Michael Allen
MooSci MooSci is a device that uses scintillation measurements from the Moon to reconstruct the ground layer turbulence profile. This information about the turbulence profile is used to help choose optimal sites for the placement of new telescopes.
Scintillation Turbulent packets of air in the atmosphere act like lenses and distort incoming light. Different sources of light will cause scintillation in different parts of the atmosphere. ○ Sun ○ Stars ○ Planets ○ Moon
Considerations for using the Moon as a source of scintillation Scintillation frequency of the Moon The lunar phase Adequate signal to noise ratio of >10^4
Mechanical Design 11 photodiode circuits Distance between each pair sets heights being profiled
Electronics Two low pass filters Voltage regulator and instrumentation amplifier
Data Collection and Reduction LabView samples all 11 channels at a frequency of 10 kHz. Python data reduction script to obtain turbulence profile
Results Current version yet to be complete Previous versions have worked and been used in site testing for the Giant Magellan Telescope
Questions?