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Vacuum ultraviolet spectroscopy --- 535 --- Far ultraviolet spectroscopy --- Ultraviolet spectroscopy --- Optics --- 535 Optics

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Photochemistry --- Vacuum ultraviolet spectroscopy --- Quantum chemistry --- Photochimie --- Spectroscopie ultraviolette sous vide --- Chimie quantique --- Congresses --- Congrès --- 541.14 <063> --- -Quantum chemistry --- -Vacuum ultraviolet spectroscopy --- -Far ultraviolet spectroscopy --- Ultraviolet spectroscopy --- Chemistry, Quantum --- Chemistry, Physical and theoretical --- Quantum theory --- Excited state chemistry --- Light --- Photolysis (Chemistry) --- Photochemistry--Congressen --- Chemical action --- -Photochemistry--Congressen --- 541.14 <063> Photochemistry--Congressen --- Congrès --- Far ultraviolet spectroscopy --- Molecular orbitals. --- Optical properties. --- Radicals (Chemistry) --- Circular dichroism --- Fragmentation reaction --- Photoelectron spectra --- Photoionization --- Quantum transition

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This volume is for practitioners, experimentalists, and graduate students in applied physics, particularly in the fields of atomic and molecular physics, who work with vacuum ultraviolet applications and are in need of choosing the best type of modern instrumentation. It provides first-hand knowledge of the state-of-the-art equipment sources and gives technical information on how to use it, along with a broad reference bibliography.

Vacuum ultraviolet spectroscopy --- Vacuum ultraviolet spectroscopy. --- Ultraviolet spectra. --- Spectrum analysis. --- Analysis, Spectrum --- Spectra --- Spectrochemical analysis --- Spectrochemistry --- Spectrometry --- Spectroscopy --- Chemistry, Analytic --- Interferometry --- Optics --- Radiation --- Wave-motion, Theory of --- Absorption spectra --- Light --- Spectroscope --- Spectrum, Ultraviolet --- Ultra-violet spectrum --- Spectrum analysis --- Far ultraviolet spectroscopy --- Ultraviolet spectroscopy --- Qualitative --- Analytical chemistry

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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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Particle accelerators and radiation based on radio-frequency (RF) cavities have significantly contributed to the advancement of science and technology in the most recent century. However, the rising costs and scales for building cutting-edge accelerators act as barriers to accessing these particle and radiation sources. Since the introduction of chirped pulse amplification technology in the 1990s, short-pulse, high-power lasers have enabled the realization of laser-driven accelerations and radiation sources. Laser-driven accelerators and radiation sources could be a viable alternative to providing compact and cost-effective particle and photon sources. An accelerating field in a plasma, driven by intense laser pulses, is typically several orders of magnitude greater than that of RF accelerators, while controlling the plasma media and intense laser pulses is highly demanding. Therefore, numerous efforts have been directed toward developing laser-driven high-quality particle beams and radiation sources with the goal of paving the way for these novel sources to be used in a variety of applications. This Special Issue covers the latest developments in laser-based ion and electron accelerators; laser-plasma radiation sources; advanced targetry and diagnostic systems for laser-driven particle accelerators; particle beam transport solutions for multidisciplinary applications; ionizing radiation dose map determination; and new approaches to laser–plasma nuclear fusion using high-intensity, short laser pulses.

spectra of laser accelerated particle beams --- mapping of radiation dose --- GEANT4 simulations --- Monte Carlo simulation --- laser-driven ion acceleration --- imaging plate --- high repetition rate target --- ion acceleration --- laser–plasma interaction --- Thomson parabola --- electromagnetic pulse --- laser electron acceleration --- laser proton acceleration --- high-intensity lasers --- non-destructive testing --- elemental analysis --- petawatt laser --- laser plasma --- laser wakefield acceleration --- compact electron accelerator --- GeV electron beam --- laser-plasma accelerator --- TNSA --- laser-accelerated protons --- magnetic beamline --- Particle Induced X-ray Emission --- laser-produced plasma --- plasma light source --- far-ultraviolet spectroscopy --- Seya–Namioka monochromator --- radiation-hydrodynamics --- collisional-radiative model --- Monte Carlo simulations --- Geant4 --- laser-accelerated ion beams --- proton–boron fusion --- laser–plasma acceleration --- α-particle beam --- n/a --- laser-plasma interaction --- Seya-Namioka monochromator --- proton-boron fusion --- laser-plasma acceleration