Don't Throw out the Sympatric Species with the Crater Lake Water: Fine-Scale
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Annual Report COOPERATIVE INSTITUTE for RESEARCH in ENVIRONMENTAL SCIENCES
2015 Annual Report COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES 2015 annual report University of Colorado Boulder UCB 216 Boulder, CO 80309-0216 COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES University of Colorado Boulder 216 UCB Boulder, CO 80309-0216 303-492-1143 [email protected] http://cires.colorado.edu CIRES Director Waleed Abdalati Annual Report Staff Katy Human, Director of Communications, Editor Susan Lynds and Karin Vergoth, Editing Robin L. Strelow, Designer Agreement No. NA12OAR4320137 Cover photo: Mt. Cook in the Southern Alps, West Coast of New Zealand’s South Island Birgit Hassler, CIRES/NOAA table of contents Executive summary & research highlights 2 project reports 82 From the Director 2 Air Quality in a Changing Climate 83 CIRES: Science in Service to Society 3 Climate Forcing, Feedbacks, and Analysis 86 This is CIRES 6 Earth System Dynamics, Variability, and Change 94 Organization 7 Management and Exploitation of Geophysical Data 105 Council of Fellows 8 Regional Sciences and Applications 115 Governance 9 Scientific Outreach and Education 117 Finance 10 Space Weather Understanding and Prediction 120 Active NOAA Awards 11 Stratospheric Processes and Trends 124 Systems and Prediction Models Development 129 People & Programs 14 CIRES Starts with People 14 Appendices 136 Fellows 15 Table of Contents 136 CIRES Centers 50 Publications by the Numbers 136 Center for Limnology 50 Publications 137 Center for Science and Technology -
Kevin Gill ‘11G
InSight: RIVIER ACADEMIC JOURNAL, VOLUME 14, NUMBER 1, FALL 2018 EXPLORING THE UNIVERSE: Meet Kevin Gill ‘11G Michelle Marrone (From Rivier Today, Fall 2018) From the comfort of his lab chair in sunny, southern California, Kevin Gill ’11G has a view into outer space. As a Science Data Software Engineer at NASA’s Jet Propulsion Laboratory (JPL), he spends his time planning and designing technology in support of environmental science and space exploration, as well as data visualization and planetary imaging. His recent work not only produced the first-ever close views of Saturn, but also contributed to NASA’s team winning an Emmy Award. Kevin earned his M.S. in Computer Science at Rivier and has been designing software to render the unique images he gathers ever since. He used an algorithm he developed during his program at Rivier to generate hypothetical images portraying Mars as a vibrant planet with oceans, an oxygen-rich atmosphere, and a green biosphere. The images went viral and within a week his work was featured on major media networks—Discovery News, Fox News, Universe Today, and the Huffington Post. His work captured NASA’s attention and paved the way for his career move. “Rivier taught me many of the algorithms and development practices I still use today at NASA,” says Kevin. “In fact, I can trace the lineage of code currently running on NASA systems directly to my final master’s project at the University.” The systems and tools he develops support a range of scientists specializing in the areas of climate, oceanography, asteroids, planetary science, and others. -
Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
PUTTING LIFE on MARS: Using Computer Graphics to Render a Living Mars
InSight: RIVIER ACADEMIC JOURNAL, VOLUME 9, NUMBER 1, SPRING 2013 PUTTING LIFE ON MARS: Using Computer Graphics to Render a Living Mars Kevin M. Gill ‘11G* Senior Software Engineer, Thunderhead.com, Manchester, NH Keywords: Computer Graphics, Mars, Life, Planetary Science, OpenGL Abstract This article describes the software, algorithms & decisions that went into the development of the Living Mars image project. This includes topics related to computer graphics, software development, astronomy, & planetary science. The purpose of the project was to create a visualization of the planet Mars as could look with a living biosphere. This makes no distinction as to whether this biosphere would represent an ancient or future, possibly terraformed planet. 1 Background Mars, named for the Roman god of war. Ancient civilizations have forever associated the planet with fear, war, and destruction. It is the color of blood, and “one of a handful of planets visible to the naked eye, and the only one of marked color, so the planet demanded attention (Pyle, 2012).” Ever since man has noticed it, there have been dreams and visions of life on Mars, from Giovanni Schiaparelli and Percival Lowell describing channels and canals to Robert A. Heinlein’s science fiction. Lowell, in particular famous for fantastic writings of Mars, asked “are physical forces alone at work there, or has evolution begotten something more complex, something not unakin to what we know on Earth as life?” (Lowell, 1895) Even more recent discoveries by NASA’s Curiosity rover have found proof that liquid water once flowed billions of years ago positing an environment that could have served host to life (Brown, 2013). -
May 2016 | Volume 15, Issue 01 | Boeing.Com/Frontiers
MAY 2016 | VOLUME 15, ISSUE 01 | BOEING.COM/FRONTIERS Solar revolution Spectrolab employees are powering the future— with sunshine MAY 2016 | 01 TABLE OF CONTENTS 12 06 Leadership Message 08 Snapshot 09 Quotables 10 Historical Perspective PHOTO: BOB FERGUSON | BOEING 12 Sweating the metal Go behind the scenes of the ongoing 737 MAX flight-test program, where the aircraft are pushed to the limit, and then some. 18 18 Desert bloom In the high desert of New Mexico, at Boeing’s site in Albuquerque, scientists and engineers are continually looking for ways to enhance modern civilization and military technologies. And at the nearby Starfire Optical Range, Boeing and the U.S. Air Force are jointly experimenting with lasers to better monitor man-made objects in orbit, much of it space debris. 28 Solar explorer A wholly owned Boeing subsidiary, Spectrolab has provided electric power to more than 600 satellites and delivered more than 4 million PHOTO: BOB FERGUSON | BOEING solar cells for communications, science and defense needs. It also provides 80 percent of the helicopter-mounted searchlights used 38 by U.S. law enforcement. 34 Great and small The Boeing AH-6 Little Bird, a light attack and reconnaissance helicopter, packs a lot of capability for its size. It is made at the Boeing site in Mesa, Ariz., alongside the bigger Apache. 38 Irish eyes are smiling Ryanair recently took delivery of its 400th 737-800, and a writer and photographer from Frontiers were on board for the flight to Ireland. 44 Strike dynasty Boeing’s new Harpoon Block II Plus is a network-enabled variant that can receive and transmit communications while in flight, allowing it to change course to strike a different target, even a moving target. -
Widespread Crater-Related Pitted Materials on Mars: Further Evidence for the Role of Target Volatiles During the Impact Process ⇑ Livio L
Icarus 220 (2012) 348–368 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Widespread crater-related pitted materials on Mars: Further evidence for the role of target volatiles during the impact process ⇑ Livio L. Tornabene a, , Gordon R. Osinski a, Alfred S. McEwen b, Joseph M. Boyce c, Veronica J. Bray b, Christy M. Caudill b, John A. Grant d, Christopher W. Hamilton e, Sarah Mattson b, Peter J. Mouginis-Mark c a University of Western Ontario, Centre for Planetary Science and Exploration, Earth Sciences, London, ON, Canada N6A 5B7 b University of Arizona, Lunar and Planetary Lab, Tucson, AZ 85721-0092, USA c University of Hawai’i, Hawai’i Institute of Geophysics and Planetology, Ma¯noa, HI 96822, USA d Smithsonian Institution, Center for Earth and Planetary Studies, Washington, DC 20013-7012, USA e NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA article info abstract Article history: Recently acquired high-resolution images of martian impact craters provide further evidence for the Received 28 August 2011 interaction between subsurface volatiles and the impact cratering process. A densely pitted crater-related Revised 29 April 2012 unit has been identified in images of 204 craters from the Mars Reconnaissance Orbiter. This sample of Accepted 9 May 2012 craters are nearly equally distributed between the two hemispheres, spanning from 53°Sto62°N latitude. Available online 24 May 2012 They range in diameter from 1 to 150 km, and are found at elevations between À5.5 to +5.2 km relative to the martian datum. The pits are polygonal to quasi-circular depressions that often occur in dense clus- Keywords: ters and range in size from 10 m to as large as 3 km. -
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CICHLIFORMES: Cichlidae (part 3) · 1 The ETYFish Project © Christopher Scharpf and Kenneth J. Lazara COMMENTS: v. 6.0 - 30 April 2021 Order CICHLIFORMES (part 3 of 8) Family CICHLIDAE Cichlids (part 3 of 7) Subfamily Pseudocrenilabrinae African Cichlids (Haplochromis through Konia) Haplochromis Hilgendorf 1888 haplo-, simple, proposed as a subgenus of Chromis with unnotched teeth (i.e., flattened and obliquely truncated teeth of H. obliquidens); Chromis, a name dating to Aristotle, possibly derived from chroemo (to neigh), referring to a drum (Sciaenidae) and its ability to make noise, later expanded to embrace cichlids, damselfishes, dottybacks and wrasses (all perch-like fishes once thought to be related), then beginning to be used in the names of African cichlid genera following Chromis (now Oreochromis) mossambicus Peters 1852 Haplochromis acidens Greenwood 1967 acies, sharp edge or point; dens, teeth, referring to its sharp, needle-like teeth Haplochromis adolphifrederici (Boulenger 1914) in honor explorer Adolf Friederich (1873-1969), Duke of Mecklenburg, leader of the Deutsche Zentral-Afrika Expedition (1907-1908), during which type was collected Haplochromis aelocephalus Greenwood 1959 aiolos, shifting, changing, variable; cephalus, head, referring to wide range of variation in head shape Haplochromis aeneocolor Greenwood 1973 aeneus, brazen, referring to “brassy appearance” or coloration of adult males, a possible double entendre (per Erwin Schraml) referring to both “dull bronze” color exhibited by some specimens and to what -
Mitochondrial ND2 Phylogeny of Tilapiines and the Evolution of Parental Care Systems in the African Cichlid Fishes
What, if Anything, is a Tilapia?ÐMitochondrial ND2 Phylogeny of Tilapiines and the Evolution of Parental Care Systems in the African Cichlid Fishes Vera Klett and Axel Meyer Department of Biology, University of Konstanz, Germany We estimated a novel phylogeny of tilapiine cichlid ®sh (an assemblage endemic to Africa and the Near East) within the African cichlid ®shes on the basis of complete mitochondrial NADH dehydrogenase subunit 2 (ND2) gene sequences. The ND2 (1,047 bp) gene was sequenced in 39 tilapiine cichlids (38 species and 1 subspecies) and in an additional 14 nontilapiine cichlid species in order to evaluate the traditional morphologically based hypothesis of the respective monophyly of the tilapiine and haplochromine cichlid ®sh assemblages. The analyses included many additional cichlid lineages, not only the so-called tilapiines, but also lineages from Lake Tanganyika, east Africa, the Neotropics and an out-group from Madagascar with a wide range of parental care and mating systems. Our results suggest, in contrast to the historical morphology-based hypotheses from Regan (1920, 1922), Trewavas (1983), and Stiassny (1991), that the tilapiines do not form a monophyletic group because there is strong evidence that the genus Tilapia is not monophyletic but divided into at least ®ve distinct groups. In contrast to this ®nding, an allozyme analysis of Pouyaud and AgneÁse (1995), largely based on the same samples as used here, found a clustering of the Tilapia species into only two groups. This discrepancy is likely caused by the difference in resolution power of the two marker systems used. Our data suggest that only type species Tilapia sparrmanii Smith (1840) should retain the genus name Tilapia. -
Bethany L. Ehlmann California Institute of Technology 1200 E. California Blvd. MC 150-21 Pasadena, CA 91125 USA Ehlmann@Caltech
Bethany L. Ehlmann California Institute of Technology [email protected] 1200 E. California Blvd. Caltech office: +1 626.395.6720 MC 150-21 JPL office: +1 818.354.2027 Pasadena, CA 91125 USA Fax: +1 626.568.0935 EDUCATION Ph.D., 2010; Sc. M., 2008, Brown University, Geological Sciences (advisor, J. Mustard) M.Sc. by research, 2007, University of Oxford, Geography (Geomorphology; advisor, H. Viles) M.Sc. with distinction, 2005, Univ. of Oxford, Environ. Change & Management (advisor, J. Boardman) A.B. summa cum laude, 2004, Washington University in St. Louis (advisor, R. Arvidson) Majors: Earth & Planetary Sciences, Environmental Studies; Minor: Mathematics International Baccalaureate Diploma, Rickards High School, Tallahassee, Florida, 2000 Additional Training: Nordic/NASA Summer School: Water, Ice and the Origin of Life in the Universe, Iceland, 2009 Vatican Observatory Summer School in Astronomy &Astrophysics, Castel Gandolfo, Italy, 2005 Rainforest to Reef Program: Marine Geology, Coastal Sedimentology, James Cook Univ., Australia, 2004 School for International Training, Development and Conservation Program, Panamá, Sept-Dec 2002 PROFESSIONAL EXPERIENCE Professor of Planetary Science, Division of Geological & Planetary Sciences, California Institute of Technology, Assistant Professor 2011-2017, Professor 2017-present; Associate Director, Keck Institute for Space Studies 2018-present Research Scientist, Jet Propulsion Laboratory, California Institute of Technology, 2011-2020 Lunar Trailblazer, Principal Investigator, 2019-present MaMISS -
Copyright by Ashley Lynn Busby 2013
Copyright by Ashley Lynn Busby 2013 The Dissertation Committee for Ashley Lynn Busby Certifies that this is the approved version of the following dissertation: PICTURING THE COSMOS: SURREALISM, ASTRONOMY, ASTROLOGY, AND THE TAROT, 1920S-1940S Committee: Linda Dalrymple Henderson, Supervisor Richard Shiff John R. Clarke Bruce J. Hunt Kimberly A. Smith PICTURING THE COSMOS: SURREALISM, ASTRONOMY, ASTROLOGY, AND THE TAROT, 1920S-1940S by Ashley Lynn Busby, B.A.; M.A. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin December 2013 Dedication To JWB Acknowledgements First, I want to thank my dissertation committee for their support of this project. John Clarke, Richard Shiff, and Bruce Hunt have helped shape my scholarly development since my arrival at the University of Texas. I am also very grateful for Kimberly Smith’s continued guidance and encouragement. During my undergraduate study at Southwestern University, her dedication to her students inspired me to pursue graduate work, and I continue to look to her as a teaching role model. As an advisor, Linda Henderson has been exemplary during my time at the university. Her scholarship on the intersections between art and science has helped show me the possibilities for my own work in this area. In addition to research pursued in the library and collections at the University of Texas at Austin, I spent the summer of 2008 completing research at the Bibliothèque nationale de France. Funding from the College of Fine Arts at the University of Texas at Austin, the Department of Art and Art History, the M.K. -
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CICHLIFORMES: Cichlidae (part 5) · 1 The ETYFish Project © Christopher Scharpf and Kenneth J. Lazara COMMENTS: v. 10.0 - 11 May 2021 Order CICHLIFORMES (part 5 of 8) Family CICHLIDAE Cichlids (part 5 of 7) Subfamily Pseudocrenilabrinae African Cichlids (Palaeoplex through Yssichromis) Palaeoplex Schedel, Kupriyanov, Katongo & Schliewen 2020 palaeoplex, a key concept in geoecodynamics representing the total genomic variation of a given species in a given landscape, the analysis of which theoretically allows for the reconstruction of that species’ history; since the distribution of P. palimpsest is tied to an ancient landscape (upper Congo River drainage, Zambia), the name refers to its potential to elucidate the complex landscape evolution of that region via its palaeoplex Palaeoplex palimpsest Schedel, Kupriyanov, Katongo & Schliewen 2020 named for how its palaeoplex (see genus) is like a palimpsest (a parchment manuscript page, common in medieval times that has been overwritten after layers of old handwritten letters had been scraped off, in which the old letters are often still visible), revealing how changes in its landscape and/or ecological conditions affected gene flow and left genetic signatures by overwriting the genome several times, whereas remnants of more ancient genomic signatures still persist in the background; this has led to contrasting hypotheses regarding this cichlid’s phylogenetic position Pallidochromis Turner 1994 pallidus, pale, referring to pale coloration of all specimens observed at the time; chromis, a name -
A Small Cichlid Species Flock from the Upper Miocene (9–10 MYA)
Hydrobiologia https://doi.org/10.1007/s10750-020-04358-z (0123456789().,-volV)(0123456789().,-volV) ADVANCES IN CICHLID RESEARCH IV A small cichlid species flock from the Upper Miocene (9–10 MYA) of Central Kenya Melanie Altner . Bettina Reichenbacher Received: 22 March 2020 / Revised: 16 June 2020 / Accepted: 13 July 2020 Ó The Author(s) 2020 Abstract Fossil cichlids from East Africa offer indicate that they represent an ancient small species unique insights into the evolutionary history and flock. Possible modern analogues of palaeolake Waril ancient diversity of the family on the African conti- and its species flock are discussed. The three species nent. Here we present three fossil species of the extinct of Baringochromis may have begun to subdivide haplotilapiine cichlid Baringochromis gen. nov. from their initial habitat by trophic differentiation. Possible the upper Miocene of the palaeolake Waril in Central sources of food could have been plant remains and Kenya, based on the analysis of a total of 78 articulated insects, as their fossilized remains are known from the skeletons. Baringochromis senutae sp. nov., B. same place where Baringochromis was found. sonyii sp. nov. and B. tallamae sp. nov. are super- ficially similar, but differ from each other in oral-tooth Keywords Cichlid fossils Á Pseudocrenilabrinae Á dentition and morphometric characters related to the Palaeolake Á Small species flock Á Late Miocene head, dorsal fin base and body depth. These findings Guest editors: S. Koblmu¨ller, R. C. Albertson, M. J. Genner, Introduction K. M. Sefc & T. Takahashi / Advances in Cichlid Research IV: Behavior, Ecology and Evolutionary Biology. The tropical freshwater fish family Cichlidae and its Electronic supplementary material The online version of estimated 2285 species is famous for its high degree of this article (https://doi.org/10.1007/s10750-020-04358-z) con- phenotypic diversity, trophic adaptations and special- tains supplementary material, which is available to authorized users.