1 / 3

3 m

Trigger, data flow and the synchronization between the Auger surface detector and the AMIGA underground muon counters. 3 m. knee. 2 nd knee. ankle. toe. e ± , . AMIGA. Auger. µ. Low energy (10 17 – 10 1 8.5 eV) enhancement for the Pierre Auger Observatory ,

ivana
Download Presentation

3 m

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Trigger, data flow and the synchronization between the Auger surface detector and the AMIGA underground muon counters 3 m knee 2nd knee ankle toe e±,  AMIGA Auger µ Low energy (1017 – 1018.5 eV) enhancement for the Pierre Auger Observatory, Detection of muon component 3m underground Zbigniew Szadkowski, University of Łódź Real Time Conference, Lisbon, 2010

  2. 80 MHz prototype – 4 segments Zbigniew Szadkowski, University of Łódź

  3. 4th generation of the Front-End CycloneIII™ FPGA 320 MHz prototype with NIOS - 2 segments only Higher sampling underground: 80 -> 320 MHz Higher sampling on the surface: 40 -> 100 MHz Two segments only: higher reliability NIOS processors both underground and on the surface: no problem of obsolescence T1 – trigger + FEBTS LVDS communication between NIOS Poster PDAQ20 Zbigniew Szadkowski, University of Łódź CycloneIII™ NIOS Development Kit

More Related