Assessment of 53Mn deposition on Earth via accelerator mass spectrometry
The 53Mn flux onto Earth is a quantity relevant for different extraterrestrial and astrophysical questions. It is a proxy for related fluxes, such as supernova-produced material or interplanetary dust particles. In this work, we performed a first attempt to assess the 53Mn flux by measuring the 53Mn...
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2018
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_09698043_v140_n_p342_Rodrigues http://hdl.handle.net/20.500.12110/paper_09698043_v140_n_p342_Rodrigues |
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paper:paper_09698043_v140_n_p342_Rodrigues2023-06-08T15:59:05Z Assessment of 53Mn deposition on Earth via accelerator mass spectrometry Deposition Extraterrestrial atmospheres Particle accelerators Upper atmosphere Accelerator mass spectrometry Interplanetary dust particles Isotopic ratios Production rates Upper limits Mass spectrometry Antarctica article atmosphere mass spectrometry The 53Mn flux onto Earth is a quantity relevant for different extraterrestrial and astrophysical questions. It is a proxy for related fluxes, such as supernova-produced material or interplanetary dust particles. In this work, we performed a first attempt to assess the 53Mn flux by measuring the 53Mn/10Be isotopic ratio in a 1400 L sample of molten Antarctic snow by AMS (Accelerator Mass Spectrometry). Using the 10Be production rate in the atmosphere, an upper limit of 5.5 × 103 atoms cm−2 yr−1 was estimated for the deposition of extraterrestrial 53Mn. This result is compatible with one of the two discrepant values existing in the literature. © 2018 Elsevier Ltd 2018 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_09698043_v140_n_p342_Rodrigues http://hdl.handle.net/20.500.12110/paper_09698043_v140_n_p342_Rodrigues |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Deposition Extraterrestrial atmospheres Particle accelerators Upper atmosphere Accelerator mass spectrometry Interplanetary dust particles Isotopic ratios Production rates Upper limits Mass spectrometry Antarctica article atmosphere mass spectrometry |
spellingShingle |
Deposition Extraterrestrial atmospheres Particle accelerators Upper atmosphere Accelerator mass spectrometry Interplanetary dust particles Isotopic ratios Production rates Upper limits Mass spectrometry Antarctica article atmosphere mass spectrometry Assessment of 53Mn deposition on Earth via accelerator mass spectrometry |
topic_facet |
Deposition Extraterrestrial atmospheres Particle accelerators Upper atmosphere Accelerator mass spectrometry Interplanetary dust particles Isotopic ratios Production rates Upper limits Mass spectrometry Antarctica article atmosphere mass spectrometry |
description |
The 53Mn flux onto Earth is a quantity relevant for different extraterrestrial and astrophysical questions. It is a proxy for related fluxes, such as supernova-produced material or interplanetary dust particles. In this work, we performed a first attempt to assess the 53Mn flux by measuring the 53Mn/10Be isotopic ratio in a 1400 L sample of molten Antarctic snow by AMS (Accelerator Mass Spectrometry). Using the 10Be production rate in the atmosphere, an upper limit of 5.5 × 103 atoms cm−2 yr−1 was estimated for the deposition of extraterrestrial 53Mn. This result is compatible with one of the two discrepant values existing in the literature. © 2018 Elsevier Ltd |
title |
Assessment of 53Mn deposition on Earth via accelerator mass spectrometry |
title_short |
Assessment of 53Mn deposition on Earth via accelerator mass spectrometry |
title_full |
Assessment of 53Mn deposition on Earth via accelerator mass spectrometry |
title_fullStr |
Assessment of 53Mn deposition on Earth via accelerator mass spectrometry |
title_full_unstemmed |
Assessment of 53Mn deposition on Earth via accelerator mass spectrometry |
title_sort |
assessment of 53mn deposition on earth via accelerator mass spectrometry |
publishDate |
2018 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_09698043_v140_n_p342_Rodrigues http://hdl.handle.net/20.500.12110/paper_09698043_v140_n_p342_Rodrigues |
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1768544145020813312 |