Sentence examples for interstellar secondary from inspiring English sources

We describe constraints on the source energy spectrum of electrons, which appears to have the same shape as that of nuclear cosmic rays, and we discuss the evidence that positrons are predominantly if not exclusively of interstellar secondary origin.

We have investigated the effect of reacceleration on interstellar flux of K-capture secondaries 49V and 51Cr.

It was noted (Zank et al. 1996) that energetic neutral H created via charge exchange in the IHS and fast solar wind could "splash" back into the interstellar medium where they would experience a secondary charge exchange.

Above about 1 GeV, models in which antiprotons are secondary products of the interactions of primary cosmic rays with the interstellar gas agree with the BESS antiproton spectrum.

The p energy spectrum measured by the recent BESS experiment shows the characteristic peak around 2 GeV, which was expected from "secondary" p's, i.e., produced in cosmic-ray interactions with the interstellar gas.

Abundances of the β-decay radioactive secondaries, produced by fragmentation of the cosmic rays during transport in the interstellar medium (ISM), depend on the time scales for spallation and escape from the Galaxy.

In order to show the importance of our results for multi-messenger studies about the physics of CR propagation, we evaluate the propagated spectra of Galactic secondary nuclei, leptons, and gamma rays produced by the interactions of CRs with the interstellar gas, exploiting the numerical codes DRAGON and GammaSky.

A major science goal is the measurement of secondary nuclei at high energy (produced by spallation reactions of heavier cosmic rays in the interstellar medium).

This task is however hampered by the existence of a secondary "background" flux of antiprotons produced in the interactions of cosmic-ray particles in the interstellar medium.

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Interstellar travel beckons, too.