Publications


On the relative humidity of the atmosphere

in The Global Circulation of the Atmosphere, Princeton University Press (2007) 6

RT Pierrehumbert


Intercomparison of tropical tropospheric humidity in GCMs with AMSU-B water vapor data

GEOPHYSICAL RESEARCH LETTERS 34 (2007) ARTN L17812

H Brogniez, RT Pierrehumbert


Investigating plausible mechanisms to trigger a deglaciation from a hard snowball Earth

COMPTES RENDUS GEOSCIENCE 339 (2007) 274-287

G Le Hir, G Ramstein, Y Donnadieu, RT Pierrehumbert


An ocean of air: A natural history of the atmosphere

NATURE 447 (2007) 911-911

RT Pierrehumbert


The dynamics behind Titan's methane clouds.

Proceedings of the National Academy of Sciences of the United States of America 103 (2006) 18421-18426

JL Mitchell, RT Pierrehumbert, DMW Frierson, R Caballero

We present results of an axisymmetric global circulation model of Titan with a simplified suite of atmospheric physics forced by seasonally varying insolation. The recent discovery of midlatitude tropospheric clouds on Titan has caused much excitement about the roles of surface sources of methane and the global circulation in forming clouds. Although localized surface sources, such as methane geysers or "cryovolcanoes," have been invoked to explain these clouds, we find in this work that clouds appear in regions of convergence by the mean meridional circulation and over the poles during solstices, where the solar forcing reaches its seasonal maximum. Other regions are inhibited from forming clouds because of dynamical transports of methane and strong subsidence. We find that for a variety of moist regimes, i.e., with the effect of methane thermodynamics included, the observed cloud features can be explained by the large-scale dynamics of the atmosphere. Clouds at the solsticial pole are found to be a robust feature of Titan's dynamics, whereas isolated midlatitude clouds are present exclusively in a variety of moist dynamical regimes. In all cases, even without including methane thermodynamics, our model ceases to produce polar clouds approximately 4-6 terrestrial years after solstices.


Modelling the primary control of paleogeography on Cretaceous climate

EARTH AND PLANETARY SCIENCE LETTERS 248 (2006) 426-437

Y Donnadieu, R Pierrehumbert, R Jacob, F Fluteau


A GEOCLIM simulation of climatic and biogeochemical consequences of Pangea breakup

GEOCHEMISTRY GEOPHYSICS GEOSYSTEMS 7 (2006) ARTN Q11019

Y Donnadieu, Y Godderis, R Pierrehumbert, G Dromart, F Fluteau, R Jacob


Using microwave observations to assess large-scale control of free tropospheric water vapor in the mid-latitudes

GEOPHYSICAL RESEARCH LETTERS 33 (2006) ARTN L14801

H Brogniez, RT Pierrehumbert


Climate Change: A Catastrophe in Slow Motion

Chicago Journal of International Law 6 (2006) 6

RT Pierrehumbert


Climate dynamics of a hard snowball Earth

JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES 110 (2005) ARTN D01111

RT Pierrehumbert


Nonnormal amplification of the thermohaline circulation

Journal of Physical Oceanography 35 (2005) 1593-1605

L Zanna, E Tziperman

A simple zonally averaged coupled ocean-atmosphere model, with a relatively high resolution in the meridional direction, is used to examine physical mechanisms leading to transient amplification of thermohaline circulation (THC) anomalies. It is found that in a stable regime, in which small perturbations eventually decay, there are optimal initial conditions leading to a dramatic amplification of initial temperature and salinity anomalies in addition to the THC amplification. The maximum amplification occurs after about 40 years, and the eventual decay is on a centennial time scale. The initial temperature and salinity anomalies are considerably amplified by factors of a few hundreds and 20, respectively. The initial conditions leading to this amplification are characterized by mutually canceling initial temperature and salinity anomalies contributions to the THC anomaly, such that the initial THC anomaly vanishes. The mechanism of amplification is analyzed and found to be the result of an interaction between a few damped (oscillatory and nonoscillatory) modes with decay time scales lying in a range of 20-800 years. The amplification mechanism is also found to be distinct from the advertive feedback leading to THC instabilities for large freshwater forcing. © 2005 American Meteorological Society.


High levels of atmospheric carbon dioxide necessary for the termination of global glaciation.

Nature 429 (2004) 646-649

RT Pierrehumbert

The possibility that the Earth suffered episodes of global glaciation as recently as the Neoproterozoic period, between about 900 and 543 million years ago, has been widely discussed. Termination of such 'hard snowball Earth' climate states has been proposed to proceed from accumulation of carbon dioxide in the atmosphere. Many salient aspects of the snowball scenario depend critically on the threshold of atmospheric carbon dioxide concentrations needed to trigger deglaciation. Here I present simulations with a general circulation model, using elevated carbon dioxide levels to estimate this deglaciation threshold. The model simulates several phenomena that are expected to be significant in a 'snowball Earth' scenario, but which have not been considered in previous studies with less sophisticated models, such as a reduction of vertical temperature gradients in winter, a reduction in summer tropopause height, the effect of snow cover and a reduction in cloud greenhouse effects. In my simulations, the system remains far short of deglaciation even at atmospheric carbon dioxide concentrations of 550 times the present levels (0.2 bar of CO2). I find that at much higher carbon dioxide levels, deglaciation is unlikely unless unknown feedback cycles that are not captured in the model come into effect.


Warming the world.

Nature 432 (2004) 677-

RT Pierrehumbert


Hydrothermal plume dynamics on Europa: Implications for chaos formation

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS 109 (2004) ARTN E03008

JC Goodman, GC Collins, J Marshall, RT Pierrehumbert


Hydrothermal plume dynamics on Europa: Implications for chaos formation

Journal of Geophysical Research E: Planets 109 (2004)

JC Goodman, GC Collins, J Marshall, RT Pierrehumbert

Hydrothermal plumes may be responsible for transmitting radiogenic or tidally generated heat from Europa's rocky interior through a liquid ocean to the base of its ice shell. This process has been implicated in the formation of chaos regions and lenticulae by melting or exciting convection in the ice layer. In contrast to earlier work, we argue that Europa's ocean should be treated as an unstratified fluid. We have adapted and expanded upon existing work describing buoyant plumes in a rotating, unstratified environment. We discuss the scaling laws governing the flow and geometry of plumes on Europa and perform a laboratory experiment to obtain scaling constants and to visualize plume behavior in a Europa-like parameter regime. We predict that hydrothermal plumes on Europa are of a lateral scale (at least 25-50 km) comparable to large chaos regions; they are too broad to be responsible for the formation of individual lenticulae. Plume heat fluxes (0.1-10 W/m2) are too weak to allow complete melt-through of the ice layer. Current speeds in the plume (3-8 mm/s) are much slower than indicated by previous studies. The observed movement of ice blocks in the Conamara Chaos region is unlikely to be driven by such weak flow. Copyright 2004 by the American Geophysical Union.


Abrupt climate change.

Science (New York, N.Y.) 299 (2003) 2005-2010

RB Alley, J Marotzke, WD Nordhaus, JT Overpeck, DM Peteet, RA Pielke, RT Pierrehumbert, PB Rhines, TF Stocker, LD Talley, JM Wallace

Large, abrupt, and widespread climate changes with major impacts have occurred repeatedly in the past, when the Earth system was forced across thresholds. Although abrupt climate changes can occur for many reasons, it is conceivable that human forcing of climate change is increasing the probability of large, abrupt events. Were such an event to recur, the economic and ecological impacts could be large and potentially serious. Unpredictability exhibited near climate thresholds in simple models shows that some uncertainty will always be associated with projections. In light of these uncertainties, policy-makers should consider expanding research into abrupt climate change, improving monitoring systems, and taking actions designed to enhance the adaptability and resilience of ecosystems and economies.


Erratum: Decay of passive scalars under the action of single scale smooth velocity fields in bounded two-dimensional domains - From non-self-similar probability distribution functions to self-similar eigenmodes (Physical Review E (2002) 66 (056302))

Physical Review E - Statistical, Nonlinear, and Soft Matter Physics 68 (2003) 199031-

J Sukhatme, RT Pierrehumbert


Glacial flow of floating marine ice in ''Snowball Earth''

JOURNAL OF GEOPHYSICAL RESEARCH-OCEANS 108 (2003) ARTN 3308

JC Goodman, RT Pierrehumbert


Risk and reason: Safety, law, and the environment

NATURE 422 (2003) 263-263

RT Pierrehumbert


Decay of passive scalars under the action of single scale smooth velocity fields in bounded two-dimensional domains: From non-self-similar probability distribution functions to self-similar eigenmodes (vol E 66, art no 056302, 2002)

PHYSICAL REVIEW E 68 (2003) ARTN 019903

J Sukhatme, RT Pierrehumbert

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