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CHARA Array Operating Procedures\\ | CHARA Array Operating Procedures\\ | ||
- | Copyright © 2005-2018 The CHARA Team\\ | + | Copyright © 2005-2019 The CHARA Team\\ |
- | Last updated: | + | Last updated: |
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- | **Chapter 1:** === = Lab Protocol | + | **Chapter 1: ** Lab Protocol\\ |
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- | Picture_28.png Picture_29.png === 1.1 Lab Rules Intro ===\\ | + | 1.1 Lab Rules Intro\\ |
- | The CHARA optics lab is a building within a building and is intended to provide thermal and vibrational stability. The main goal of the CHARA lab rules is to keep all optics and equipment safe from any hazards. The crucial issue being misalignment of anything. The amount of dust and dander must be kept to a minimum. | + | The CHARA optics lab is a building within a building and is intended to provide thermal and vibrational stability. The main goal of the CHARA lab rules is to keep all optics and equipment safe from any hazards. The crucial issue being misalignment of anything. The amount of dust and dander must be kept to a minimum. |
- | A high-powered infrared laser is used for the delay line metrology. This is an eye hazard, so before entering the lab check to make sure the red light above the door is not on. If the laser is activated, it is a must to put on IR-protective goggles. If you are not sure, wear the goggles. | + | |
+ | 1.2 The Metrology Laser\\ | ||
+ | A high-powered infrared laser is used for the delay line metrology. This is an eye hazard, so before entering the lab check to make sure the red light above the door is not on. If the laser is activated, it is a must to put on IR-protective goggles. If you are not sure, wear the goggles. | ||
+ | |||
+ | 1.3 General Lab Rules\\ | ||
Please remember that:\\ | Please remember that:\\ | ||
Procedures in the lab must be followed closely and failure to follow these rules will result in loss of lab privileges.\\ | Procedures in the lab must be followed closely and failure to follow these rules will result in loss of lab privileges.\\ | ||
- | * Before entering the lab, you must have a reason or tasks at hand. * Lab booties/ | + | * Before entering the lab, you must have a reason or tasks at hand. |
+ | |||
+ | * Lab booties/ | ||
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- | **Chapter 2:** Version 2. August | + | **Chapter 2:** |
- | These are routine tasks to be performed in and around the lab every evening to prepare the array for regular observations. | + | |
- | Go into building, | + | 27 AUG 2012 by Judit, |
+ | |||
+ | Preparations in the Lab Prior to Observing\\ | ||
+ | These are routine tasks to be performed in and around the lab every evening to prepare the array for regular observations. | ||
+ | |||
+ | 2.1 Starting the vacuum pump for the light pipes | ||
+ | |||
+ | Go into vacuum pump shack. Flip on power switch for pump (wait for blower to go on) Open valve slowly (parallel to pipe means open) Note if fan cords are plugged into wall outlet to keep pumps cool. Note oil temperature when you start up. Oil temps below 20º C make for a labored start. Inform Larry if the oil temp is low and the heater did not run to bring the temp up before starting.\\ | ||
+ | Go into lab building, check pressures on Vacmon display. If pressure is higher than 100 torr in any of the lines, pump those lines only one at a time. Open valve a little, then come back to open fully. When all lines to be used are well below 100 torr, open all those valves. The final pressure should be 0.5 - 1.0 Torr in each line. The pump will normally bring all 6 lines down to .2-.3 Torr. The S1 and S2 lines leak the most during the day and will read the highest in the afternoon when you return, usually around 10 and 20 Torr. Note any unusual vacuum readings as they can indicate a leak beyond what is normal. Sometimes a line isn't pumped down the night before and can read higher than 30 Torr. Pump the highest ones down first as stated above. | ||
+ | |||
+ | 2.2 Filling IR cameras with LN2\\ | ||
Fill both chambers on the NIRO camera. Use the gloves and glasses provided on the shelf with the funnels and the thermos. It will normally take 1 liter of LN2 in the outer chamber and 1/2 liter in the inner chamber. Fill it until the LN2 bubbles out of the top. This camera is normally kept cool all the time, exceptions will be noted.\\ | Fill both chambers on the NIRO camera. Use the gloves and glasses provided on the shelf with the funnels and the thermos. It will normally take 1 liter of LN2 in the outer chamber and 1/2 liter in the inner chamber. Fill it until the LN2 bubbles out of the top. This camera is normally kept cool all the time, exceptions will be noted.\\ | ||
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- | Fill the other dewars ONLY if you were specifically asked to do so. Other IR cameras: JouFLU and Cali (the blue dewar on the JouFLU table).\\ | + | Record that you filled the camera |
- | \\ | + | |
- | Record that you filled the cameras | + | 2.3 Alignment of the light path to the telescopes\\ |
Go into the lab. The green alignment laser on the light source table is used. To open necessary guis, use laptops or the two tablets inside lab. Tablets are the newest hand held units and are located on the west and south walls plugged into chargers.\\ | Go into the lab. The green alignment laser on the light source table is used. To open necessary guis, use laptops or the two tablets inside lab. Tablets are the newest hand held units and are located on the west and south walls plugged into chargers.\\ | ||
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- | 2.3.1 In the lab (Beam Combination area) * Turn on power switch for alignment laser, and turn the key. * Above the tiptilt camera, turn on the Pico 3 controller.\\ | + | 2.3.1 In the lab (Beam Combination area) Turn on power switch for alignment laser, and turn the key. Above the tiptilt camera, turn on the Pico 3 controller. |
- | 2.3.2 Check the laser spots on the E table (at North wall of Beam Switching area) * on Laser Filter gui, select ND 0.0 * make sure VEGA periscope is UP * open LASER shutter on the SHUTTERS gui and open shutters for the beams you are going to use * using the VISBEAMS gui, move the laser to the first beam pair you will check, ie. Beams 1& | + | |
- | If the telescopes were used on the same beam on the previous night, the next steps may be very close and not need much if any adjustment.\\ | + | 2.3.2 Laser alignment to east table |
+ | |||
+ | Check the laser spots on the E table target | ||
+ | If the telescopes were used on the same beam on the previous night, the next steps may be very close and should | ||
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- | 2.3.3 Next check the dichroic | + | 2.3.3 dichroic |
- | 2.3.4 Check the spot on the rail target | + | |
- | 2.3.5 The periscope covers | + | NOTE: As of 2017 Jul 05, please align the dichroics following the instructions in {{: |
+ | |||
+ | \\ | ||
+ | 2.3.4 Checking | ||
+ | |||
+ | Put the rail target onto delay lines (toward back of the room from home sensor) | ||
+ | |||
+ | 2.3.5 IR alignments | ||
+ | \\ | ||
+ | 2.3.6 M10 Alignment | ||
+ | |||
+ | Go to a computer anywhere to check the beam remotely at the telescopes. Check Vacuum Monitor that the vacuum is below 20 torr. Open telescope gui from pull down menu. Click TV [ON] to open the camera window and click [M10AL] to change view to the M10 alignment view, click [M7 open] to open the M7 mirror cover. Center bright spot in beam on the black reference spot. You may need to adjust the IRIS or the TV brightness to see the bright spot well. [BEAM] cycles the iris from open to closed and gives a good idea of where the center of the spot is. To adjust the position, use Pico 2 to select, for example, E2M10 → [MOVE] (use large steps ~ 100). Note that the up, down, left, and right buttons do no correspond to the actual directions the spot will move. When the spot is centered, click [M7 close] to close the mirror cover * click TV [OFF] to close the window | ||
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- | 2.3.6 M10 Alignment: | ||
- | Go to a computer anywhere to check the beam remotely at the telescopes. * look at Vacuum Monitor, check that the vacuum is below 20 torr * open telescope gui from pull down menu * click TV [ON] to open the camera window * click [M10AL] to change view to the M10 alignment view, click [M7 open] to open the M7 mirror cover * you want to center bright spot in beam on the black reference spot * may need to adjust the IRIS to see the bright spot well. [BEAM] cycles the iris from open to closed and gives a good idea of where the center of the spot is. * to adjust the position, use Pico 2 to select, for example, E2M10 → [MOVE] (use large steps ~ 100) * Note that the up, down, left, and right buttons do no correspond to the actual directions the spot will move * when the spot is centered, click [M7 close] to close the mirror cover * click TV [OFF] to close the window\\ | ||
2.3.7 Labao wfs camera covers and labao shutters\\ | 2.3.7 Labao wfs camera covers and labao shutters\\ | ||
- | The labao camera covers should be kept off, but put the covers on gently any time when you need to put the small corner cubes in place at the BRTs to work with the internal sources to protect the cameras.\\ | ||
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- | **Covers on** when doing the following alignment steps in the lab: * IR mirror check to CLIMB or MIRC with alignment laser * beam combiner alignments with white light source | + | **Put the Covers on** gently |
+ | |||
+ | **Covers off** after you remove | ||
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- | The labao cameras (just like the tiptilt camera) are safe during pop changes as long as you do not open any labao shutters. You will notice increased counts on the labao cameras (just like in the tiptilt camera) whenever ND=0 alignment laser is going through the system, but this is not harmful as long as the labao shutters are closed. While observing none of the labao shutters need to be or should be opened. As usual, dim the laser after you are done with the pop change to protect any camera in the lab from ghost reflections and scattered laser light. | + | The labao cameras (just like the tiptilt camera) are safe during pop changes as long as you do not open any labao shutters. You will notice increased counts on the labao cameras (just like in the tiptilt camera) whenever ND=0 alignment laser is going through the system, but this is not harmful as long as the labao shutters are closed. While observing none of the labao shutters need to be or should be opened. As usual, dim the laser after you are done with the pop change to protect any camera in the lab from ghost reflections and scattered laser light. |
+ | |||
+ | 2.4 Alignment of the IR light toward beam combiners | ||
The IR mirrors on the beam samplers can be adjusted using Pico 2 controller to targets depending on which IR beam combiner is to be used.\\ | The IR mirrors on the beam samplers can be adjusted using Pico 2 controller to targets depending on which IR beam combiner is to be used.\\ | ||
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For CLIMB 1 and CLIMB 2, the removable 6-beam target should be placed in the clamps on the CLIMB table. This also applies to aligning CLIMB for fringe tracking for VEGA or fringe finding for PAVO.\\ | For CLIMB 1 and CLIMB 2, the removable 6-beam target should be placed in the clamps on the CLIMB table. This also applies to aligning CLIMB for fringe tracking for VEGA or fringe finding for PAVO.\\ | ||
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- | For MIRC or JouFLU, the same target should be placed in the clamps on the MIRC table. | + | For MIRCX, the same target should be placed in the clamps on the MIRCX table. |
- | Go to OPLE racks * turn on OPLE Power on top unit (top of left most rack) This is the VME. * then turn on power for surge protector (bottom of left most rack) * turn on power for amplifiers for cart movement and cable pullers and once the central red light on the VME rack goes out, turn on the Burleigh amplifiers for telescopes that will be used.\\ | + | |
- | On computer outside lab, bring up Primary Ople Server | + | 2.5 Starting up OPLE and Metrology |
- | Go inside lab to check carts * from pull-down menu, under GTK, open Primary OPLE GUI * click on [STATUS] | + | |
- | Check delay line wires on carts, sure nothing is on tracks\\ | + | Go to OPLE racks and turn on OPLE Power on top unit (top of left most rack) This is the VME. Turn on power for surge protector (bottom of left most rack), turn on power for amplifiers for cart movement and cable pullers and once the central red light on the VME rack goes out, turn on the Burleigh amplifiers for telescopes that will be used.\\ |
+ | To test cart motions: | ||
+ | Check delay line wires on carts, | ||
+ | \\ | ||
+ | On the Metrology table inside the lab, turn on two blue amplifiers for metrology laser (on button is labeled " | ||
+ | |||
+ | 2.6 Final steps in the lab | ||
+ | |||
+ | If using CLASSIC or CLIMB, turn on the black box above the NIRO computer, and then turn on the silver box below it on the same cart. Remove cover on camera. After lab is completely setup, you need to take off tiptilt cover if using lab tiptilt, but do so with only the dim lights on and the laser shutter closed so as not to blast CCD with light. | ||
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- | On the Metrology table inside the lab * Turn on two blue amplifiers for metrology laser (on button is labeled " | + | **Chapter 3: ** |
- | Back To Main Menu **Chapter 3: ** (edited 2012Aug29 | + | |
- | fig_monitors_new.jpg * Things should | + | 17 DEC 2019 by Norm |
- | Open Cosmic Debris, CD for short, | + | |
- | Set the instrument and settings on Cosmic Debris | + | Setting up Computer in the Control Room |
- | Establish connection between tiptilt and the telescopes. | + | |
- | Finish setting up tiptilt GUIs * Click re-open on the Tiptilt GUI. This will update the TT labels on the TT viewing screens from B1,B2,etc to the telescope names * Click on the [SERVO CONTROL] tab on the tiptilt GUI to bring up a second window and move to screen 5 with the telescope guis. * The Servo Control GUI allows you to turn ON the servo for the TT loop and make biases for individual beams (DBIAS and ZBIAS) | + | 3.1 General Overview of Control Room computer setup |
- | Turning on the metrology laser * Make sure that no one is in the lab. * Turn the Laser on using the metrology laser GUI. The [Laser Power] button will go from red to green. | + | |
- | Home each of the active carts * The carts must be homed before observing or else fringes will not be found. Do not forget this step or endless frustration will follow. | + | There are six computer screens which are now horizontally arrayed. |
+ | |||
+ | 3.2 Setting up for observing | ||
+ | |||
+ | Turn on the following from the POWER GUI: To change the setting on the power GUI, unclick LOCK, make change, re-click LOCK. Under RACK_2, turn on [METSCOPE] (button will turn green when ON). If observing with CLASSIC, turn on [NIRO CPU] and [CLS-DITH] on RACK_2. | ||
+ | |||
+ | 3.3 Servers | ||
+ | |||
+ | Servers can be opened | ||
+ | |||
+ | 3.4 Open Telescope guis, or obsgtks from icons on desktop | ||
+ | |||
+ | 3.5 Open GUIs required for observing from the menu under GTK or the desktop icons: Open Primary OPLE gui, Open Classic, Climb1, or Climb2 gui if needed, Open LDC1 and LDC2 if VEGA or PAVO programs are observing. | ||
+ | |||
+ | 3.6 Using the Cosmic Debris job sequencer | ||
+ | |||
+ | Open Cosmic Debris, CD for short, from the desktop icon. | ||
+ | Set the instrument and settings on Cosmic Debris. | ||
+ | Establish connection between tiptilt and the telescopes. | ||
+ | Finish setting up tiptilt GUIs * Click re-open on the Tiptilt GUI. This will update the TT labels on the TT viewing screens from B1,B2,etc to the telescope names. | ||
+ | |||
+ | 3.7 Turn on metrology laser and home the carts | ||
+ | |||
+ | Make sure that no one is in the lab. Turn the Laser on using the metrology laser GUI. The [Laser Power] button will go from red to green. | ||
+ | Home each of the active carts. | ||
+ | |||
+ | 3.8 Synchronizing the clocks | ||
+ | |||
+ | Synchronizing the clocks is very important for positional calculations of the telescopes and ople carts. | ||
+ | |||
+ | 3.9 | ||
+ | |||
+ | The following windows should be opened on computer screen | ||
+ | |||
+ | 3.10 | ||
+ | |||
+ | See the instruments page for information about starting different instruments at the beginning of the night:\\ | ||
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- | **Chapter 4: ** === = Observing Conditions ====\\ | + | **Chapter 4: ** === = Observing Conditions ====\\ |
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- | Picture_4.png | + | Picture_4.png === 4.1 Observing Conditions Intro ===\ \ In opening the CHARA Array, conditions should be, for the most part, ideal. If the weather is questionable, |
- | \ | + | |
- | In opening the CHARA Array, conditions should be, for the most part, ideal. If the weather is questionable, | + | |
- | \ | + | |
- | Only open the telescopes if the humidity is steady or dropping, at 75% or below. If the roofs outside the control room are ever dripping, then the telescopes should not be opened or should be closed immediately. If when starting out, the RH is above 80%, do not open unless it drops to below 75% and stays there for at least 30 minutes. If you do open after that, be wary and watch the RH, and if it starts rising, be prepared to close. Closing up takes about 10 minutes, so be ready for that. The array operator is in charge of protecting the telescopes and makes the final decision on whether the conditions are safe to open. If the RH is low at the beginning of the night, and rises after you are already open, the array operator should inform the PI around 70-75%, and start closing between 80-85%. Other humidity warning signs are: 1) water dripping off the OPLE building (or wet spots on the asphalt straight down from the eaves); 2) cold, clammy feel to metal objects such as railings; and 3) dew forming on the parked cars. It is important to note that the humidity can rise from 50% to 80% in as little as 10 minutes, so please keep a close eye on the rate of change of the humidity plots. It can also rain from passing clouds when the humidity is quite low, even 50% RH or lower. If in doubt, stay closed. === 4.3 Dust ===\ | + | |
- | \ | + | |
- | Gauging the airborne dust is problematic because you need a bright light and a relatively dark night. In general, you want to look in the bottom 0.5 meter of the light column. There will be a diffuse column lit up by the beam – don’t worry about it, just follow the dust glints. If you can count the dust glints, the conditions are safe to observe. If it looks like a blizzard, close up. If any of the dust glints shine with an orange or a peach hue, or the dust glints look abnormally large, the dust is probably ash – close up immediately. Ash seriously degrades bare aluminum coatings. Dust and wind go together. But, just because it is calm, the dust conditions might still be bad. If it was windy a few days earlier, it could have kicked up a lot of dust, which can take several days to settle. Finally, during late spring to early summer, conifer tree pollen can be problematic. If particulates are borderline please email the CHARA day staff so they can clean the optics as soon as possible. === 4.4 Wind ===\ | + | |
- | \ | + | |
- | Wind has the effect of degrading the seeing as well as kicking up dust. The wind effects are amplified in the tunnel between the OPLE building and the office building, so look for other places to gauge the wind conditions. The intersection of the road and the trail to the eastern telescopes is a good place to gauge conditions. To be on the safe side, we only observe under calm to light breeze conditions (gusts less than about 10 knots, or 15 kph). Windy conditions we try to avoid. If you can hear the gusts from your desk, it is too windy to observe. If you hear whistling from the light pipe supports, it is too windy to observe. If you hear the signs on the chain banging, it is too windy to observe. Occasionally you will hear the wind rustling the tops of the tall trees, but it is calm at ground level. This is a symptom of chaotic wind conditions, and almost always happens during windy episodes (Santa Anas, onshore flows, etc.), during which you shouldn’t observe – the seeing will be bad anyway. Be cautious about opening if wind gusts are above 15-20 kph; winds this high are usually correlated with bad seeing and poor data quality. Telescopes and domes should be closed if the wind gusts get up to 30 kph. This will protect the optics from branches and debris that can be blown in from the surrounding trees. === 4.5 Snow ===\\ | + | |
Because of the nature of the snow that falls on Mount Wilson, it is usually not a problem. If snow/wind conditions are such that drifting occurs, don’t open up. If there is still any snow stuck to the telescope dome itself, don’t open up. If there is snow still on the trees and branches procede with caution and make a visual assessment. Otherwise, you are free to observe (assuming the humidity, dust, and wind conditions allow it). === 4.6 Essential Observing Links === * 150-Foot Solar Tower Current TowerCam Image ([[http:// | Because of the nature of the snow that falls on Mount Wilson, it is usually not a problem. If snow/wind conditions are such that drifting occurs, don’t open up. If there is still any snow stuck to the telescope dome itself, don’t open up. If there is snow still on the trees and branches procede with caution and make a visual assessment. Otherwise, you are free to observe (assuming the humidity, dust, and wind conditions allow it). === 4.6 Essential Observing Links === * 150-Foot Solar Tower Current TowerCam Image ([[http:// | ||
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- | {{: | + | |
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- | **Chapter 6:** === = Procedure for Shutting Down at the End of the Night ==== === 6.1 End Night Sequence Introduction ===\\ | + | **Chapter 6:** === = Procedure for Shutting Down at the End of the Night ==== === 6.1 End Night Sequence Introduction ===\\ |
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The End Night sequence on Cosmic Debris can be used to end observing and stow the telescopes, carts, and domes. It will only stow the active scopes, carts, and domes, so if there are other scopes open, make them active in the Configure tab of CD or stow them manually with the procedure below, 6.4 Manually Stowing the Telescopes === 6.2 Start the end night sequence on Cosmic Debris === * Clear the job queue on Cosmic Debris. * Press the [END NIGHT] button on Cosmic Debris. This will close all the shutters, stow the active telescopes, close the telescope mirror covers, send the OPLE carts to the back switch, close the OPLE socket, and archive the accumulated data for the night. * NOTE: The End Night Sequence will NOT close the dome slits so these will have to be closed manually after all of the telescope mirror covers are closed. It will also not send inactive carts back. Update the configuration with any inactive scopes to make sure those carts can be sent back manually as well. * The Cosmic Debris status window will indicate when the end night sequence is complete. You can close Cosmic Debris after you have sent out the Observing Report. * If you use the End Night sequence to stow the telescopes and close mirror covers, remember to do a visual check of all telescopes using the check list in step 6.4 below before turning off the power for the telescopes and closing the telescope GUIs.\\ | The End Night sequence on Cosmic Debris can be used to end observing and stow the telescopes, carts, and domes. It will only stow the active scopes, carts, and domes, so if there are other scopes open, make them active in the Configure tab of CD or stow them manually with the procedure below, 6.4 Manually Stowing the Telescopes === 6.2 Start the end night sequence on Cosmic Debris === * Clear the job queue on Cosmic Debris. * Press the [END NIGHT] button on Cosmic Debris. This will close all the shutters, stow the active telescopes, close the telescope mirror covers, send the OPLE carts to the back switch, close the OPLE socket, and archive the accumulated data for the night. * NOTE: The End Night Sequence will NOT close the dome slits so these will have to be closed manually after all of the telescope mirror covers are closed. It will also not send inactive carts back. Update the configuration with any inactive scopes to make sure those carts can be sent back manually as well. * The Cosmic Debris status window will indicate when the end night sequence is complete. You can close Cosmic Debris after you have sent out the Observing Report. * If you use the End Night sequence to stow the telescopes and close mirror covers, remember to do a visual check of all telescopes using the check list in step 6.4 below before turning off the power for the telescopes and closing the telescope GUIs.\\ | ||
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In addition to paper observing logs, CHARA offers the option of using electronic logs. At minimum, we request that you fill out the date, UT time, target name, and any comments that would be relevant for subsequent reduction. This information will be useful for building and maintaining the CHARA archive:\\ | In addition to paper observing logs, CHARA offers the option of using electronic logs. At minimum, we request that you fill out the date, UT time, target name, and any comments that would be relevant for subsequent reduction. This information will be useful for building and maintaining the CHARA archive:\\ | ||
- | CHARA Electronic Logs | + | CHARA Electronic Logs === 6.3 Shutdown Checklist Introduction ===\\ |
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It is important to make sure the array gets shutdown properly at the end of the night. This includes stowing the telescopes, closing the mirror covers and domes, powering down equipment, and covering the cameras. Each day many employees are working on various systems from any number of different locations around the Array. Any CHARA equipment left on or exposed, can cause damage to other systems or be damaged itself. It is critical that the array is shut down consistently from night to night. Listed below are the procedures for shutting down the array. Please make sure that the Array is secure at the end of the night. === 6.4 Manually stowing the telescopes === * Unlock the tiptilt beams using the Tiptilt servo control GUI. * Turn the telescope TVs to SPY1 so that you can watch the telescopes. * On the Control Tab of the telescope GUI, click [STOW]. This will send the telescope and dome to the stow position. * When the telescopes reach an elevation above 70 degrees, you can begin closing the mirror covers. * M1 CLOSE * M3 CLOSE * M5 CLOSE * M7 CLOSE * Finder CLOSE Note that W2 and E1? covers need a second click to close. * Visually inspect the telescopes using SPY2 to make sure that the mirror covers close properly. Check the Telescope Monitor for mirror cover status. * After all of the mirror covers finish closing, close the dome slits by clicking [SLIT CLOSE] on the telescope control tab for each telescope dome that is open. * Close the dome enclosures by clicking [CLOSE] on the cylinder GUI. Watch that each reads .000 or .001 when closed. * Check that the telescopes moved to their stow positions in EL and AZ: * EL 90.0 deg, AZ 55.9 deg for E1 and E2 * EL 90.0 deg, AZ 99.3 deg for W1 and W2 * EL 90.0 deg, AZ 82.0 deg for S1 and S2 * Turn off the power for [TEL AZ], [TEL EL] and [TIP/TILT] for the active scopes using the Power GUI. * Visually check all telescopes in the spycams to make sure all covers and slits are closed. * Leave the telescope GUIs open until the End Night Sequence is finished. (Cosmic Debris will turn on the TVs and the SpyCams during the End Night Sequence.) * If the humidity is high, make sure that the heaters are turned on. === 6.5 Send the OPLE carts to the back of the rails === * Click the OL and MAN buttons for the active carts on the OPLE GUI Control Tab so that the buttons turn green. * Turn the carts OFF using the OPLE GUI. * Click BACK on the OPLE GUI to send the carts to the back. * Watch OPLE Server for Back Switch indicator to light up with an " | It is important to make sure the array gets shutdown properly at the end of the night. This includes stowing the telescopes, closing the mirror covers and domes, powering down equipment, and covering the cameras. Each day many employees are working on various systems from any number of different locations around the Array. Any CHARA equipment left on or exposed, can cause damage to other systems or be damaged itself. It is critical that the array is shut down consistently from night to night. Listed below are the procedures for shutting down the array. Please make sure that the Array is secure at the end of the night. === 6.4 Manually stowing the telescopes === * Unlock the tiptilt beams using the Tiptilt servo control GUI. * Turn the telescope TVs to SPY1 so that you can watch the telescopes. * On the Control Tab of the telescope GUI, click [STOW]. This will send the telescope and dome to the stow position. * When the telescopes reach an elevation above 70 degrees, you can begin closing the mirror covers. * M1 CLOSE * M3 CLOSE * M5 CLOSE * M7 CLOSE * Finder CLOSE Note that W2 and E1? covers need a second click to close. * Visually inspect the telescopes using SPY2 to make sure that the mirror covers close properly. Check the Telescope Monitor for mirror cover status. * After all of the mirror covers finish closing, close the dome slits by clicking [SLIT CLOSE] on the telescope control tab for each telescope dome that is open. * Close the dome enclosures by clicking [CLOSE] on the cylinder GUI. Watch that each reads .000 or .001 when closed. * Check that the telescopes moved to their stow positions in EL and AZ: * EL 90.0 deg, AZ 55.9 deg for E1 and E2 * EL 90.0 deg, AZ 99.3 deg for W1 and W2 * EL 90.0 deg, AZ 82.0 deg for S1 and S2 * Turn off the power for [TEL AZ], [TEL EL] and [TIP/TILT] for the active scopes using the Power GUI. * Visually check all telescopes in the spycams to make sure all covers and slits are closed. * Leave the telescope GUIs open until the End Night Sequence is finished. (Cosmic Debris will turn on the TVs and the SpyCams during the End Night Sequence.) * If the humidity is high, make sure that the heaters are turned on. === 6.5 Send the OPLE carts to the back of the rails === * Click the OL and MAN buttons for the active carts on the OPLE GUI Control Tab so that the buttons turn green. * Turn the carts OFF using the OPLE GUI. * Click BACK on the OPLE GUI to send the carts to the back. * Watch OPLE Server for Back Switch indicator to light up with an " |