOD" signal is also needed.
A keyed power switch will be installed to turn off power.
Ethernet connection to the network is also needed.
The cables will pass down from the box into a wireway on the floor.
A strain relief of nature yet to be decided will be installed
on the wall.
One possibility is a piece of unistrut mounted on the wall with
long bolt to which coils of the unused cables can be hung.
The cover of the floor wireway will have to be cut to allow access
to the cables.
Hour Angle
Ripout: All the present motors, clutches,
differentials, gears and encoders will
be removed from the HA drive plate.
Wires can be cut as the items will not be re-used.
The only thing left will be, of course, the worm.
Unused cables will be removed.
Install: A belt pulley will be installed on the right of the worm.
This pulley has been machined to the proper diameter.
The motor mount will be mounted using an adapter plate into
the existing holes below
the right side of the gear.
The position encoder will be mounted directly off the left end of the worm
drive.
An adapter plate will be made to so the encoder mount can mount in
the existing screws and be at the correct location.
It is coupled to the worm using a xxx coupler.
A piece of unistrut will be mounted on the flanges on the drive cabin
using clamps.
East and west limit switches will be mounted on sliders.
These contain two levels (regular and failsafe).
Shorter pieces of unistrut will be mounted with molly screws in the
existing one inch diameter holes in the worm gear.
A dog will be mounted on this unistrut to set the activation point.
It is an MDM responsibility to set this point.
??A magnetic strip will be cemented on half the worm gear.
A Hall effect sensor mounted on the unistrut will act as the
home flag. This will be used to resolve the ambiguity in the
encoder index mark to determine the exact home position.
There are four cables: C1-limits, C2-encoder, C3-halls, and C4-motor that
will pass through the base of the telescope.
A small junction box maybe installed to consolidate the home flag and limit
connections.
A xx-diameter hole will be drilled to accommodate these cables.
This hole must also accommodate cables going to declination and
beyond.
The cables will then run into the pit, and through the pipes going
into the control room.
West Box and Primary Mirror Cover
Ripout: The existing
west box will be removed.
The paddle will be disconnected and possibly used later.
Obsolete cables will be removed.
Install: New receptacles will be installed
to supply 117 v.a.c. power that is used by instruments.
A new box
will be installed in the same location.
The new box will do the following:
- have manual mirror opener switches
- contain mirror opener circuits
- act as junction box for cables temperature sensors
- contain the tilt limit sensor
To install the mirror cover opener.
- the central drive bar between the cranks will be removed
- the cranks
on both sides will be replaced with a pulley
- the motor plate
will be mounted below
- motor drive cables connected to the West box
- closed limit switches will be mounted on both leaves using the
holes from the center guide plate
- open limit switches will be installed somehow
- all limit switches connected to West box
There are four cables: C17-mirror cover, C18-mirror cover power, C19-tilt,
C23-tel temp that will be dressed around the primary, down the
telescope center tube, out the HA cage and to the Control Box.
East Box and Dome Azimuth
Ripout:The the two existing
Dome control boxes
will be removed.
The two existing dome azimuth motors will be replaced.
The three vertical BX going upward from the box.
The vertical conduit from the floor will be preserved as it
has 117 v.a.c. power.
Install: A new box will be installed.
The box will contain:
- The klaxon
- an ESTOP switch
- the dome drive
- controls to manually turn the dome left and right
- slit controls to be determined
The 117 volt floor controls can go through the existing conduit
on the bottom.
The control cables will go through the semi circular conduit
to the control box.
For the dome azimuth drive:
- three phase versions of the dome drive motors
- A new encoder on the right angle drive
will be replaced see MDM007
- A three ABB phase drive will be installed in the "East Box"
- A homing switch dog will be installed at the slip ring location
The three phase drive will be supplied by the normal 117 v.ac.
mains power (non-UPS);this is already present in the conduit to the
existing boxes.
Great care in the wiring of this drive to the motors is needed
as it can radiate a lot of unwanted noise.
Cables C9-encoder and C12-encoder will be routed through the
semi-circular conduit to the control box.
Semi Circular Conduit
Install: A run of 1-1/2 inch IMT conduit will be
installed going from near
the slip rings on the upper east side of the dome, running
along the top of dome wall to the south where there will
be a sweep 90 and another run down to the cable inlet to
the control room.
A junction box will be installed at the top end.
It isn't clear what to do at the bottom end.
How is this conduit grounded?
North Box
Ripout: The present
North relay box will be
removed.
The only thing to be salvaged is the control wire that controls
the motion of the floor.
A temporary control box will have to fabricated for temporary use.
The wire from the floor switch can be cut.
All unused cables will be removed.
Install: A new much smaller box will be installed at some yet
to be specified location. One possibility is on the floor
itself at which point flexible conduit will have to be installed.
This box will have:
- floor control buttons
- push button to override the floor interlock to allow telescope motion
- junction between floor and pier interlocks to C27
The cable C27-interlocks will run down the large floor channel
southward to the control room.
Declination
Ripout:
All the present motors, clutches, gears and encoders will
be removed from the Declination drive plate.
All old cables will be removed from the central cable run.
Install:
- a belt pulley will be attached to one side of the worm
- the drive motor will be mounted to the side
- the position encoder will be mounted directly off the left end of the worm
drive
- north and south limit switches will be mounted somewhere, these will
contain two levels
- a homing device will be installed, one possible design is an optical
sensor with 180 degrees of black tape on the declination gear
The location of the motor holder has yet to be determined.
There are four wires (C5-limits, C6-encoder, C7-Halls, and C8- motor)
that will be dressed down through the axis and out
through the hour angle gear and onward to the Control Box.
Focus
Ripout: The existing
SloSyn drive motor.
Keep the limits switches.
All present cables.
Install:
- servo gearmotor with an internal encoder.
- the existing limit switches will be re-used
The motor mount will have to be designed and fabricated when
the motor is removed.
Three cables (C12 - limits, C13- encoder, C14 - motor) will have to be dressed
down the telescope sides, down the center tube of the telescope,
through the hole in the hour angle cabin and finally to
the control box.
Pier Interlock
Install:
A stainless steel cable will be installed from the top of
West pier down to the bottom where it will be connected
to a pull limit switch.
The top mounting will look like ???.
The bottom mounting will look like this.
Pulleys may be used if needed.
A turnbuckle tightner and other rigging has been purchased.
The limit switch will connect to the North box where it will
then go to the control box.
A second pull limit switch has been purchased for the East side, but
it isn't clear whether this need to be installed.
Temperature sensors
Install:
Temperature sensors (AD590s) will be installed at
various parts of the telescope these will be wired to
the West box and then connected to the Control Box
via cable C25.
At least one of the sensors will be mounted in a hole drilled
in the large tubes going up to the secondary.
The sensor will be covered with insulation so it will respond
to the metal temperature.
Another will be placed near the primary mirror.
Note the following will be installed after "local" observers
have returned.
The following will be needed for "remote" observers.
Slit Opener
This one is really vague since I don't know how the slit opener works.
The following things will be done.
- The slip rings will powered from the 117 v.a.c from the East Box
- RS485 telemetry and the Open signal will be wired to the Control Box
- The new control box
connected in place of the existing one
The C15-RS485 cable will be routed through the semi-circular conduit
to the control room.
One cable (cable C15) is then needed to go to the control box.
Weather station
I propose installing a tower at the South west corner of the
building.
See the location on the Dome sketch or
in this silly graphic.
The tower will a triangular radio tower set in a small concrete pier
similar to that shown here.
It will be twenty feet high which puts it about 11 feet above the
pony wall.
The top will have a lightning rod connected to the ground lead
that is already in place.
The weather instruments will be placed about a foot below on
a horizontal cross spar.
While this is not ideal weather indicating location, it should
be easy to erect, service and cable.
The following things have to be done:
- The above tower erected
- A new hole for the cables bored in the the building.
- Vaisala WXT510 weather station installed on conduit
- Vaisala DRD11a precipitation sensor installed on horizontal strut
- Cloud sensor installed on cross strut
- RS-485 connected (cable C22)
- Cloud sensor connected (cable C24)
- Precipitation sensor connected (cable C26)
MDM index