You've reached Manoj Joshi's SECOND little
gas** station on the web.
That's me on the rocking chair, with my shotgun, smoking my pipe, yip.
**gasoline: n, a volatile flammable mixture of hydrocarbons (hexane and heptane and octane etc.) derived from petroleum; used mainly as a fuel in internal-combustion engines [syn: gasolene, gas, petrol])
I'm the project manager of the QUEST project's earth system model QESM.
Here's a link to the QESM wiki page (password required to enter)
The following things are what I used to get
paid to do- I still do research on these topics:
Climate modelling
I used to be a research scientist at the
Hadley
Centre for Climate Change, doing earth system
science and climate model development, from carbon cycle modelling to
coupled-ocean atmosphere processes in the tropics, to looking at
mechanisms behind land surface temperature feedbacks under climate
change, and climatic effects of volcanic eruptions.
Coupled Ocean-Atmosphere Processes in the North Atlantic
Region
I've coupled a simplified high-resolution (1/6° -
1/12°) shallow-water ocean model of the Atlantic Ocean to the IGCM in order to
investigate the North Atlantic storm track, as well as the potential
changes in the thermohaline circulation. The advantages of this approach
is that it allows the representation of small-scale features like ocean
Kelvin waves and the Gulfstream, but is not as computationally intensive
as running state-of-the-art coupled multilayer global ocean models.
Water vapour in the stratosphere
I'm looking at how
volcanic eruptions change water vapour transport.
It's known that volcanic eruptions act to dry out the upper troposphere, but
the effect on the lower stratosphere might be to make it wetter.
Volcanic eruptions could explain a significant part of the observed increase in
stratospheric water vapour concentrations since 1960. I'm also looking
at the dynamical effects of stratospheric water vapour changes.
Refining metrics of climate change
Radiative
forcing is an example of such a metric (or measure) that is utilised
in the Kyoto Protocol. However, as a measure of climate change, it has
its flaws, so we're trying to find improved metrics of global warming
related to radiative forcing. The METRIC project
website explains more. Click on the publications link at the bottom
of this webpage for references to papers that the METRIC team have
produced.
Terrestrial planetary atmospheres
A lot of my career
has been spent researching the circulation and evolution of the Martian
(and Venusian) atmospheres. Before coming to Reading I spent 4 years
working in this
group. And before that I did a PhD at this place.
Extrasolar planets
This research is about modelling
the atmospheres of planets that nobody has actually found yet! I know
this sounds quite dodgy but there is a reason. Astronomers tend
to concentrate searches for planets around G-type stars like the sun,
rather than smaller M-stars (commonly called red dwarf stars), even
though M stars constitute 80% of all main sequence stars. Some of the
reasons for this are unavoidable given limitations in
technology. However, other reasons for this bias are based on
assumptions about the nature of the geophysics of planets orbiting M
stars which may be flawed. The modelling work aimed to highlight such
flaws.
And finally, obligatory
self-publicity:
Here are some of my publications
An article about the extrasolar planet research appeared in New Scientist in 2001. Read it here.