منابع مشابه
The ALTO Project at IPN Orsay
In order to probe neutron rich radioactive noble gases produced by photo-fission, a PARRNe1 experiment (Production d’Atomes Radioactifs Riches en Neutrons) has been carried out at CERN. The incident electron beam of 50 MeV was delivered by the LIL machine: LEP Injector Linac. The experiment allowed to compare under the same conditions two production methods of radioactive noble gases: fission i...
متن کاملThe Alto Tandem and Isol Facility at IPN Orsay
Alto is an infrastructure for experimental nuclear physics in France that comprises both an on-line isotope-separation facility based on the photofission of uranium and a stableion beam facility based on a 14.5-MV tandem accelerator. The isotope-separation on-line section of Alto is dedicated to the production of neutron-rich radioactive ion beams (RIB) from the interaction of the γ-flux induce...
متن کاملThe ALTO facility at IPN Orsay and study of neutron rich nuclei in the vincinity of 78Ni
The ALTO facility at IPN Orsay is based on a linear electron accelerator (50 MeV, 10μA) dedicated to the production of neutron rich radiactive beams by photofission of a thick uranium carbide target paced on an ISOL line. The construction of the facility has ended in december 2005 and the first on-line tests have been carried out in mid-2006. The production of fission fragments after separation...
متن کاملPhoto-fission for the production of radioactive beams ALTO project
In order to probe neutron rich radioactive noble gases produced by photo-fission, a PARRNe-1 experiment (Production d Atomes Radioactifs Riches en Neutrons) has been carried out at CERN. The incident electron beam of 50 MeV was delivered by the LIL machine: LEP Injector Linac. The experiment allowed us to compare under the same conditions two production methods of radioactive noble gases: fissi...
متن کاملThe Night-sky at the Calar Alto Observatory
We present a characterization of the main properties of the night-sky at the Calar Alto observatory for the time period between 2004 and 2007. We use optical spectrophotometric data, photometric calibrated images taken in moonless observing periods, together with the observing conditions regularly monitored at the observatory, such as atmospheric extinction and seeing. We derive, for the first ...
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ژورنال
عنوان ژورنال: Physics of Atomic Nuclei
سال: 2003
ISSN: 1063-7788,1562-692X
DOI: 10.1134/1.1601741