PoS - Proceedings of Science
Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Solar & Heliospheric. SH-Transient solar phenomena (SEP, GLE, Forbush decreases)
Cosmogenic isotopes Be-7, Be-10, C-14, Na-22 and Cl-36 in the atmosphere: Altitudinal profiles of yield functions
S. Poluianov,* G. Kovaltsov, A. Mishev, I. Usoskin
*corresponding author
Full text: pdf
Pre-published on: September 05, 2017
Published on: August 03, 2018
Abstract
Production of isotopes by cosmic rays in the Earth’s atmosphere plays a key role in many studies in solar physics, geophysics, archeology and other fields. For those purposes, precise quantitative modeling of their production is crucial, and high-resolution altitudinal profiles of production rates are in high demand. Here we present detailed and consistent yield functions of isotopes Be-7, Be-10, C-14, Na-22 and Cl-36 produced by energetic particles in the atmosphere. Comparison
of reconstructions of the Be-10 deposition flux in 1951-2013 and around 775 AD with ice core measurements is shown for illustration of application of our yield functions.
DOI: https://doi.org/10.22323/1.301.0124
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.