PALEO-PGEM V1.0: a Statistical Emulator of Pliocene–Pleistocene Climate
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AMOC Variability, a Key Factor in Emission Reduction Scenarios
UTRECHT UNIVERSITY MSC CLIMATE PHYSICS INSTITUTE FOR MARINE AND ATMOSPHERIC RESEARCH UTRECHT 5 AMOC variability, a key factor in emission reduction scenarios 10 Author: J.M. Valentí Muelas [6515886] Supervisor: Prof. Dr. Ir. H.A. Dijkstra 15 June 2020. Contents 1 Introduction 2 2 Methods 4 2.1 Carbon Cycle Model................................................4 5 2.2 Emission reduction pathways............................................5 2.3 Model........................................................7 2.4 Climate sensitivity & Feedbacks..........................................8 2.5 Model diagnostics.................................................. 10 3 Results 12 10 3.1 Basic variables................................................... 12 3.2 AMOC....................................................... 14 3.3 GMST-AMOC correlation............................................. 19 4 Discussion and Conclusions 21 4.1 GMST response to emission reduction....................................... 21 15 4.2 AMOC Collapse.................................................. 22 4.3 Conclusions..................................................... 24 Appendix A: Tables 28 Appendix B: Complementary figures 29 1 Abstract The climate system response to emission reduction shows time dependencies when evaluated in terms of global mean sur- face temperature (GMST). The Atlantic meridional overturning circulation (AMOC) variability may be forcing a non-linear behaviour on GMST response to emission reduction. In this study, emission reduction is evaluated with -
Referee 1 1 2 Many Thanks for the Constructive Suggestions. Our
1 Referee 1 2 3 Many thanks for the constructive suggestions. Our responses are in red text 4 below. 5 6 The paper describes PLASIM-GENIE a new intermediate-complexity 7 Atmosphere- Ocean Earth System Model, designed for simulations of millenium+ 8 length. The new model is well suited for studies of long-term climate change, its 9 simulation of present-day climate is acceptable, its formulation is mostly 10 described well, and I recommend publication subject to the following changes 11 being made. 12 13 1. It’s not 100% clear whether or not this model has a carbon cycle, and what 14 aspects of this are turned on or off. The model is described as an AOGCM 15 (suggesting no C-cycle), but section 2.1 and others do allude to the simulation of 16 different carbon pools on land, which is slightly confusing. I presume there is 17 some sort of diagnostic C-cycle which does not affect atmospheric CO2, but does 18 affect vegetation. However GENIE- 1 does contain a fully interactive C-cycle. The 19 abstract, introduction, section 2.1 and other sections have to be clearer about 20 which parts of the C-cycle are on or off. Any flexibility in the C-cycle (ie: being 21 run in a diagnostic mode to simulation terrestrial pools but without affecting the 22 ocean and atmosphere) should be noted, as potential users of this AOGCM would 23 be interested in this. 24 25 As suggested, we have added flexibility to the run the terrestrial carbon cycle in 26 diagnostic mode. -
Multiple Climate States of Habitable Exoplanets: the Role of Obliquity and Irradiance
The Astrophysical Journal, 844:147 (13pp), 2017 August 1 https://doi.org/10.3847/1538-4357/aa7a03 © 2017. The American Astronomical Society. All rights reserved. Multiple Climate States of Habitable Exoplanets: The Role of Obliquity and Irradiance C. Kilic1,2,3, C. C. Raible1,2,3, and T. F. Stocker1,2,3,4 1 Climate and Environmental Physics, Physics Institute, University of Bern, Switzerland; [email protected] 2 Centre for Space and Habitability, University of Bern, Switzerland 3 Oeschger Centre for Climate Change Research, University of Bern, Switzerland Received 2017 April 3; revised 2017 May 29; accepted 2017 June 14; published 2017 August 1 Abstract Stable, steady climate states on an Earth-size planet with no continents are determined as a function of the tilt of the planet’s rotation axis (obliquity) and stellar irradiance. Using a general circulation model of the atmosphere coupled to a slab ocean and a thermodynamic sea ice model, two states, the Aquaplanet and the Cryoplanet, are found for high and low stellar irradiance, respectively. In addition, four stable states with seasonally and perennially open water are discovered if comprehensively exploring a parameter space of obliquity from 0° to 90° and stellar irradiance from 70% to 135% of the present-day solar constant. Within 11% of today’s solar irradiance, we find a rich structure of stable states that extends the area of habitability considerably. For the same set of parameters, different stable states result if simulations are initialized from an aquaplanet or a cryoplanet state. This demonstrates the possibility of multiple equilibria, hysteresis, and potentially rapid climate change in response to small changes in the orbital parameters. -
The Super X-Ray Laser
The DESY research magazine – Issue 01/16 ZOOM – The DESY research magazine | Issue 01/16 The DESY research – femto The super X-ray laser Breakthrough in crystallography The DESY research centre Nanostructures DESY is one of the world’s leading particle accelerator centres. Researchers use the large‑scale facilities at DESY to explore the microcosm in all its variety – ranging from the assemble themselves interaction of tiny elementary particles to the behaviour of innovative nanomaterials and the vital processes that take place between biomolecules. The accelerators and detectors that Why van Gogh’s DESY develops and builds at its locations in Hamburg and Zeuthen are unique research Sunflowers are wilting tools. The DESY facilities generate the most intense X‑ray radiation in the world, accelerate particles to record energies and open up completely new windows onto the universe. DESY is a member of the Helmholtz Association, Germany’s largest scientific organisation. femto 01/16 femto 01/16 Imprint femto is published by Translation Deutsches Elektronen‑Synchrotron DESY, TransForm GmbH, Cologne a research centre of the Helmholtz Association Ilka Flegel Editorial board address Cover picture Notkestraße 85, 22607 Hamburg, Germany Dirk Nölle, DESY Tel.: +49 40 8998‑3613, fax: +49 40 8998‑4307 e‑mail: [email protected] Printing and image processing Internet: www.desy.de/femto Heigener Europrint GmbH ISSN 2199‑5192 Copy deadline Editorial board March 2016 Till Mundzeck (responsible under press law) Ute Wilhelmsen Contributors to this issue Frank Grotelüschen, Kristin Hüttmann Design and production Diana von Ilsemann The planet simulator A new high-pressure press at DESY’s X-ray source PETRA III can simulate the interior of planets and synthesise new materials. -
Vplanet: the Virtual Planet Simulator
VPLanet: The Virtual Planet Simulator Rory Barnes1,2, Rodrigo Luger2,3, Russell Deitrick2,4, Peter Driscoll2,5, David Fleming1,2, Hayden Smotherman1,2, Thomas R. Quinn1,2, Diego McDonald1,2, Caitlyn Wilhelm1,2, Benjamin Guyer1,2, Victoria S. Meadows1,2, Patrick Barth6, Rodolfo Garcia1,2, Shawn D. Domagal-Goldman2,7, John Armstrong2,8, Pramod Gupta1,2, and The NASA Virtual Planetary Laboratory 1Astronomy Dept., U. of Washington, Box 351580, Seattle, WA 98195 2NASA Virtual Planetary Laboratory 3Center for Computational Astrophysics, 6th Floor, 162 5th Ave, New York, NY 10010 4Astronomisches Institut, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland 5Department of Terrestrial Magnetism, Carnegie Institute for Science, 5241 Broad Branch Road, NW, Washington, DC 20015 6Max Planck Institute for Astronomy, Heidelberg, Germany 7NASA Goddard Space Flight Center, Mail Code 699, Greenbelt, MD, 20771 8Department of Physics, Weber State University, 1415 Edvaldson Drive, Dept. 2508, Ogden, UT 84408-2508 Overview. VPLanet is software to simulate the • BINARY: Orbital evolution of a circumbinary planet evolution of an arbitrary planetary system for billions of from Leung & Lee (2013). years. Since planetary systems evolve due to a myriad • GalHabit: Evolution of wide binaries due to the of processes, VPLanet unites theories developed in galactic tide and passing stars (Heisler & Tremaine Earth science, stellar astrophysics, planetary science, 1986; Rickman et al. 2008; Kaib et al. 2013). and galactic astronomy. VPLanet can simulate a generic • SpiNBody: N-body integrator. planetary system, but is optimized for those with • DistOrb: 2nd and 4th order secular models of orbital potentially habitable worlds. VPLanet is open source evolution (Murray & Dermott 1999). -
Arxiv:2005.01740V1 [Astro-Ph.EP] 4 May 2020 18.8 (Winters Et Al
Draft version May 6, 2020 Preprint typeset using LATEX style emulateapj v. 12/16/11 A COUPLED ANALYSIS OF ATMOSPHERIC MASS LOSS AND TIDAL EVOLUTION IN XUV IRRADIATED EXOPLANETS: THE TRAPPIST-1 CASE STUDY Juliette Becker1,2,3, *, Elena Gallo1, Edmund Hodges-Kluck4, Fred C. Adams1,3, Rory Barnes5,6 1Department of Astronomy, University of Michigan, Ann Arbor, MI 48104, USA 2Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 3Department of Physics, University of Michigan, Ann Arbor, MI 48104, USA 4Code 662, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA 5Department of Astronomy, University of Washington, Seattle, WA, USA 6NASA Virtual Planetary Laboratory, USA and *51 Pegasi b Fellow Draft version May 6, 2020 ABSTRACT Exoplanets residing close to their stars can experience evolution of both their physical structures and their orbits due to the influence of their host stars. In this work, we present a coupled analysis of dynamical tidal dissipation and atmospheric mass loss for exoplanets in XUV irradiated environments. As our primary application, we use this model to study the TRAPPIST-1 system, and place constraints on the interior structure and orbital evolution of the planets. We start by reporting on a UV continuum flux measurement (centered around ∼ 1900 Angstroms) for the star TRAPPIST-1, based on 300 ks of Neil Gehrels Swift Observatory data, and which enables an estimate of the XUV-driven thermal escape arising from XUV photo-dissociation for each planet. We find that the X-ray flaring luminosity, −4 measured from our X-ray detections, of TRAPPIST-1 is 5.6 ×10 L∗, while the full flux including non- −5 flaring periods is 6.1 ×10 L∗, when L∗ is TRAPPIST-1's bolometric luminosity. -
Global Weat Her Prediction and High-End Computing at NASA
Global Weat her Prediction and High-End Computing at NASA Shian-Jiann Lin, Robert Atlas, and Kao-San Yeh* NASA Goddard Space Flight Center *Corresponding author address: Dr. Kao-San Yeh Code 900.3, NASA Goddard Space Flight Center, Greenbelt, MD 20771 E-mail: [email protected] August 18th, 2003 Abstract We demonstrate current capabilities of the NASA finite-volume General Circulation Model an high-resolution global weather prediction, and discuss its development path in the foreseeable future. This model can be regarded as a prototype of a future NASA Earth modeling system intended to unify development activities cutting across various disciplines within the NASA Earth Science Enterprise. 1 1. Introduction NASA’s goal for an Earth modeling system is to unify the model development activities that cut across various disciplines within the Earth Science Enterprise. Applications of the Earth modeling system include, but are not limited to, weather and chemistry-climate change predictions, and atmospheric and oceanic data assimilation. Among these applications, high-resolution global weather prediction requires the highest temporal and spatial resolution, and hence demands the most capability of a high-end computing system. In the continuing quest to improve and perhaps push to the limit of the predictability of the weather (see the related side bar), we are adopting more physically based algorithms with much higher resolution than those in earlier models. We are also including additional physical and chemical components that have not been coupled to the modeling system previously. As a comprehensive high-resolution Earth modeling system will require enormous computing power, it is important to design all component models efficiently for modern parallel computers with distributed-memory platforms. -
Molecular Factory: Gravityflow
Partnership with PlantForm Corporation MOLECULAR FACTORY: GRAVITYFLOW 2015 Starting point: PlantForm Corporation: Canadian biotech company producing biosimilar drugs and vaccines through GMO agrobacteria infiltration of the tobacco plant Nicotiana Benthamiana. Intravision patent: Vacuum PlantForm patent: Biosimilar infiltration of transgenic Herceptin in transgenic tobacco tobacco plant. The GravityFlow system - a “high-tech/ low-tech” The Intravision Timeline: Projects: We the Roots AI Farmer Toronto pilot Pilot facility in assistant operational Paris France operational Intravision GravityFlow Intravision New Jersey & AI Deep GROUP system GREENS Welland facilities Learning/pattern established invented established complete Recognition starts 1998 2009 2016 2018 2019 2020 2022 Eurostar on Photosystem NSERC grant on Reserach on GMO Barley, sealed research Romaine salad micro-algae ORF, Iceland chamber. and beans started (PS1000) Photobiolgy on Cooperation Photosystem fish in CESRF sealed research aquaculture UoGuelph chamber. (PS2000) Research: Tech-transfer Space Research: 2010 Intravision and CESRF cooperation. The hypobaric Guelph Blue-Box plant chambers developed to understand if terrestrial food-plants can be grown in low at- mospheric pressures / smaller planets than Earth like on Mars or on the Moon. Evolution of Intravision Technology: Snapshots from the development of plant research LED-lighting and research-chambers. 2009: ORF Genetics, Iceland. 2011: INTICE, with CESRF UoGuelph. 2015: MAPS, with CESRF UoGuelph. GMO barely for production of cytokines Production of food for manned space Food production prototype for KISR, EUROSTAR research funding. travel. Canadian Space Agency funding. Kuwait Institute of Scientific Research 2016: PhotoSystem; CESRF UoGuelph. 2018: Planet Simulator, McMaster U. 2019: MELISSA photo-bioreactor, Sealed Plant Research chamber, prototype, Simulate environment on a planet - prior LED retrofit of photo-bioreactor, Internal development project to the establishment of an athmosphere. -
COOPERATIVE INSTITUTE for RESEARCH in ENVIRONMENTAL SCIENCES University of Colorado at Boulder UCB 216 Boulder, CO 80309-0216
CELEB ra TING 0 OF ENVI R ONMENT A L RESE arc H years 4 COOPERATIVE INSTITUTE FOR RESEARCH ANNU A L REPO R T IN ENVIRONMENTAL SCIENCES University of Colorado at Boulder i 00 2 8 COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES University of Colorado at Boulder UCB 216 Boulder, CO 80309-0216 Phone: 303-492-1143 Fax: 303-492-1149 email: [email protected] http://cires.colorado.edu ANNU A L REPO R T ST A FF Suzanne van Drunick, Coordinator Jennifer Gunther, Designer Katy Human, Editor COVE R PHOTO Pat and Rosemarie Keough part of traveling photographic exhibit Antarctica—Passion and Obsession Sponsored by CIRES in celebration of 40th Anniversary ii From the Director 2 Executive Summary and Research Highlights 4 The Institute Year in Review 12 Contributions to NOAA’s Strategic Vision 13 Administration and Funding 16 Creating a Dynamic Research Environment 21 CIRES People and Projects 26 Faculty Fellows Research 27 Scientific Centers 58 Education and Outreach 68 Visiting Fellows 70 Innovative Research Projects 73 Graduate Student Research Fellowships 83 Diversity and Undergraduate Research Programs 85 Theme Reports 86 Measures of Achievement: Calendar Year 2007 146 Publications by the Numbers 147 Refereed publications 148 Non-refereed Publications 172 Refereed Journals in which CIRES Scientists Published 179 Honors and Awards 181 Service 185 Appendices 188 Governance and Management 189 Personnel Demographics 193 Acronyms and Abbreviations 194 CIRES Annual Report 2008 1 From the Director 2 CIRES Annual Report 2008 am very proud to present the new CIRES annual report for fiscal year 2008. It has been another exciting year with numerous accomplishments, Iawards, and continued growth in our research staff and budget. -
ITCZ Splitting and the Influence of Large-Scale Eddy Fields on The
Journal of the Meteorological Society of Japan, Vol. 89, No. 5, pp. 399–411, 2011 399 DOI:10.2151/jmsj.2011-501 ITCZ Splitting and the Influence of Large-Scale Eddy Fields on the Tropical Mean State Eileen DAHMS Max Planck Institute for Meteorology, Hamburg, Germany Meteorological Institute, KlimaCampus, University of Hamburg, Germany Hartmut BORTH, Frank LUNKEIT and Klaus FRAEDRICH Meteorological Institute, KlimaCampus, University of Hamburg, Germany (Manuscript received 21 April 2010, in final form 12 December 2010) Abstract A spectral aqua-planet atmospheric general circulation model (AGCM) is forced with a series of zonally constant sea surface temperature (SST) distributions which are symmetric about the equator. For every oceanic forcing, the AGCM is run twice; a first time keeping all spectral modes and a second time with only the zonally symmetric ones. Parameterizations and boundary conditions remain the same in all cases thus allowing a consistent comparison of 3-D and 2-D flows. The comparative study shows that the structure of the tropical mean state of the full model is basically captured by the zonally symmetric model and that eddy fields merely modify this structure. This shows that the structure of the tropical mean state is mainly determined by the shape of the effective SST forcing. We confirm previous studies where the shape and strength of the Hadley circulation is comparable in the 3-D and 2-D experiments for cases with a well pronounced single ITCZ. So the underestimation of the Hadley circulation often found in idealized zonally symmetric models is not only due to the neglect of large-scale eddy fields. -
April 16, 2021
april 16, 2021 The Apeiron is an ancient term offered by Anaximander of Miletus in the 6th century B.C. that embraces the spirit of this forum. As with the Apeiron, which is infinite and boundless, all inclusive, eternal, and unaging, this forum is designed to be inclusive with respect to student research, scholarship, creative activities, and community engagement. It is dedicated to the proposition that students are capable of work that knows no limits and transcends all boundaries. Each student participant in the Washburn University Apeiron has worked on his or her project under the supervision of a faculty mentor. The projects, which have been reviewed by the faculty, demonstrate creativity, originality, and a level of work superior to that normally expected of students. Today’s presenters exemplify the spirit of the Apeiron. www.washburn.edu/apeiron __ The Greek Alphabet_ ___ Alpha Nu Beta Xi Gamma Omicron Delta Pi Epsilon Rho Zeta Sigma Eta Tau Theta Upsilon Iota Phi Kappa Chi Lambda Psi Mu Omega ______________________________________________________________________________ Original cover art designed by Christina Noland. Table of Contents Page Schedule of Events ……………………………………………………………… 2 Fine Arts Performance ………………………………………………………….. 3 Oral Presentation Schedule-at-a-Glance ………………………………………... 4 Oral Presentations I ……………………………………………………………... 5 Oral Presentations II …………………………………………………………… 10 Poster Presentations ……………………………………………………………. 13 Apeiron Committee ……………………………………………………………. 22 Special Thanks ………………………………………………………………… 23 Index of Presenters and Mentors ………………………………………………. 24 1 April 16, 2021 Schedule of Events 10:00 a.m. – 10:10 a.m. Welcome* Courtney Sullivan, Chair, Apeiron Committee Join: https://live.remo.co/e/washburn-university-apeiron-2021 Recognition of Student Designers* Gloriänna Noland and Christina Noland, Designers of Apeiron Poster and Program Cover Art 10:10 a.m. -
Air Dispersion Modelling of Stack Emissions
Enemalta Air dispersion modelling of stack emissions First phase final report Authors Calori G., Tinarelli G., Radice P., Costa M., Pozzi C., Finardi S. Ref. ARIANET R2013.25 December 2013 (final revision: June 2014) ARIANET s.r.l. via Gilino, 9 – 20128 Milano – ITALY tel. +39-02-27007255 – +39-02-25708084 – http://www.aria-net.it Cap. Soc. € 90.000.00 i.v. – R.E.A. n° 1635752 – Codice Fiscale e Partita IVA 03079010967 Enemalta - Air dispersion modelling of stack emissions Report ARIANET R2013.25 Authors: Calori G., Tinarelli G., Radice P., Costa M., Pozzi C., Finardi S. Customer: Enemalta Corporation Central Administration Building, Church Wharf, Marsa MRS 1000, Malta Reference number: GN/DPS/T/3015/2012 ARIANET R2013.25 Page I Enemalta - Air dispersion modelling of stack emissions Non-technical summary Scope: Electricity for the Maltese Islands is provided by Enemalta Corporation, the state-owned energy utility, which currently operates two power stations: Marsa (MPS) and Delimara (DPS), with a total installed electrical capacity of 720 MW, provided by a mix of conventional steam units, gas turbines and a new combined cycle diesel engines block at DPS. According to plans, MPS is expected to be progressively shut down during 2013 and 2014, and a 200 MW submarine interconnection to the European grid, to be finally commissioned and handed over to Enemalta. Enemalta carried out an air dispersion modelling study for DPS in 2011 as part of the IPPC obligations. However, the revised Delimara IPPC permit requires that this dispersion model is updated to reflect changes in the combustion plants and the installation of the cable interconnector.