2003 - Astronomia - Università degli Studi di Firenze

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References: 1. EUSO - Extreme Universe Space Observatory, Original Proposal for the ESA F2/F3 Missions, 2. January 2000 O. Catalano, M. C. Maccarone, B. Sacco, L. Scarsi, EUSO - Extreme Universe Space Observatory, Proc. 27th ICRC, Hamburg, Germany, August 2001, Copernicus Gesellschaft, Vol.HE, pp.835-838, 2001 3. O. Catalano, EUSO - Extreme Universe Space Observatory: general assembly and ISS 4. accommodation, Proc. 27th ICRC, Hamburg, Germany, August 2001, Copernicus Gesellschaft, Vol.HE, pp.843-846, 2001 A. Gherardi, E. Pace, R. Ciaranfi, S. Bottai, G. Landi, The EUSO experiment: status of micro-cell tests, EUSO-IT DFF 400/02/03, Dipartimento di Fisica, Università di Firenze, 2003 5. A. Gherardi, R. Ciaranfi, E. Pace, S. Bottai, G. Landi, Preliminary analysis of the R7600-03-M64 MAPMT response to the nitrogen UV emission wavelength, EUSO-IT DFF 402/5/03, Dipartimento di Fisica, Università di Firenze, 2003 6. M. Ameri, F. Cadoux, R. Cereseto, G. Corti, S. Cuneo, P. Musico, E. Pace, A. Petrolini, P. Pollovio, F. Pratolongo, F. Siccardi, A. Vinci, R&D mechanical studies of the photon detector microcells and modules for the euso experiment, INFN/TC-03/13, 2003 7. L. Gambicorti, V. Bratina, P. Mazzinghi, E. Pace, M. Focardi, Improved collection efficiency of the MAPMT R8900 by UV filter optical adapters, EUSO-IT DASS TR2-2003, Dipartimento di Astronomia e Scienza dello Spazio, Università di Firenze, 2003 8. L. Gambicorti, P. Mazzinghi, E. Pace, UV filtering optical adapters to enhance the collection efficiency of MAPMT R8900, EUSO-IT DASS TR4-2003, Dipartimento di Astronomia e Scienza dello Spazio, Università di Firenze, 2003 9. E. Pace, Proposal for the EUSO Instrument Calibration System, Tech. Rep. TR1-2003, Dipartimento di Astronomia e Scienza dello Spazio, Università di Firenze, 2003 10. L. Gambicorti, G. Corti, E. Pace, Study report on the in orbit calibration of the EUSO telescope, EUSO-IT DASS TR3-2003, Dipartimento di Astronomia e Scienza dello Spazio, Università di Firenze, 2003 XUVLab activity summary 2003 space projects 05
UVCI The HERSCHEL payload with the two UVCI coronagraphs Aground based version of the UVCI coronagraph (see session HERSCHEL pag. 03) has been approved for funding in 2002 by the Italian Ministry for the University and Research (MIUR). The MIUR project is thought for the development of a ground-based UVCI prototype with as many components as possible that are also qualified for use in the sounding rocket version. Due to the impossibility of observing the EUV lines from earth, the ground based UVCI will need only a visible light channel, that nevertheless has to be optimized even for EUV radiation, in order to be a reliable test for the space project. Moreover this version of the coronagraph will give a proof of principle for the efficiency of the liquid crystals polarizer [1], useful to measure the visible light linear polarization; it is an innovative solution for a space mission, and it has been used only once for earth based observations [2]. As for the space version of UVCI, the XUVLab is responsible for the stray light analysis, for the tolerance analysis and for the procurement of the CCD detectors. Along the lines of the work done for space version, thorough stray light and tolerance analysis will be performed during 2004. References: 1. L. Zangrilli, Polarimetria di lamine a cristalli liquidi a ritardo variabile, Master in applied optics thesis, University of Padova, 2003 2. R. M. MacQueen et al., The high altitude observatory coronagraph/polarimeter on the Solar Maximum Mission, Sol.Phys., 65, 91, 1980 XUVLab activity summary 2003 space projects 06
Page 1: TECHNICAL REPORT SERIES No. TR5-200
Page 4 and 5: Presentation by the coordinators of
Page 6 and 7: HERSCHEL The Helium Resonant Scatte
Page 10 and 11: SPECTRE The SPECTRE (SPECtroheliogr
Page 12 and 13: Figure 1. Sketch of a filter lens a
Page 14 and 15: HERSCHEL optical design The HERSCHE
Page 16 and 17: Diamond and semiconductor processin
Page 18 and 19: Diamond detectors The use of wide b
Page 20 and 21: Charge coupled devices (CCDs) The 2
Page 22 and 23: The LabVIEW software interface has
Page 24 and 25: Clean room 3 Clean room 2 An air co
Page 26 and 27: 0.3 m normal incidence Czerny-Turne
Page 28 and 29: Radiation sources Detectors
Page 30 and 31: Educational and training activities
Page 32 and 33: Staff Rosaria Brescia Ph. D. studen
Page 34 and 35: Emanuele Pace Researcher pace@arcet
Page 36 and 37: Publications Referred publications
Page 38 and 39: Technical reports (T1) L. Gambicort

2003 - Astronomia - Università degli Studi di Firenze

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