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Dive into the research topics where Peter H. Haynes is active.

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Featured researches published by Peter H. Haynes.


Reviews of Geophysics | 1995

Stratosphere-troposphere exchange

James R. Holton; Peter H. Haynes; Michael E. McIntyre; Anne R. Douglass; Richard B. Rood; Leonhard Pfister

In the past, studies of stratosphere-troposphere exchange of mass and chemical species have mainly emphasized the synoptic- and small-scale mechanisms of exchange. This review, however, includes also the global-scale aspects of exchange, such as the transport across an isentropic surface (potential temperature about 380 K) that in the tropics lies just above the tropopause, near the 100-hPa pressure level. Such a surface divides the stratosphere into an “overworld” and an extratropical “lowermost stratosphere” that for transport purposes need to be sharply distinguished. This approach places stratosphere-troposphere exchange in the framework of the general circulation and helps to clarify the roles of the different mechanisms involved and the interplay between large and small scales. The role of waves and eddies in the extratropical overworld is emphasized. There, wave-induced forces drive a kind of global-scale extratropical “fluid-dynamical suction pump,” which withdraws air upward and poleward from the tropical lower stratosphere and pushes it poleward and downward into the extratropical troposphere. The resulting global-scale circulation drives the stratosphere away from radiative equilibrium conditions. Wave-induced forces may be considered to exert a nonlocal control, mainly downward in the extratropics but reaching laterally into the tropics, over the transport of mass across lower stratospheric isentropic surfaces. This mass transport is for many purposes a useful measure of global-scale stratosphere-troposphere exchange, especially on seasonal or longer timescales. Because the strongest wave-induced forces occur in the northern hemisphere winter season, the exchange rate is also a maximum at that season. The global exchange rate is not determined by details of near-tropopause phenomena such as penetrative cumulus convection or small-scale mixing associated with upper level fronts and cyclones. These smaller-scale processes must be considered, however, in order to understand the finer details of exchange. Moist convection appears to play an important role in the tropics in accounting for the extreme dehydration of air entering the stratosphere. Stratospheric air finds its way back into the troposphere through a vast variety of irreversible eddy exchange phenomena, including tropopause folding and the formation of so-called tropical upper tropospheric troughs and consequent irreversible exchange. General circulation models are able to simulate the mean global-scale mass exchange and its seasonal cycle but are not able to properly resolve the tropical dehydration process. Two-dimensional (height-latitude) models commonly used for assessment of human impact on the ozone layer include representation of stratosphere-troposphere exchange that is adequate to allow reasonable simulation of photochemical processes occurring in the overworld. However, for assessing changes in the lowermost stratosphere, the strong longitudinal asymmetries in stratosphere-troposphere exchange render current two-dimensional models inadequate. Either current transport parameterizations must be improved, or else, more likely, such changes can be adequately assessed only by three-dimensional models.


Reviews of Geophysics | 2001

The quasi‐biennial oscillation

Mark P. Baldwin; Lesley J. Gray; Timothy J. Dunkerton; Kevin Hamilton; Peter H. Haynes; William J. Randel; James R. Holton; M. J. Alexander; Isamu Hirota; T. Horinouchi; Dylan B. A. Jones; Jonathan S. Kinnersley; C. Marquardt; Kaoru Sato; Masaaki Takahashi

The quasi-biennial oscillation (QBO) dominates the variability of the equatorial stratosphere (∼16–50 km) and is easily seen as downward propagating easterly and westerly wind regimes, with a variable period averaging approximately 28 months. From a fluid dynamical perspective, the QBO is a fascinating example of a coherent, oscillating mean flow that is driven by propagating waves with periods unrelated to that of the resulting oscillation. Although the QBO is a tropical phenomenon, it affects the stratospheric flow from pole to pole by modulating the effects of extratropical waves. Indeed, study of the QBO is inseparable from the study of atmospheric wave motions that drive it and are modulated by it. The QBO affects variability in the mesosphere near 85 km by selectively filtering waves that propagate upward through the equatorial stratosphere, and may also affect the strength of Atlantic hurricanes. The effects of the QBO are not confined to atmospheric dynamics. Chemical constituents, such as ozone, water vapor, and methane, are affected by circulation changes induced by the QBO. There are also substantial QBO signals in many of the shorter-lived chemical constituents. Through modulation of extratropical wave propagation, the QBO has an effect on the breakdown of the wintertime stratospheric polar vortices and the severity of high-latitude ozone depletion. The polar vortex in the stratosphere affects surface weather patterns, providing a mechanism for the QBO to have an effect at the Earths surface. As more data sources (e.g., wind and temperature measurements from both ground-based systems and satellites) become available, the effects of the QBO can be more precisely assessed. This review covers the current state of knowledge of the tropical QBO, its extratropical dynamical effects, chemical constituent transport, and effects of the QBO in the troposphere (∼0–16 km) and mesosphere (∼50–100 km). It is intended to provide a broad overview of the QBO and its effects to researchers outside the field, as well as a source of information and references for specialists. The history of research on the QBO is discussed only briefly, and the reader is referred to several historical review papers. The basic theory of the QBO is summarized, and tutorial references are provided.


Journal of the Atmospheric Sciences | 1991

On the downward control of extratropical diabatic circulations by eddy-induced mean zonal forces

Peter H. Haynes; Michael E. McIntyre; Theodore G. Shepherd; C. J. Marks; Keith P. Shine

Abstract The situation considered is that of a zonally symmetric model of the middle atmosphere subject to a given quasi-steady zonal force F, conceived to be the result of irreversible angular momentum transfer due to the upward propagation and breaking of Rossby and gravity waves together with any other dissipative eddy effects that may be relevant. The models diabatic heating is assumed to have the qualitative character of a relaxation toward some radiatively determined temperature field. To the extent that the force F may be regarded as given, and the extratropical angular momentum distribution is realistic, the extratropical diabatic mass flow across a given isentropic surface may be regarded as controlled exclusively by the F distribution above that surface (implying control by the eddy dissipation above that surface and not, for instance, by the frequency of tropopause folding below). This “downward control” principle expresses a critical part of the dynamical chain of cause and effect governin...


Journal of the Atmospheric Sciences | 1987

On the Evolution of Vorticity and Potential Vorticity in the Presence of Diabatic Heating and Frictional or Other Forces

Peter H. Haynes; Michael E. McIntyre

Abstract Some consequences of regarding potential vorticity as a tracer are considered. It is shown that neither diabatic heating, nor frictional forces, nor external forces such as might be used to model gravity-wave drag, can bring about any net transport or Rossby-Ertel potential vorticity (PV) across an isotropic surface—notwithstanding the diabatic, cross-isentropic transport of mass and chemical tracers. Nor can PV be created or destroyed within a layer bounded by two isentropic surface. It can only be transported along the layer. and diluted or concentrated by cross-isentropic mass inflow or outflow. This constitutes a systematic difference between the behavior of PV and that of other tracers, recognition of which simplifies thinking about PV budgets and gives insight into the relationships between dynamical processes, departures from radiatively determined temperatures, and chemical tracer transport including stratosphere-troposphere exchange. The results just stated are true by virtue of the way ...


Journal of Geophysical Research | 2000

Effective diffusivity as a diagnostic of atmospheric transport: 2. Troposphere and lower stratosphere

Peter H. Haynes; Emily Shuckburgh

The effective diffusivity diagnostic is used to analyze the isentropic transport and mixing properties of observed winds in the upper troposphere and the lower stratosphere (300–450 K), following the approach described in part 1 [Haynes and Shuckburgh, this issue]. Local minima in effective diffusivity on isentropic surfaces in the range 330–400 K indicate transport barriers in each hemisphere associated with the extratropical tropopause. The strongest part of these “tropopause barriers” are coincident with the core of the subtropical jet at about 350 K. They are shown to have a seasonal evolution in which they are strongest in winter and considerably weakened by the monsoon circulations in summer. The barrier in the Southern Hemisphere is seen to be generally stronger than that in Northern Hemisphere during the same season. The minimum value of effective diffusivity on each isentropic surface is proposed as a new definition of the tropopause. This effective-diffusivity definition corresponds most closely to potential vorticity (PV) values of ±2 PVU at 330 K, ±2.5 PVU at 350 K, and ±4.5 PVU at 370 K (with larger values being more appropriate during the summer monsoon period), rather than to the conventional tropopause definition of a single PV value at all levels. It is also demonstrated that the lower limit of the barrier at the stratospheric polar-vortex edge, i.e., the “sub-vortex” transition, varies in altitude throughout the winter. In the Antarctic the transition generally occurs at 380 K and is sometimes as low as 350 K. In the Arctic the transition is higher, rarely occurring below 400 K and frequently occurring above 450 K.


Journal of Geophysical Research | 2000

Effective diffusivity as a diagnostic of atmospheric transport: 1. Stratosphere

Peter H. Haynes; Emily Shuckburgh

The transport and mixing properties of the isentropic flow in the lower and middle stratosphere are analyzed by using observed winds to advect a tracer on isentropic surfaces in the range 400–850 K. The effective diffusivity diagnostic introduced by Nakamura and collaborators is applied to the tracer field in order to identify barriers to transport and mixing regions, and to follow their seasonal evolution. Large effective diffusivity corresponds to strong mixing, and small effective diffusivity corresponds to weak mixing, i.e., to barriers. The effective diffusivity shows, in the winter stratosphere of each hemisphere, the evolution of the vortex-edge barrier and the midlatitude surf zone, and also the extent of any mixing within the vortex. At low latitudes in the stratosphere there is a region of low effective diffusivity whose latitudinal width varies with height, broadening substantially from 400 K to 550 K. The low values of effective diffusivity in this “tropical-reservoir” region imply little isentropic transport into or out of it. There is a strong seasonal cycle to the reservoir, which has different forms at 400 K, 450–600 K, and above 650 K, determined by the relative influences of tropospheric synoptic eddies and stratospheric planetary waves. Comparison of effective diffusivity between the Northern Hemisphere winters 1996/1997 and 1997/1998 shows strong differences at low latitudes according to the phase of the quasi-biennial oscillation (QBO). When there are QBO easterlies, there is a broad region of very low effective diffusivity at low latitudes. When there are QBO westerlies, there are very low values of effective diffusivity at low latitudes within the westerlies themselves but larger values at their edges.


Journal of the Atmospheric Sciences | 1997

The Vertical-Scale Cascade in Atmospheric Tracers due to Large-Scale Differential Advection

Peter H. Haynes; Jerome Anglade

Abstract Reduction in the vertical scale of atmospheric tracer fields occurs as a result of quasi-horizontal stirring by the large-scale flow, provided that the flow varies in the vertical. This scale reduction and the implications for dissipation and mixing are here analyzed using simple mathematical models. The first is based on a steady linear flow and gives simple insight into the interaction between horizontal strain, vertical shear, and diffusion. The second is a simple random-straining model, with random vertical shear being added to a horizontal random strain field. Analytical progress is possible in the limit where the correlation time for the flow is small or large compared to the inverse strain itself. Numerical integration allows investigation of the intermediate case. In all cases the vertical scale decreases exponentially fast, at the same rate as the horizontal scale, with the rate, say S, being controlled by the statistics of the horizontal strain field. As this exponential decrease occurs...


Journal of Fluid Mechanics | 1991

The stability of a two-dimensional vorticity filament under uniform strain

David G. Dritschel; Peter H. Haynes; M. N. Juckes; Theodore G. Shepherd

The quantitative effects of uniform strain and background rotation on the stability of a strip of constant vorticity (a simple shear layer) are examined. The thickness of the strip decreases in time under the strain, so it is necessary to formulate the linear stability analysis for a time-dependent basic flow. The results show that even a strain rate γ (scaled with the vorticity of the strip) as small as 0.25 suppresses the conventional Rayleigh shear instability mechanism, in the sense that the r.m.s. wave steepness cannot amplify by more than a certain factor, and must eventually decay. For γ < 0.25 the amplification factor increases as γ decreases; however, it is only 3 when γ e 0.065. Numerical simulations confirm the predictions of linear theory at small steepness and predict a threshold value necessary for the formation of coherent vortices. The results help to explain the impression from numerous simulations of two-dimensional turbulence reported in the literature that filaments of vorticity infrequently roll up into vortices. The stabilization effect may be expected to extend to two- and three-dimensional quasi-geostrophic flows.


Physics of Fluids | 2003

Diagnosing transport and mixing using a tracer-based coordinate system

Emily Shuckburgh; Peter H. Haynes

The advection-diffusion equation for the concentration of a tracer may be transformed into a pure diffusion equation by using the area inside concentration contours as a coordinate. The corresponding effective diffusivity depends on the geometry of the tracer field, which is determined by the underlying flow. Recent studies have used effective diffusivity, calculated from a suitable tracer, as a qualitative indicator of the transport and mixing properties of a given flow. Here we show that the effective diffusivity may further be used as a quantitative diagnostic of transport and mixing. We use a family of incompressible two-dimensional time-periodic flows as a test-bench and compare the calculated effective diffusivity with other diagnostics. The results demonstrate how the effective diffusivity accurately captures the location and character of barrier and mixing regions. We also show that the effective diffusivity parameterizes the transport of particles relative to the tracer-based coordinates. These r...


Journal of Geophysical Research | 2001

The impact of the mixing properties within the Antarctic stratospheric vortex on ozone loss in spring

Adrian M. Lee; Howard K. Roscoe; Anna E. Jones; Peter H. Haynes; Emily Shuckburgh; Martin W. Morrey; Hugh C. Pumphrey

Calculations of equivalent length from an artificial advected tracer provide new insight into the isentropic transport processes occurring within the Antarctic stratospheric vortex. These calculations show two distinct regions of approximately equal area: a strongly mixed vortex core and a broad ring of weakly mixed air extending out to the vortex boundary. This broad ring of vortex air remains isolated from the core between late winter and midspring. Satellite measurements of stratospheric H2O confirm that the isolation lasts until at least mid-October. A three-dimensional chemical transport model simulation of the Antarctic ozone hole quantifies the ozone loss within this ring and demonstrates its isolation. In contrast to the vortex core, ozone loss in the weakly mixed broad ring is not complete. The reasons are twofold. First, warmer temperatures in the broad ring prevent continuous polar stratospheric cloud (PSC) formation and the associated chemical processing (i.e., the conversion of unreactive chlorine into reactive forms). Second, the isolation prevents ozone-rich air from the broad ring mixing with chemically processed air from the vortex core. If the stratosphere continues to cool, this will lead to increased PSC formation and more complete chemical processing in the broad ring. Despite the expected decline in halocarbons, sensitivity studies suggest that this mechanism will lead to enhanced ozone loss in the weakly mixed region, delaying the future recovery of the ozone hole.

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Peter Hitchcock

National Center for Atmospheric Research

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J. G. Esler

University College London

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William J. Randel

National Center for Atmospheric Research

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