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chara:operating_procedures [2020/01/21 21:33]
charaobs old revision restored (2020/01/17 20:42)
chara:operating_procedures [2021/06/02 18:49]
gail_stargazer
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 [[:chara:operating_procedures#observing_conditions|Observing Conditions]]\\ [[:chara:operating_procedures#observing_conditions|Observing Conditions]]\\
 [[:chara:operating_procedures#going_on_sky|Going on Sky]]\\ [[:chara:operating_procedures#going_on_sky|Going on Sky]]\\
-[[:chara:operating_procedures#procedure_for_shutting_down_at_the_end_of_the_night|Procedure for Shutting Down the Array]]\\+[[:chara:night_time_pop_changes|Night-time POP Changes]]\\ 
 +[[:chara:operating_procedures#procedure_for_shutting_down_at_the_end_of_the_night|Procedure for Shutting Down the Array]] 
 \\ \\
 __**SUPPLEMENTAL INFORMATION**__ \\ __**SUPPLEMENTAL INFORMATION**__ \\
 [[:chara:remote_observing|Remote Observing]]\\ [[:chara:remote_observing|Remote Observing]]\\
-[[:chara:power_outage|Power Outage]]\\+[[:chara:power_outage|Shutting Down prior to a Power Outage]]\\ 
 +[[:chara:power_recovery|Recovering from a Power Outage]]\\ 
 +[[:chara:trouble_shooting|Trouble Shooting]]\\ 
 +[[:chara:text_commands_for_chara_guis|Text Commands for CHARA GUIs]]\\
 {{:chara:files:dailylabcheck.pdf|Daily Alignment Check Procedure}} \\ {{:chara:files:dailylabcheck.pdf|Daily Alignment Check Procedure}} \\
 {{:chara:files:co-phase2019.pdf|Co-phasing with the CHARA phase reference}} \\ {{:chara:files:co-phase2019.pdf|Co-phasing with the CHARA phase reference}} \\
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 [[https://docs.google.com/document/d/1TnLxWaAw42DZwh7l6_wPfe_CpIfT935_aShK0ymBX1o|WFS TT Alignment and Usage]]\\ [[https://docs.google.com/document/d/1TnLxWaAw42DZwh7l6_wPfe_CpIfT935_aShK0ymBX1o|WFS TT Alignment and Usage]]\\
 [[https://docs.google.com/document/d/1UY5C8Pkbi_yd448aF_TXXE9KFkwjd5VK3LALvkFahjQ/|Coude alignment (daytime)]]\\ [[https://docs.google.com/document/d/1UY5C8Pkbi_yd448aF_TXXE9KFkwjd5VK3LALvkFahjQ/|Coude alignment (daytime)]]\\
-{{:chara:files:s2_new_finder_camera-r1.docx|New S2 Finder Instructions}} \\ +{{:chara:files:tiptilt_splitters_change.pdf|Tip-tilt Splitters Change}} 
-[[:chara:night_time_pop_changes|Night-time POP Changes]]\\+ 
 +[[:chara:coude_alignment_procedure|Coude alignment procedure]] - 2021Jun01 
 [[:chara:azimuth_coude_alignments|Azimuth coudé alignments]]\\ [[:chara:azimuth_coude_alignments|Azimuth coudé alignments]]\\
-{{:chara:files:tiptilt_splitters_change.pdf|Tip-tilt Splitters Change}} \\ 
-[[:chara:trouble_shooting|Trouble Shooting]]\\ 
 [[:chara:horizons|Telescope Horizon Limits]]\\ [[:chara:horizons|Telescope Horizon Limits]]\\
 [[:chara:restarting_servers|Restarting Servers]]\\ [[:chara:restarting_servers|Restarting Servers]]\\
 \\ \\
 **__INSTRUMENTS__ ** \\ **__INSTRUMENTS__ ** \\
-[[:chara:instruments|Instrument Manuals]]\\ 
 [[:chara:instruments|Observing Logs]]\\ [[:chara:instruments|Observing Logs]]\\
 [[:chara:fringe_offsets|Recent fringe offsets]]\\ [[:chara:fringe_offsets|Recent fringe offsets]]\\
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 \\ \\
 CHARA Array Operating Procedures\\ CHARA Array Operating Procedures\\
-Copyright © 2005-2019 The CHARA Team\\ +Copyright © 2005-2020 The CHARA Team\\ 
-Last updated: 2019-12-17\\+Last updated: 2020-1-22\\
 \\ \\
 \\ \\
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 \\ \\
 \\ \\
-**Chapter 1: ** Lab Protocol\\+**Chapter 1: ** 
 +=== Lab Protocol === 
 \\ \\
 1.1 Lab Rules Intro 1.1 Lab Rules Intro
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 \\ \\
 **Chapter 2:** **Chapter 2:**
 +=== Preparations in the Lab Prior to Observing ===
  
 27 AUG 2012 by Judit, Current version 17 JAN 2020 by Norm 27 AUG 2012 by Judit, Current version 17 JAN 2020 by Norm
  
-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. Note that there is a new Daily Alignment Check Procedure for configurations that do not change night to night. Use it instead of the full alignment given here.
-These are routine tasks to be performed in and around the lab every evening to prepare the array for regular observations. Note that there is a new alignment protocol for configurations that do not change night to night. Use it instead of the full alignment given here.+
  
 2.1 Starting the vacuum pump for the light pipes 2.1 Starting the vacuum pump for the light pipes
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 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. 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\\+2.2 Filling NIRO 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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 \\ \\
 **Chapter 3: ** **Chapter 3: **
 +=== Setting up Computer in the Control Room ===
  
-17 DEC 2019 by Norm +Updated 17 DEC 2019 by Norm
- +
-Setting up Computer in the Control Room+
  
 3.1 General Overview of Control Room computer setup 3.1 General Overview of Control Room computer setup
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 \\ \\
 \\ \\
-**Chapter 4: **Observing Conditions+**Chapter 4: ** 
 +=== Observing Conditions ===
  
 \\ \\
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 National Weather Service ([[http://forecast.weather.gov/MapClick.php?site=lox&textField1=34.2231&textField2=-118.0587&smap=1#.VKsuq2TF8rO|http://forecast.weather.gov]]) Mount Wilson weather and 5 day forecast National Weather Service ([[http://forecast.weather.gov/MapClick.php?site=lox&textField1=34.2231&textField2=-118.0587&smap=1#.VKsuq2TF8rO|http://forecast.weather.gov]]) Mount Wilson weather and 5 day forecast
  
-CHARA telescopes spy cams and weather graph ([[http://astro.gsu.edu/~weather/chara_scopes.html|http://www.astro.gsu.edu]]) Status of each CHARA telescope+CHARA telescopes spy cams and weather graph ([[http://astro.gsu.edu/~weather/chara_scopes.html|http://www.astro.gsu.edu]]) Status of each CHARA telescope and the All-sky camera.
  
-Mount Wilson HP Wren Cameras ([[http://hpwren.ucsd.edu/cameras/wilson.html|http://hpwren.ucsd.edu/cameras/wilson.html]])+Mount Wilson HP Wren Cameras ([[http://hpwren.ucsd.edu/cameras/wilson.html|http://hpwren.ucsd.edu/cameras/wilson.html]]) 360º view of mountain in color and IR
  
 Aerospace Corporation weather station ([[http://www.weatherlink.com/user/mocam/index.php?view=summary&headers=1|http://www.weatherlink.com/user/mocam]]) Another local station, always current. Aerospace Corporation weather station ([[http://www.weatherlink.com/user/mocam/index.php?view=summary&headers=1|http://www.weatherlink.com/user/mocam]]) Another local station, always current.
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 \\ \\
 \\ \\
-**Chapter 5:** Going on Sky+**Chapter 5:** 
 +=== Going on Sky ===
  
 5.1 Opening the Telescope Domes and enclosures\\ 5.1 Opening the Telescope Domes and enclosures\\
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 [[:chara:operating_procedures|Back to Main Menu]]\\ [[:chara:operating_procedures|Back to Main Menu]]\\
 \\ \\
-**Chapter 6:** === = Procedure for Shutting Down at the End of the Night+**Chapter 6:** 
 +=== Procedure for Shutting Down at the End of the Night ===
  
 6.1 End Night Sequence Introduction\\ 6.1 End Night Sequence Introduction\\
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 6.2 Start the end night sequence on Cosmic Debris 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 M1 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.\\+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 active 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 M1 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.\\
 A list of observed targets and an Observing Report is now automatically generated as part of the End Night Sequence. Click [END NIGHT], then [REPORT] on Cosmic Debris to generate this automatic report email. The report will include the headings: PI name, Program, Observers, Baselines, Weather and Seeing data, and targets on which data was collected. Complete the Observers and Baselines entries, add comments to the bottom of the report and put your name at the end. Check with the observer for completeness of the target list. Some observers will send you comments of their own. Add those to the report. Cut and paste this into an email to CHARA Obs and send it. When the function works, you can also hit the SEND button at the bottom of the report to email this report to the CHARA OBS list.\\ A list of observed targets and an Observing Report is now automatically generated as part of the End Night Sequence. Click [END NIGHT], then [REPORT] on Cosmic Debris to generate this automatic report email. The report will include the headings: PI name, Program, Observers, Baselines, Weather and Seeing data, and targets on which data was collected. Complete the Observers and Baselines entries, add comments to the bottom of the report and put your name at the end. Check with the observer for completeness of the target list. Some observers will send you comments of their own. Add those to the report. Cut and paste this into an email to CHARA Obs and send it. When the function works, you can also hit the SEND button at the bottom of the report to email this report to the CHARA OBS list.\\
 Note: Classic, CLIMB, FLUOR and PAVO will automatically send the target information to Cosmic Debris after data is acquired. For MIRCx, the [DATA ACQUIRED] button can be clicked on Cosmic Debris after each data sequence is finished or it can be done by the MIRCx operator from his or her station.\\ Note: Classic, CLIMB, FLUOR and PAVO will automatically send the target information to Cosmic Debris after data is acquired. For MIRCx, the [DATA ACQUIRED] button can be clicked on Cosmic Debris after each data sequence is finished or it can be done by the MIRCx operator from his or her station.\\
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 6.4 Manually stowing the telescopes 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 and domes stow. 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 50 degrees, you can begin closing the mirror covers. M1 CLOSE, M3 CLOSE, M5 CLOSE, M7 CLOSE, Finder CLOSE Note that W2 and E1? finder 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 the M1, M3 and finder 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.+Unlock the tiptilt beams using the Tiptilt servo control GUI. Turn the telescope TVs to SPY1 so that you can watch the telescopes and domes stow. 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 50 degrees, you can begin closing the mirror covers. M1 CLOSE, M3 CLOSE, M5 CLOSE, M7 CLOSE, Finder CLOSE Note that W2 and E1? finder covers and the W1 and W2 M7 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 the M1, M3 and finder 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 Spy Cam 2 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 6.5 Send the OPLE carts to the back of the rails
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 6.6 Finish shutting down in the control room 6.6 Finish shutting down in the control room
  
-If using Classic or CLIMB, check to make sure the dither is off by looking at the dither status in the CLASSIC/CLIMB server. If necessary, this can be turned off from the dither tab on the Classic/CLIMB GUI. They are off when gray. Shut off [METSCOPE], [NIRO CPU], and [CLS-DITH], or [CLM-DITH] if used on the POWER gui. Close the OPLE, Tiptilt, CLIMB/CLASSIC GUIs Close the OPLE, Tiptilt, and CLIMB/CLASSIC servers, type CTRL+C, then Y, Visually check all telescopes in the spycams to make sure all covers and slits are closed. Turn the TV OFF. Leave GPS server and the Telescope Servers open and running+If using Classic or CLIMB, check to make sure the dither is off by looking at the dither status in the CLASSIC/CLIMB server. If necessary, this can be turned off from the dither tab on the Classic/CLIMB GUI. They are off when gray. Shut off [METSCOPE], [NIRO CPU], and [CLS-DITH], or [CLM-DITH] if used on the POWER gui. Close the OPLE, Tiptilt, CLIMB/CLASSIC GUIs Close the OPLE, Tiptilt, and CLIMB/CLASSIC servers, type CTRL+C, then Y, Visually check all telescopes in the spycams to make sure all covers and slits are closed. Turn the TV OFF. Leave GPS, Metrol, and Vacmon servers and the Telescope servers open and running
  
 6.7 Shutting down the Lab\\ 6.7 Shutting down the Lab\\
chara/operating_procedures.txt · Last modified: 2023/09/01 02:50 by gail_stargazer