10  The Primary Mirror Air-Conditioning System

10.1) Introduction
10.2) Hardware Description
10.2.1) The Sensors
10.2.2) The Cooling Units
10.3) The Control System
10.4) The User Interfacde and Controlling the Primary Mirror AC
10.4.1) Settings Sub-Window
10.4.2) Status Sub-Window
10.4.3) A Word on Dew Point, Mirror Cooling & Safety
10.5) Graphical Display of Environmental Parameters
10.6) Raw Data For Environmental Parameters


10.1  Introduction

The primary mirror is cooled to reduce the effect of "mirror seeing". When the mirror is warmer than the ambient air temperature, currents can deteriorate the seeing, adding 0.4" for every 1 C. The mirror should ideally be slightly cooler than the ambient air but when this condition cannot be met it is best to have the mirror considerably cooler than ambient. The best seeing is obtained when the dome air is continuously flushed with the ambient air. Make sure that the louvers and garage door are fully open and that the passageway doors are closed.

10.2  Hardware Description

10.2.1  The Sensors

The environment of the telescope and the ambient dome air are monitored by seven digital temperature sensors and three humidity sensors. 

The following points are monitored:

10.2.2  The Cooling Units

The air-conditioning unit is located outside to the south-east corner of the dome. This unit cools the refrigerant, turning it into a liquid. The cold liquid is then pumped to a series of coils located under the dome floor. A fan draws ambient dome air in through a floor register (located to the east of the telescope), passing across the cold coils, and reaches the primary mirror through a flexible insulated hose. A deflector at the end of the hose prevents "cold spots" from forming on the mirror. The air at the mirror-end of the hose is approximately 12 degrees C cooler than ambient during the summer months, and only 4 degrees cooler than ambient during the coldest winter months.

10.3  The Control System

Environmental parameters are passed along to the TCS Control System PC via two secondary (box b & box c) and one primary (box a) interface boxes.  Box b resides next to the AC system under the floor in the dome.  It is responsible for temperature readouts from the AC duct and coil.  It also provides control signals to the AC system via a relay bank.  Box c is easily visible on the north edge of the primary mirror cell.  It is responsible for the remainder of the environmental parameters.  It also transfers mirror cover status, which in turn provides interlocks to the AC system when the telescope is in use (AC system is overridden when the mirror covers are open).  Both of these boxes communicate via RJ45 cables with box a, which is located in the computer room.  Box a connects via USB to the TCS Control System PC, where the user interfaces with the system.  Using the Up/Down arrows on box a toggles the display through the various environmental parameters as well as the mirror cover status and AC system status.  The other buttons are unused.

Figure 10-1: Primary Interface Box (box a)
weather interface


10.4 The User Interface and Controlling the Primary Mirror AC

The user interface for environmental monitoring and control can be accessed from Options>Environmental Data/Control on the TCS Control System GUI.  This will bring up the window seen in Figure 10-2, below.  Typically, this window is left open on the desktop. 

Serial Port settings should load automatically as long as "Enable" and "Auto Enable" are checked (default).  If for some reason the settings are lost, they can be entered by clicking the "Settings" button.  Serial Port paramters are:

Just ignore the warning that the port is not available.  With the system enabled, functionality can be verified by simply watching the temperature values.  If they update, things are running.

Figure 10-2: Environmental Data/Control, Settings/Status
env1


10.4.1 Settings Sub-Window

The settings section of the page provides the user with control of the primary mirror AC system.  Typically, seeing can be optimized by cooling the mirror 1-2 degrees C lower than the ambient temperature during the night.  A good rule-of-thumb is to check for the low temperature for the previous night and cool to one degree lower than that.  To enter the desired temperature, enter the value in the 'Mirror Temperature Set Point" window and hit <enter>.  You should hear a chime.  The system will work to cool the mirror 1C lower than the desired set point before shitting the AC off.  The mirror is then allowed to warm to 1C above the desired set point before the system turns the AC back on.  This limits the duty cycle, and thusly the wear-and-tear on the AC system.  As an example, if the demand temperature is set to 10C, the system will cool until reaching 9C.  The AC will then shut off and remain off until the mirror reaches a temperature of 11C.

The settings section also provides for a series of override options.  Users should never have to force-set any components of the system so these should not be touched.

10.4.2 Status Sub-Window

The status section of the page provides the user with all the telescope environmental parameters, mirror cover status and AC system status. 

10.4.3 A Word on Dew Point, Mirror Cooling & Safety

The primary mirror cooling system will limit cooling to within 2 degrees of the dew point.  This is a safety to reduce the otential for condensation forming on the mirror surface.  However, the routine currently utilizes the dew point calculated using the temperature and humidity values at the center section of the telescope.  This tends to produce dew point readings that are a few degrees lower than seen outside.  If the humidity is relatively high (greater than ~60%), it is advisable to check the dew point value outside via the Weather Station Display (Figure 10-3) and set the mirror temperature setpoint accordingly.  Sensors for monitoring temperature and humidity (dew point) outside may be added to the system at a later date.

It should also be noted that some forecast weather systems, as well as monsoonal activity (seen from late June through early September) can result in quickly rising dew point.  For this reason, when observing when there is a chance of precipitable weather, it is highly advisable to keep close watch of outside dew point and adjust the mirror cooling accordingly.

Figure 10-3: Weather Station Display
weather display

10.5 Graphical Display of Environmental Parameters

The second tab on the Environmental Data/Control window provides graphical displays of any or all environmental parameters.  The system defaults to showing all trends, however some, such as Secondary, AC Coil and AC Ducts can be de-selected.  Whenever the TCS Control System software is restarted, the plots are wiped from memory and start new. 

Figure 10-4: Graphs Tab of the Environmental Data/Control Window
graphs

The plots provide a good reference for determining a set point for the mirror cooling.

Note that when observing starts in the early evening, the mirror warms up as it is exposed to the evening air, whose temperature is falling. When set correctly, the primary should remain below the dome ambient for the whole night, being about 0.5 degrees below at the end of the night.

10.6 Raw Data for Environmental Parameters

The last tab on the Environmental Data/Control window provides a spreadsheet display of all raw environmental data.  If desired, the data can be saved to file.

Figure 10-5: Reports Tab of hte Environmental Data/Control Window
Raw Data



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Updated: 2018Sep20 (Galayda/MDM)