Sentence examples for proton ratio from inspiring English sources

A fully time-dependent cosmic ray modulation model based on the numerical solution of Parker's transport equation is used to study the amount of particle drifts needed to explain the observed 1.2 GV electron to Helium ratio at Earth and the 2.5 GV electron to proton ratio (e/p) observed by the KET instrument on the Ulysses spacecraft.

Ions are ubiquitous, whereby any molecule with an unbalanced electron to proton ratio results in a net positive or negative electrical charge [ 1].

Using this information together with the latest heliospheric diffusion coefficients, the electron to positron, proton to anti-proton, and electron to proton ratios are computed with a comprehensive numerical diffusive shock and drift modulation model for a simulated heliosphere.

The polymerisation degree of PBLG was determined to be 40 by comparing proton ratios between PEG (−OCH2CH2–: δ=3.7 p.p.m).

As explained by UCLA astrophysicist Edward Wright, the Big Bang would have fizzled in the first second had the neutron- to-proton ratio been just a wee bit more or less than it was.

However, hot fusion reactions tend to produce more neutron-rich products because the actinides have the highest neutron-to-proton ratios of any elements that can presently be made in macroscopic quantities.

The solutions collected from the polarizer outputs were analyzed by H NMR spectroscopy using PEP/PLAC vinyl/methyl proton intensities' ratio.

pH-weighted signal was quantified using amide proton transfer ratio (APTR*) (Chappell et al., 2013; Tee et al., 2014) where low values represent intracellular acidosis.

GPC and 1H NMR analyses of the free pSBMA before and after the acid treatment revealed no difference in the polymer retention time, MW, PDI or the proton integration ratio between the backbone methyl group (C CH3) and the side chain methyl group (N CH3).

In order to maintain stability, the neutron-to-proton (n/p) ratio in nuclei must increase with increasing proton number.

I will present the results of black hole accretion simulations that treat electrons as a separate fluid and show how physically-motivated electron heating rates result in simulated electron temperature distributions that are significantly different from the constant electron-to-proton temperature ratio assumed in previous work.