![]() ![]() ![]() Ensure demand reflect the needs of the MOB and proactively coordinate with CSC to ensure needs are met.Advise SM on stock levels and liaise with DSM/staff to ensure sufficient stock levels are maintained.Monitor individual training and advise on training requirements.Provide Recurrent Training for MOB personnel.Audit and control aircraft Servicing Sets for correctness and completeness of aircraft maintenance carried out at 1st and 2nd Line.Enforce policies, procedures and directives established by the Company.Ensuring personnel adhere to airworthiness rules and standards in the TAM/MPM, technical publications, and standard procedures.Ensure aircraft maintenance personnel requirements are identified, and personnel are assigned, to support aircraft maintenance and operations.Advise Site Manager on Monthly Aircraft Availability, Mission Reliability, as well cause factors and corrective actions.Plan, supervise corrective and preventive maintenance on MOB aircraft to ensure PIM inspections remain on schedule to meet FCFCL date or better.Ensuring that the Site Manager is briefed on the current status of MOB corrective and scheduled aircraft maintenance.Ensuring aircraft maintenance is adequately scheduled to provide mission capable aircraft to meet flight schedule.Communicate with Squadron Operations staff for all aircraft maintenance and support issues.Position: Associate Professor at CNS, the University of Tokyo since June, 2014 – present Assistant Professor at Institute of Particle and Nuclear Study, KEK from October 2004 to May 2014.Įducation: Doctorate Degree in Science from The University of Tokyo in April 2004.Ĭommunity service: Hold several prestigious positions in Japan, which include Chairman of the RCNP P-PAC (2019-2021), Board Member of the RCNP P-PAC (2016-2017), Chairman of the Unstable Nuclei Division of the Future Project Steering Committee, Japan Nuclear Physics Forum (2016-present), Scientific secretary of JPS Division of Experimental Nuclear Physics (2018-2019), Chairman of RIBF Users Executive Committee (UEC) (2014-2016), Member of RIBF Users Executive Committee (UEC) (2013-2017).Īwards: Japan Nuclear Physics Forum Award for Outstanding Young Physicists in the Experimental Nuclear Physics (2005). In the talk, the speaker will introduce the system of OEDO and discuss the surrogate reactions on 79Se and 130Sn. In spring 2022, we applied this method to the (d,p) reaction with the decelerated 130Sn beam at OEDO to reveal the condition to form the second peak at r-process. This was the first experiment to determine the gamma emission probability without detecting gamma rays. The gamma emission probability was obtained directly from the residual nuclei. The outgoing residues were identified by the first half of the SHARAQ spectrometer. The recoil particles were detected by the SSD-CsI array. The decelerated 79Se was focused on a CD2 target. To determine the CN reaction rate via studying the gamma emission probability, we conducted the (d,p) surrogate reaction on 79Se at the Optimized Energy Degrading Optics (OEDO) beamline – a deceleration and focusing element – at RIBF. In the CN reaction, the gamma emission probability around the neutron threshold is a key quantity. In particular, the peak structure in the abundance is governed by the neutron capture reaction around in the freezing-out phase, where the compound neutron (CN) capture reaction plays an important role. Although the neutron capture rate is the one of the most important to determine the neutron density at the final stage, they have not been well studied experimentally because both the neutron and the nuclei are short-lived. To understand the r-process, several nuclear physics parameters are demanded. ![]() The study on the origin is boosted by a recent finding of kilonova following the discovery of the gravitational wave. Origin of the element in the universe is one of the big questions in modern physics. Place: Meeting room on the 6th floor, Technique Building Nobuaki IMAI (CNS, the University of Tokyo) Title: OEDO Beam Line at RIBF and Its Physics Program
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