Circling in on Convective Organization

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Circling in on Convective Organization. / Härter, Jan Olaf Mirko; Böing, Steven J.; Henneberg, Olga Cassandra; Nissen, Silas Boye.

In: Geophysical Research Letters, Vol. 46, 21.06.2019, p. 1-11.

Research output: Contribution to journalLetterResearchpeer-review

Harvard

Härter, JOM, Böing, SJ, Henneberg, OC & Nissen, SB 2019, 'Circling in on Convective Organization', Geophysical Research Letters, vol. 46, pp. 1-11. https://doi.org/10.1029/2019GL082092

APA

Härter, J. O. M., Böing, S. J., Henneberg, O. C., & Nissen, S. B. (2019). Circling in on Convective Organization. Geophysical Research Letters, 46, 1-11. https://doi.org/10.1029/2019GL082092

Vancouver

Härter JOM, Böing SJ, Henneberg OC, Nissen SB. Circling in on Convective Organization. Geophysical Research Letters. 2019 Jun 21;46:1-11. https://doi.org/10.1029/2019GL082092

Author

Härter, Jan Olaf Mirko ; Böing, Steven J. ; Henneberg, Olga Cassandra ; Nissen, Silas Boye. / Circling in on Convective Organization. In: Geophysical Research Letters. 2019 ; Vol. 46. pp. 1-11.

Bibtex

@article{068f0286bf8f4232a1aeb32634b9285c,
title = "Circling in on Convective Organization",
abstract = "Cold pools (CPs) contribute to convective organization. However, it is unclear by which mechanisms organization occurs. By using a particle method to track CP gust fronts in large eddy simulations, we characterize the basic collision modes between CPs. Our results show that CP interactions, where three expanding gust fronts force an updraft, are key at triggering new convection. Using this, we conceptualize CP dynamics into a parameter-free mathematical model: circles expand from initially random points in space. Where two expanding circles collide, a stationary front is formed. However, where three expanding circles enclose a single point, a new expanding circle is seeded. This simple model supports three fundamental features of CP dynamics: precipitation cells constitute a spatially interacting system, CPs come in generations, and scales steadily increase throughout the diurnal cycle. Finally, this model provides a framework for how CPs act to cause convective self-organization, clustering, and extremes.",
author = "H{\"a}rter, {Jan Olaf Mirko} and B{\"o}ing, {Steven J.} and Henneberg, {Olga Cassandra} and Nissen, {Silas Boye}",
year = "2019",
month = jun,
day = "21",
doi = "10.1029/2019GL082092",
language = "English",
volume = "46",
pages = "1--11",
journal = "Geophysical Research Letters",
issn = "0094-8276",
publisher = "Wiley-Blackwell",

}

RIS

TY - JOUR

T1 - Circling in on Convective Organization

AU - Härter, Jan Olaf Mirko

AU - Böing, Steven J.

AU - Henneberg, Olga Cassandra

AU - Nissen, Silas Boye

PY - 2019/6/21

Y1 - 2019/6/21

N2 - Cold pools (CPs) contribute to convective organization. However, it is unclear by which mechanisms organization occurs. By using a particle method to track CP gust fronts in large eddy simulations, we characterize the basic collision modes between CPs. Our results show that CP interactions, where three expanding gust fronts force an updraft, are key at triggering new convection. Using this, we conceptualize CP dynamics into a parameter-free mathematical model: circles expand from initially random points in space. Where two expanding circles collide, a stationary front is formed. However, where three expanding circles enclose a single point, a new expanding circle is seeded. This simple model supports three fundamental features of CP dynamics: precipitation cells constitute a spatially interacting system, CPs come in generations, and scales steadily increase throughout the diurnal cycle. Finally, this model provides a framework for how CPs act to cause convective self-organization, clustering, and extremes.

AB - Cold pools (CPs) contribute to convective organization. However, it is unclear by which mechanisms organization occurs. By using a particle method to track CP gust fronts in large eddy simulations, we characterize the basic collision modes between CPs. Our results show that CP interactions, where three expanding gust fronts force an updraft, are key at triggering new convection. Using this, we conceptualize CP dynamics into a parameter-free mathematical model: circles expand from initially random points in space. Where two expanding circles collide, a stationary front is formed. However, where three expanding circles enclose a single point, a new expanding circle is seeded. This simple model supports three fundamental features of CP dynamics: precipitation cells constitute a spatially interacting system, CPs come in generations, and scales steadily increase throughout the diurnal cycle. Finally, this model provides a framework for how CPs act to cause convective self-organization, clustering, and extremes.

U2 - 10.1029/2019GL082092

DO - 10.1029/2019GL082092

M3 - Letter

VL - 46

SP - 1

EP - 11

JO - Geophysical Research Letters

JF - Geophysical Research Letters

SN - 0094-8276

ER -

ID: 222869445