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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Publicado: 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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spelling 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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