Thirty Years of Quo Vadis 

Brian Lo –  

“Quo Vadis”, Latin for “Where are you marching?”, is an annual event held in the Department of Meteorology in which mostly 2nd year PhD students showcase their work to other members in the department. The event provides the opportunity for students to present research in a professional yet friendly environment. Quo Vadis talks usually focus on a broad overview of the project and the questions they are trying to address, the work done so far to address those questions and especially an emphasis on where ongoing research is heading (as the name of the event suggests).  Over the years, presenters have been given constructive feedback from their peers and fellow academics on presentation style and their scientific work. 

This year’s Quo Vadis was held on 1st March 2022 as a hybrid event. Eleven excellent in-person talks covering a wide range of topics were delivered in the one-day event. The two sessions in the morning saw talks that ranged from synoptic meteorology such as atmospheric blocking to space weather-related topics on the atmosphere of Venus, whereas the afternoon session had talks that varied from storms, turbulence, convection to energy storage!  

Every year, anonymous staff judges attend the event and special recognition is given to the best talk. The winning talk is selected based on criteria including knowledge of the subject matter, methods and innovativeness, results, presentation style and ability to answer questions after the presentation. This year, the judges were faced with a difficult decision due to the high standard of cutting-edge research presented in which presenters “demonstrated excellent knowledge of their subject matter, reached conclusions that were strongly supported by their results, produced well-structured presentations, and answered their questions well.” 

This year’s Quo Vadis winner is Natalie Ratcliffe. She gave an impressive presentation titled “Using Aircraft Observations and modelling to improve understanding of mineral dust transport and deposition processes”. The judging panel appreciated the combination of observations and modelling in her work and were impressed by her ability to motivate and communicate her findings in an engaging way. In addition to the winner, three honourable mentions were made this year. These went to Hannah Croad, Brian Lo and James Fallon whose talks were on arctic cyclones, using radar observations in the early identification of severe convection and weather impacts on energy storage respectively. 

Being the first in-person event for a long time, Quo Vadis 2022 was a huge success thanks to our organisers Lauren James and Elliott Sainsbury. Having run for 30 years, Quo Vadis remains a highlight and an important rite of passage for PhD students in the meteorology department. Having presented at this year’s event, I found that summarising a year’s worth of research work in 12 minutes and making it engaging for a general audience is always a challenge. The audience at any level attending the event would at the very least appreciate the diversity of the PhD work within an already specialised field of meteorology. Who knows how Quo Vadis will evolve in the coming 30 years? Long may it continue! 

The Social Metwork in 2021

James Fallon –
Brian Lo – 

Hello readers, and a happy new year to you all! (ok we’re a bit late on that one… but regardless we both wish you a great start to 2022!)

We have really enjoyed reading and publishing all of the posts submitted over the last year, and following all of the research conducted by PhD students in the Reading department of Meteorology. There have been posts on conferences, papers, visitors, and much more, finishing with the heralded Met dept. Pantomime!

Thank you to everyone who has contributed to the Social Metwork over this past year. We are really looking forward to new submissions this term – and whether you are a veteran contributor or have never written for a blog before, we really encourage you to get in touch and write for us 🙂

In the last year, the blog has had over 7900 visitors from all over the world!

Map of visitors to the social metwork in 2021

Compared to 2020 we have seen Brazil and Australia enter the top 10 highest number of readers at 144 and 118 views respectively. And leading with the top 3 number of views are United Kingdom (6495), United States (1134) and China (361).

In case you missed any posts, or want to look through your favourites, here are all of the posts from 2021:

January – Adriaan Hilbers – Carl Haines – Sophia Moreton

February – Chloe Brimicombe – Linda van Garderen – James Fallon & Brian Lo – Lewis Blunn

March – Sophie Cuckow – Brian Lo – Alec Vessey

April – Carl Haines – Daniel Ayers

May – Max Coleman & Chloe Brimicombe – James Fallon

June – Kaja Milczewska – Brian Lo & Chloe Brimicombe

July – Andrea Marcheggiani – Lily Greig – Hannah Croad – Gwyneth Matthews & Helen Hooker

August – Harriet Turner

[ no submissions ]

October – Charlie Suitters – Haonan Ren – Emanuele Gentile – Shammi Akhter

November – Gabriel M P Perez – Helen Hooker – Isabel Smith

December – Kieran Pope – Natalie Ratcliffe

Panto 2021: Hybrid edition – Semi-Lagrangian Rhapsody! 

Charlie Suitters –
Hannah Croad –
Isabel Smith –
Natalie Ratcliffe –

The pantomime has been one of the highlights of the year for the last 3 decades in the Met department. This is put on by the PhD students, and usually performed in person at the end of the Autumn term. Despite the ongoing COVID-19 pandemic, the panto is going from strength to strength, with a virtual instalment in 2020, and adapting to the hybrid format this year. It’s amazing to see the department tradition continue.  

This year the four of us (Charlie Suitters, Hannah Croad, Isabel Smith and Natalie Ratcliffe) agreed to organise the panto. It was clear that the panto this year would need to cater for both people joining in person and virtually, and with the lingering uncertainty of the covid situation in the UK, we came to a group decision to pre-record the performance in advance. This would provide the best viewing experience for everyone, and provided a contingency if the covid situation worsened. In hindsight, this was a good decision. 

This year’s panto was called Semi-Lagrangian Rhapsody, an idea based on the story of the band Queen. On Thursday 9th December 2021 we screened our pre-recorded pantomime in a hybrid format, with people watching both in the Madejski lecture theatre on campus and at home via Teams (probably in their pyjamas). Our story begins with our research group, Helen Dacre, Keith Shine, and Hilary Weller, on the lookout for a fourth member. In an episode of Mets Factor, the group sit through terrible auditions from Katrina and the Rossby Waves, Wet Wet Wet, the Weather Girls and Jedward (comprised of John Methven and Ed Hawkins), before finally stumbling upon Thorwald Stein (aka Eddy Mercury). The research group QUEEN (Quasi-Useful atmosphEric Electricity Nowcasting) is formed. Inspired by an impromptu radiosonde launch on the MSc field trip and skew-Ts (Chris knows!), QUEEN develop a Semi-Lagrangian convection scheme for lightning. Our narrator, SCENARIO administrator Wendy Neale, tells the story of the ups and downs of QUEENs journey, culminating in a presentation of their Semi-Lagrangian Rhapsody to the world at the AMS conference.  

Natalie suggested the idea for the panto, and we all agreed that it was a great idea – especially with the potential for lots of Queen songs! Once we had our storyline, next came the script writing. This was a daunting task, but working as a team we managed to produce a decent first draft in one intensive script-writing week, full of amazing terrible meteorology puns. Whilst writing the script we decided on the best Queen songs for the plot (and for reasons that we cannot explain/remember, a Rebecca Black song too). Now it was time to alter the lyrics, which was a lot of fun! Only once we had written the songs did we actually consider the complexity of Freddie Mercury’s voice and how we, a bunch of non-musically talented PhD students, were going to attempt to do these songs any justice. It was too late to go back though, and we had to break the news to the band. Thankfully they were up to the challenge! 

From week 6 onwards, we were able to start recording scenes; we were lucky that we were able to film in-person in and around the Met Department. We were still able to include students who weren’t in Reading at the time by writing in virtual parts into the panto. This worked perfectly well given the very hybrid nature of life currently anyway. 

Like last year, we wanted to start earlier as we knew that we needed to be finished at least a week – preferably more – before the big night to give time to edit everything in time (there were still a couple of late nights just before the big night). The final late night session did lead to the incredible slow-mo shot of Nicki Robinson (Charlie) turning around in Bohemian Rhapsody, so there is something that can be said about late-night-induced-insanity!  

Come week 10, we had nearly finished all of our filming and only had the songs left to record. We arrived at the London Road music rooms not yet having heard any of the band’s rehearsals. They sounded amazing. Many thanks to James and Gabriel who had been organising the band throughout the term. Then we started singing and immediately reduced the quality! But with a bit of practice around the piano, we started to improve, though the beginning of Bohemian Rhapsody was still a little questionable… With lots of pizza, we managed to record all of the songs in two nights! The band did an amazing job to put up with our musical incompetence (we are so very sorry). 

Over the next week, our three video editors worked hard to put the whole panto together and I hope you agree that they did a good job. This all led up to the big night where we were able to offer a small pre-panto reception in the Met coffee room before the panto started (somewhat attempting to mirror the normal pre-panto buffet). Apart from one slip up in scene 4 (my apologies hehe – Natalie), the screening went nearly perfectly with very few hybrid IT complications. Additionally, we had the return of an in-person performance of Mr Mets by our own Jon Shonk, and a heartwarming singing performance from the staff, organised by Chris Holloway and Keith Shine. Not only were we gifted this, but we were able to enjoy an in-person after-party in the coffee room with DJ Shonk. Of course there were a few Queen songs scattered in the mix, though we realised we struggled to remember the original lyrics and were only able to sing the panto versions! Following the story of Queen may have been a good idea, but have we forever ruined their songs for ourselves forever now? Quite possibly… 

And on that bombshell, we’d like to thank everyone who was involved in this panto, whether that be those who we convinced to act, sing, play in the band, help organise the event or even just come along to the screening. The whole process of creating this panto was exhausting, but so incredibly fun. I (Natalie) am so glad I did it and had a great time, but I now understand the ‘I’ve done my time’ sentiment of the previous organisers. (Hannah) Organising the panto was a lot of work, but so much fun (see bloopers). This has been a really rewarding experience, to see it all come together on the night, and to contribute to a fantastic department tradition. 

This year we sold tickets for the in-person showing and asked for donations to the David Grimes Trust from those viewing from home. Thank you to everyone who has already donated. Your generosity is greatly appreciated. We have managed to raise £170 for the David Grimes Trust. If you would like to donate still, please find our email with details on how to do so from Hannah Croad. 

Thank you to everyone who watched Semi-Lagrangian Rhapsody on Thursday, we hope you had a fun evening whether you watched at home or in-person! 

Cloud-Radiation Interactions and Their Contributions to Convective Self-Aggregation 

Kieran Pope –

Convective self-aggregation is the process by which initially randomly scattered convection becomes spontaneously clustered in space despite uniform initial conditions. This process was first identified in numerical models, however it is relevant to real world convection (Holloway et al., 2017). Tropical weather is dominated by convection, and the degree of convective aggregation has important consequences for weather and climate. A more organised regime is associated with reduced cloudiness, increased longwave emission to space (Bretherton et al., 2005), and a higher frequency of long-lasting extreme precipitation events (Bao and Sherwood, 2019).

Because of its relevance to weather and climate, self-aggregation has been the focus of many recent studies. However, there is still much debate as to the processes that cause aggregation. There is great variability in the rate and degree of aggregation between models, and there remains uncertainty as to how aggregation is affected by climate change (Wing et al., 2020). Previous studies have shown that feedbacks between convection and shortwave & longwave radiation are key drivers and maintainers of aggregation (e.g. Wing & Cronin 2016), and that interactive radiation in models is essential for aggregation to occur (Muller & Bony 2015).

This blog summarises results from the first paper from my PhD (Pope et al., 2021), where we develop and use a framework to analyse how radiative interactions with different cloud types contribute to aggregation. We analyse self-aggregation within a set of three idealised simulations of the UK Met Office Unified Model (UM). The simulations are configured in radiative-convective equilibrium over three fixed sea surface temperatures (SSTs) of 295, 300 and 305 K. They are convection permitting models that are 432 × 6048 km2 in size with a 3 km horizontal grid spacing. The simulations neglect the earth’s rotation, so they approximately represent convection over tropical oceans within a warming climate.

Our analysis framework is based on that used in Wing and Emanuel (2014) which uses the variance of vertically-integrated frozen moist static energy (FMSE) as a measure of aggregation. FMSE is a measure of the total energy an air parcel has if all the water (vapour and frozen) was converted to liquid, neglecting its velocity. Variations in vertically-integrated FMSE come from perturbations in temperature and humidity. As aggregation increases, moist regions get moister and dry regions get drier, so the variance of vertically-integrated FMSE increases.

The problem with using FMSE variance as an aggregation metric is that it is highly sensitive to SST. A warmer atmosphere can hold more water vapour via the Clausius-Clapeyron relationship. This means there is a greater difference in FMSE between the moist and dry regions for higher-SST simulations, so the variance of FMSE is typically much greater for higher SSTs. To account for this problem, we normalise FMSE between hypothetical upper and lower limits which are functions of SST. This gives a value of normalised FMSE between 0 and 1.

Wing and Emanuel (2014) derive a budget equation for the rate of change of FMSE variance which shows how different processes contribute to aggregation. By rederiving their equation for normalised FMSE , we get:

\displaystyle \frac{1}{2}\frac{\partial\widehat{h'}_n^2}{\partial t} = \widehat{h'}_nLW'_n + \widehat{h'}_nSW'_n + \widehat{h'}_nSEF'_n - \widehat{h'}_n\nabla_h\cdot\widehat{\textbf{u}h_n}

where \widehat{h} is vertically-integrated FMSE, LW and SW are the net atmospheric column longwave and shortwave heating rates, SEF is the surface enthalpy flux, made up of the surface latent and sensible heat fluxes, and \nabla h \cdot \widehat{\textbf{u}h} is the horizontal divergence of the \widehat{h} flux. Primes (') indicate local anomalies from the instantaneous domain mean. The subscript (_n) denotes a normalised variable which is the original variable divided by the difference between the hypothetical upper and lower limits of \widehat{h}. The equation shows that the rate of change of \widehat{h'}_n variance (left hand side term) is driven by interactions between \widehat{h}_n anomalies and anomalies in normalised net longwave heating, shortwave heating, surface fluxes and advection.

We use the variance of \widehat{h}_n as our aggregation metric. Hovmöller plots of \widehat{h}_n are shown in Figure 1 for each of our SSTs. In these plots, \widehat{h}_n is averaged along the short axis of our domains. The plots show how initially randomly-distributed convection organises into bands which expand until the point where there are 4 to 5 quasi-stationary bands of moist convective regions separated by dry subsiding regions. This demonstrates that once our domains become fully-aggregated, the degree of aggregation appears similar. Figure 2a shows time series of each of the variance of \widehat{h}_n, and shows that the variance of non-normalised \widehat{h}_n is ~4 times greater for our 305 K simulations compared to our 295 K simulation. Figure 2b shows time series of the variance of \widehat{h}_n. From this, we can see the convection aggregates faster as SST increases, yet the degree of aggregation remains similar via this metric once the convection is fully aggregated. Values of \widehat{h}_n variance around 10-4 or lower correspond to randomly scattered convection, whereas values greater that 10-3 are associated with strongly aggregated convection.

Figure 3: Maps of (a) cloud condensed water path, (b) vertically-integrated FMSE anomaly, (c) longwave heating anomaly, (d) shortwave heating anomaly. Snapshots at day 100 of the 300 K simulation.

To understand the processes contributing to aggregation, we have to look to Equation 1. We mainly focus on the two radiative terms on the right hand side. The terms show that regions in which the radiative anomalies and the \widehat{h}_n anomalies have the same sign contribute to aggregation. We can start to get an intuitive understanding of this concept by looking at maps of these variables. Figure 3b-d show maps of \widehat{h'}_n, LW' and SW'. We can see SW' and \widehat{h'} are closely correlated since SW' is mainly determined by the shortwave absorption by water vapour. Clouds have little effect on the shortwave heating rates, with ~90% of the shortwave heating rate in cloudy regions being due to absorption by water vapour. LW' is closely linked to cloud condensed water path (Figure 3a). This is because the majority of our clouds are high-topped clouds which, due to their cold cloud tops, are able to prevent longwave radiation escaping to space, so they are associated with positive longwave heating anomalies.

The sensitivity of the budget terms to both aggregation and SST can be seen in Figure 4. This figure is made by creating 50 bins of \widehat{h}_n variance and then averaging the budget terms in space and time for each bin and for each SST. Where the terms are positive, they are helping to increase aggregation. Where they are negative, the terms are opposing aggregation. The terms tend to increase in magnitude since every term has \widehat{h'}_n as a factor, which increases with aggregation by definition.

Figure 4: Terms in Equation 1 vs normalised FMSE variance for each SST

In general, we find the longwave term is the dominant driver of aggregation, being insensitive to SST during the growth phase of aggregation. Once the aggregation is mature, the longwave term remains the dominant maintainer of aggregation, however its contribution to aggregation maintenance decreases with SST. The shortwave term is initially small at early times but becomes a key maintainer of aggregation within highly-aggregated environments. This is because humidity variations are initially small, so there is little variation in shortwave heating. Once the convection is aggregated, moist regions are very moist and dry regions are very dry, so there is a large difference in shortwave heating between moist and dry regions. The variations in shortwave heating remain very similar with SST, meaning shortwave heating anomalies contribute the same amount to non-normalised \widehat{h} variance. Therefore, shortwave heating contributes less to aggregation at higher SSTs because they contribute to a smaller fraction of \widehat{h} anomalies. The radiative terms are balanced by the surface flux term (negative because there is greater evaporation in dry regions) and the advection term (negative because circulations tend to smooth out \widehat{h'}_n gradients). The decrease in the magnitude of the radiative terms with SST is balanced by the surface flux and advection terms becoming more positive with SST.

To understand the behaviour of the longwave term, we define different cloud types based on the vertical profile of cloud, assigning one cloud type per grid box in a similar way to Hill et al. (2018). We define a lower and upper level pressure threshold, assigning cloud below the lower threshold to a “Low” category, cloud above the upper threshold to a “High” category, and cloud in between to a “Mid” category. If cloud occurs in more than one of these layers, then it is assigned to a combined category. In total, there are eight cloud types: Clear, Low, Mid, Mid & Low, High, High & Low, High & Mid, and Deep. We can then find each cloud type’s contribution to the longwave term by multiplying the cloud’s mean [Equation] covariance by its domain fraction.

To see how the cloud type contributions change with aggregation, we define a Growth phase and Mature phase of aggregation. The Growth phase has \widehat{h}_n variance between 3\times10^{-4} and 4\times10^{-4} and the Mature phase has \widehat{h} variance between 1.5\times10^{-3} and 2\times 10^{-3}. The contribution of longwave interactions with each cloud type to aggregation during these two phases is shown in Figure 5a, with their mean LW'\times\widehat{h'} covariance and fraction shown in Figures 5b & c.

Figure 5: Mean (a) contribution to the longwave term in Equation 1, (b) normalised longwave-FMSE covariance, (c) cloud fraction for the Growth phase (dots) and Mature phase (open circles). Data points for each category are in order of SST increasing to the right.

We find that longwave interactions with high-topped clouds and clear regions drive aggregation during the Growth phase (Figure 5a). This is because high clouds are abundant, have positive longwave heating anomalies and occur in moist, high \widehat{h} environments. The clear regions are the most abundant category, have typically negative longwave heating anomalies and tend to occur in low \widehat{h} regions, so their LW'\times\widehat{h'} covariance is positive. During the Growth phase, there is little SST sensitivity within each category. During the Mature phase, longwave interactions with high-topped cloud remain the main maintainer of aggregation however their contribution decreases with SST. This sensitivity is mainly because there is a greater decrease in high-topped cloud fraction with aggregation as SST increases. This also has consequences for the LW'\times\widehat{h'} covariance of the clear regions. As high-topped cloud fraction reduces, the domain-mean longwave cooling increases. This makes the radiative cooling of the clear regions less anomalous, resulting in an increasingly negative LW'\times\widehat{h'} covariance during the Mature phase as SST increases.

There is great variability in the degrees of aggregation within numerical models, which has important consequences for weather and climate modelling (Wing et al. 2020). With cloud-radiation interactions being crucial for aggregation, understanding how these interactions vary between models may help to explain the differences in aggregation. This study provides a framework by which a comparison of cloud-radiation interactions and their contributions to convective self-aggregation between models and SSTs can be achieved.

Page Break 


Bao, J., & Sherwood, S. C. (2019). The role of convective self-aggregation in extreme instantaneous versus daily precipitation. Journal of Advances in Modeling Earth Systems11(1), 19– 33. 

Bretherton, C. S., Blossey, P. N., & Khairoutdinov, M. (2005). An energy-balance analysis of deep convective self-aggregation above uniform SST. Journal of the Atmospheric Sciences62(12), 4273– 4292. 

Hill, P. G., Allan, R. P., Chiu, J. C., Bodas-Salcedo, A., & Knippertz, P. (2018). Quantifying the contribution of different cloud types to the radiation budget in Southern West Africa. Journal of Climate31(13), 5273– 5291. 

Holloway, C. E., Wing, A. A., Bony, S., Muller, C., Masunaga, H., L’Ecuyer, T. S., & Zuidema, P. (2017). Observing convective aggregation. Surveys in Geophysics38(6), 1199– 1236. 

Muller, C., & Bony, S. (2015). What favors convective aggregation and why? Geophysical Research Letters42(13), 5626– 5634. 

Pope, K. N., Holloway, C. E., Jones, T. R., & Stein, T. H. M. (2021). Cloud-radiation interactions and their contributions to convective self-aggregation. Journal of Advances in Modeling Earth Systems13, e2021MS002535. 

Wing, A. A., & Cronin, T. W. (2016). Self-aggregation of convection in long channel geometry. Quarterly Journal of the Royal Meteorological Society142(694), 1– 15. 

Wing, A. A., & Emanuel, K. A. (2014). Physical mechanisms controlling self-aggregation of convection in idealized numerical modeling simulations. Journal of Advances in Modeling Earth Systems6(1), 59– 74. 

Wing, A. A., Stauffer, C. L., Becker, T., Reed, K. A., Ahn, M.-S., Arnold, N., & Silvers, L. (2020). Clouds and convective self-aggregation in a multi-model ensemble of radiative-convective equilibrium simulations. Journal of Advances in Modeling Earth Systems12(9), e2020MS0021380. 

2021 Academic Visiting Scientist – Tim Woolings 

Isabel Smith –

Every year, the Met PhD students at the University of Reading invite a scientist from a different university to learn from and talk to about their own project. This year we had the renowned Professor Tim Woolings, who currently researches and teaches at the University of Oxford. Tim’s interests generally revolve around large scale atmospheric dynamics and understanding the impacts of climate change on such features. We, as Met PhD students, were very excited and extremely thankful that Tim donated a week of his time (4th-8th of October) and travelled from Oxford for hybrid events within the Met. building. Tim told us of his own excitement to be back visiting Reading, after completing his PhD here, on isentropic modelling of the atmosphere, and staying on as a researcher and part of the department until 2013.  

The week started with Tim presenting “Jet Stream Trends” at the Dynamical Research Group, known as Hoskin’s Half Hour. A large number of PhD students, post-doctorates and supervisors attended, which was to be expected considering Tim has a book dedicated on Jet streams. After a quick turnaround, he spoke at the departmental lunch time seminar on “The role of Rossby waves in polar weather and climate”. Here, Tim did an initial review on Rossby wave theory and then talked about his current fascinating research on the relevance of them within the polar atmosphere. The rest of Tim’s Monday consisted of lunch at park house with Robert Lee and the organising committee, Charlie Suitters, Hannah Croad and Isabel Smith (within picture). Later that evening Tim visited the Three Tuns pub with other staff members, for an important staff meeting! The PhD networking social with Tim on Thursday was a great evening where 15 to20 students were able to discuss Tim’s research in a less formal setting within Park House pub.  

Tim Woolings (2nd left) and the visiting scientist organising committee

Tim’s Tuesday, Wednesday (morning) and Thursday consisted of virtual and in-person one on one 15-minute meetings with PhD students. Here students explained their research projects and Tim gave them a refreshing outsider perceptive. On Wednesday afternoon, after Tim attended the High-Resolution Climate Modelling research group, he talked about his career in PhD group (A research group for PhD students only, where PhD students present to each other.). Tim explained how his PhD did not work as well as he had initially hoped, and the entire room felt a great weight of relief. His advice on keeping calm and looking for the bigger picture was heard by us all.  

On Friday the 8th, a mini conference was put on and six students got to the “virtual” and literal stage and presented their current findings. Topics ranged from changes to Arctic cyclones, blocking, radar and Atmospheric dust. The conference and the week itself were both great successes, with PhD students leaving with inspiring questions to help aid their current studies. All at the University of Reading Department of Meteorology were extremely grateful and we thoroughly enjoyed having Tim here. We wish him all the best in his future endeavours and hope he comes back soon! 

COP Climate Action Studio 2021 and a visit to the Green Zone, Glasgow  

Helen Hooker 


SCENARIO DTP and the Walker Academy offered PhD students the opportunity to take part in the annual COP Climate Action Studio (COPCAS) 2021. COPCAS began with workshops on the background of COP, communication and interviewing skills and an understanding of the COP26 themes and the (massive!) schedule. James Fallon and Kerry Smith were ‘on the ground’ in the Blue Zone, Glasgow in week 1 of COP26, followed by Gwyn Matthews and Jo Herschan during week 2. Interviews were arranged between COP26 observers, and COPCAS participants back in Reading who were following COP26 events in small groups through livestream. Students summarised the varied and interesting findings by writing blog posts and engaging with social media.

Figure 1: COPCAS in action.   

Motivation, training and week 1 

Personally, I wanted to learn more about the COP process and to understand climate policy implementation and action (or lack thereof). I was also interested to learn more about anticipatory action and forecast based financing, which relate to my research. After spending 18 months working remotely in my kitchen, I wanted to meet other students and improve formulating and asking questions! I found the initial training reassuring in many ways, especially finding out that so many people have dedicated themselves to drive change and find solutions. During the first week of COP26 we heard about so many positive efforts to combat the climate crisis from personal actions to community schemes, and even country wide ambitious projects such as reforestation in Costa Rica. A momentum seemed to be building with pledges to stop deforestation and to reduce methane emissions.

Green Zone visit 

Figure 2: Green Zone visit included a weekend full of exhibitors, talks, films and panel discussions plus a giant inflatable extracting COvia bouncing!

During the middle weekend of COP26, some of us visited the Green Zone in Glasgow. This was a mini version of the Blue Zone open to the public and offered a wide variety of talks and panel discussions. Stand out moments for me: a photograph of indigenous children wearing bamboo raincoats, measuring the length of Judy Dench’s tree, the emotive youth speakers from Act4Food Act4Change and the climate research documentary Arctic Drift where hundreds of scientists onboard a ship carried out research whilst locked into the polar winter ice-flow.  


During COPCAS I wrote blogs about: a Green Zone event from Space4climate, an interview by Kerry Smith with SEAChange (a community-based project in Aberdeenshire aiming to decarbonise old stone buildings) and Sports for climate action. I also carried out an interview arranged by Jo with WWF on a food systems approach to tackling climate change.

Ultimately though, the elephant in the large COP26 Blue Zone room had been there all along…

Interview with Anne Olhoff, Emissions Gap Report (EGR) 2021 Chief scientific editor and Head of Strategy, Climate Planning and Policy, UNEP DTU Partnership.

Figure 3: Source: UNEP Emissions Gap Report 2021 updated midway through week two of COP26 accounting for new pledges. 

Time is running out, midway through the second week of COP26, the United Nations Environmental Partnership (UNEP) presented its assessment on the change to global temperature projections based on the updated pledges so far agreed in Glasgow.  

Pledges made prior to COP26 via Nationally Determined Contributions (NDCs) put the world on track to reach a temperature increase of 2.7C by the end of the century. To keep the Paris Agreement of keeping warming below 1.5C this century, global greenhouse gas emissions must be reduced by 55% in the next eight years. At this point in COP26, updated pledges now account for just an 8% reduction – this is 7 times too small to keep to 1.5C and 4 times too small to keep to 2C. Updated projections based on COP26 so far now estimate a temperature rise of 2.4C by 2100. Net-zero pledges could reduce this by a further 0.5C, however plans are sketchy and not included in NDCs. So far just five of the G20 countries are on a pathway to net-zero.

Anne’s response regarding policy implementation in law: 

“Countries pledge targets for example for 2030 under the UN framework for climate change and there’s no international law to enforce them, at least not yet. Some countries have put net-zero policies into law, which has a much bigger impact as the government can be held accountable for the implementation of their pledges.” 

Following my own shock at the size of the emissions gap, I asked Anne if she feels there has been any positive changes in recent years: 

“I do think we have seen a lot of change, actually…the thing is, things are not moving as fast as they should. We have seen change in terms of the commitment of countries and the policy development and development in new technology needed to achieve the goals, these are all positive developments and here now, changing the whole narrative, just 2 years ago no one would have thought we’d have 70 countries setting net-zero emission targets…we are also seeing greater divergence between countries, between those making the effort to assist the green transition such as the UK, EU and others, and those further behind the curve such as China, Brazil and India. It’s important to help these countries transition very soon, peaking emissions and rapidly declining after that.”   

I asked Anne how countries on track can support others: 

“A lot of the great things here (at COP) is to strengthen that international collaboration and sharing of experiences, it’s an important function of the COP meeting, but we need to have the political will and leadership in the countries to drive this forward.” 


The momentum that was apparent during the first week of COP26 seemed to have stalled with this update. Despite the monumental effort of so many scientists, NGOs, individuals and those seeking solutions from every conceivable angle, the pledges made on fossil fuel reduction are still so far from what is needed. And at the final hour (plus a day), the ambition to ‘phaseout’ burning coal was changed to ‘phasedown’ and the financial contributions from developed nations pledged to cover loss and damage to countries not responsible for, but impacted now by climate change, have not been realised. I think this is the first time I have really felt the true meaning of ‘climate justice’. Perhaps we do need a planet law, as it seems our political leaders, do not have the will.

Overall, the COPCAS experience has been enjoyable, slightly overwhelming and emotional! It has been great to work together and to share the experiences of those in the Blue zone. It was also an amazing learning experience; I think I have barely touched the surface of the entire COP process and I would still like to understand more.

Climate Science and Power 

Gabriel M P Perez – 


Climate science, especially climate-change science, is increasingly becoming a source of power in society and integrating politics. As an academic in meteorology, I started realising how possibly other scientists and I rarely think about how our profession fits in the power networks that constitute politics; on the contrary, it seems that we often think about our scientific outputs as something detached from the wheels of history.  

In this essay, I paint a picture of how climate science relates to the main sources of power in the civic sphere by building upon some of my recent readings in history of ideas and philosophy. I also discuss a few past and recent instances where alleged “apolitical” scientific discourse was moulded to support politics of domination and exclusion. By better understanding the relationships of power surrounding our science, we can be more confident that our scientific outputs will contribute more positively to society at large.  

The participation of climate-change science in politics is not exactly new: it has existed for at least three or four decades. However, up until the early 2010s, the hypothesis of anthropogenic global warming still faced a few challenges in the scientific realm. Perhaps the last of these challenges was the alleged 1998-2014 warming hiatus – climate scientists had to answer to the public and come to an agreement as to why the increase in global temperatures appeared to halt. Now, in the second decade of the 21st century, anthropogenic warming is a consensus and the most relevant contenders of climate science are found in the political realm. 

Historical background

In the seminal text “A discourse on the method of correctly conducting one’s reason and seeking truth in sciences”, Descartes proposes a method of pure reason to conduct scientific research. He proposes that the inquisitive individual should start by forgetting everything he learned and start deriving basic truths from simple logical statements and build up from that to provide scientific answers to more complex questions using “pure reason”. This text was one of the starting points of a scientific revolution and helped build the bases of modern science. Although epistemology quickly moved on from the Cartesian thought, it still affects the way we do science. After years in academia, trained scientists grow to believe that their scientific outputs are disconnected from the other spheres of society and the networks of power. This “apolitical” mindset will then affect, for example, our ideas, hypotheses and communications regarding climate change.  

The historian of ideas Michel Foucault in his book “The Order of Things”, deconstructs the idea that the scientific discourse is independent of the surrounding socio-economic environment. He argues that the scientific discourse is inherently tied to the “lenses” by which scientists of a certain time are capable of analysing the physical world. Foucault calls these lenses “epistemes”. The epistemes are the ways of thinking in each stage of history that define what is acceptable scientific discourse. Let us take Descartes’ Discourse as an example of that: the author lived in a highly religious time, and, although in Parts 1 to 3 of the Discourse he describes his method of “pure reason”, in Part 4 he employs his method to argue for the existence of God: this would not be acceptable scientific discourse in the 21st century. Therefore, even the brightest minds are subject to having their scientific discourse shaped by the epistemes of their time. 

For some scientists, accepting that our science is shaped by factors outside of the realm of pure reason may be uncomfortable. However, embracing our episteme and the historical forces that drive scientific paradigm shifts may aid us in producing and communicating science in ways that are more likely to impact society positively; this could also help prevent distortions and misuses of the power stemming from our science.

For example, the scientific consensus has been distorted in the past to provide an intellectual background to the darkest side of environmentalism: “ecofascism”, a political model that, in the early 20th century, used environmentalism to justify white supremacy and genocide of indigenous peoples (see the New Yorker article “Environmentalism’s Racist History” by Jedediah Purdy). Sadly, such distortions of environmental sciences are not buried in the past, on the opposite, they are gaining popularity in certain extremist groups (Lawton, 2019; Taylor, 2019) and even influencing today’s politics: the Portuguese ecofascist party was an important early supporter of the current Brazilian president Jair Bolsonaro, whose policies are ironically accelerating the deforestation of the Amazon rainforest (Pereira, 2020). In United States politics, we have recently seen in the media the eco-fascist “shaman” invading the White House after Donal Trump’s defeat. 

The power relations of climate science 

Power can be defined as the ability to have others do as you would. Evoking Foucault one more time, there are two kinds of power: the repressive and normalising power. Repressive power is a second-rate type of power that requires the use of force to control the actions of others.  Normalising power, on the other hand, is silent, non-aggressive, and much more effective than repressive power. Normalising power controls what other people want. If you have normalising power over others, they will do as you would because you have succeeded in making them want the same as you. As climate researchers, our scientific output is a growing source of normalising power. More and more people and governments want to do what climate science says is better for life on Earth. Therefore, “power” hereafter refers to “normalising power”. 

Power is present in all spheres of human relations (e.g., family, workplace and institutions). Here we will discuss power in the civic sphere, i.e., the power of having groups of people or societies do as you would. The civics educator Eric Liu suggests that power emanates from six sources. Here, I list four of these sources that I deem most relevant to climate science and discuss some ways that they relate to it: 

  1. Ideas Ideas, hypotheses and theories about the physics, impacts, mitigation and adaptation of climate change emanate almost exclusively from academia.  This directly places climate scientists from top institutions as raw sources of power that shape how people and governments think, behave and act towards climate change.  Combining David Hume’s proposition that ideas come from the impressions one has had throughout their lives and Foucault’s theory of epistemes, we may come to the conclusion that this source of power (i.e., scientific ideas) might not be as purely rational as one might have hoped. 
  2. Wealth Since ideas stem from academia, it is important to remember that most top institutions are in the wealthy nations of the Global North. Moreover, most scientists in these institutions were born and raised in the same wealthy nations. Naturally, the bulk of scientific outputs, both in terms of results and communications, are tied to the episteme, or “ways of thinking”, of this particular set of scientists.    Wealth is also related to science through the sources of research funding. Decisions regarding the allocation of research funds are often made by boards composed by either: 
  • Scientists in wealthy countries or 
  • Influential individuals outside academia 

A controversial example of B is the influence that Bill and Melinda Gates, through their foundation, exert over the World Health Organisation, having a disproportionate influence on scientific and public health decisions (Wadman, 2007). The issue is that Bill and Melinda’s suggestions are often not aligned with the public’s best interest or the scientific consensus, but rather with the personal motivations of these individuals. The power of wealth in climate-related negotiations is further evidenced when we notice that ideas such as climate debt (Warlenius, 2018) are typically ignored by current and former imperialist nations. These ideas were advocated by Global South agents in the widely ignored “World People’s Conference on Climate Change and the Rights of Mother Earth” held in Bolivia in 2010. 

  1. Numbers Climate activists, when numerous enough, have the power to pressure or convince governments and individuals to act according their beliefs. These beliefs are largely based on climate-change scientific literature. Scientists sometimes also take a more direct approach and practise environmental activism of some sort. 
  2. State action Governments are themselves a source of civic power but also subject to the other sources of power (i.e., ideas, wealth and numbers). Democratic states, as representatives of the people, have the power to directly and indirectly influence climate change by reducing (or increasing) emissions, funding climate research, educating the future generations, and many others. The governmental action, in its turn, is constrained by law in states under “Rechtsstaat” (or “the rule of law”). This raises the question: are lawmakers, prosecutors, judges and other agents well equipped to make decisions around climate change? In the next decades, it is not hard to imagine climate scientists being consulted regarding climate-change litigation in national or international courts. A few weeks ago, for example, the Brazilian president Jair Bolsonaro was accused of crimes against humanity at the International Criminal Court; his policies were said to be “directly connected to the negative impacts of climate change around the world”. 


In this essay, I have outlined and attempted to disentangle a few existing and emerging power relations around climate change. I argue that as climate scientists we are sources of power in society. Therefore, we should be aware of our own “ways of thinking”, or “epistemes”, and remember that these are driven by external factors. Those external factors have the ability to shape our ideas, hypotheses and communications regarding climate change. Being aware of our role in the complex network of power known as politics could maximise the positive impact of the power stemming from our scientific outputs. Hopefully, this awareness could help prevent this power from being misdirected to support politics of domination and exclusion. Moreover, as the impacts of climate change are increasingly damaging to life on Earth, it is likely that in the next decade’s climate scientists involve themselves with litigation in national and international courts of justice. It is, therefore, timely for us to be aware of our roles in all levels of politics. 

References and further reading

Descartes, Rene. A discourse on the method of correctly conducting one’s reason and seeking truth in science. 1637

Foucault, Michel. The order of things. 1966.

Lawton, Graham. “The rise of real eco-fascism.” New Scientist 243.3243 (2019): 24.

Pereira, Eder Johnson de Area Leão, et al. “Brazilian policy and agribusiness damage the Amazon rainforest.” Land Use Policy 92 (2020): 104491.

Purdy, Jedediah. Environmentalism’s racist history. The New Yorker. 2015

Taylor, Blair. “Alt-right ecology: Ecofascism and far-right environmentalism in the United States.” The Far Right and the Environment. Routledge, 2019. 275-292.

Wadman, Meredith. “Biomedical philanthropy: state of the donation.” Nature 447.7142 (2007): 248-251.

Warlenius, Rikard. “Decolonizing the atmosphere: The climate justice movement on climate debt.” The Journal of Environment & Development 27.2 (2018): 131-155.

Eric Liu Ted Talk about civic power:

List of resources about climate debt:

History of ecofascism:

NCAS Climate Modelling Summer School

Shammi Akhter –

The Virtual Climate Modelling Summer School covers the fundamental principles of climate modelling. The school is run for 2 weeks in the September of each year by the leading researchers from the National Centre for Atmospheric Science (NCAS) and from the Department of Meteorology at the University of Reading. I attended the school mainly because I have recently started using climate models in the second aspect of my research work and also because one of my supervisors recommended this to me.

What happened during the first week?

In the first week, lecturers introduced us to numerical methods used in climate models and we had a practical assignment implementing a chosen numerical method of our own in Python. We mostly worked individually on our projects that week. There were also lectures on convection parameterisation and statistical analysis for climate models.

What happened during the second week?

Figure 1: Earth energy budget comparison diagram between control (red) and flat earth (green) experiments produced by me in week 2.

In week two, with the assistance of NCAS and university scientists, we analysed climate model outputs. I personally was involved in the Flat Earth experiment- in which we tested the effect of changing surface elevation for terrain such as mountains, high plateaus on the climate. In this experiment, the perturbation is imposed by reducing the elevation of mountains to sea level. There were eight people in our team. As you may know, we PhD students have the occasional opportunity to do research collaboratively with other students in Reading Meteorology and encourage our teammates. For this reason, it felt very nice to me to work as the part of a research group. I was amazed by how we had been able to produce a small good piece of scientific work just within a matter of days due to our team effort. In Figure 1, I have presented a small part of our work which is the global energy budget comparison between a control experiment and the flat earth experiment (where the elevation of the mountains has been reduced to sea level). Along with our practical, we also attended some lectures on the ocean dynamics and physics, water in the climate system and land-atmosphere coupling and surface energy balance during this week.

How was it like to socialize with people virtually?

We used the during the lunchtime and after work to socialize. I was a bit surprised though that I was the only student joining the and as a result I always had to hang out (virtually) with NCAS and university scientists all the time. I rather consider it a blessing for me as there was no competition to introduce myself to the professionals. I even received a kind offer from one of our professors to assist him as a teaching assistant in his course in the department.

Concluding Remarks

I learnt about some of the basic concepts of climate modelling and I hope to use these things in my research someday. It was also very refreshing to talk to and work with other students as well as the scientists. While working in a group in week 2, I once again realized there are so many things we can accomplish if we work together and encourage each other.