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Details of Award

NERC Reference : NE/S015167/1

How does the aurora heat the upper atmosphere?

Fellowship Award

Fellow:
Dr DK Whiter, University of Southampton, Sch of Physics and Astronomy
Science Area:
Atmospheric
Overall Classification:
Panel B
ENRIs:
Environmental Risks and Hazards
Global Change
Science Topics:
Atmospheric chemistry
Aurora
Electric fields
Electron precipitation
Energetic particles
Ionosphere
Iono - thermosphere coupling
Magneto - ionosphere coupling
Mesosphere
Solar activity
Themosphere
Upper Atmos Process & Geospace
Solar & Solar-Terrestrial Phys
Abstract:
My research will study the aurora, a beautiful display caused by energetic particles from space hitting the Earth's atmosphere at about 40 million mph. The aurora typically deposits 50 GW of power into the atmosphere, comparable to the electricity consumption of the UK. This huge energy source has considerable influence on the temperature and composition of the upper atmosphere, particularly in polar regions. The aurora is therefore one of many ingredients needed for computer simulations of the whole atmosphere, which predict changes to Earth's climate and to concentrations of gases such as ozone. Intense currents flow within and around aurora, heating the atmosphere just as an electric current heats a resistor. This heating has dramatic effects on the upper atmosphere, but several fundamental aspects remain undetermined. Previously it has been very difficult to measure the temperature of the atmosphere at auroral heights; it is too high for weather balloons, but too low for spacecraft. However, I recently made the exciting discovery, through experiment and theory, that the ratio of brightnesses of two specific auroral colours depends on the temperature of the atmosphere; therefore by observing these wavelengths in the aurora we can calculate the temperature. My idea is to use extremely sensitive cameras equipped with colour filters to make maps of atmospheric temperature, just like a thermal imaging camera. These temperature maps can be combined with radar measurements of the upper atmosphere to estimate the electrical conductivity, which is an important property influencing the flow of electric current through near-Earth space and the atmosphere. A computer simulation will help me to understand how different types of aurora are produced, what electric currents they generate, and how the aurora affects the temperature and chemistry of the upper atmosphere.
Period of Award:
1 Oct 2019 - 30 Sep 2024
Value:
£529,819
Authorised funds only
NERC Reference:
NE/S015167/1
Grant Stage:
Awaiting Event/Action
Scheme:
Research Fellowship
Grant Status:
Active
Programme:
IRF

This fellowship award has a total value of £529,819  

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FDAB - Financial Details (Award breakdown by headings)

DI - Other CostsIndirect - Indirect CostsDI - StaffDA - Estate CostsDA - Other Directly AllocatedDI - T&S
£28,606£196,463£217,498£40,094£5,070£42,088

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