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Cosmic rays - Congresses. --- Galactic cosmic rays - Congresses. --- Supernovae - Congresses. --- Interstellar matter - Congresses. --- Astrophysics - Congresses. --- Cosmic rays --- Galactic cosmic rays --- Supernovae --- Interstellar matter --- Astrophysics
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Nuclear astrophysics --- Cosmic rays --- Congresses --- Nuclear astrophysics - Congresses --- Cosmic rays - Congresses
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A Search for Muon Neutrino to Electron Neutrino Oscillations in the MINOS Experiment is a tour de force that summarizes, clearly and in some depth, much of Ochoa’s vast body of work which has had a major impact on MINOS. The centerpiece of the thesis is the search for muon neutrino to electron neutrino oscillations, which would indicate a non-zero mixing angle between the first and third neutrino generations (θ13), currently the “holy grail” of neutrino physics. The optimal extraction of the electron neutrino oscillation signal is based on the novel “library event matching” (LEM) method which Ochoa developed and implemented together with colleagues at Caltech and at Cambridge, which improves MINOS’ reach for establishing an oscillation signal over any other method. LEM will now be the basis for MINOS’ final results, and will likely keep MINOS at the forefront of this field until it completes its data taking in 2011. Ochoa and his colleagues also developed the successful plan to run MINOS with a beam tuned for antineutrinos, to make a sensitive test of CPT symmetry by comparing the inter-generational mass splitting for neutrinos and antineutrinos. Ochoa’s in-depth, creative approach to the solution of a variety of complex experimental problems is an outstanding example for graduate students and longtime practitioners of experimental physics alike. Some of the most exciting results in this field to emerge in the near future may find their foundations in this thesis, for which Ochoa was awarded the National Prize for Youth of Mexico in 2009. This Doctoral Thesis has been accepted by California Institute of Technology, Pasadena, USA.
Cosmic rays -- Congresses. --- Neutrinos -- Congresses. --- Neutrino interactions --- Neutrinos --- Physics --- Physical Sciences & Mathematics --- Nuclear Physics --- Atomic Physics --- Neutrinos. --- Oscillations. --- Neutret --- Physics. --- Elementary particles (Physics). --- Quantum field theory. --- Particle acceleration. --- Elementary Particles, Quantum Field Theory. --- Particle Acceleration and Detection, Beam Physics. --- Numerical and Computational Physics. --- Cycles --- Fluctuations (Physics) --- Vibration --- Leptons (Nuclear physics) --- Neutrons --- Quantum theory. --- Numerical and Computational Physics, Simulation. --- Particles (Nuclear physics) --- Acceleration (Mechanics) --- Nuclear physics --- Quantum dynamics --- Quantum mechanics --- Quantum physics --- Mechanics --- Thermodynamics --- Acceleration --- Natural philosophy --- Philosophy, Natural --- Physical sciences --- Dynamics --- Relativistic quantum field theory --- Field theory (Physics) --- Quantum theory --- Relativity (Physics) --- Elementary particles (Physics) --- High energy physics --- Nuclear particles --- Nucleons --- Main Injector Neutrino Oscillation Search
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This book is the result of a working group sponsored by ISSI in Bern, which was initially created to study possible ways to calibrate a Far Ultraviolet (FUV) instrument after launch. In most cases, ultraviolet instruments are well calibrated on the ground, but unfortunately, optics and detectors in the FUV are very sensitive to contaminants and it is very challenging to prevent contamination before and during the test and launch sequences of a space mission. Therefore, ground calibrations need to be confirmed after launch and it is necessary to keep track of the temporal evolution of the sensitivity of the instrument during the mission. The studies presented here cover various fields of FUV spectroscopy with the exclusion of direct solar UV spectroscopy, including a catalog of stellar spectra, data-sets of lunar Irradiance, observations of comets and measurements of the interplanetary background. Detailed modeling of the interplanetary background is presented as well. This work also includes comparisons of older data-sets with current ones. This raises the question of the consistency of the existing data-sets. Previous experiments have been calibrated independently and comparison of the data-sets may lead to inconsistencies. The authors have tried to check that possibility in the data-sets and when relevant, suggest a correction factor for the corresponding data.
Heliosphere (Astrophysics) -- Congresses. --- Solar cosmic rays -- Congresses. --- Solar flares -- Congresses. --- Astronomy & Astrophysics --- Physical Sciences & Mathematics --- Astrophysics --- Astronomical instruments --- Vacuum ultraviolet spectroscopy. --- Far ultraviolet detectors. --- Stars --- Calibration. --- Spectra. --- Spectrum of the stars --- Stellar spectra --- Far ultraviolet spectroscopy --- Astronomy --- Instruments, Astronomical --- Instruments --- Physics. --- Observations, Astronomical. --- Space sciences. --- Spectroscopy. --- Microscopy. --- Extraterrestrial Physics, Space Sciences. --- Spectroscopy and Microscopy. --- Astronomy, Observations and Techniques. --- Observations. --- Analysis, Microscopic --- Light microscopy --- Micrographic analysis --- Microscope and microscopy --- Microscopic analysis --- Optical microscopy --- Optics --- Analysis, Spectrum --- Spectra --- Spectrochemical analysis --- Spectrochemistry --- Spectroscopy --- Chemistry, Analytic --- Interferometry --- Radiation --- Wave-motion, Theory of --- Absorption spectra --- Light --- Spectroscope --- Science and space --- Space research --- Cosmology --- Science --- Astronomical observations --- Observations, Astronomical --- Natural philosophy --- Philosophy, Natural --- Physical sciences --- Dynamics --- Qualitative --- Ultraviolet detectors --- Ultraviolet spectroscopy --- Optical instruments --- Physical instruments --- Scientific apparatus and instruments --- Space optics --- Astrophysics. --- Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). --- Astronomical physics --- Cosmic physics --- Physics --- Astronomy—Observations. --- Spectrometry --- Analytical chemistry --- Solar system. --- Spectrum analysis. --- Space Physics.
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