Events and Seminars 2016/2017

School seminars

All seminars will take place from 13:00 to 14.00 in the Williamson Building G.03 lecture theatre.  These seminars are open to all and are a good opportunity to meet your fellow students and staff. 

For details of previous seminars please see our seminar archive.


Wednesday 1 February 2017 - Jos Barlow (Lancaster University)

Title: Revealing the impact of disturbance on tropical forest biota

Abstract: Tropical forests hold much of the world's terrestrial biodiversity yet are threatened by deforestation and forest disturbance. While the impacts of deforestation are well known and widely reported, we have a much poorer understanding of the more cryptic loss of biodiversity caused by to disturbances such as selective logging, fires, hunting and fragmentation. I outline their impacts using a large data set of plants, birds and dung beetles sampled in 36 catchments in the Brazilian state of Pará. Catchments retaining more than 69–80% forest cover lost more conservation value from disturbance than from forest loss. For example, a 20% loss of primary forest, the maximum level of deforestation allowed on Amazonian properties under Brazil’s Forest Code5, resulted in a 39–54% loss of conservation value. Species that were most affected by disturbance had the highest conservation or functional value. These results demonstrate why disturbance needs to be addressed by policy and management.

Wednesday 8 February 2017 - Sigurjon Jonsson (King Abdullah University of Science and Technology, Saudi Arabia)

Title: Rifting in Iceland and in the Red Sea observed using satellite geodesy

Abstract: Extension at divergent plate boundaries is episodic and occurs during rifting events. As most divergent plate boundaries are located on the sea floor, rifting events are challenging to study and near-field data of past events are limited. In this talk, I will present our results of studying recent rifting events in the Red Sea region and in Iceland that provide a rare glimpse of this type of activity. Three volcanic eruptions occurred in the southern Red Sea during the past several years, on Jebel at Tair Island (2007-8) and within the Zubair archipelago (2011-12 and 2013). On Jebel at Tair we find evidence for temporarily varying stress field orientations within the island’s volcanic edifice that appear isolated from the regional Red Sea stress field. The two eruptions in the Zubair archipelago resulted in the formation of two new islands and were fed by dike intrusions much larger than the small size of the new islands might suggest. Together these eruptions and several seismic swarms indicate that the southern Red Sea has been experiencing an episode of rifting with multiple diking events and meter-scale extension and shows that this plate boundary is more active than previously thought. The 2014-15 Bárðarbunga rifting event in central Iceland originated from the Bárðarbunga central volcano located under the Vatnajökull ice cap. Magma propagated over 40 km to the northeast from the caldera and well beyond the periphery of the glacier where the intrusion eventually made it to the surface and produced a large lava field. We used high-resolution satellite radar images to map the near-field deformation within and around a reactivated graben between the glacier’s edge and the eruption site. We find that the meter-scale opening across the graben was accompanied with a significant amount of left-lateral shear motion. The left-lateral shear is in accordance with the mis-alignment of the rift segment to the overall plate motion in the region and implies that pre-existing fracture zones play a key role in controlling dike emplacements in rifts.


Wednesday 15 February 2017 - Alexandre Anesio (Bristol)

Title: How microorganisms melt glaciers

Abstract: It is now recognised that large expanses of ice in the polar regions are inhabited by active microbial communities forming one of the biomes of Earth. Microbes on ice are diverse, play an important role in the cycling of nutrients and can even modify the physical environment they live. For instance, microbial processes at the surface of glaciers and ice sheets can lead to the accumulation of labile dissolved and particulate organic carbon and this in turn have consequences to ice wastage and the delivery of nutrients to adjacent ecosystems.  Liquid water also occurs at the beds of temperate and polythermal glaciers, as well as large sectors of polar ice sheets. In contrast with glacial surface environments, subglacial habitats have higher rock:water ratios, higher contact times between the bedrock and water, and a lack of light and redox potential that tend towards anoxic conditions, particularly during periods with long hydraulic residence times. Iron and sulphur reduction and oxidation, and production of methane are a few examples of processes in subglacial habitats that are important at local and potentially global scales. 

Wednesday 22 February 2017 - John Plane (Leeds)

Title: Cosmic Dust and the Earth’s Atmosphere

Abstract: Cosmic dust particles are produced in the solar system from the sublimation of comets as they orbit close to the sun, and also from collisions between asteroids in the belt between Mars and Jupiter. Dust particles enter the atmosphere at hyperthermal velocities (11 – 72 km s-1), and ablate at heights between 80 and 120 km in the mesosphere/lower thermosphere (MLT). The resulting metallic vapours (Fe, Mg, Si and Na etc.) then oxidize and recondense to form nm-size particles, termed “meteoric smoke particles (MSPs)”. MSPs are too small to sediment downwards and so are transported by the general circulation of the atmosphere, taking roughly 4 years to reach the surface. Smoke particles play a potentially important role as condensation nuclei of noctilucent ice clouds in the mesosphere, and polar stratospheric clouds in the lower stratosphere, where they also facilitate freezing of the clouds. There are also potential implications for climate, as the input of bio-available cosmic Fe in the Southern Ocean can increase biological productivity and stimulate CO2 drawdown from the atmosphere. However, current estimates of the magnitude of the cosmic dust mass input rate into the Earth’s atmosphere range from 2 to over 200 tonnes per day, depending on whether the measurements are made in space, in the middle atmosphere, or in polar ice cores. This nearly 2 order-of-magnitude discrepancy indicates that there must be serious flaws in the interpretation of observations that have been used to make the estimates. Furthermore, given this degree of uncertainty, the significance of these potential atmospheric impacts remains speculative. 
In this seminar I will describe the results of a large study designed to determine the size of the cosmic dust input rate using a self-consistent treatment of cosmic dust from the outer solar system to the Earth’s surface. An astronomical model which tracks the evolution of dust from various sources into the inner solar system was combined with a chemical ablation model to determine the rate of injection of metallic vapours into the atmosphere. Constraining these coupled models with lidar measurements of the vertical fluxes of Na and Fe in the MLT, and the rate of accretion of cosmic spherules at the South Pole, indicates that about 40 tonnes of dust enters the atmosphere each day, of which ~18% ablates. The subsequent atmospheric chemistry of the ablated metallic vapours is then examined using the Whole Atmosphere Community Climate Model (WACCM), coupled with the aerosol microphysics model CARMA to treat the interplay of meteoric smoke particles with the stratospheric sulphate layer. While the optical extinction of meteoric smoke in the lower mesosphere, and of refractory material in polar stratospheric clouds is satisfactorily modelled, two problems remain. First, the injection rate of Na and Fe atoms is too large (by a factor between 5 and 10) for WACCM to replicate the observed metal atom layer densities in the MLT. It appears that vertical transport by eddy diffusion has to be significantly supplemented by chemical transport produced by unresolved (sub-grid) gravity waves (this process will significantly affect the transport of other species such as atomic O through the MLT). The second problem is that the rate of deposition of MSPs at polar latitudes is substantially underestimated by the model, indicating that there may be an efficient process for removing particles directly from the lower stratospheric winter polar vortex to the surface.
Underpinning the model development are three novel experimental systems developed at Leeds:  a Meteor Ablation Simulator, which measures the evaporation of metals from cosmic dust particles that are flash heated to over 2800 K; a Time-of-Flight mass spectrometer with laser photo-ionization which is used to study the reactions of neutral metallic compounds in the gas phase; and a flowing afterglow experiment to study the dissociative recombination of metallic ions with electrons.

Wednesday 1 March 2017 - Andrew Cundy (Southampton)

Title: From nano to macro: developing scalable remediation methods for problem sites and contaminants"

Abstract: The effective management of contaminated soil and waters is a major issue globally, with significant areas of land and volumes of waste and water contaminated by inorganic, organic and radioactive substances at levels that may pose a risk to human health and the wider environment. This presentation explores recent work aimed at developing scalable and practical remediation and management methods for problem sites and contaminants (including radionuclides), involving nano-based geochemical methods and large area “green” remediation strategies.

Wednesday 8 March 2017 - speaker to be confirmed

Wednesday 15 March 2017 - Linda Kirstein (Edinburgh)

Title: Boron Isotopes

Wednesday 22 March 2017 - Tom Lachlan Cope (BAS)

Wednesday 29 March 2017 - Andreas Petzold (Jülich)

Wednesday 3 May 2017 - Gerald Roberts (Birkbeck)

Title: Earthquake histories through the Holocene from 36Cl cosmogenic exposure dating and structural geology, central Italy

Abstract: The talk will present observations of the recent Mw 6.1-6.6 earthquakes in central Italy and show how these relate to the pattern of active faults in the region and their Holocene slip-rates. 36Cl cosmogenic exposure dating of fault planes will be presented to show that earthquakes are clustered in time with periods of many thousands of years with no earthquakes interspersed with periods of the same duration containing several earthquakes. The observations and 36Cl results will be used to form an overview of how fault systems evolve and how seismic hazard ought to be conveyed to at risk populations.

Wednesday 10 May 2017 - Laura Wilcox (University of Reading)

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