'Polar angle' diaporamas de présentation

PARAMETRIC EQUATIONS AND POLAR COORDINATES

10. PARAMETRIC EQUATIONS AND POLAR COORDINATES. PARAMETRIC EQUATIONS & POLAR COORDINATES. A coordinate system represents a point in the plane by an ordered pair of numbers called coordinates. PARAMETRIC EQUATIONS & POLAR COORDINATES.

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Polar Coordinate System CALCULUS-III

Polar Coordinate System CALCULUS-III. Dr. Farhana Shaheen. Polar Coordinate System.

1.88k views • 102 slides

Electrostatic force due to spherical shell of charge

Electrostatic force due to spherical shell of charge. (field point). (source point). ?. R. Q. z. Electrostatic force due to spherical shell of charge. ?. R. z. Electrostatic force due to spherical shell of charge. ?. R. z. Electrostatic force due to spherical shell of charge. ?. R.

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Kinematics of p + n ? w p? p 0 g p reaction

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SOLAR SYSTEM C H A O S

SOLAR SYSTEM C H A O S. (with emphasis on the resonant asteroids). CHAOS = Extreme Sensibility to Initial Conditions. Long-term predictability impaired by the existence of singularities associated with unstable periodic orbits. Solutions that, at a given moment, are very close, become

532 views • 41 slides

Giulia Manca (University of Liverpool) On behalf of the CDF collaboration

Search for Squark and Gluino Production In Missing Energy+Jets at CDF. Giulia Manca (University of Liverpool) On behalf of the CDF collaboration. SUSY05, Durham (UK) 18-23 July 2005. Outline. 2. CDF and the Tevatron Theory and Motivation Analysis strategy Kinematic selection Results

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Luminosity Measurement at the International Linear Collider

Luminosity Measurement at the International Linear Collider. Iftach Sadeh Tel Aviv University ( On behalf of the FCAL collaboration ). December 28 th 2008. http://alzt.tau.ac.il/~sadeh/ sadeh@alzt.tau.ac.il. Overview. 2. The International Linear Collider (ILC).

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Search for the omega-mesic nuclei at SPring-8 LEPS

CHIRAL05 @RIKEN, 17 Feb. 2005. Search for the omega-mesic nuclei at SPring-8 LEPS. Norihito Muramatsu RCNP, Osaka University. Contents. Concepts of the omega-mesic nuclei search in photoreaction Experimental setups including newly introduced deep-UV laser

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Starter

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Projectile Motion-Starter

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Production of Two Vector Bosons, especially Diffractive

Production of Two Vector Bosons, especially Diffractive. ? Standard Model direct (non-Higgs, top) VV Production Higgs Production and Decay ? VV , especially DPE Related Processes at Tevatron VV at the LHC ... importance of pots.

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IPN Orsay, 20 September 2004

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Lecture #13

Lecture #13. Multiple representations of data. Complex numbers. imaginary. 3 + 2 i. 2. 13. atan(2/3). real. 3. How do we have them both ?. We tag the data:. ( ' rectangular 3 2) ( ' polar (sqrt 13) (atan 2 3)). How do we have them both ?. We tag the data:.

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Mike Crenshaw (Georgia State University) Steve Kraemer (Catholic University of America)

Mass Outflows from AGN in Emission and Absorption. Mike Crenshaw (Georgia State University) Steve Kraemer (Catholic University of America). NGC 4151. Six HST /STIS echelle observations (0.2'' x 0.2''): 1999 July - 2002 May Simultaneous HST, FUSE , and CXO observations in 2002 May.

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Target

r / mm. Target. 4. r max = 150 mm. 3. 2. 135. 1. Beam. 95. 1. 55. 2. 3. 4. 25. 5. 6. -230. -170. 6 disk layers 4 barrel layers Silicon detectors : Hybrid pixel detectors Double - sided microstrip detectors. 20. 40. 70. 100. 160. 230. z / mm. Target. Beam.

261 views • 15 slides

Anti-reflection optical coatings

Anti-reflection optical coatings Anti-reflection coatings are frequently used to reduce the Fresnel reflection. For normal incidence, the intensity reflection coefficient for normal incidence is. For normal incidence, the Fresnel reflection can be reduced to zero if.

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Starter

Starter. Vector Addition Lab. If you are on the ground, what three pieces of information do you need to locate a flying aircraft?. Practice . Graphical Addition. Pick a scale 2. Draw B on the head of A using a protractor and ruler.

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Recent progress and plans for Snowmass

Recent progress and plans for Snowmass. study dependence of vertex charge reconstruction on energy and polar angle results shown are for standard detector only, for Snowmass will compare with following geometries :

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Detector Alignment Thomas Naumann DESY Zeuthen

Detector Alignment Thomas Naumann DESY Zeuthen. Detector alignment and calibration often imply least squares fits with many parameters : n global parameters of calibration, n = 10 ... 10.000 m local parameters of the data model of an object (e.g. tracks) where m = k x l with

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Cherenkov Ring Reconstruction

D IRC, Particle Identification for B A B AR. D etection of I nternally R eflected C herenkov light

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