Optics of Balloon Experimental Twin Telescope for Infrared Interferometry (BETTII): Delay Lines and Alignment

التفاصيل البيبلوغرافية
العنوان: Optics of Balloon Experimental Twin Telescope for Infrared Interferometry (BETTII): Delay Lines and Alignment
المؤلفون: Dhabal, Arnab, Rinehart, Stephen A, Rizzo, Maxime J, Mundy, Lee, Fixsen, Dale, Sampler, Henry, Mentzell, Eric, Veach, Todd, Silverberg, Robert F, Furst, Stephen, Dow, Thomas, Ade, Peter, Tucker, Carole
المصدر: SPIE Proceedings. 9907
بيانات النشر: United States: NASA Center for Aerospace Information (CASI), 2016.
سنة النشر: 2016
مصطلحات موضوعية: Astrophysics
الوصف: We present the optics of Balloon Experimental Twin Telescope for Infrared Interferometry (BETTII) as it gets ready for launch. BETTII is an 8-meter baseline far-infrared (30-90 microns) interferometer mission with capabilities of spatially resolved spectroscopy aimed at studying star formation and galaxy evolution. The instrument collects light from its two arms, makes them interfere, divides them into two science channels (30-50 microns and 60-90 microns), and focuses them onto the detectors. It also separates out the NIR light (1-2.5 microns) and uses it for tip-tilt corrections of the telescope pointing. Currently, all the optical elements have been fabricated, heat treated, coated appropriately and are mounted on their respective assemblies. We are presenting the optical design challenges for such a balloon borne spatio-spectral interferometer, and discuss how they have been mitigated. The warm and cold delay lines are an important part of this optics train. The warm delay line corrects for path length differences between the left and the right arm due to balloon pendulation, while the cold delay line is aimed at introducing a systematic path length difference, thereby generating our interferograms from where we can derive information about the spectra. The details of their design and the results of the testing of these opto-mechanical parts are also discussed. The sensitivities of different optical elements on the interferograms produced have been determined with the help of simulations using FRED software package. Accordingly, an alignment plan is drawn up which makes use of a laser tracker, a CMM, theodolites and a LUPI interferometer.
نوع الوثيقة: Report
اللغة: English
تدمد: 0277-786X
Relation: An Overview of the Mid-Infrared Spectro-Interferometer MATISSE: Science, Concept, and Current Status
DOI: 10.1117/12.2230218
URL الوصول: https://ntrs.nasa.gov/citations/20170006225
ملاحظات: NNG17PT01A
رقم الانضمام: edsnas.20170006225
قاعدة البيانات: NASA Technical Reports
الوصف
تدمد:0277786X
DOI:10.1117/12.2230218