AuxTel Weather Constraints

This page defines the different types of operational constraints due to weather.

For a full study of wind on image quality, refer to SIT-Com TN-126.

Operating conditions used to define the Rubin construction project are found in LTS-54.

As commissioning gets underway, the operating conditions will be better constrained, and different situations will apply to the Main telescope and Auxiliary Telescope.

Deciding to open

Before opening the dome to take on-sky data or for cooling, observers must take care to inspect the weather conditions. Humidity (especially the dew point difference), cloud cover, and wind speed are the three largest determining factors for safety of the telescope and equipment.

Observers should inspect the forecast for the night, and review the weather trends on the Rubin weather station in LOVE or Chronograph, and the Gemini weather station (currently unavailable due to cyberattack). The Rubin weather data is updated every 0.5 seconds. The Rubin weather data is viewed in LOVE, in the “Weather Station Component” view. The wind is displayed both as an integer and plotted on a vector graph.

The Gemini weather data updates every 30 seconds. The Gemini wind speed data reported is the average over the previous 10 minutes.

NOIRLab also hosts additional links to Cerro Pachón weather, including site webcams, and the SOAR weather station (currently unavailable due to cyberattack).

If the humidity is above 70%, go outside and look for incoming cloud fronts, and inspect the buildings and cars for condensation. Be more cautious to open if there will not be someone in the control room to monitor changing weather conditions, e.g. opening before going to dinner, or leaving the control room to complete another task.

Warning

Vent gates:

The vent gates on the first floor of the AuxTel dome can add turbulence if winds are high. Close the vent gates if wind speeds are above 10 m/s. This value is less than they can physically stand, but this avoids cross talk in the dome.

Note

Extraction fan use:

The extraction fan on vent gate 3 can operate at 50-100% power for initial cooling. During on-sky operations, the extraction fan must be run at 20-25% power. If winds are over 8 m/s, the extraction fan should be turned off. If humidity is rising quickly, or >= 65%, (to be revised) the extraction fan should be turned off to avoid drawing in more moisture through the dome.

Wind

The predominant wind direction at the summit is from the northwest or ~300 degrees. The majority of the time, the wind comes up from the coast and blows through the Elqui River valley, arriving to the summit. If the direction changes frequently, or has completely changed direction from 300 degrees, use caution as this likely indicates a frontal system and unstable atmospheric conditions.

Mount jitter becomes much more frequent in cases of gusty wind. High mount error is characterized as error over 0.25, which calculated and displayed in RubinTV as mount motion image degradation. The figure below shows an example of the mount moving erratically in wind speeds over 10 m/s.

../../_images/Windy_AuxTel.png

Over the year of 2023, the median wind speed is plotted against the number of mount failures due to wind. When the wind velocity averages higher than 8 m/s, winds begin to noticeably impact mount performance and image quality.

../../_images/Wind_mount_failures.png

Using this information, the following guidelines are imposed:

Wind speeds less than 8 m/s (measured over the last 10 data points):
  • This is safe operation range for AuxTel.

    No restrictions in observing are needed.

Wind speeds between 8 and 15 m/s (measured over the last 10 data points):
  • If the observer has control to choose targets, observe out of the wind.

    Report that the scheduler configuration needs to be changed, or change the scheduler program you are running. Skip over any observing blocks that point the telescope directly into, or 90 degrees offset from, the dominant direction of the wind.

  • Close the vent gate(s) at winds over 12 m/s.

Note

Opposite rule:

The optimum place to point when there are winds over 8 m/s is 180 degrees offset from the dominant wind direction.

Wind speeds greater than 15 m/s (measured over the last 10 data points):
  • Observers should close once wind gusts have become greater than 15 m/s.

    If mount jitter is occurring frequently in all parts of the sky, close the dome. Before deciding to open again, ensure that sustained winds have dropped below the closure limits for more than 15 minutes. Reset the timer if the wind jumps over 15 m/s again.

Warning

Dome drop-down shutter:

The AuxTel dome shutter has a drop-down shutter that opens like a flap, causing it to extend further past the dome structure. It is opened when observing targets below 25 degrees elevation. The drop-down shutter is susceptible to wind gusts, and should be closed if gusts reach over 8 m/s.

Humidity and dew point

Higher relative humidity is not an absolute determination of closure, but observers must pay close attention when humidity is over 70%, or if it begins to suddenly trend upward.

Humidity above 65%:

  • Turn off the extraction fan and close vent gates.

Humidity above 70%:
  • Observers must treat this range with extra caution.

    Take time to go outside and inspect vehicles, buildings, and look for falling drops from the roof. Be mindful of local humidity changes between AuxTel and the main telescope building. Because AuxTel is more exposed, there is more air mixing which creates a small buffer against condensation compared to the Rubin building. If the ambient temperature is cooler, especially during winter time, the condensation risk on metal surfaces is higher.

The quantity that is more important than relative humidity is the dew point temperature and the dew point difference. The dew point temperature is the ambient air temperature at which relative humidity will reach 100% - the air is completely saturated with water vapor. You can calculate the dew point temperature using this online tool. The dew point difference is the difference between the dew point temperature and the coldest structure in the telescope dome.

Example:

Dew point temperature = 8 degrees C.

AuxTel M1 temperature = 11 degrees C.

Truss temperature = 4 degrees C.

Dew point difference = 4 degrees C.

In the example, the dew point difference is 4 degrees C, which is in safe operational range. For any object or structure that is above the dew point temperature, there is less condensation risk. Water condenses on the coldest surface.

Dew point difference is > 2.5 degrees C:

  • Normal operations may continue.

Dew point difference is between 2 degrees and 2.5 degrees C:
  • Observers must consider closing.

    Go outside and check condensation on buildings and vehicles. If wet, advise to close.

Dew point difference is 2 degrees C or less:

  • Close immediately.

Observers must wait for the dew point temperature or humidity to recover from the closure limits for at least 15 minutes before opening again.

Note

If humidity has dropped during the night, before opening the dome slit, consider performing a quick dome drain procedure. Rotate the closed dome several times in both directions, exercising large slews. This can remove some of the water droplets that might have accumulated on the metal surface.

Cloud cover

Until DIMM flux measurements are imported into Rubin TV or in the EFD, or the wavefront sensors of LSSTCam are available, determining safe or unsafe cloud coverage is a bit of an un-tested process.

AuxTel has continued observing happily in 2.5 magnitudes of extinction, given that most targets are typically \(\leq 8\,mag\).

The biggest threat of cloud cover is lower-atmosphere condensation, or virga, which is rain and moisture that falls from a cloud, but evaporates before it hits ground level. Virga appears like streaks of rain or whips on the bottom of different types of cumulus clouds. Winds can bring this moisture into the dome, or it can condense on the dome roof and fall through the slit.

If clouds are present in the all-sky camera - which is mounted next to Earthcam on Piñon - be mindful of further cloud accumulation and the direction they are coming from.

Aggregate data by going outside and looking around the sky. During bright time, look along the glowing cloud edges for wisps.

The Gemini cloud cameras are useful to evaluate how low the clouds are. Cloud camera images update every 30 seconds during the night. The Gemini cloud cameras begin exposing when the sun is ~6 degrees below horizon. In the North East camera, verify that the clouds are not below the mountain peaks. If clouds are at this low elevation, and they are also overhead the telescope, these is a moisture risk.

Note

The Gemini cloud cameras and the all-sky cameras do not always represent reality. Due to the longer exposure times, stars can appear brighter in the images, so extinction is not as bad as it seems. If possible, take the opportunity to go outside and compare the cloud cameras to real life.

Moon avoidance

If the scheduler is choosing targets that point directly into the direction of the moon, alert support staff or change the scheduler program. If engineering tasks are being run that are not measuring sky brightness, choose targets out of the direction of the moon. Be mindful of scattered moonlight during heavy cloud cover. Data may be degraded.

This procedure was last modified Dec 16, 2024.