(1)日球层外的星际宇宙射线光谱和(2)本地介质中的星际宇宙射线光谱:它们是一样的吗?

E. Orlando
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引用次数: 1

摘要

星际宇宙射线(CR)光谱就在日球层外,由于CR的直接测量,太阳调制给出了不确定性。星际CR光谱在局部介质(即在太阳周围~1 kpc范围内)可以间接获得,这要归功于对星际辐射的观测,包括无线电/微波以及CR与星际介质和银河系磁场相互作用产生的伽马射线。对这些星际辐射的观测是了解银河系不同地方CR密度和光谱的宝贵工具。这些光谱的推导依赖于模型假设。直到最近,人们才相信,在考虑了太阳调制和传播效应之后,直接测量到的CR与整个银河系的CR相似。然而,目前的精确数据是不一致的,并提出了重大挑战。日球层外的星际CR光谱和本地介质中的星际CR光谱是否相同,这是一个最近再次提出的问题。我们在此介绍我们为回答这个问题所作的努力和我们最近取得的成果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Interstellar cosmic-ray spectra (1) just outside the heliosphere and (2) in the local medium: are they the same?
Interstellar cosmic ray (CR) spectra just outside the heliosphere are accessible thanks to direct measurements of CR, with uncertainties given by the solar modulation. Interstellar CR spectra in the local medium (i.e. within ~1 kpc around the Sun) are indirectly accessible thanks to observations of interstellar emissions in radio/microwaves and in gamma rays produced by CR interactions with the interstellar medium and the Galactic magnetic field. Observations of these interstellar emissions are an invaluable tool for understanding densities and spectra of CR in different places of our Galaxy. The derivation of these spectra depends on model assumptions. Until recently it was believed that CR as directly measured were resembling CR throughout the Galaxy, after accounting for solar modulation and propagation effects. However, present precise data are discordant and are posing significant challenges. Whether interstellar CR spectra just outside the heliosphere and in the local medium are the same is a question that has recently opened again. We present here our effort in answering this question and our recent results.
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