logging in or signing up ruggiero Jolene Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINTLite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 7 Category: Entertainment License: All Rights Reserved Like it (0) Dislike it (0) Added: September 27, 2007 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... Premium member Presentation Transcript SCL for 1-MW AGS Upgrade: SCL for 1-MW AGS Upgrade Alessandro G. Ruggiero Brookhaven National Laboratory NuFact 03 Workshop Columbia University, New York June 5-11, 2003Slide2: Goal & ComparisonUpgrade with the AGS Booster ?: Upgrade with the AGS Booster ?Slide4: Upgrade with Super–Conducting LinacSlide5: Why a Super-Conducting LinacSlide6: The 1.2-GeV SCL for the 1-MW AGS UpgradeSlide7: SCL LayoutSlide8: Front-EndSlide9: SCL Site and LayoutSlide10: Injector and AGS Parameters for 1-MW UpgradeSlide11: SCL ComponentsSlide12: A Cryo-ModuleSlide13: Warm Insertions (why warm?)Slide14: General Parameters of SCL SectionsSlide15: Other SCL ParametersSlide16: Project CostSlide17: Super Neutrino Beam Geographical LayoutSlide18: 3-D Neutrino Super Beam PerspectiveSlide19: Advantages of a Very Long Baseline neutrino oscillations result from the factor sin2(Dm322 L / 4E) modulating the n flux for each flavor (here nm disappearance) the oscillation period is directly proportional to distance and inversely proportional to energy with a very long baseline actual oscillations are seen in the data as a function of energy the multiple-node structure of the very long baseline allows the Dm322 to be precisely measured by a wavelength rather than an amplitude (reducing systematic errors)Slide20: BNL Homestake Super Neutrino Beam You do not have the permission to view this presentation. In order to view it, please contact the author of the presentation.
ruggiero Jolene Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINTLite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 7 Category: Entertainment License: All Rights Reserved Like it (0) Dislike it (0) Added: September 27, 2007 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... Premium member Presentation Transcript SCL for 1-MW AGS Upgrade: SCL for 1-MW AGS Upgrade Alessandro G. Ruggiero Brookhaven National Laboratory NuFact 03 Workshop Columbia University, New York June 5-11, 2003Slide2: Goal & ComparisonUpgrade with the AGS Booster ?: Upgrade with the AGS Booster ?Slide4: Upgrade with Super–Conducting LinacSlide5: Why a Super-Conducting LinacSlide6: The 1.2-GeV SCL for the 1-MW AGS UpgradeSlide7: SCL LayoutSlide8: Front-EndSlide9: SCL Site and LayoutSlide10: Injector and AGS Parameters for 1-MW UpgradeSlide11: SCL ComponentsSlide12: A Cryo-ModuleSlide13: Warm Insertions (why warm?)Slide14: General Parameters of SCL SectionsSlide15: Other SCL ParametersSlide16: Project CostSlide17: Super Neutrino Beam Geographical LayoutSlide18: 3-D Neutrino Super Beam PerspectiveSlide19: Advantages of a Very Long Baseline neutrino oscillations result from the factor sin2(Dm322 L / 4E) modulating the n flux for each flavor (here nm disappearance) the oscillation period is directly proportional to distance and inversely proportional to energy with a very long baseline actual oscillations are seen in the data as a function of energy the multiple-node structure of the very long baseline allows the Dm322 to be precisely measured by a wavelength rather than an amplitude (reducing systematic errors)Slide20: BNL Homestake Super Neutrino Beam