TY - JOUR
T1 - The Two Diurnal Modes of Tropical Upward Motion
AU - Ruppert, James H.
AU - Klocke, Daniel
N1 - Funding Information:
J. H. R. acknowledges funding for this research from the National Science Foundation (Grant AGS-1524844) and Alexander von Humboldt Foundation/Stiftung. D. K. acknowledges funding through the Hans Ertel Center for Weather Research (HErZ). This German research network of universities, research institutions, and DWD is funded by the BMVI (Federal Ministry of Transport and Digital Infrastructure). We thank Claudia Stephan and three anonymous reviewers for their highly constructive comments, Felicia Brisc of Climate Visualization Laboratory (Center for Earth System Research and Sustainability) for creating and sharing the online animation, and the DWD and the Deutsches Klimarechenzentrum (DKRZ) for providing vital supercomputing resources. All model source code, start data, and postprocessing software used in this study are available online; to ensure reproducibility, representative model output and documentation of the model and software versions employed herein can be obtained with no restrictions from the Max Planck Society at the website (https://pure.mpg.de/pubman/faces/ HomePage.jsp).
Funding Information:
J.?H.?R. acknowledges funding for this research from the National Science Foundation (Grant AGS-1524844) and Alexander von Humboldt Foundation/Stiftung. D.?K. acknowledges funding through the Hans Ertel Center for Weather Research (HErZ). This German research network of universities, research institutions, and DWD is funded by the BMVI (Federal Ministry of Transport and Digital Infrastructure). We thank Claudia Stephan and three anonymous reviewers for their highly constructive comments, Felicia Brisc of Climate Visualization Laboratory (Center for Earth System Research and Sustainability) for creating and sharing the online animation, and the DWD and the Deutsches Klimarechenzentrum (DKRZ) for providing vital supercomputing resources. All model source code, start data, and postprocessing software used in this study are available online; to ensure reproducibility, representative model output and documentation of the model and software versions employed herein can be obtained with no restrictions from the Max Planck Society at the website (https://pure.mpg.de/pubman/faces/HomePage.jsp).
Publisher Copyright:
©2019. American Geophysical Union. All Rights Reserved.
PY - 2019/3/16
Y1 - 2019/3/16
N2 - This study describes a new mechanism governing the diurnal variation of vertical motion in tropical oceanic heavy rainfall zones, such as the intertropical convergence zone. In such regions, the diurnal heating of widespread anvil clouds due to shortwave radiative absorption enhances upward motion in these upper layers in the afternoon. This radiatively driven ascent promotes an afternoon maximum of anvil clouds, indicating a diurnal cloud-radiative feedback. The opposite occurs at nighttime: While rainfall exhibits a dominant peak at night-early morning, the boundary layer rooted upward motion and latent heating tied to this peak are forced to be more bottom heavy by the nighttime anomalous radiative cooling at upper levels. This mechanism therefore favors the stratiform top-heavy heating mode during daytime and suppresses it nocturnally. These diurnal circulation signatures arise from microphysical-radiative feedbacks that manifest on the scales of organized deep convection, which may ultimately impact the daily mean radiation budget.
AB - This study describes a new mechanism governing the diurnal variation of vertical motion in tropical oceanic heavy rainfall zones, such as the intertropical convergence zone. In such regions, the diurnal heating of widespread anvil clouds due to shortwave radiative absorption enhances upward motion in these upper layers in the afternoon. This radiatively driven ascent promotes an afternoon maximum of anvil clouds, indicating a diurnal cloud-radiative feedback. The opposite occurs at nighttime: While rainfall exhibits a dominant peak at night-early morning, the boundary layer rooted upward motion and latent heating tied to this peak are forced to be more bottom heavy by the nighttime anomalous radiative cooling at upper levels. This mechanism therefore favors the stratiform top-heavy heating mode during daytime and suppresses it nocturnally. These diurnal circulation signatures arise from microphysical-radiative feedbacks that manifest on the scales of organized deep convection, which may ultimately impact the daily mean radiation budget.
UR - https://www.scopus.com/pages/publications/85062796708
UR - https://www.scopus.com/pages/publications/85062796708#tab=citedBy
U2 - 10.1029/2018GL081806
DO - 10.1029/2018GL081806
M3 - Article
AN - SCOPUS:85062796708
SN - 0094-8276
VL - 46
SP - 2911
EP - 2921
JO - Geophysical Research Letters
JF - Geophysical Research Letters
IS - 5
ER -