Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
Menu
Juno Jupiter image

Tim Palmer

Emeritus

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Predictability of weather and climate
Tim.Palmer@physics.ox.ac.uk
Telephone: 01865 (2)72897
Robert Hooke Building, room S43
  • About
  • Publications

Singular vectors, metrics, and adaptive observations

JOURNAL OF THE ATMOSPHERIC SCIENCES 55:4 (1998) 633-653

Authors:

TN Palmer, R Gelaro, J Barkmeijer, R Buizza
More details from the publisher

The ECMWF Ensemble Prediction System

Meteorological Applications Wiley 4:4 (1997) 301-304

Authors:

TN Palmer, J Barkmeijer, R Buizza, T Petroliagis
More details from the publisher

Predictability of a Coupled Model of ENSO Using Singular Vector Analysis. Part II: Optimal Growth and Forecast Skill

Monthly Weather Review American Meteorological Society 125:9 (1997) 2057-2073

Authors:

Yan Xue, MA Cane, SE Zebiak, TN Palmer
More details from the publisher
More details

Potential use of the ECMWF Ensemble Prediction System in cases of extreme weather events

Meteorological Applications Wiley 4:1 (1997) 69-84

Authors:

T Petroliagis, R Buizza, A Lanzinger, TN Palmer
More details from the publisher

A study of the predictability of tropical pacific SST in a coupled atmosphere-ocean model using singular vector analysis: The role of the annual cycle and the ENSO cycle

Monthly Weather Review 125:5 (1997) 831-845

Authors:

YQ Chen, DS Battisti, TN Palmer, J Barsugli, ES Sarachik

Abstract:

The authors examine the sensitivity of the Battisti coupled atmosphere-ocean model - considered as a forecast model for the E1 Niño-Southern Oscillation (ENSO) - to perturbations in the sea surface temperature (SST) field applied at the beginning of a model integration. The spatial structures of the fastest growing SST perturbations are determined by singular vector analysis of an approximation to the propagator for the linearized system. Perturbation growth about the following four reference trajectories is considered: (i) the annual cycle, (ii) a freely evolving model ENSO cycle with an annual cycle in the basic state, (iii) the annual mean basic state, and (iv) a freely evolving model ENSO cycle with an annual mean basic state. Singular vectors with optimal growth over periods of 3, 6, and 9 months are computed. The magnitude of maximum perturbation growth is highly dependent on both the phase of the seasonal cycle and the phase of the ENSO cycle at which the perturbation is applied and on the duration over which perturbations are allowed to evolve. However, the spatial structure of the optimal perturbation is remarkably insensitive to these factors. The structure of the optimal perturbation consists of an east-west dipole spanning the entire tropical Pacific basin superimposed on a north-south dipole in the eastern tropical Pacific. A simple physical interpretation for the optimal pattern is provided. In most cases investigated, there is only one structure that exhibits growth. Maximum perturbation growth takes place for integrations that include the period June-August, and the minimum growth for integrations that include the period January-April. Maxima in potential growth also occur for forecasts of ENSO onset and decay, while minima occur for forecasts initialized during the beginning of a warm event, after the transition from a warm to a cold event, and continuing through the cold event. The physical processes responsible for the large variation in the amplitude of the optimal perturbation growth are identified. The implications of these results for the predictability of short-term climate in the tropical Pacific are discussed.
More details from the publisher
More details

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 45
  • Page 46
  • Page 47
  • Page 48
  • Current page 49
  • Page 50
  • Page 51
  • Page 52
  • Page 53
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet