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description Publicationkeyboard_double_arrow_right Article , Preprint 2016IOP Publishing ARC | Representation theory of ..., NSERCARC| Representation theory of diagram algebras and logarithmic conformal field theory ,NSERCAuthors: Alexi Morin-Duchesne; Jørgen Rasmussen; Philippe Ruelle;Alexi Morin-Duchesne; Jørgen Rasmussen; Philippe Ruelle;The central charge of the dimer model on the square lattice is still being debated in the literature. In this paper, we provide evidence supporting the consistency of a $c=-2$ description. Using Lieb's transfer matrix and its description in terms of the Temperley-Lieb algebra $TL_n$ at $\beta = 0$, we provide a new solution of the dimer model in terms of the model of critical dense polymers on a tilted lattice and offer an understanding of the lattice integrability of the dimer model. The dimer transfer matrix is analysed in the scaling limit and the result for $L_0-\frac c{24}$ is expressed in terms of fermions. Higher Virasoro modes are likewise constructed as limits of elements of $TL_n$ and are found to yield a $c=-2$ realisation of the Virasoro algebra, familiar from fermionic $bc$ ghost systems. In this realisation, the dimer Fock spaces are shown to decompose, as Virasoro modules, into direct sums of Feigin-Fuchs modules, themselves exhibiting reducible yet indecomposable structures. In the scaling limit, the eigenvalues of the lattice integrals of motion are found to agree exactly with those of the $c=-2$ conformal integrals of motion. Consistent with the expression for $L_0-\frac c{24}$ obtained from the transfer matrix, we also construct higher Virasoro modes with $c=1$ and find that the dimer Fock space is completely reducible under their action. However, the transfer matrix is found not to be a generating function for the $c=1$ integrals of motion. Although this indicates that Lieb's transfer matrix description is incompatible with the $c=1$ interpretation, it does not rule out the existence of an alternative, $c=1$ compatible, transfer matrix description of the dimer model. Comment: 54 pages. v2: minor corrections
Journal of Physics A... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu15 citations 15 popularity Average influence Average impulse Top 10% Powered by BIP!
more_vert Journal of Physics A... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2017Springer Science and Business Media LLC NSERC, EC | THREEPLE, ARC | Discovery Projects - Gran... +2 projectsNSERC ,EC| THREEPLE ,ARC| Discovery Projects - Grant ID: DP150104327 ,ARC| Quantum entanglement using slow-light-enhanced nonlinearity ,ARC| Nonlinear optical phononics: harnessing sound and light in nonlinear nanoscale circuitsLucia Caspani; Chunle Xiong; Benjamin J. Eggleton; Daniele Bajoni; Marco Liscidini; Matteo Galli; Roberto Morandotti; David J. Moss;AbstractThe ability to generate complex optical photon states involving entanglement between multiple optical modes is not only critical to advancing our understanding of quantum mechanics but will play a key role in generating many applications in quantum technologies. These include quantum communications, computation, imaging, microscopy and many other novel technologies that are constantly being proposed. However, approaches to generating parallel multiple, customisable bi- and multi-entangled quantum bits (qubits) on a chip are still in the early stages of development. Here, we review recent advances in the realisation of integrated sources of photonic quantum states, focusing on approaches based on nonlinear optics that are compatible with contemporary optical fibre telecommunications and quantum memory platforms as well as with chip-scale semiconductor technology. These new and exciting platforms hold the promise of compact, low-cost, scalable and practical implementations of sources for the generation and manipulation of complex quantum optical states on a chip, which will play a major role in bringing quantum technologies out of the laboratory and into the real world.
CORE (RIOXX-UK Aggre... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu182 citations 182 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!
visibility 17visibility views 17 download downloads 195 Powered bymore_vert CORE (RIOXX-UK Aggre... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type 2020 Italy, United States, Spain, Netherlands, Spain, United Kingdom, Italy, United Kingdom, France, ItalyCambridge University Press (CUP) EC | FirstDawn, NSERC, EC | MAGCOW +6 projectsEC| FirstDawn ,NSERC ,EC| MAGCOW ,NSF| Expanding interdisciplinary research at the Center for Gravitational Wave Astronomy ,ARC| Discovery Early Career Researcher Award - Grant ID: DE170100356 ,ARC| ARC Future Fellowships - Grant ID: FT130101086 ,EC| COSMOFLAGS ,NSF| Support of LIGO Data Analysis Activities at the University of Texas at Brownsville ,EC| AstroFIt2Amanda Weltman; Philip Bull; Stefano Camera; Katharine Kelley; Hamsa Padmanabhan; Jonathan R. Pritchard; Alvise Raccanelli; Signe Riemer-Sørensen; Lijing Shao; Sambatra Andrianomena; E. Athanassoula; David Bacon; Rennan Barkana; Gianfranco Bertone; Camille Bonvin; Albert Bosma; Marcus Brüggen; Carlo Burigana; Céline Bœhm; Francesca Calore; Jose A. R. Cembranos; Chris Clarkson; R. M. T. Connors; A. de la Cruz-Dombriz; Peter K. S. Dunsby; José Fonseca; Nicolao Fornengo; Daniele Gaggero; Ian Harrison; Julien Larena; Yin-Zhe Ma; Roy Maartens; M. Méndez-Isla; Soumya D. Mohanty; Steven G. Murray; David Parkinson; Alkistis Pourtsidou; Peter J. Quinn; Marco Regis; Prasenjit Saha; Martin Sahlén; Mairi Sakellariadou; J. Silk; T. Trombetti; Franco Vazza; Tejaswi Venumadhav; Francesca Vidotto; Francisco Villaescusa-Navarro; Yue-Fei Wang; Christoph Weniger; Laura Wolz; Fupeng Zhang; Bryan Gaensler;The Square Kilometre Array (SKA) is a planned large radio interferometer designed to operate over a wide range of frequencies, and with an order of magnitude greater sensitivity and survey speed than any current radio telescope. The SKA will address many important topics in astronomy, ranging from planet formation to distant galaxies. However, in this work, we consider the perspective of the SKA as a facility for studying physics. We review four areas in which the SKA is expected to make major contributions to our understanding of fundamental physics: cosmic dawn and reionisation; gravity and gravitational radiation; cosmology and dark energy; and dark matter and astroparticle physics. These discussions demonstrate that the SKA will be a spectacular physics machine, which will provide many new breakthroughs and novel insights on matter, energy, and spacetime. A. Racanelli has received funding from the People Programme (Marie Curie Actions) of the European Union H2020 Programme under REA grant agreement number 706896 (COSMOFLAGS). Funding for this work was partially provided by the Spanish MINECO under MDM-2014-0369 of ICCUB (Unidad de Excelencia ‘Maria de Maeztu’). Square Kilometre Array: et al. arXiv:1810.02680v3 Peer reviewed
Caltech Authors arrow_drop_down Recolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2020Spiral - Imperial College Digital RepositoryArticle . 2019Data sources: Spiral - Imperial College Digital RepositoryRecolector de Ciencia Abierta, RECOLECTAArticle . 2020Data sources: Recolector de Ciencia Abierta, RECOLECTAOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2020Data sources: OA@INAF - Istituto Nazionale di AstrofisicaPublications of the Astronomical Society of AustraliaOther literature type . Article . 2020License: https://www.cambridge.org/core/termsadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu172 citations 172 popularity Top 1% influence Top 10% impulse Top 0.1% Powered by BIP!
visibility 8visibility views 8 download downloads 42 Powered bymore_vert Caltech Authors arrow_drop_down Recolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2020Spiral - Imperial College Digital RepositoryArticle . 2019Data sources: Spiral - Imperial College Digital RepositoryRecolector de Ciencia Abierta, RECOLECTAArticle . 2020Data sources: Recolector de Ciencia Abierta, RECOLECTAOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2020Data sources: OA@INAF - Istituto Nazionale di AstrofisicaPublications of the Astronomical Society of AustraliaOther literature type . Article . 2020License: https://www.cambridge.org/core/termsadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1017/pasa.2019.42&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2018 United KingdomAmerican Geophysical Union (AGU) NSERC, ARC | Discovery Indigenous - Gr..., ARC | Tracking the response of ...NSERC ,ARC| Discovery Indigenous - Grant ID: IN140100050 ,ARC| Tracking the response of the Australian climate to abrupt climate changeKristen K. Beck; Michael-Shawn Fletcher; Patricia Gadd; Henk Heijnis; Krystyna M. Saunders; Gavin Simpson; Atun Zawadzki;doi: 10.1002/2017jg004135
AbstractCritical transitions in ecosystem states are often sudden and unpredictable. Consequently, there is a concerted effort to identify measurable early warning signals (EWS) for these important events. Aquatic ecosystems provide an opportunity to observe critical transitions due to their high sensitivity and rapid response times. Using palaeoecological techniques, we can measure properties of time series data to determine if critical transitions are preceded by any measurable ecosystem metrics, that is, identify EWS. Using a suite of palaeoenvironmental data spanning the last 2,400 years (diatoms, pollen, geochemistry, and charcoal influx), we assess whether a critical transition in diatom community structure was preceded by measurable EWS. Lake Vera, in the temperate rain forest of western Tasmania, Australia, has a diatom community dominated by Discostella stelligera and undergoes an abrupt compositional shift at ca. 820 cal yr BP that is concomitant with increased fire disturbance of the local vegetation. This shift is manifest as a transition from less oligotrophic acidic diatom flora (Achnanthidium minutissimum, Brachysira styriaca, and Fragilaria capucina) to more oligotrophic acidic taxa (Frustulia elongatissima, Eunotia diodon, and Gomphonema multiforme). We observe a marked increase in compositional variance and rate‐of‐change prior to this critical transition, revealing these metrics are useful EWS in this system. Interestingly, vegetation remains complacent to fire disturbance until after the shift in the diatom community. Disturbance taxa invade and the vegetation system experiences an increase in both compositional variance and rate‐of‐change. These trends imply an approaching critical transition in the vegetation and the probable collapse of the local rain forest system.
Journal of Geophysic... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/2017jg004135&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu24 citations 24 popularity Top 10% influence Average impulse Top 10% Powered by BIP!
visibility 6visibility views 6 download downloads 91 Powered bymore_vert Journal of Geophysic... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/2017jg004135&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2014Elsevier BV NSERC, ARC | Generalised topological s...NSERC ,ARC| Generalised topological spacesAuthors: Robin Cockett; Richard Garner;Robin Cockett; Richard Garner;Restriction categories were introduced to provide an axiomatic setting for the study of partially defined mappings; they are categories equipped with an operation called restriction which assigns to every morphism an endomorphism of its domain, to be thought of as the partial identity that is defined to just the same degree as the original map. In this paper, we show that restriction categories can be identified with \emph{enriched categories} in the sense of Kelly for a suitable enrichment base. By varying that base appropriately, we are also able to capture the notions of join and range restriction category in terms of enriched category theory. Comment: 29 pages
Theoretical Computer... arrow_drop_down Theoretical Computer ScienceArticle . 2014add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.tcs.2013.12.018&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu6 citations 6 popularity Average influence Average impulse Average Powered by BIP!
more_vert Theoretical Computer... arrow_drop_down Theoretical Computer ScienceArticle . 2014add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.tcs.2013.12.018&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 Italy, Netherlands, United Kingdom, Italy, FranceCambridge University Press (CUP) NSERC, NWO | Nature's Purest "Clean Ma..., NSF | NANOGrav Physics Frontier... +3 projectsNSERC ,NWO| Nature's Purest "Clean Machine": Deconstructing the Pulsar Magnetosphere ,NSF| NANOGrav Physics Frontier Center ,ARC| ARC Centres of Excellence - Grant ID: CE170100004 ,EC| MeerTRAP ,EC| ALERTMatthew Bailes; Andrew Jameson; F. Abbate; Ewan Barr; N. D. R. Bhat; L. Bondonneau; M. Burgay; Sarah Buchner; Fernando Camilo; David Champion; Ismaël Cognard; Paul Demorest; Paulo C. C. Freire; T. Gautam; M. Geyer; J. M. Griessmeier; Lucas Guillemot; H. Hu; Fabian Jankowski; Simon Johnston; Aris Karastergiou; Ramesh Karuppusamy; D. Kaur; Michael Keith; Michael Kramer; J. van Leeuwen; Marcus E. Lower; Yogesh Maan; Maura McLaughlin; B. W. Meyers; Stefan Oslowski; L. S. Oswald; Aditya Parthasarathy; Timothy T. Pennucci; Bettina Posselt; Andrea Possenti; Scott M. Ransom; Daniel J. Reardon; Alessandro Ridolfi; C. T. G. Schollar; M. Serylak; G. Shaifullah; M. Shamohammadi; Ryan Shannon; Charlotte Sobey; X. Song; Renée Spiewak; Ingrid H. Stairs; Benjamin Stappers; W. van Straten; Andrzej Szary; Gilles Theureau; V. Venkatraman Krishnan; Patrick Weltevrede; Norbert Wex; T. D. Abbott; G. Adams; J. P. Burger; R. R. G. Gamatham; M. Gouws; D. M. Horn; B. Hugo; A. F. Joubert; Jason Manley; K. McAlpine; S. S. Passmoor; A. Peens-Hough; Z. R. Ramudzuli; A. Rust; S. Salie; L. C. Schwardt; R. Siebrits; G. Van Tonder; V. van Tonder; M. G. Welz;We describe system verification tests and early science results from the pulsar processor (PTUSE) developed for the newly-commissioned 64-dish SARAO MeerKAT radio telescope in South Africa. MeerKAT is a high-gain (~2.8 K/Jy) low-system temperature (~18 K at 20cm) radio array that currently operates from 580-1670 MHz and can produce tied-array beams suitable for pulsar observations. This paper presents results from the MeerTime Large Survey Project and commissioning tests with PTUSE. Highlights include observations of the double pulsar J0737-3039A, pulse profiles from 34 millisecond pulsars from a single 2.5h observation of the Globular cluster Terzan 5, the rotation measure of Ter5O, a 420-sigma giant pulse from the Large Magellanic Cloud pulsar PSR J0540-6919, and nulling identified in the slow pulsar PSR J0633-2015. One of the key design specifications for MeerKAT was absolute timing errors of less than 5 ns using their novel precise time system. Our timing of two bright millisecond pulsars confirm that MeerKAT delivers exceptional timing. PSR J2241-5236 exhibits a jitter limit of <4 ns per hour whilst timing of PSR J1909-3744 over almost 11 months yields an rms residual of 66 ns with only 4 min integrations. Our results confirm that the MeerKAT is an exceptional pulsar telescope. The array can be split into four separate sub-arrays to time over 1000 pulsars per day and the future deployment of S-band (1750-3500 MHz) receivers will further enhance its capabilities. 20 pages, 16 Figures, 4 Tables, accepted for publication in PASA
NARCIS arrow_drop_down Publications of the Astronomical Society of Australia; Oxford University Research ArchiveOther literature type . Article . 2020 . 2023License: https://www.cambridge.org/core/termsOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2020Data sources: OA@INAF - Istituto Nazionale di Astrofisicaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu97 citations 97 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!
more_vert NARCIS arrow_drop_down Publications of the Astronomical Society of Australia; Oxford University Research ArchiveOther literature type . Article . 2020 . 2023License: https://www.cambridge.org/core/termsOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2020Data sources: OA@INAF - Istituto Nazionale di Astrofisicaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1017/pasa.2020.19&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Preprint , Article 2021Elsevier BV NSERC, ARC | Discovery Projects - Gran...NSERC ,ARC| Discovery Projects - Grant ID: DP190100977Authors: Pu Gao; Catherine Greenhill;Pu Gao; Catherine Greenhill;The switch chain is a well-studied Markov chain which can be used to sample approximately uniformly from the set $\Omega(\boldsymbol{d})$ of all graphs with a given degree sequence $\boldsymbol{d}$. Polynomial mixing time (rapid mixing) has been established for the switch chain under various conditions on the degree sequences. Amanatidis and Kleer introduced the notion of strongly stable families of degree sequences, and proved that the switch chain is rapidly mixing for any degree sequence from a strongly stable family. Using a different approach, Erd\H{o}s et al. recently extended this result to the (possibly larger) class of P-stable degree sequences, introduced by Jerrum and Sinclair in 1990. We define a new notion of stability for a given degree sequence, namely $k$-\emph{stability}, and prove that if a degree sequence $\boldsymbol{d}$ is 8-stable then the switch chain on $\Omega(\boldsymbol{d})$ is rapidly mixing. We also provide sufficient conditions for P-stability, strong stability and 8-stability. Using these sufficient conditions, we give the first proof of P-stability for various families of heavy-tailed degree sequences, including power-law degree sequences, and show that the switch chain is rapidly mixing for these families. We further extend these notions and results to directed degree sequences. Comment: 32 pages, 6 figures. This version addresses referee comments
arXiv.org e-Print Ar... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.dam.2020.12.004&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu2 citations 2 popularity Average influence Average impulse Average Powered by BIP!
more_vert arXiv.org e-Print Ar... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.dam.2020.12.004&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2014 United StatesCopernicus GmbH ARC | Tropospheric ozone and ai..., NSERCARC| Tropospheric ozone and air quality in Australia ,NSERCCamille Viatte; Kimberly Strong; James W. Hannigan; E. Nussbaumer; Louisa K. Emmons; Stephanie Conway; Clare Paton-Walsh; J Hartley; J. S. Benmergui; John C. Lin;We investigate Arctic tropospheric composition using ground-based Fourier transform infrared (FTIR) solar absorption spectra, recorded at the Polar Environment Atmospheric Research Laboratory (PEARL, Eureka, Nunavut, Canada, 80°05' N, 86°42' W) and at Thule (Greenland, 76°53' N, −68°74' W) from 2008 to 2012. The target species, carbon monoxide (CO), hydrogen cyanide (HCN), ethane (C2H6), acetylene (C2H2), formic acid (HCOOH), and formaldehyde (H2CO) are emitted by biomass burning and can be transported from mid-latitudes to the Arctic. By detecting simultaneous enhancements of three biomass burning tracers (HCN, CO, and C2H6), ten and eight fire events are identified at Eureka and Thule, respectively, within the 5-year FTIR time series. Analyses of Hybrid Single Particle Lagrangian Integrated Trajectory (HYSPLIT) model back-trajectories coupled with Moderate Resolution Imaging Spectroradiometer (MODIS) fire hotspot data, Stochastic Time-Inverted Lagrangian Transport (STILT) model footprints, and Ozone Monitoring Instrument (OMI) UV aerosol index maps, are used to attribute burning source regions and travel time durations of the plumes. By taking into account the effect of aging of the smoke plumes, measured FTIR enhancement ratios were corrected to obtain emission ratios and equivalent emission factors. The means of emission factors for extratropical forest estimated with the two FTIR data sets are 0.40 ± 0.21 g kg−1 for HCN, 1.24 ± 0.71 g kg−1 for C2H6, 0.34 ± 0.21 g kg−1 for C2H2, and 2.92 ± 1.30 g kg−1 for HCOOH. The emission factor for CH3OH estimated at Eureka is 3.44 ± 1.68 g kg−1. To improve our knowledge concerning the dynamical and chemical processes associated with Arctic pollution from fires, the two sets of FTIR measurements were compared to the Model for OZone And Related chemical Tracers, version 4 (MOZART-4). Seasonal cycles and day-to-day variabilities were compared to assess the ability of the model to reproduce emissions from fires and their transport. Good agreement in winter confirms that transport is well implemented in the model. For C2H6, however, the lower wintertime concentration estimated by the model as compared to the FTIR observations highlights an underestimation of its emission. Results show that modeled and measured total columns are correlated (linear correlation coefficient r > 0.6 for all gases except for H2CO at Eureka and HCOOH at Thule), but suggest a general underestimation of the concentrations in the model for all seven tropospheric species in the high Arctic.
Caltech Authors arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5194/acpd-14-26349-2014&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu26 citations 26 popularity Top 10% influence Average impulse Average Powered by BIP!
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Preprint 2016Copernicus GmbH NSERC, ARC | The carbon cycle and clim..., ARC | Discovery Projects - Gran... +3 projectsNSERC ,ARC| The carbon cycle and climate: new approaches to atmospheric measurements and modelling ,ARC| Discovery Projects - Grant ID: DP140101552 ,ARC| High resolution Fourier transform infrared spectrometer for atmospheric remote sensing and laboratory spectroscopy ,ARC| Discovery Early Career Researcher Award - Grant ID: DE140100178 ,ARC| Innovative measurement and modelling of greenhouse fluxes at regional scales across AustraliaA. Ostler; Ralf Sussmann; Prabir K. Patra; Sander Houweling; Marko De Bruine; Gabriele Stiller; Florian J. Hänel; Johannes Plieninger; Philippe Bousquet; Yi Yin; Marielle Saunois; Kaley A. Walker; Nicholas M. Deutscher; David W. T. Griffith; Thomas Blumenstock; Frank Hase; Thorsten Warneke; Zhiting Wang; Rigel Kivi; John Robinson;doi: 10.5194/amt-2016-90
Abstract. The distribution of methane (CH4) in the stratosphere can be a major driver of spatial variability in the dry-air column-averaged CH4 mixing ratio (XCH4), which is being measured increasingly for the assessment of CH4 surface emissions. Chemistry-transport models (CTMs) therefore need to simulate the tropospheric and stratospheric fractional columns of XCH4 accurately for estimating surface emissions from XCH4. Simulations from three CTMs are tested against XCH4 observations from the Total Carbon Column Network (TCCON). We analyze how the model-TCCON agreement in XCH4 depends on the model representation of stratospheric CH4 distributions. Model equivalents of TCCON XCH4 are computed with stratospheric CH4 fields from both the model simulations and from satellite-based CH4 distributions from MIPAS (Michelson Interferometer for Passive Atmospheric Sounding) and MIPAS CH4 fields adjusted to ACE-FTS (Atmospheric Chemistry Experiment Fourier Transform Spectrometer) observations. In comparison to simulated model fields we find an improved model-TCCON XCH4 agreement for all models with MIPAS-based stratospheric CH4 fields. For the Atmospheric Chemistry Transport Model (ACTM) the average XCH4 bias is significantly reduced from 38.1 ppb to 13.7 ppb, whereas small improvements are found for the models TM5 (Transport Model, version 5; from 8.7 ppb to 4.3 ppb), and LMDz (Laboratoire de Météorologie Dynamique model with Zooming capability; from 6.8 ppb to 4.3 ppb), respectively. MIPAS stratospheric CH4 fields adjusted to ACE-FTS reduce the average XCH4 bias for ACTM (3.3 ppb), but increase the average XCH4 bias for TM5 (10.8 ppb) and LMDz (20.0 ppb). These findings imply that the range of satellite-based stratospheric CH4 is insufficient to resolve a possible stratospheric contribution to differences in total column CH4 between TCCON and TM5 or LMDz. Applying transport diagnostics to the models indicates that model-to-model differences in the simulation of stratospheric transport, notably the age of stratospheric air, can largely explain the inter-model spread in stratospheric CH4 and, hence, its contribution to XCH4. This implies that there is a need to better understand the impact of individual model transport components (e.g., physical parameterization, meteorological data sets, model horizontal/vertical resolution) on modeled stratospheric CH4.
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For further information contact us at helpdesk@openaire.eu1 citations 1 popularity Average influence Average impulse Average Powered by BIP!
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You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2019 France, United StatesAmerican Astronomical Society NSERC, ARC | Discovery Projects - Gran..., NSF | Cosmological Research wit... +1 projectsNSERC ,ARC| Discovery Projects - Grant ID: DP150103208 ,NSF| Cosmological Research with the 10-meter South Pole Telescope ,NSF| Center for Cosmological PhysicsMarco P. Viero; Christian L. Reichardt; Bradford Benson; Lindsey Bleem; James J. Bock; John E. Carlstrom; C. L. Chang; H-M. Cho; T. M. Crawford; A. T. Crites; T. de Haan; M. A. Dobbs; W. B. Everett; Elizabeth George; N. W. Halverson; N. L. Harrington; G. P. Holder; W. L. Holzapfel; Zhen Hou; J. D. Hrubes; Lloyd Knox; Adrian T. Lee; Daniel M. Luong-Van; Daniel P. Marrone; Jeff McMahon; S. S. Meyer; Marius Millea; L. M. Mocanu; Joseph J. Mohr; Lorenzo Moncelsi; Stephen Padin; C. Pryke; J. E. Ruhl; K. K. Schaffer; Paolo Serra; Erik Shirokoff; Z. K. Staniszewski; Antony A. Stark; K. T. Story; Keith Vanderlinde; Joaquin Vieira; R. Williamson; Michael Zemcov;We present measurements of the power spectra of cosmic infrared background (CIB) and cosmic microwave background (CMB) fluctuations in six frequency bands. Maps at the lower three frequency bands, 95, 150, and 220 GHz (3330, 2000, 1360 $\mu$m) are from the South Pole Telescope, while the upper three frequency bands, 600, 857, and 1200 GHz (500, 350, 250 $\mu$m) are observed with Herschel/SPIRE. From these data, we produce 21 angular power spectra (six auto- and fifteen cross-frequency) spanning the multipole range $600 \le \ell \le 11,000$. Our measurements are the first to cross-correlate measurements near the peak of the CIB spectrum with maps at 95 GHz, complementing and extending the measurements from Planck Collaboration et al. (2014) at 218, 550, and 857 GHz. The observed fluctuations originate largely from clustered, infrared-emitting, dusty star-forming galaxies, the CMB, and to a lesser extent radio galaxies, active galactic nuclei, and the Sunyaev-Zel'dovich effect. Comment: 21 pages, 3 figures; Accepted by ApJS (updated to accepted version)
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For further information contact us at helpdesk@openaire.eu8 citations 8 popularity Top 10% influence Average impulse Average Powered by BIP!
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description Publicationkeyboard_double_arrow_right Article , Preprint 2016IOP Publishing ARC | Representation theory of ..., NSERCARC| Representation theory of diagram algebras and logarithmic conformal field theory ,NSERCAuthors: Alexi Morin-Duchesne; Jørgen Rasmussen; Philippe Ruelle;Alexi Morin-Duchesne; Jørgen Rasmussen; Philippe Ruelle;The central charge of the dimer model on the square lattice is still being debated in the literature. In this paper, we provide evidence supporting the consistency of a $c=-2$ description. Using Lieb's transfer matrix and its description in terms of the Temperley-Lieb algebra $TL_n$ at $\beta = 0$, we provide a new solution of the dimer model in terms of the model of critical dense polymers on a tilted lattice and offer an understanding of the lattice integrability of the dimer model. The dimer transfer matrix is analysed in the scaling limit and the result for $L_0-\frac c{24}$ is expressed in terms of fermions. Higher Virasoro modes are likewise constructed as limits of elements of $TL_n$ and are found to yield a $c=-2$ realisation of the Virasoro algebra, familiar from fermionic $bc$ ghost systems. In this realisation, the dimer Fock spaces are shown to decompose, as Virasoro modules, into direct sums of Feigin-Fuchs modules, themselves exhibiting reducible yet indecomposable structures. In the scaling limit, the eigenvalues of the lattice integrals of motion are found to agree exactly with those of the $c=-2$ conformal integrals of motion. Consistent with the expression for $L_0-\frac c{24}$ obtained from the transfer matrix, we also construct higher Virasoro modes with $c=1$ and find that the dimer Fock space is completely reducible under their action. However, the transfer matrix is found not to be a generating function for the $c=1$ integrals of motion. Although this indicates that Lieb's transfer matrix description is incompatible with the $c=1$ interpretation, it does not rule out the existence of an alternative, $c=1$ compatible, transfer matrix description of the dimer model. Comment: 54 pages. v2: minor corrections
Journal of Physics A... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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