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Sarah Stoebner University of Hawai’i at Hilo Mentor: Billie Chitwood. Temperature Effects on the Pointing of Antennas at the Submillimeter Array. SMA Why? Background Project Results. Outline. The Submillimeter Array Mauna Kea, Hawai’i. Important Project. -Daytime observations
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Sarah Stoebner University of Hawai’i at Hilo Mentor: Billie Chitwood Temperature Effects on the Pointing of Antennas at the Submillimeter Array
SMA • Why? • Background • Project • Results Outline
Important Project -Daytime observations -Most temperature variation -Metal heats up it expands -Variation of expansion affects pointing -Pointing important for astronomical data -Other factors cause pointing errors -Correct for factors that cause large error -Pointing Model -Too expensive to correct for all
Primary Reflector Reflector Mount Sensor
Snapshotson July 25, 2007 Snapshot of Jupiter at sunset (7:32PM) Snapshot of Jupiter a few hours later (10:13PM)
Arcturus Altair Deneb Jupiter Vega
Results In Azimuth: The pixel difference was 1.6 pixels With 1.252” per pixel the pointing error caused by temperature was 1.878” In Elevation: The pixel difference was 3.5 pixels With 1.252” per pixel the pointing error caused by temperature was 4.381”
Acknowledgments • Billie Chitwood • Nimesh Patel • Erin Brassfield • SMA Staff • Sarah Anderson • Scott Seagroves • Hilary O’Bryan • This work has been supported by the National Science Foundation Science and Technology Center for Adaptive Optics, managed by the University of California at Santa Cruz under cooperative agreement No. AST - 9876783.
Azimuth Error Elevation Error ΔEl = El´ + S cos(El) + I cos(Az) + I sin(Az) + I cos(2(Az)) + I sin(2(Az)) + Qel Other Pointing Errors ΔAz cos(El) = Az´ cos(El) + C + L sin (El) +I sin(El) sin(Az) + I sin(El) cos(Az) + I sin(El) sin(2(Az)) + I sin(El) cos(2(Az))+ M cos(El) sin(Az) + M cos(El) cos(Az) + M cos(El) sin(2(Az)) + M cos(El) cos(2(Az)) + M cos(El) sin(3(Az)) + M cos(El) cos(3(Az))+ Qaz +RMaz