The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes.

Bekki Y, Cameron RH, Gizon L.

DOI: 10.1126/sciadv.adk5643
Published: 2024-03-27
Container: Sci Adv
Publisher: Not recorded
Open access: yes

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Cite this work

BibTeX

@article{allodium:10.1126/sciadv.adk5643,
  title = {The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes.},
  author = {Bekki Y and  Cameron RH and  Gizon L.},
  year = {2024},
  journal = {Sci Adv},
  doi = {10.1126/sciadv.adk5643},
  url = {https://doi.org/10.1126/sciadv.adk5643}
}

RIS

TY  - JOUR
TI  - The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes.
AU  - Bekki Y
AU  -  Cameron RH
AU  -  Gizon L.
PY  - 2024
JO  - Sci Adv
DO  - 10.1126/sciadv.adk5643
UR  - https://doi.org/10.1126/sciadv.adk5643
ER  -

APA

Y, B., RH, C., & L., G. (2024). The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes.. Sci Adv. https://doi.org/10.1126/sciadv.adk5643

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europe-pmc · retrieved 2026-09-26T00:04:53.375Z