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Seminars

How Much Does Sea Ice Affect Arctic Precipitation?

Professor Xiahong Feng

Dartmouth College

Global climate is influenced by the Arctic hydrologic cycle, which is, in part, regulated by sea ice through its control on evaporation and precipitation. However, the quantitative link between precipitation and sea ice extent is poorly constrained. This talk presents observational evidence for the response of precipitation to sea ice reduction and assesses the sensitivity of the response. Changes in the proportion of moisture sourced from the Arctic with sea ice change in the Canadian Arctic and Greenland Sea regions over the past two decades are inferred from annually averaged deuterium excess (d-excess) measurements from six sites. Other influences on the Arctic hydrologic cycle, such as the strength of meridional transport, are assessed using the North Atlantic Oscillation index. We find that the independent, direct effect of sea ice on the increase of the percentage of Arctic sourced moisture (or Arctic moisture proportion, AMP) is 18.2 ± 4.6% and 10.8 ± 3.6%/100,000 km2 sea ice lost for each region, respectively, corresponding to increases of 10.9 ± 2.8% and 2.7 ± 1.1%/1 °C of warming in the vapor source regions. The moisture source changes likely result in increases of precipitation and changes in energy balance, creating significant uncertainty for climate predictions.

Wednesday 8 May 2024, 12.00pm
Room 314, Science III Building
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Seminars

Concepts of quantum machine learning

Associate Professor Christopher Gies

Institut für Theoretische Physik, Universitat Bremen

The seminar will give a glimpse into the vibrant field of quantum machine learning (QML)— its underlying quantum- mechanical principles, hardware implementations, and potential advantages over classical systems. QML has gained substantial interest as a quantum technology application capable of taking advantage of the noisy intermediate scale quantum (NISQ) devices of the current era, i.e. systems operating with tens to hundreds of imperfect qubits.

A particular focus will be on reservoir computing, which utilizes physical systems as artificial (quantum) neural networks to process information. Like in conventional machine learning, an input u(t) undergoes processing within the network to yield an output y(t). Only by training the output weights W, even small quantum systems can approximate non-linear functions of the input data due to the exponentially large Hilbert space dimension.

WEDNESDAY 1 May, 12:00PM, Room 314, Science III Building, University of Otago
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Media Events News Seminars

Waves in a Plasma Ocean: Wave-Particle Interactions Throughout the Solar System

Associate Professor Allison Jaynes

University of Iowa

All planetary and smaller bodies in our solar system are embedded in a sea of plasma, like boulders in a terrestrial ocean. Their surfaces or magnetic fields run into this ocean of space plasma, generated primarily by our Sun, and create a whole range of fascinating effects as a result.

The American Physical Society’s Katherine E. Weimer Award winner talks about the plasma ocean of our solar system, from aurora and “killer electrons” to the furthest reaches of space exploration.

This talk will be accessible to all backgrounds, knowledge of Physics not required.

WEDNESDAY 17 April, 5:00PM, Archway 3, University of Otago

 

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News

Unveiling the secrets of the aurora and other dark-sky emissions

Dr Maxime Grandin

Academy of Finland Postdoctoral Researcher
Finnish Centre of Excellence in Research of Sustainable Space (FORESAIL) Department of Physics
University of Helsinki
Finland

A fascinating natural phenomenon, auroral displays are the result of the interaction between charged particles precipitating from space and the upper atmospheric constituents. Characterising the fluxes of precipitating particles and understanding the mechanisms behind optical emissions still proves challenging and is an active field of research in space physics. After briefly introducing the chain of processes starting at the Sun and leading to auroral emissions in the Earth’s atmosphere, I will focus on two of my ongoing research interests. First, I will discuss how the precipitating electron fluxes have different properties depending on where they occur in the auroral oval. Second, I will talk about how participatory science is becoming a powerful way to gain new insight into dark-sky emission processes, and review recent discoveries it has enabled in space physics. I will advertise an ongoing collaboration aiming at internationalising participatory science initiatives and connecting the communities of aurora hunters together.

WEDNESDAY 6 MARCH, 12:00PM, ROOM 314 SCIENCE III BUILDING
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Seminars

Photonic Crystal Ring Resonators for Tailored Optical Microcombs

Dr Ewan Lucas

Research Fellow, Laboratoire Interdisciplinaire Carnot de Bourgogne

Nonlinear-wave mixing in optical microresonators offers a promising avenue for compact optical-frequency microcomb generation [1]. These microcombs have rapidly found applications across diverse fields, including optical frequency synthesis and high-capacity data communication systems. A fundamental characteristic of microcombs is their spectral profile, which is principally determined by the resonator’s dispersion. An illustrative example is the sech2 spectrum of dissipative Kerr solitons that emerges under anomalous group-velocity dispersion.

Concurrently, photonic crystal ring resonators (PhCR) have emerged as a flexible way of tailoring of optical microcavities [2]. These ring resonators introduce a corrugation to the inner wall of the waveguide, enabling precise and independent control of cavity mode resonance frequencies while preserving a high quality factor (Q). This innovative approach offers mode-by-mode frequency splitting capabilities, vastly expanding the design space for managing the nonlinear dynamics of optical states, such as Kerr solitons.

This presentation explores the advantages of this enhanced control, initially focusing on the control and generation of microcombs in the normal dispersion regime. I also demonstrate the creation of a ‘meta-dispersion’ resonator by selectively manipulating the resonance of multiple modes with a PhCR. The nonlinear modeling of these structures unveils new comb states and instabilities.
Furthermore, by embedding the governing equation of the system into a genetic algorithm, we efficiently pinpoint a dispersion profile that yields a microcomb closely aligned with a user-defined target spectrum [3].

References
[1] T. J. Kippenberg et al. “Dissipative Kerr solitons in optical microresonators”. Science 361.6402 (2018).
[2] S.-P. Yu et al. “Spontaneous pulse formation in edgeless photonic crystal resonators”. Nat. Phot. 15.6 (2021).
[3] E. Lucas, et al. “Tailoring microcombs with inverse-designed, meta-dispersion microresonators”. Nat. Photon. 1–8 (2023) doi:10.1038/s41566-023-01252-7.

Friday 15 December, 12:00pm, Room 314 Science III Building

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Media Events News

Potential drivers of the recent large Antarctic ozone holes

Despite public perception, the Antarctic ozone hole has been remarkably massive and long-lived over the past years, and University of Otago researchers believe there are factors beyond CFCs that are contributing. In their ground breaking work just published in Nature Communications, University of Otago Physicists Hannah Kessenich, Annika Seppälä, and Craig Rodger analysed ozone levels from 2004 to 2022, and found there is much less ozone in the centre of the Antarctic ozone hole compared to 19 years ago. While overall Antarctic ozone is recovering due to the Montreal Protocol that banned the harmful ozone depleting CFCs, the slow ozone recovery is focused on the outer parts of the ozone hole.

The Otago team used 20 years of satellite data from the Microwave Limb Sounder instrument on the NASA Aura satellite (https://aura.gsfc.nasa.gov) to identify what drivers the continued ozone depletion in the ozone hole core, and their study highlights the pressing need for comprehensive and ongoing monitoring of the ozone hole due to the critical role the ozone layer plays in protecting life on earth.

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News

2023 Hector Medal Award to Niels Kjærgaard

On November 15 The Royal Society held its Christchurch event to celebrate 2023 Research Honours. At the event Niels was awarded the Hector Medal for fundamental scientific studies on atomic collisions and light scattering using ultracold gases.

The Hector medal is an award for outstanding work in chemical, physical or mathematical and information sciences by a researcher in New Zealand, awarded annually. Niels will join a distinguished list of recipients since 1912, including Ernest Rutherford, Te Rangi Hiroa (Peter H. Buck), John Newton Dodd, Roy Patrick Kerr, Daniel Frank Walls, Paul Terence Callaghan and Richard Blaikie.

Find out more about the award at the Royal Society Media Release:

“Professor Niels Kjærgaard has been awarded the Hector Medal by Royal Society Te Apārangi for his outstanding contribution to the advancement of scientific understanding of fundamental particles, through experimental studies of atomic collisions and light-scattering using ultracold gases.”

Congratulations Niels!

Find out more about the research, visit the website for Kjærgaard Lab.

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News

Promotions 2023

Congratulations to Annika Seppälä, Jono Squire, and Paul Muir on your successful promotions in 2023!

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Media Events Seminars

2023 Dan Walls Medal Public Lecture: Maths powers black holes, the Universe and everything

Prof. David Wiltshire

University of Canterbury

Sixty years ago New Zealander Roy Kerr helped revolutionize physics, achieving what had eluded scientists for 47 years. He discovered the solution to Einstein’s equations defining space around a rotating star or black hole. He combined advanced mathematics with one key simplifying insight: All bodies collapsing under their own gravity inevitably rotate faster.

The Kerr solution became the basis for revolutions first in fundamental physics in the 1960s, in astronomy in the 1970–80s, and in cosmology in the 1990s and beyond. The discoveries of gravitational waves from colliding black holes, first in 2015, and then from colliding neutron stars in 2017, mean that decades of further scientific revolutions are just beginning.

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News

Transient Array Radio Telescope to be adopted by Square Kilometre Array

What started as an idea in 2014 by Dr Tim Molteno to develop the world’s smallest radio telescope in his Department of Physics laboratory at the University of Otago, is now being rolled out across eight partner nations of the Square Kilometre Array project in Southern Africa! The open-source, low-cost radio telescope called the ‘Transient Array Radio Telescope’ has been chosen by the South African Radio Astronomy Observatory as the ideal technology to build radio astronomy capacity on the continent.