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Storms and convection on Uranus and Neptune: impact of methane abundance revealed by a 3D cloud-reso...

Storms and convection on Uranus and Neptune: impact of methane abundance revealed by a 3D cloud-reso...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3105553338

Storms and convection on Uranus and Neptune: impact of methane abundance revealed by a 3D cloud-resolving model

About this item

Full title

Storms and convection on Uranus and Neptune: impact of methane abundance revealed by a 3D cloud-resolving model

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2024-09

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Uranus and Neptune have atmospheres dominated by molecular hydrogen and helium. In the upper troposphere, methane is the third main molecule and condenses, yielding a vertical gradient in CH4. This condensable species being heavier than H2 and He, the resulting change in mean molecular weight due to condensation comes as a factor countering dry and...

Alternative Titles

Full title

Storms and convection on Uranus and Neptune: impact of methane abundance revealed by a 3D cloud-resolving model

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_3105553338

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3105553338

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2409.02091

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