### Abstract

Atmospheric convection has the striking capability to organize itself into a hierarchy of cloud clusters and super-clusters on scales ranging from the convective cell of a few kilometres to planetary scale disturbances such as the Madden–Julian oscillation. It is widely accepted that this phenomenon is due in large part to the two-way coupling between convective processes and equatorially trapped waves and planetary scale flows in general. However, the physical mechanisms responsible for this multiscale organization and the associated across-scale interactions are poorly understood. The two main peculiarities of the tropics are the vanishing of the Coriolis force at the equator and the abundance of mid-level moisture. Here we test the effect of these two physical properties on the organization of convection and its interaction with gravity waves in a simplified primitive equation model for flows parallel to the equator. Convection is represented by deterministic as well as stochastic multicloud models that are known to represent organized convection and convectively coupled waves quite well. It is found here that both planetary rotation and mid-troposphere moisture are important players in the diminishing of organized convection and convectively coupled gravity wave activity in the subtropics and mid-latitudes. The meridional mean circulation increases with latitude while the mean zonal circulation is much shallower and is dominated by mid-level jets, reminiscent of a second baroclinic mode circulation associated with a congestus mode instability in the model. This is consistent with the observed shallow Hadley and Walker circulations accompanied by congestus cloud decks in the higher latitude tropics and sub-tropics. Moreover, deep convection activity in the stochastic model simulations becomes very patchy and unorganized as the computational domain is pushed towards the subtropics and mid-latitudes. This is consistent with previous work based on cloud resolving modeling simulations on smaller domains.

Original language | English (US) |
---|---|

Pages (from-to) | 937-960 |

Number of pages | 24 |

Journal | Climate Dynamics |

Volume | 44 |

Issue number | 3-4 |

DOIs | |

State | Published - 2014 |

### Fingerprint

### Keywords

- Congestus clouds
- Convectively coupled waves
- Organized convection
- Rotation effects
- Stochastic parametrization
- Tropical circulation

### ASJC Scopus subject areas

- Atmospheric Science

### Cite this

*Climate Dynamics*,

*44*(3-4), 937-960. https://doi.org/10.1007/s00382-014-2222-5

**Effects of rotation and mid-troposphere moisture on organized convection and convectively coupled gravity waves.** / Majda, Andrew J.; Khouider, Boualem; Frenkel, Yevgeniy.

Research output: Contribution to journal › Article

*Climate Dynamics*, vol. 44, no. 3-4, pp. 937-960. https://doi.org/10.1007/s00382-014-2222-5

}

TY - JOUR

T1 - Effects of rotation and mid-troposphere moisture on organized convection and convectively coupled gravity waves

AU - Majda, Andrew J.

AU - Khouider, Boualem

AU - Frenkel, Yevgeniy

PY - 2014

Y1 - 2014

N2 - Atmospheric convection has the striking capability to organize itself into a hierarchy of cloud clusters and super-clusters on scales ranging from the convective cell of a few kilometres to planetary scale disturbances such as the Madden–Julian oscillation. It is widely accepted that this phenomenon is due in large part to the two-way coupling between convective processes and equatorially trapped waves and planetary scale flows in general. However, the physical mechanisms responsible for this multiscale organization and the associated across-scale interactions are poorly understood. The two main peculiarities of the tropics are the vanishing of the Coriolis force at the equator and the abundance of mid-level moisture. Here we test the effect of these two physical properties on the organization of convection and its interaction with gravity waves in a simplified primitive equation model for flows parallel to the equator. Convection is represented by deterministic as well as stochastic multicloud models that are known to represent organized convection and convectively coupled waves quite well. It is found here that both planetary rotation and mid-troposphere moisture are important players in the diminishing of organized convection and convectively coupled gravity wave activity in the subtropics and mid-latitudes. The meridional mean circulation increases with latitude while the mean zonal circulation is much shallower and is dominated by mid-level jets, reminiscent of a second baroclinic mode circulation associated with a congestus mode instability in the model. This is consistent with the observed shallow Hadley and Walker circulations accompanied by congestus cloud decks in the higher latitude tropics and sub-tropics. Moreover, deep convection activity in the stochastic model simulations becomes very patchy and unorganized as the computational domain is pushed towards the subtropics and mid-latitudes. This is consistent with previous work based on cloud resolving modeling simulations on smaller domains.

AB - Atmospheric convection has the striking capability to organize itself into a hierarchy of cloud clusters and super-clusters on scales ranging from the convective cell of a few kilometres to planetary scale disturbances such as the Madden–Julian oscillation. It is widely accepted that this phenomenon is due in large part to the two-way coupling between convective processes and equatorially trapped waves and planetary scale flows in general. However, the physical mechanisms responsible for this multiscale organization and the associated across-scale interactions are poorly understood. The two main peculiarities of the tropics are the vanishing of the Coriolis force at the equator and the abundance of mid-level moisture. Here we test the effect of these two physical properties on the organization of convection and its interaction with gravity waves in a simplified primitive equation model for flows parallel to the equator. Convection is represented by deterministic as well as stochastic multicloud models that are known to represent organized convection and convectively coupled waves quite well. It is found here that both planetary rotation and mid-troposphere moisture are important players in the diminishing of organized convection and convectively coupled gravity wave activity in the subtropics and mid-latitudes. The meridional mean circulation increases with latitude while the mean zonal circulation is much shallower and is dominated by mid-level jets, reminiscent of a second baroclinic mode circulation associated with a congestus mode instability in the model. This is consistent with the observed shallow Hadley and Walker circulations accompanied by congestus cloud decks in the higher latitude tropics and sub-tropics. Moreover, deep convection activity in the stochastic model simulations becomes very patchy and unorganized as the computational domain is pushed towards the subtropics and mid-latitudes. This is consistent with previous work based on cloud resolving modeling simulations on smaller domains.

KW - Congestus clouds

KW - Convectively coupled waves

KW - Organized convection

KW - Rotation effects

KW - Stochastic parametrization

KW - Tropical circulation

UR - http://www.scopus.com/inward/record.url?scp=84939890232&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84939890232&partnerID=8YFLogxK

U2 - 10.1007/s00382-014-2222-5

DO - 10.1007/s00382-014-2222-5

M3 - Article

AN - SCOPUS:84939890232

VL - 44

SP - 937

EP - 960

JO - Climate Dynamics

JF - Climate Dynamics

SN - 0930-7575

IS - 3-4

ER -