H, He, Li, and Be isotopes in the PAMELA space experiment, according to the flight data of 2006–2008

被引：0

作者：

Bogomolov E.A. ^{[1
]}

Vasilyev G.I. ^{[1
]}

Krut’kov S.Y. ^{[1
]}

Menn W. ^{[2
]}

Nikonov N.N. ^{[1
]}

Formato V. ^{[3
]}

机构：

[1] Ioffe Institute, Russian Academy of Sciences, St. Petersburg

[2] Department of Physics, University Siegen, Siegen

[3] University of Trieste, Trieste

来源：

Bulletin of the Russian Academy of Sciences: Physics | 2015年 / 79卷 / 03期

基金：

俄罗斯基础研究基金会;

关键词：

Compendex;

D O I：

10.3103/S1062873815030120

中图分类号：

学科分类号：

摘要：

The results from measurements of the isotopic composition of nuclei from hydrogen to beryllium in galactic cosmic rays observed in the orbital experiment near the solar activity minimum in 2006–2008 by analyzing the loss of nucleus ionization with the rigidity known from measuring the trajectories for particles passed through the device without nuclear interaction in the multilayer calorimeter of the PAMELA magnetic spectrometer are presented. The results from measurements are compared to existing experimental and calculated data. © 2015, Allerton Press, Inc.

引用

页码：302 / 305

页数：3