Earth's Stratosphere and Microbial Life
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CARI-7 Documentation: Radiation Transport in the Atmosphere
DOT/FAA/AM-21/5 Office of Aerospace Medicine Washington, DC 20591 CARI Documentation: Radiation Transport in the Atmosphere Kyle Copeland Civil Aerospace Medical Institute Federal Aviation Administration Oklahoma City, OK 73125Location/Address March 2021 Final Report NOTICE This document is disseminated under the sponsorship of the U.S. Department of Transportation in the interest of information exchange. The United States Government assumes no liability for the contents thereof. _________________ This publication and all Office of Aerospace Medicine technical reports are available in full-text from the Civil Aerospace Medical Institute’s publications Web site: (www.faa.gov/go/oamtechreports) Technical Report Documentation Page 1. Report No. 2. Government Accession No. 3. Recipient's Catalog No. DOT/FAA/AM-21/5 4. Title and Subtitle 5. Report Date CARI-7 DOCUMENTATION: RADIATION TRANSPORT IN March 2021 THE ATMOSPHERE 6. Performing Organization Code 7. Author(s) 8. Performing Organization Report No. Copeland, K. 9. Performing Organization Name and Address 10. Work Unit No. (TRAIS) Civil Aerospace Medical Institute FAA 11. Contract or Grant No. 12. Sponsoring Agency name and Address 13. Type of Report and Period Covered Office of Aerospace Medicine Federal Aviation Administration 800 Independence Ave., S.W. Washington, DC 20591 14. Sponsoring Agency Code 15. Supplemental Notes 16. Abstract Primary cosmic radiation from both the Sun and interstellar space enters Earth's atmosphere in varying amounts. Outside of Earth's atmosphere, cosmic radiation is modulated by solar activity and Earth's magnetic field. Once the radiation enters Earth's atmosphere, it interacts with Earth's atmosphere in the same manner regardless of its point of origin (solar or galactic). -
Global Ionosphere-Thermosphere-Mesosphere (ITM) Mapping Across Temporal and Spatial Scales a White Paper for the NRC Decadal
Global Ionosphere-Thermosphere-Mesosphere (ITM) Mapping Across Temporal and Spatial Scales A White Paper for the NRC Decadal Survey of Solar and Space Physics Andrew Stephan, Scott Budzien, Ken Dymond, and Damien Chua NRL Space Science Division Overview In order to fulfill the pressing need for accurate near-Earth space weather forecasts, it is essential that future measurements include both temporal and spatial aspects of the evolution of the ionosphere and thermosphere. A combination of high altitude global images and low Earth orbit altitude profiles from simple, in-the-medium sensors is an optimal scenario for creating continuous, routine space weather maps for both scientific and operational interests. The method presented here adapts the vast knowledge gained using ultraviolet airglow into a suggestion for a next-generation, near-Earth space weather mapping network. Why the Ionosphere, Thermosphere, and Mesosphere? The ionosphere-thermosphere-mesosphere (ITM) region of the terrestrial atmosphere is a complex and dynamic environment influenced by solar radiation, energy transfer, winds, waves, tides, electric and magnetic fields, and plasma processes. Recent measurements showing how coupling to other regions also influences dynamics in the ITM [e.g. Immel et al., 2006; Luhr, et al, 2007; Hagan et al., 2007] has exposed the need for a full, three- dimensional characterization of this region. Yet the true level of complexity in the ITM system remains undiscovered primarily because the fundamental components of this region are undersampled on the temporal and spatial scales that are necessary to expose these details. The solar and space physics research community has been driven over the past decade toward answering scientific questions that have a high level of practical application and relevance. -
A Moderately Boron-Tolerant Candidatus Novel Soil Bacterium Lysinibacillus Pakistanensis Sp
Pak. J. Bot., 45(SI): 41-50, January 2013. A MODERATELY BORON-TOLERANT CANDIDATUS NOVEL SOIL BACTERIUM LYSINIBACILLUS PAKISTANENSIS SP. NOV. CAND., ISOLATED FROM SOYBEAN (GLYCINE MAX L.) RHIZOSPHERE RIFAT HAYAT1,2,3*, IFTIKHAR AHMED2*, JAYOUNG PAEK4, MUHAMMAD EHSAN1, 2, MUHAMMAD IQBAL2 AND YOUNG H. CHANG4* 1Department of Soil Science & SWC, PMAS Arid Agriculture University, Rawalpindi, 46300, Pakistan 2Plant Biotechnology Program, National Institute for Genomics and Advanced Biotechnology (NIGAB), National Agricultural Research Center (NARC), Park Road, Islamabad-45500, Pakistan 3Institute of Molecular and Cellular Biosciences, The University of Tokyo, Yayoi 1-1-1, Bunkyo-ku, Tokyo 113-8657, Japan 4Korean Collection of Type Cultures, Biological Resource Center, KRIBB, 52 Oeundong, Daejeon 305-806, Republic of Korea *Correspondence E-mail: [email protected]; [email protected]; [email protected] Abstract A Gram-positive, motile, rod-shaped, endospore-forming and moderately boron (B) tolerant novel candidatus strain, designated as NCCP-54T, was isolated from rhizospheric soil of soybean (Glycine max L.) sampled from the experimental area of Research Farm, PMAS Arid Agriculture University, Rawalpindi, Pakistan. To delineate its taxonomic position, the strain was subject to polyphasic characterization. Cells of the strain NCCP-54T can grow at 10-45○C (optimum at 28○C) at pH ranges of 6.5-9.0 (optimum at pH 7.0) and in 0-6% NaCl (w/v) in tryptic soya agar medium. It can also tolerate 150 mM boric acid in agar medium; however, optimum growth occurs in the absence of boric acid. Based on 16S rRNA gene sequence analysis, strain NCCP-54T showed highest similarity to Lysinibacillus xylanilyticus KCTC13423T (99.1%), Lysinibacillus fusiformis KCTC3454T (98.5%), Lysinibacillus boronitolerans KCTC13709T (98.4%), Lysinibacillus parviboronicapiens KCTC13154T (97.8%), and Lysinibacillus sphaericus KCTC3346T (97.5%) and less than 97% with other closely related taxa. -
Marina Galand
Thermosphere - Ionosphere - Magnetosphere Coupling! Canada M. Galand (1), I.C.F. Müller-Wodarg (1), L. Moore (2), M. Mendillo (2), S. Miller (3) , L.C. Ray (1) (1) Department of Physics, Imperial College London, London, U.K. (2) Center for Space Physics, Boston University, Boston, MA, USA (3) Department of Physics and Astronomy, University College London, U.K. 1." Energy crisis at giant planets Credit: NASA/JPL/Space Science Institute 2." TIM coupling Cassini/ISS (false color) 3." Modeling of IT system 4." Comparison with observaons Cassini/UVIS 5." Outstanding quesAons (Pryor et al., 2011) SATURN JUPITER (Gladstone et al., 2007) Cassini/UVIS [UVIS team] Cassini/VIMS (IR) Credit: J. Clarke (BU), NASA [VIMS team/JPL, NASA, ESA] 1. SETTING THE SCENE: THE ENERGY CRISIS AT THE GIANT PLANETS THERMAL PROFILE Exosphere (EARTH) Texo 500 km Key transiLon region Thermosphere between the space environment and the lower atmosphere Ionosphere 85 km Mesosphere 50 km Stratosphere ~ 15 km Troposphere SOLAR ENERGY DEPOSITION IN THE UPPER ATMOSPHERE Solar photons ion, e- Neutral Suprathermal electrons B ion, e- Thermal e- Ionospheric Thermosphere Ne, Nion e- heang Te P, H * + Airglow Neutral atmospheric Exothermic reacAons heang IS THE SUN THE MAIN ENERGY SOURCE OF PLANERATY THERMOSPHERES? W Main energy source: UV solar radiaon Main energy source? EartH Outer planets CO2 atmospHeres Exospheric temperature (K) [aer Mendillo et al., 2002] ENERGY CRISIS AT THE GIANT PLANETS Observed values at low to mid-latudes solsce equinox Modeled values (Sun only) [Aer -
Stratosphere-Troposphere Coupling: a Method to Diagnose Sources of Annular Mode Timescales
STRATOSPHERE-TROPOSPHERE COUPLING: A METHOD TO DIAGNOSE SOURCES OF ANNULAR MODE TIMESCALES Lawrence Mudryklevel, Paul Kushner p R ! ! SPARC DynVar level, Z(x,p,t)=− T (x,p,t)d ln p , (4) g !ps x,t p ( ) R ! ! Z(x,p,t)=− T (x,p,t)d ln p , (4) where p is the pressure at the surface, R is the specific gas constant and g is the gravitational acceleration s g !ps(x,t) where p is the pressure at theat surface, the surface.R is the specific gas constant and g is the gravitational acceleration Abstract s Geopotentiallevel, Height Decomposition Separation of AM Timescales p R ! ! at the surface. This time-varying geopotentialZ( canx,p,t be)= decomposed− T into(x,p a,t cli)dmatologyln p , and anomalies from the(4) climatology AM timescales track seasonal variations in the AM index’s decorrelation time6,7. For a hydrostatic fluid, geopotential height may be describedg !p sas(x ,ta) function of time, pressure level Timescales derived from Annular Mode (AM) variability provide dynamical and ashorizontalZ(x,p,t position)=Z (asx,p a )+temperatureδZ(x,p,t integral). Decomposing from the Earth’s the temperature surface to a andgiven surface pressure pressure fields inananalogous insight into stratosphere-troposphere coupling and are linked to the strengthThis of time-varying level, geopotentialwhere can beps is decomposed the pressure at into the a surface, climatologyR is the and specific anomalies gas constant from and theg is climatology the gravitational acceleration NCEP, 1958-2007 level: ^ a) o (yL ) d) o AM responses to climate forcings. -
Hohonu Volume 5 (PDF)
HOHONU 2007 VOLUME 5 A JOURNAL OF ACADEMIC WRITING This publication is available in alternate format upon request. TheUniversity of Hawai‘i is an Equal Opportunity Affirmative Action Institution. VOLUME 5 Hohonu 2 0 0 7 Academic Journal University of Hawai‘i at Hilo • Hawai‘i Community College Hohonu is publication funded by University of Hawai‘i at Hilo and Hawai‘i Community College student fees. All production and printing costs are administered by: University of Hawai‘i at Hilo/Hawai‘i Community College Board of Student Publications 200 W. Kawili Street Hilo, Hawai‘i 96720-4091 Phone: (808) 933-8823 Web: www.uhh.hawaii.edu/campuscenter/bosp All rights revert to the witers upon publication. All requests for reproduction and other propositions should be directed to writers. ii d d d d d d d d d d d d d d d d d d d d d d Table of Contents 1............................ A Fish in the Hand is Worth Two on the Net: Don’t Make me Think…different, by Piper Seldon 4..............................................................................................Abortion: Murder-Or Removal of Tissue?, by Dane Inouye 9...............................An Etymology of Four English Words, with Reference to both Grimm’s Law and Verner’s Law by Piper Seldon 11................................Artifacts and Native Burial Rights: Where do We Draw the Line?, by Jacqueline Van Blarcon 14..........................................................................................Ayahuasca: Earth’s Wisdom Revealed, by Jennifer Francisco 16......................................Beak of the Fish: What Cichlid Flocks Reveal About Speciation Processes, by Holly Jessop 26................................................................................. Climatic Effects of the 1815 Eruption of Tambora, by Jacob Smith 33...........................Columnar Joints: An Examination of Features, Formation and Cooling Models, by Mary Mathis 36.................... -
Bacillus Safensis FO-36B and Bacillus Pumilus SAFR-032: a Whole Genome Comparison of Two Spacecraft Assembly Facility Isolates
bioRxiv preprint doi: https://doi.org/10.1101/283937; this version posted April 24, 2018. The copyright holder for this preprint (which was not certified by peer review) is the author/funder. All rights reserved. No reuse allowed without permission. 1 Bacillus safensis FO-36b and Bacillus pumilus SAFR-032: A Whole Genome 2 Comparison of Two Spacecraft Assembly Facility Isolates 3 Madhan R Tirumalai1, Victor G. Stepanov1, Andrea Wünsche1, Saied Montazari1, 4 Racquel O. Gonzalez1, Kasturi Venkateswaran2, George. E. Fox1§ 5 1Department of Biology and Biochemistry, University of Houston, Houston, TX, 77204-5001. 6 2 Biotechnology & Planetary Protection Group, NASA Jet Propulsion Laboratories, California 7 Institute of Technology, Pasadena, CA, 91109. 8 9 §Corresponding author: 10 Dr. George E. Fox 11 Dept. Biology & Biochemistry 12 University of Houston, Houston, TX 77204-5001 13 713-743-8363; 713-743-8351 (FAX); email: [email protected] 14 15 Email addresses: 16 MRT: [email protected] 17 VGS: [email protected] 18 AW: [email protected] 19 SM: [email protected] 20 ROG: [email protected] 21 KV: [email protected] 22 GEF: [email protected] 1 bioRxiv preprint doi: https://doi.org/10.1101/283937; this version posted April 24, 2018. The copyright holder for this preprint (which was not certified by peer review) is the author/funder. All rights reserved. No reuse allowed without permission. 23 Keywords: Planetary protection, Bacillus endospores, extreme radiation resistance, peroxide 24 resistance, genome comparison, phage insertions 25 26 Background 27 Microbial persistence in built environments such as spacecraft cleanroom facilities [1-3] is often 28 characterized by their unusual resistances to different physical and chemical factors [1, 4-7]. -
Bioprospection of Cellulolytic and Lipolytic South Atlantic Deep-Sea Bacteria
Electronic Journal of Biotechnology ISSN: 0717-3458 http://www.ejbiotechnology.info DOI: 10.2225/vol15-issue5-fulltext-17 RESEARCH ARTICLE Bioprospection of cellulolytic and lipolytic South Atlantic deep-sea bacteria Estácio Jussie Odisi1 · Marcela Bruschi Silvestrin1 · Rodrigo Yoji Uwamori Takahashi1 · Marcus Adonai Castro da Silva1 · André Oliveira de Souza Lima1 1 Universidade do Vale do Itajaí, Centro de Ciências Tecnológicas da Terra e do Mar, Itajaí, SC, Brazil Corresponding author: [email protected] Received June 6, 2012 / September 3, 2012 Published online: September 15, 2012 © 2012 by Pontificia Universidad Católica de Valparaíso, Chile Abstract Background: Cellulases and lipases have broad industrial application, which calls for an urgent exploration of microorganisms from extreme environments as valuable source of commercial enzyme. In this context, the present work describes the bioprospection and identification of deep-sea bacteria that produce cellulases and lipases, as well their optimal temperature of activity. Results: The first step of this study was the screening of cellulolytic and lipolytic deep-sea bacteria from sediment and water column, which was conducted with substrates linked with 4-Methylumbelliferyl. Among the 161 strains evaluated, 40 were cellulolytic, 23 were lipolytic and 5 exhibited both activities. Cellulolytic and lipolytic bacteria are more common in sediment than at the water column. Based on the ability to produce cellulases and lipases three isolates were selected and identified (16S rRNA sequencing) as Bacillus stratosphericus, B. aerophilus and B. pumilus. Lipases of strain B. aerophilus LAMA 582 exhibited activity at a wide temperature range (4º to 37ºC) and include psychrophilic behaviour. Strain Bacillus stratosphericus LAMA 585 can growth in a rich (Luria Bertani) and minimal (Marine Minimal) medium, and does not need an inducer to produce its mesophilic cellulases and lipases. -
Summary of a Program Review Held at Huntsville, Alabama October 19-21, 1982
Summary of a program review held at Huntsville, Alabama October 19-21, 1982 - TECH LIBRARY KAFEI, NM lllllllsllllllRlRllffllilrml OOSSE!?b NASA Conference Publication 2259 NASA/MSFCFY-82 Atmospheric Processes Research Review Compiled by Robert E. Turner George C. Marshall Space Flight Center Marshall Space Flight Center, Alabama Summary of a program review held at Huntsville, Alabama October 19-21, 1982 National Aeronautics and Space Administration Sclontlflc and Tochnlcal InformatIon Branch 1983 ACKNOWLEDGMENTS The productive inputs and comments from the participants and attendees in the Atmospheric Processes Research Review contributed very much to the success of the review. The opportunity provided for everyone to become better acquainted with the work of other investigators and to see how the research relates to the overall objective of NASA's Atmospheric Processes Research Program was an important aspect of the review. Appreciation is expressed to all those who participated in the review. The organizers trust that participation will provide each with a better frame of reference from which to proceed with the next year's research activities. ii PREFACE Each year NASA supports research in various disciplinary program areas. The coordination and exchange of information among those sponsored by NASA to conduct research studies are important elements of each program. The Office of Space Science and Applications and the Office of Aeronautics and Space Technology, via Announcements of Opportunity (AO), Application Notices (AN),etc., invites interested investigators throughout the country to communicate their research ideas within NASA and in institutions. The proposals in the Atmospheric Processes Research area selected and assigned to the NASA Marshall Space Flight Center's (MSFC's) Atmospheric Sciences Division for technical monitorship, together with the research efforts included in the FY-82 MSFC Research and Technology Operating Plan (RTOP1 I are the source of principal focus for the NASA/MSFC FY-82 Atmospheric Processes Research Review. -
The Stratopause Evolution During Different Types of Sudden Stratospheric Warming Event
Clim Dyn DOI 10.1007/s00382-014-2292-4 The stratopause evolution during different types of sudden stratospheric warming event Etienne Vignon · Daniel M. Mitchell Received: 18 February 2014 / Accepted: 5 August 2014 © The Author(s) 2014. This article is published with open access at Springerlink.com Abstract Recent work has shown that the vertical struc- Keywords Stratopause · Sudden stratospheric warming · ture of the Arctic polar vortex during different types of MERRA data · Polar vortex · sudden stratospheric warming (SSW) events can be very Middle atmospheric circulation distinctive. Specifically, SSWs can be classified into polar vortex displacement events or polar vortex splitting events. This paper aims to study the Arctic stratosphere during 1 Introduction such events, with a focus on the stratopause using the Mod- ern Era-Restrospective analysis for Research and Applica- The stratopause is characterised by a reversal of the atmos- tions reanalysis data set. The reanalysis dataset is compared pheric lapse rate at around 50 km (~1 hPa). While strato- against two independent satellite reconstructions for valida- spheric ozone heating is responsible for the stratopause pres- tion purposes. During vortex displacement events, the strat- ence at sunlit latitudes, westward gravity wave drag (and to opause temperature and pressure exhibit a wave-1 structure a lesser extent, stationary gravity wave drag) maintains the and are in quadrature whereas during vortex splitting events stratopause in the polar night jet (Hitchman et al. 1989). they exhibit a wave-2 structure. For both types of SSW the Indeed, the westward and stationary gravity wave (GW) temperature anomalies at the stratopause are shown to be breaking induces a mesospheric meridional flow toward the generated by ageostrophic vertical motions. -
A DNA Ligase from the Psychrophile Pseudoalteromonas Haloplanktis Gives Insights Into the Adaptation of Proteins to Low Temperatures
Eur. J. Biochem. 267, 3502±3512 (2000) q FEBS 2000 A DNA ligase from the psychrophile Pseudoalteromonas haloplanktis gives insights into the adaptation of proteins to low temperatures D. Georlette1,Z.O.JoÂnsson2,3, F. Van Petegem4, J.-P. Chessa1, J. Van Beeumen4,U.HuÈ bscher2 and C. Gerday1 1Laboratory of Biochemistry, Institute of Chemistry, B6a Universite de LieÁge, Sart-Tilman, Belgium; 2Institute of Veterinary Biochemistry, UniversitaÈtZuÈrich-Irchel, ZuÈrich, Switzerland; 3Department of Pathology, Brigham & Women's Hospital, Boston, MA, USA; 4Laboratory for Protein Biochemistry and Protein Engineering, Department of Biochemistry Physiology and Microbiology, Gent, Belgium The cloning, overexpression and characterization of a cold-adapted DNA ligase from the Antarctic sea water bacterium Pseudoalteromonas haloplanktis are described. Protein sequence analysis revealed that the cold- adapted Ph DNA ligase shows a significant level of sequence similarity to other NAD1-dependent DNA ligases and contains several previously described sequence motifs. Also, a decreased level of arginine and proline residues in Ph DNA ligase could be involved in the cold-adaptation strategy. Moreover, 3D modelling of the N-terminal domain of Ph DNA ligase clearly indicates that this domain is destabilized compared with its thermophilic homologue. The recombinant Ph DNA ligase was overexpressed in Escherichia coli and purified to homogeneity. Mass spectroscopy experiments indicated that the purified enzyme is mainly in an adenylated form with a molecular mass of 74 593 Da. Ph DNA ligase shows similar overall catalytic properties to other NAD1-dependent DNA ligases but is a cold-adapted enzyme as its catalytic efficiency (kcat/Km) at low and moderate temperatures is higher than that of its mesophilic counterpart E. -
ESSENTIALS of METEOROLOGY (7Th Ed.) GLOSSARY
ESSENTIALS OF METEOROLOGY (7th ed.) GLOSSARY Chapter 1 Aerosols Tiny suspended solid particles (dust, smoke, etc.) or liquid droplets that enter the atmosphere from either natural or human (anthropogenic) sources, such as the burning of fossil fuels. Sulfur-containing fossil fuels, such as coal, produce sulfate aerosols. Air density The ratio of the mass of a substance to the volume occupied by it. Air density is usually expressed as g/cm3 or kg/m3. Also See Density. Air pressure The pressure exerted by the mass of air above a given point, usually expressed in millibars (mb), inches of (atmospheric mercury (Hg) or in hectopascals (hPa). pressure) Atmosphere The envelope of gases that surround a planet and are held to it by the planet's gravitational attraction. The earth's atmosphere is mainly nitrogen and oxygen. Carbon dioxide (CO2) A colorless, odorless gas whose concentration is about 0.039 percent (390 ppm) in a volume of air near sea level. It is a selective absorber of infrared radiation and, consequently, it is important in the earth's atmospheric greenhouse effect. Solid CO2 is called dry ice. Climate The accumulation of daily and seasonal weather events over a long period of time. Front The transition zone between two distinct air masses. Hurricane A tropical cyclone having winds in excess of 64 knots (74 mi/hr). Ionosphere An electrified region of the upper atmosphere where fairly large concentrations of ions and free electrons exist. Lapse rate The rate at which an atmospheric variable (usually temperature) decreases with height. (See Environmental lapse rate.) Mesosphere The atmospheric layer between the stratosphere and the thermosphere.