Cargando…
Introduction to the AMS Experiment
<!--HTML-->Following the pioneering experiments (ATIC, BESS, CREAM, HEAT, PAMELA, …), using a magnetic spectrometer (AMS) on ISS is a unique way to provide precision long term measurements of primordial high energy charged cosmic rays. AMS was installed on the Station in May 2011. Up to no...
| Autor principal: | |
|---|---|
| Lenguaje: | eng |
| Publicado: |
2015
|
| Materias: | |
| Acceso en línea: | http://cds.cern.ch/record/2009160 |
| _version_ | 1780946448899112960 |
|---|---|
| author | Prof. TING, Samuel |
| author_facet | Prof. TING, Samuel |
| author_sort | Prof. TING, Samuel |
| collection | CERN |
| description | <!--HTML-->Following the pioneering experiments (ATIC, BESS, CREAM, HEAT, PAMELA, …), using a magnetic spectrometer (AMS) on ISS is a unique way to provide precision long term measurements of primordial high energy charged cosmic rays. AMS was installed on the Station in May 2011. Up to now, 60 billion events have been collected. 40 billion events have been partially analysed. AMS is scheduled to be on the Station until at least 2024. By then AMS will have collected close to 200 billion events. The detector properties and the analysis methods will be introduced.
|
| id | cern-2009160 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2015 |
| record_format | invenio |
| spelling | cern-20091602022-11-02T22:09:43Zhttp://cds.cern.ch/record/2009160engProf. TING, SamuelIntroduction to the AMS ExperimentAMS DAYS AT CERN - The Future of Cosmic Ray Physics and Latest ResultsConferences<!--HTML-->Following the pioneering experiments (ATIC, BESS, CREAM, HEAT, PAMELA, …), using a magnetic spectrometer (AMS) on ISS is a unique way to provide precision long term measurements of primordial high energy charged cosmic rays. AMS was installed on the Station in May 2011. Up to now, 60 billion events have been collected. 40 billion events have been partially analysed. AMS is scheduled to be on the Station until at least 2024. By then AMS will have collected close to 200 billion events. The detector properties and the analysis methods will be introduced. oai:cds.cern.ch:20091602015 |
| spellingShingle | Conferences Prof. TING, Samuel Introduction to the AMS Experiment |
| title | Introduction to the AMS Experiment |
| title_full | Introduction to the AMS Experiment |
| title_fullStr | Introduction to the AMS Experiment |
| title_full_unstemmed | Introduction to the AMS Experiment |
| title_short | Introduction to the AMS Experiment |
| title_sort | introduction to the ams experiment |
| topic | Conferences |
| url | http://cds.cern.ch/record/2009160 |
| work_keys_str_mv | AT proftingsamuel introductiontotheamsexperiment AT proftingsamuel amsdaysatcernthefutureofcosmicrayphysicsandlatestresults |