Author: David Michael Weldon
Publisher:
ISBN:
Category :
Languages : en
Pages : 49
Book Description
Measurement of the Sigma- Polarization in the Process Pi- + P Til Sigma- + K+.
Author: David Michael Weldon
Publisher:
ISBN:
Category :
Languages : en
Pages : 49
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 49
Book Description
Measurement of the [Sigma]− Polarization in the Process [pi]−+p[right Arrow][Sigma]−+[Kappa].
Author: David Michael Weldon
Publisher:
ISBN:
Category :
Languages : en
Pages : 49
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 49
Book Description
MEASUREMENT OF THE SIGMA- POLARIZATION IN THE REACTION Pi- + P--]IGMA- + K
Author:
Publisher:
ISBN:
Category :
Languages : en
Pages : 14
Book Description
The average polarization of the?− produced in the reaction?− + p →?− + K has been measured between center-of-mass angles 134{sup o} and 166{sup o} for an incident?− momentum of 1145 MeV/c. A polarized proton target was used, and the?− polarization was found by measuring the difference in the production-rate of K+ mesons for protons polarized along the production-plane normal and against it. Spark chambers were used to record the?− and K+ trajectories, and the?− momentum was obtained from a magnetic spectrometer while the K+ momentum was obtained from a range telescope. Each event was kinematically reconstructed in a one constraint fit to help eliminate events produced from protons bound in heavy nuclei of the target. The?− polarization was found to be -0.36 ± 0.46.
Publisher:
ISBN:
Category :
Languages : en
Pages : 14
Book Description
The average polarization of the?− produced in the reaction?− + p →?− + K has been measured between center-of-mass angles 134{sup o} and 166{sup o} for an incident?− momentum of 1145 MeV/c. A polarized proton target was used, and the?− polarization was found by measuring the difference in the production-rate of K+ mesons for protons polarized along the production-plane normal and against it. Spark chambers were used to record the?− and K+ trajectories, and the?− momentum was obtained from a magnetic spectrometer while the K+ momentum was obtained from a range telescope. Each event was kinematically reconstructed in a one constraint fit to help eliminate events produced from protons bound in heavy nuclei of the target. The?− polarization was found to be -0.36 ± 0.46.
Scientific and Technical Aerospace Reports
Author:
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 660
Book Description
Lists citations with abstracts for aerospace related reports obtained from world wide sources and announces documents that have recently been entered into the NASA Scientific and Technical Information Database.
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 660
Book Description
Lists citations with abstracts for aerospace related reports obtained from world wide sources and announces documents that have recently been entered into the NASA Scientific and Technical Information Database.
Nuclear Science Abstracts
Author:
Publisher:
ISBN:
Category : Nuclear energy
Languages : en
Pages : 1534
Book Description
Publisher:
ISBN:
Category : Nuclear energy
Languages : en
Pages : 1534
Book Description
Nuclear Science Abstracts
Author:
Publisher:
ISBN:
Category : Nuclear energy
Languages : en
Pages : 918
Book Description
Publisher:
ISBN:
Category : Nuclear energy
Languages : en
Pages : 918
Book Description
Measurement of the Polarized Structure Function Sigma {sub LT'} for (p{rvec E}, E'p) Pi° in the Delta (1232) Resonance Region
Author:
Publisher:
ISBN:
Category :
Languages : en
Pages :
Book Description
The polarized longitudinal-transverse structure function [sigma]{sub LT'} has been measured for the first time in the [Delta](1232) resonance region at Q2 = 0.40 and 0.65 GeV2. Data for the p{rvec e}, e'p [pi]° reaction were taken at Jefferson Lab with the CEBAF Large Acceptance Spectrometer (CLAS) using longitudinally polarized electrons at an energy of 1.515 GeV. Evidence for interference between resonant and non-resonant amplitudes is discussed using a partial wave analysis. Comparison with previous beam asymmetry measurements at MAMI indicate a deviation from the predicted Q2 dependence of [sigma]{sub LT'} using recent phenomenological models.
Publisher:
ISBN:
Category :
Languages : en
Pages :
Book Description
The polarized longitudinal-transverse structure function [sigma]{sub LT'} has been measured for the first time in the [Delta](1232) resonance region at Q2 = 0.40 and 0.65 GeV2. Data for the p{rvec e}, e'p [pi]° reaction were taken at Jefferson Lab with the CEBAF Large Acceptance Spectrometer (CLAS) using longitudinally polarized electrons at an energy of 1.515 GeV. Evidence for interference between resonant and non-resonant amplitudes is discussed using a partial wave analysis. Comparison with previous beam asymmetry measurements at MAMI indicate a deviation from the predicted Q2 dependence of [sigma]{sub LT'} using recent phenomenological models.
Polarimetric Synthetic Aperture Radar
Author: Irena Hajnsek
Publisher: Springer Nature
ISBN: 3030565041
Category : Technology & Engineering
Languages : en
Pages : 304
Book Description
This open access book focuses on the practical application of electromagnetic polarimetry principles in Earth remote sensing with an educational purpose. In the last decade, the operations from fully polarimetric synthetic aperture radar such as the Japanese ALOS/PalSAR, the Canadian Radarsat-2 and the German TerraSAR-X and their easy data access for scientific use have developed further the research and data applications at L,C and X band. As a consequence, the wider distribution of polarimetric data sets across the remote sensing community boosted activity and development in polarimetric SAR applications, also in view of future missions. Numerous experiments with real data from spaceborne platforms are shown, with the aim of giving an up-to-date and complete treatment of the unique benefits of fully polarimetric synthetic aperture radar data in five different domains: forest, agriculture, cryosphere, urban and oceans.
Publisher: Springer Nature
ISBN: 3030565041
Category : Technology & Engineering
Languages : en
Pages : 304
Book Description
This open access book focuses on the practical application of electromagnetic polarimetry principles in Earth remote sensing with an educational purpose. In the last decade, the operations from fully polarimetric synthetic aperture radar such as the Japanese ALOS/PalSAR, the Canadian Radarsat-2 and the German TerraSAR-X and their easy data access for scientific use have developed further the research and data applications at L,C and X band. As a consequence, the wider distribution of polarimetric data sets across the remote sensing community boosted activity and development in polarimetric SAR applications, also in view of future missions. Numerous experiments with real data from spaceborne platforms are shown, with the aim of giving an up-to-date and complete treatment of the unique benefits of fully polarimetric synthetic aperture radar data in five different domains: forest, agriculture, cryosphere, urban and oceans.
Materials Science for Dentistry
Author: B W Darvell
Publisher: Elsevier
ISBN: 1845696670
Category : Technology & Engineering
Languages : en
Pages : 687
Book Description
Approx.688 pages Approx.688 pages
Publisher: Elsevier
ISBN: 1845696670
Category : Technology & Engineering
Languages : en
Pages : 687
Book Description
Approx.688 pages Approx.688 pages
Turbulence in the Solar Wind
Author: Roberto Bruno
Publisher: Springer
ISBN: 3319434403
Category : Science
Languages : en
Pages : 270
Book Description
This book provides an overview of solar wind turbulence from both the theoretical and observational perspective. It argues that the interplanetary medium offers the best opportunity to directly study turbulent fluctuations in collisionless plasmas. In fact, during expansion, the solar wind evolves towards a state characterized by large-amplitude fluctuations in all observed parameters, which resembles, at least at large scales, the well-known hydrodynamic turbulence. This text starts with historical references to past observations and experiments on turbulent flows. It then introduces the Navier-Stokes equations for a magnetized plasma whose low-frequency turbulence evolution is described within the framework of the MHD approximation. It also considers the scaling of plasma and magnetic field fluctuations and the study of nonlinear energy cascades within the same framework. It reports observations of turbulence in the ecliptic and at high latitude, treating Alfvénic and compressive fluctuations separately in order to explain the transport of mass, momentum and energy during the expansion. Further, existing models are compared with direct observations in the heliosphere. The problem of self-similar and anomalous fluctuations in the solar wind is then addressed using tools provided by dynamical system theory and discussed on the basis of available models and observations. The book highlights observations of Yaglom’s law in solar wind turbulence, which is one of the most important findings in fully developed turbulence and directly related to the long-lasting and still unsolved problem of solar wind plasma heating. Lastly, it includes a short chapter dedicated to the kinetic range of fluctuations, which has recently been receiving more attention from the space plasma community, since this is inherently related to turbulent energy dissipation and consequent plasma heating. It particularly focuses on the nature and role of the fluctuations populating this frequency range, and discusses several model predictions and recent observational findings in this context.
Publisher: Springer
ISBN: 3319434403
Category : Science
Languages : en
Pages : 270
Book Description
This book provides an overview of solar wind turbulence from both the theoretical and observational perspective. It argues that the interplanetary medium offers the best opportunity to directly study turbulent fluctuations in collisionless plasmas. In fact, during expansion, the solar wind evolves towards a state characterized by large-amplitude fluctuations in all observed parameters, which resembles, at least at large scales, the well-known hydrodynamic turbulence. This text starts with historical references to past observations and experiments on turbulent flows. It then introduces the Navier-Stokes equations for a magnetized plasma whose low-frequency turbulence evolution is described within the framework of the MHD approximation. It also considers the scaling of plasma and magnetic field fluctuations and the study of nonlinear energy cascades within the same framework. It reports observations of turbulence in the ecliptic and at high latitude, treating Alfvénic and compressive fluctuations separately in order to explain the transport of mass, momentum and energy during the expansion. Further, existing models are compared with direct observations in the heliosphere. The problem of self-similar and anomalous fluctuations in the solar wind is then addressed using tools provided by dynamical system theory and discussed on the basis of available models and observations. The book highlights observations of Yaglom’s law in solar wind turbulence, which is one of the most important findings in fully developed turbulence and directly related to the long-lasting and still unsolved problem of solar wind plasma heating. Lastly, it includes a short chapter dedicated to the kinetic range of fluctuations, which has recently been receiving more attention from the space plasma community, since this is inherently related to turbulent energy dissipation and consequent plasma heating. It particularly focuses on the nature and role of the fluctuations populating this frequency range, and discusses several model predictions and recent observational findings in this context.