PPT-The COS FUV Lifetime Adjustment Plan
Author : alida-meadow | Published Date : 2016-07-07
Alessandra Aloisi for the COSSTIS team with input from DMassa SPenton CProffitt COliveira ROsten SOsterman DSahnow 17 November 2011 SPACE TELESCOPE
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The COS FUV Lifetime Adjustment Plan: Transcript
Alessandra Aloisi for the COSSTIS team with input from DMassa SPenton CProffitt COliveira ROsten SOsterman DSahnow 17 November 2011 SPACE TELESCOPE. cos eV RF RF RF RF RF RF RF RF RF RF eV eV cos cos cos cos RF RF RF RF RF eV eV eV RF RF RF RF RF RF RF eV eV cos cos cos 66 65 RF RF RF RF RF eV eV cos sin 66 65 5666 566 56 56 566 56 66 65 66 00 NA NA NA NA Resident 44 and Under 26000 26000 26000 27600 NA Resident 45 to 50 21000 21000 21000 13200 NA Resident 51 to 55 16000 16000 16000 9900 NA Resident 56 to 60 11000 11000 11000 6600 NA Resident 61 to 64 6000 6000 6000 35 MCS320IntroductiontoSymbolicComputationSpring2007 [diff(cos(t),t);#differentiationoftheformulacos(t) [diff(cos,t);#wrong! [D(cos(t));#alsowrong [D(cos);#differentiationofthecosinefunctionThefollowingi 20.sin( + )=sin cos +sin cos 21.sin( )=sin cos sin cos 22.cos( + )=cos cos sin cos 23.cos( )=cos cos +sin cos 24.tan( + )=tan +tan 1 tan tan 25.tan( )=tan tan 1+tan tan DoubleAngl WorksupportedbytheNationalScienceFoundationwhichof3formsatermcantake.The rstformis )sinh()cos( )sinh()sin(.(2)Thesecondformis kysinh(k )sinh()sin( )sin()cos()cos()cos( )sin()sin( M(i)sin1002+sin(i) N(i)cos(i)sin1002A12=NPi=1sin2(i)sin(i)cos(i) (M(i)sin100)2 sin(i)cos(i) (N(i)cos(i)sin100)2A13=NPi=1 sin(i)cos(i)cos(i) (M(i)sin100)2A22=NPi=1sin(i)sin(i) M( Intercomparison. Project (. GeoMIP. ). Giovanni . Pitari. . V. Aquila, . S. . Tilmes. , . I. . Cionni. , N. De Luca, Di . Genova. , and D. . Iachetti. Participating Models. Source of . geoengineering. Approach. :. Collaborators. :. Accomplishments. :. Development of high reflectivity coatings to increase system throughput, particularly in the far-UV . (FUV) spectral . range. Study other dielectric fluoride coatings and other deposition technologies such as Ion Beam Sputtering (IBS) that is expected to produce the nearest to ideal morphology optical thin film coatings and thus low scatter.. (dx0)2+(dy0)2=Z0d0q (1 cos0)2+sin20=21 2Z0d0p 1 cos0= 23 2hp 1+cos0i0=4241 s 1+cos 235:Thetotallengthofthependulumis`,thepartthatisstillstraightattimethaslength` ,andsothecoordinatesoft JOSEPH AJELLO. JPL. MICHAEL STEVENS. NRL. JACQUES GUSTIN. LPAP. GREG HOLSCLAW. CU. TODD BRADLEY. UCF. team meeting: . january. 2010. T. b. LIMB MODEL, RECENT LAB ANALYSIS & UVIS OBSERVATIONS . SUBMITTED FUV LIMB PAPER (T. About the COS-TC Toolkit. Digging in to the content. Applying understanding: Video clips and discussion. Online . version. Additional resources: Facilitator’s guide. . and the . Herman family scenario. Isabel Dietrich. Falko. Dressler. ACM Transaction on Sensor Networks, 2009. Presented by Group 6 . Tianyi. Pan. Why Limited Lifetime for WSNs?. 2. Various application domains. Wildlife monitoring. Precision agriculture. JOSEPH AJELLO. JPL. MICHAEL STEVENS. NRL. ROBERT WEST. JPL. JACQUES GUSTIN. LPAP. GREG HOLSCLAW. CU. TODD BRADLEY. UCF. agu. : . dEC. 2011. TITAN PROTON PLASMA (0.1 keV-4 . MeV. ) & SOLAR XUV GENERATES . JOSEPH AJELLO. JPL. MICHAEL STEVENS. NRL. ROBERT WEST. JPL. JACQUES GUSTIN. LPAP. GREG HOLSCLAW. CU. TODD BRADLEY. UCF. Team meeting: Jan20112. TITAN PROTON PLASMA (0.1 keV-4 . MeV. ) & SOLAR XUV GENERATES .
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