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4M Project

Funded by UK NERC

People: John Plane, Martyn Chipperfield, Wuhu Feng, Erin Dawkins

Description:
Changes in the mesosphere are an important signal of climate change, and there is increasing evidence that accurate Simulations of changes to the Earth's climate require models with a well resolved and accurate stratosphere and mesosphere. Metal species in the upper atmosphere offer a unique way of observing this region and accuracy of climate models in this domain. The major source of metals in the upper atmosphere is the ablation of the roughly 50 tonnes of interplanetary dust that enters each day from space. This gives rise to the layer of metal atoms and ions that occur globally in the upper mesosphere/lower thermosphere (MLT) region between about 75 and 120 km. The purpose of this NERC funded project is to insert the chemistry of four metals - Na, Fe, Ca and Mg - into a global chemistry-climate model NCAR WACCM in order to use these layers as probes of chemistry and dynamics in the MLT, and to examine the response of the metal layers to the solar cycle, solar proton events, noctilucent clouds and climate change in the middle atmosphere.
Here are five objectives of this project:

  • 1) Determine the ablation flux profiles of individual meteoric metal atoms and ions as a function of altitude, latitude, time-of-day, season and solar cycle; our project partner Dr. Diego Janches will work out based on the look up tables of the elemental ablation profiles for Na, Fe, Ca, Mg and Si produced from Leeds CABMOD model.

 

  • 2) Obtain a near-global data set on the Na, Fe, Ca and K metal atom and ion using UV-NIR dayglow observations with the limb-scanning SCIAMACHY spectrometer on ENVISAT

 

  • 3) Assess the importance of dynamical transport caused by dissipating gravity waves on minor constituents in the MLT. Does this need to be parameterised in General Circulation Models?
  • 4) Develop the first global model of the meteoric metals by inserting the chemistry of Na, Fe, Ca and Mg into the Whole Atmosphere Chemistry Model (WACCM) with project partner Dr. Dan Marsh Validate by comparison with lidar and satellite observations.

 

  • 5) Investigate the likely impact of the solar cycle and climate change on the MLT distributions of all four metals. Investigate the impact of the resolved and improved mesosphere on stratospheric ozone and climate.

 

Link to Leeds 4M workshop 16-18th May 2011

 


Here shows the first preliminary comparison of the annual Na total column abundance from satellite measurements (top panel) and WACCM simulation with Na chemistry (bottom panel). Overall, the model agrees well with the observations but differences still exist. Further detailed investigation is carrying on. .

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WACCM Na chemistry simulation. Comparison with lidar measurements at Starfire Optical Range (35N).

 

Picture2.emf

WACCM Fe chemistry simulation. Comparison with lidar measurements at Rothera station (67S).

 

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Zonal mean Mg+ (top) and Mg (bottom) profile from WACCM Mg chemistry simulation in January.