Cargando…
Design and test results of the AMS RICH detector
The AMS-02 detector will operate for at least 3 years on the International Space Station, measuring cosmic ray spectra at about 400 km above sea level over a wide range of geomagnetic latitude. The proximity focusing ring imaging \v{C}erenkov counter of AMS-02 will measure the particle velocity $\be...
| Autor principal: | |
|---|---|
| Lenguaje: | eng |
| Publicado: |
2002
|
| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1016/S0920-5632(03)91007-3 http://cds.cern.ch/record/590245 |
| _version_ | 1780899648796360704 |
|---|---|
| author | Casadei, D. |
| author_facet | Casadei, D. |
| author_sort | Casadei, D. |
| collection | CERN |
| description | The AMS-02 detector will operate for at least 3 years on the International Space Station, measuring cosmic ray spectra at about 400 km above sea level over a wide range of geomagnetic latitude. The proximity focusing ring imaging \v{C}erenkov counter of AMS-02 will measure the particle velocity $\beta$ with $\approx 0.1%$ uncertainty, making possible to discriminate Beryllium isotopes up to about 15 GeV/nucl. In addition its charge measurement will allow to study the elemental composition of cosmic rays up to Iron. A prototype of the RICH detector was tested with cosmic rays and on a ion beam accelerated by SPS, at CERN (October 2002). |
| id | cern-590245 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2002 |
| record_format | invenio |
| spelling | cern-5902452019-09-30T06:29:59Zdoi:10.1016/S0920-5632(03)91007-3http://cds.cern.ch/record/590245engCasadei, D.Design and test results of the AMS RICH detectorParticle Physics - ExperimentThe AMS-02 detector will operate for at least 3 years on the International Space Station, measuring cosmic ray spectra at about 400 km above sea level over a wide range of geomagnetic latitude. The proximity focusing ring imaging \v{C}erenkov counter of AMS-02 will measure the particle velocity $\beta$ with $\approx 0.1%$ uncertainty, making possible to discriminate Beryllium isotopes up to about 15 GeV/nucl. In addition its charge measurement will allow to study the elemental composition of cosmic rays up to Iron. A prototype of the RICH detector was tested with cosmic rays and on a ion beam accelerated by SPS, at CERN (October 2002).The AMS-02 detector will operate for at least 3 years on the International Space Station, measuring cosmic ray spectra at about 400 km above sea level over a wide range of geomagnetic latitude. The proximity focusing ring imaging \v{C}erenkov counter of AMS-02 will measure the particle velocity $\beta$ with $\approx 0.1%$ uncertainty, making possible to discriminate Beryllium isotopes up to about 15 GeV/nucl. In addition its charge measurement will allow to study the elemental composition of cosmic rays up to Iron. A prototype of the RICH detector was tested with cosmic rays and on a ion beam accelerated by SPS, at CERN (October 2002).The AMS-02 detector will operate for at least 3 years on the International Space Station, measuring cosmic ray spectra at about 400 km above sea level over a wide range of geomagnetic latitude. The proximity focusing ring imaging \v{C}erenkov counter of AMS-02 will measure the particle velocity $\beta$ with $\approx 0.1%$ uncertainty, making possible to discriminate Beryllium isotopes up to about 15 GeV/nucl. In addition its charge measurement will allow to study the elemental composition of cosmic rays up to Iron. A prototype of the RICH detector was tested with cosmic rays and on a ion beam accelerated by SPS, at CERN (October 2002).The AMS-02 detector will operate for at least 3 years on the International Space Station, measuring cosmic ray spectra at about 400 km above sea level over a wide range of geomagnetic latitude. The proximity focusing ring imaging \v{C}erenkov counter of AMS-02 will measure the particle velocity $\beta$ with $\approx 0.1%$ uncertainty, making possible to discriminate Beryllium isotopes up to about 15 GeV/nucl. In addition its charge measurement will allow to study the elemental composition of cosmic rays up to Iron. A prototype of the RICH detector was tested with cosmic rays and on a ion beam accelerated by SPS, at CERN (October 2002).The AMS-02 detector will operate for at least 3 years on the International Space Station, measuring cosmic ray spectra at about 400 km above sea level over a wide range of geomagnetic latitude. The proximity focusing ring imaging \v{C}erenkov counter of AMS-02 will measure the particle velocity $\beta$ with $\approx 0.1%$ uncertainty, making possible to discriminate Beryllium isotopes up to about 15 GeV/nucl. In addition its charge measurement will allow to study the elemental composition of cosmic rays up to Iron. A prototype of the RICH detector was tested with cosmic rays and on a ion beam accelerated by SPS, at CERN (October 2002).hep-ex/0211018oai:cds.cern.ch:5902452002-11-07 |
| spellingShingle | Particle Physics - Experiment Casadei, D. Design and test results of the AMS RICH detector |
| title | Design and test results of the AMS RICH detector |
| title_full | Design and test results of the AMS RICH detector |
| title_fullStr | Design and test results of the AMS RICH detector |
| title_full_unstemmed | Design and test results of the AMS RICH detector |
| title_short | Design and test results of the AMS RICH detector |
| title_sort | design and test results of the ams rich detector |
| topic | Particle Physics - Experiment |
| url | https://dx.doi.org/10.1016/S0920-5632(03)91007-3 http://cds.cern.ch/record/590245 |
| work_keys_str_mv | AT casadeid designandtestresultsoftheamsrichdetector |