Sentence examples for ray component from inspiring English sources

Based on the isotopic composition of the anomalous cosmic ray component, the ISM flowing into the heliosphere has a solar composition (Section 3).

Since the RMSDS is a function of propagation time and optical power of each ray component, more precise results must be obtained considering multiple wavelength of the illumination LEDs, wavelength-dependent responsivity of receiver, and wavelength-dependent reflectance coefficients.

In order to better understand the physics of acceleration, it is imperative to measure separately the spectrum of each cosmic ray component and to determine accurately the "knee" in the spectrum.

The galactic cosmic ray component of the space radiation environments at aircraft altitudes and on the International Space Station (ISS) were measured by practically identical silicon active detectors in May August 2001.

There were several gamma ray and neutron detectors, although few survived the blast, with all the gauges within 200 feet of ground zero being destroyed, but enough data was recovered to measure the gamma ray component of the ionizing radiation.

This is because there are strong LOS optical ray components caused by the LED headlamp in the V2V cases.

The thermal neutron beam axis is perpendicular to the D+ beam line in order to reduce the fast neutron and the γ ray components in the imaging beam.

For the high latitude and polar ionosphere, however, intervals III, IV and V are also significant since they contain solar cosmic ray and anomalous cosmic ray components.

Time resolved measurements have the advantage of isolating trapped proton and galactic cosmic ray components as was essential to transport code validation in Shuttle data analysis.

In Section 3 we use the Alpha Magnetic Spectrometer (AMS) data to differentiate these two cosmic ray spectral components; these two cosmic ray components excite magnetic irregularity spectra in the plasma, and the ensuing secondary spectra can explain anti-protons, lower energy positrons, and other secondary particles.

By measuring the amount of deflection for a given level of current, in 1890 Schuster was able to estimate the charge-to-mass ratio of the ray components.