logging in or signing up ruggiero Pumbaa Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINT 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: 5 Category: Entertainment License: All Rights Reserved Like it (0) Dislike it (0) Added: September 05, 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, 2003 Slide2: Goal andamp; Comparison Upgrade with the AGS Booster ?: Upgrade with the AGS Booster ? Slide4: Upgrade with Super–Conducting Linac Slide5: Why a Super-Conducting Linac Slide6: The 1.2-GeV SCL for the 1-MW AGS Upgrade Slide7: SCL Layout Slide8: Front-End Slide9: SCL Site and Layout Slide10: Injector and AGS Parameters for 1-MW Upgrade Slide11: SCL Components Slide12: A Cryo-Module Slide13: Warm Insertions (why warm?) Slide14: General Parameters of SCL Sections Slide15: Other SCL Parameters Slide16: Project Cost Slide17: Super Neutrino Beam Geographical Layout Slide18: 3-D Neutrino Super Beam Perspective Slide19: 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 Pumbaa Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINT 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: 5 Category: Entertainment License: All Rights Reserved Like it (0) Dislike it (0) Added: September 05, 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, 2003 Slide2: Goal andamp; Comparison Upgrade with the AGS Booster ?: Upgrade with the AGS Booster ? Slide4: Upgrade with Super–Conducting Linac Slide5: Why a Super-Conducting Linac Slide6: The 1.2-GeV SCL for the 1-MW AGS Upgrade Slide7: SCL Layout Slide8: Front-End Slide9: SCL Site and Layout Slide10: Injector and AGS Parameters for 1-MW Upgrade Slide11: SCL Components Slide12: A Cryo-Module Slide13: Warm Insertions (why warm?) Slide14: General Parameters of SCL Sections Slide15: Other SCL Parameters Slide16: Project Cost Slide17: Super Neutrino Beam Geographical Layout Slide18: 3-D Neutrino Super Beam Perspective Slide19: 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