Welcome to Manoj Joshi's personal (ish) webpage

If you think I'm going to discuss personal stuff on a medium read by every nutter from Berkshire to Brisbane, you must be crazy yourself. This web page confines itself to work.

I'm a university lecturer affiliated with NCAS Climate


From 2012 I work in Environmental Sciences in the University of East Anglia


Here are my areas of research and past roles

Earth system modelling and climate
I was project manager of the QUEST project's earth system model QESM

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.

The land/sea warming contrast
It's well-known that the land warms more than the ocean under climate- but it's less known that the differing thermal inertias of ocean and land are not mainly responsible for this. I've looked at mechanisms underlying this phenomenon under a range of climate forcings.
This is a collaboration with Jonathan Gregory and Hugo Lambert amongst others

Stratospheric change and climate change
A key interest of mine is understanding how the stratosphere mitigates the climate and Earth system response to different radiative drivers or forcings, such as solar variability, volcanic aerosol or water vapour. At the moment I'm examining the effect of radiative vs dynamic effects of solar variability on climate as part of SOLCI. I've also been involved with looking at how the stratosphere changes extratropical response to ENSO (see publications).

Water vapour in the stratosphere
I'm looking at how stratospheric water vapour affects climate. 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 involved with examining other effects of stratospheric water vapour.
Also see The radiation/climate group website
and the The stratosphere/climate group website

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.

Coupled Ocean-Atmosphere Processes
I'm looking at the effect of stochastic processes in the ocean component of the FAMOUS climate model. In the past I've examined the effect of coupling 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.

More recently I've collaborated on work that examined the effect of chlorophyll blooms on SST biases in the Arabian Sea and its effect on the South Asian monsoon.

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
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.

And I suppose I have to mention El Nino and ashes cricket in Australia