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Modeling Atmospheric Transport of Cosmogenic Radionuclide $^{10}$Be Using GEOS‐Chem 14.1.1 and ECHAM...

Modeling Atmospheric Transport of Cosmogenic Radionuclide $^{10}$Be Using GEOS‐Chem 14.1.1 and ECHAM...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_hal_primary_oai_HAL_hal_04724633v1

Modeling Atmospheric Transport of Cosmogenic Radionuclide $^{10}$Be Using GEOS‐Chem 14.1.1 and ECHAM6.3‐HAM2.3: Implications for Solar and Geomagnetic Reconstructions

About this item

Full title

Modeling Atmospheric Transport of Cosmogenic Radionuclide $^{10}$Be Using GEOS‐Chem 14.1.1 and ECHAM6.3‐HAM2.3: Implications for Solar and Geomagnetic Reconstructions

Publisher

American Geophysical Union

Journal title

Geophysical research letters, 2024-01, Vol.51 (2)

Language

English

Formats

Publication information

Publisher

American Geophysical Union

More information

Scope and Contents

Contents

A prerequisite to applying $^{10}$Be in natural archives for solar and geomagnetic reconstructions is to know how 10 Be deposition reflects atmospheric production changes. However, this relationship remains debated. To address this, we use two state‐of‐the‐art global models GEOS‐Chem and ECHAM6.3‐HAM2.3 with the latest beryllium production model. D...

Alternative Titles

Full title

Modeling Atmospheric Transport of Cosmogenic Radionuclide $^{10}$Be Using GEOS‐Chem 14.1.1 and ECHAM6.3‐HAM2.3: Implications for Solar and Geomagnetic Reconstructions

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_hal_primary_oai_HAL_hal_04724633v1

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_hal_primary_oai_HAL_hal_04724633v1

Other Identifiers

ISSN

0094-8276

E-ISSN

1944-8007

DOI

10.1029/2023GL106642

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