Signature Properties of Water: Their Molecular Electronic Origins
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Ice Ic” Werner F
Extent and relevance of stacking disorder in “ice Ic” Werner F. Kuhsa,1, Christian Sippela,b, Andrzej Falentya, and Thomas C. Hansenb aGeoZentrumGöttingen Abteilung Kristallographie (GZG Abt. Kristallographie), Universität Göttingen, 37077 Göttingen, Germany; and bInstitut Laue-Langevin, 38000 Grenoble, France Edited by Russell J. Hemley, Carnegie Institution of Washington, Washington, DC, and approved November 15, 2012 (received for review June 16, 2012) “ ” “ ” A solid water phase commonly known as cubic ice or ice Ic is perfectly cubic ice Ic, as manifested in the diffraction pattern, in frequently encountered in various transitions between the solid, terms of stacking faults. Other authors took up the idea and liquid, and gaseous phases of the water substance. It may form, attempted to quantify the stacking disorder (7, 8). The most e.g., by water freezing or vapor deposition in the Earth’s atmo- general approach to stacking disorder so far has been proposed by sphere or in extraterrestrial environments, and plays a central role Hansen et al. (9, 10), who defined hexagonal (H) and cubic in various cryopreservation techniques; its formation is observed stacking (K) and considered interactions beyond next-nearest over a wide temperature range from about 120 K up to the melt- H-orK sequences. We shall discuss which interaction range ing point of ice. There was multiple and compelling evidence in the needs to be considered for a proper description of the various past that this phase is not truly cubic but composed of disordered forms of “ice Ic” encountered. cubic and hexagonal stacking sequences. The complexity of the König identified what he called cubic ice 70 y ago (11) by stacking disorder, however, appears to have been largely over- condensing water vapor to a cold support in the electron mi- looked in most of the literature. -
A Primer on Ice
A Primer on Ice L. Ridgway Scott University of Chicago Release 0.3 DO NOT DISTRIBUTE February 22, 2012 Contents 1 Introduction to ice 1 1.1 Lattices in R3 ....................................... 2 1.2 Crystals in R3 ....................................... 3 1.3 Comparingcrystals ............................... ..... 4 1.3.1 Quotientgraph ................................. 4 1.3.2 Radialdistributionfunction . ....... 5 1.3.3 Localgraphstructure. .... 6 2 Ice I structures 9 2.1 IceIh........................................... 9 2.2 IceIc........................................... 12 2.3 SecondviewoftheIccrystalstructure . .......... 14 2.4 AlternatingIh/Iclayeredstructures . ........... 16 3 Ice II structure 17 Draft: February 22, 2012, do not distribute i CONTENTS CONTENTS Draft: February 22, 2012, do not distribute ii Chapter 1 Introduction to ice Water forms many different crystal structures in its solid form. These provide insight into the potential structures of ice even in its liquid phase, and they can be used to calibrate pair potentials used for simulation of water [9, 14, 15]. In crowded biological environments, water may behave more like ice that bulk water. The different ice structures have different dielectric properties [16]. There are many crystal structures of ice that are topologically tetrahedral [1], that is, each water molecule makes four hydrogen bonds with other water molecules, even though the basic structure of water is trigonal [3]. Two of these crystal structures (Ih and Ic) are based on the same exact local tetrahedral structure, as shown in Figure 1.1. Thus a subtle understanding of structure is required to differentiate them. We refer to the tetrahedral structure depicted in Figure 1.1 as an exact tetrahedral structure. In this case, one water molecule is in the center of a square cube (of side length two), and it is hydrogen bonded to four water molecules at four corners of the cube. -
Vibrational Spectra of Light and Heavy Water with Application to Neutron Cross Section Calculations J
CORE Metadata, citation and similar papers at core.ac.uk Provided by CONICET Digital Vibrational spectra of light and heavy water with application to neutron cross section calculations J. I. Marquez Damian, D. C. Malaspina, and J. R. Granada Citation: J. Chem. Phys. 139, 024504 (2013); doi: 10.1063/1.4812828 View online: http://dx.doi.org/10.1063/1.4812828 View Table of Contents: http://jcp.aip.org/resource/1/JCPSA6/v139/i2 Published by the AIP Publishing LLC. Additional information on J. Chem. Phys. Journal Homepage: http://jcp.aip.org/ Journal Information: http://jcp.aip.org/about/about_the_journal Top downloads: http://jcp.aip.org/features/most_downloaded Information for Authors: http://jcp.aip.org/authors Downloaded 11 Jul 2013 to 200.0.233.52. This article is copyrighted as indicated in the abstract. Reuse of AIP content is subject to the terms at: http://jcp.aip.org/about/rights_and_permissions THE JOURNAL OF CHEMICAL PHYSICS 139, 024504 (2013) Vibrational spectra of light and heavy water with application to neutron cross section calculations J. I. Marquez Damian,1,a) D. C. Malaspina,2 and J. R. Granada1,b) 1Neutron Physics Department and Instituto Balseiro, Centro Atómico Bariloche, CNEA, Argentina 2Department of Biomedical Engineering and Chemistry of Life Processes Institute, Northwestern University, 2145 Sheridan Road, Evanston, Illinois 60208, USA (Received 4 June 2013; accepted 19 June 2013; published online 11 July 2013) The design of nuclear reactors and neutron moderators require a good representation of the interac- tion of low energy (E < 1 eV) neutrons with hydrogen and deuterium containing materials. These models are based on the dynamics of the material, represented by its vibrational spectrum. -
The Incredible Lightness of Water Vapor
1 The Incredible Lightness of Water Vapor ∗ 2 Da Yang and Seth Seidel 3 University of California, Davis 4 Lawrence Berkeley National Laboratory, Berkeley ∗ 5 Corresponding author address: Da Yang, 253 Hoagland Hall, Davis, CA 95616. 6 E-mail: [email protected] Generated using v4.3.2 of the AMS LATEX template 1 ABSTRACT 7 The molar mass of water vapor is significantly less than that of dry air. This 8 makes a moist parcel lighter than a dry parcel of the same temperature and 9 pressure. This effect is referred to as the vapor buoyancy effect and has of- 10 ten been overlooked in climate studies. We propose that this effect increases 11 Earth’s outgoing longwave radiation (OLR) and stabilizes Earth’s climate. 12 We illustrate this mechanism in an idealized tropical atmosphere, where there 13 is no horizontal buoyancy gradient in the free troposphere. To maintain the 14 uniform buoyancy distribution, temperature increases toward dry atmosphere 15 columns to compensate reduction of vapor buoyancy. The temperature differ- 16 ence between moist and dry columns would increase with climate warming 17 due to increasing atmospheric water vapor, leading to enhanced OLR and 18 thereby stabilizing Earth’s climate. We estimate that this feedback strength 2 19 is about O(0.2 W/m /K), which compares with cloud feedbacks and surface 20 albedo feedbacks in current climate. 2 21 1. Introduction 22 How fast would Earth’s climate respond to increasing CO2 (Manabe and Wetherald 1975; Flato 23 et al. 2013; Collins et al. 2013)? Why is tropical climate more stable than extratropical climate 24 (Holland and Bitz 2003; Polyakov et al. -
Jökulhlaups in Skaftá: a Study of a Jökul- Hlaup from the Western Skaftá Cauldron in the Vatnajökull Ice Cap, Iceland
Jökulhlaups in Skaftá: A study of a jökul- hlaup from the Western Skaftá cauldron in the Vatnajökull ice cap, Iceland Bergur Einarsson, Veðurstofu Íslands Skýrsla VÍ 2009-006 Jökulhlaups in Skaftá: A study of jökul- hlaup from the Western Skaftá cauldron in the Vatnajökull ice cap, Iceland Bergur Einarsson Skýrsla Veðurstofa Íslands +354 522 60 00 VÍ 2009-006 Bústaðavegur 9 +354 522 60 06 ISSN 1670-8261 150 Reykjavík [email protected] Abstract Fast-rising jökulhlaups from the geothermal subglacial lakes below the Skaftá caul- drons in Vatnajökull emerge in the Skaftá river approximately every year with 45 jökulhlaups recorded since 1955. The accumulated volume of flood water was used to estimate the average rate of water accumulation in the subglacial lakes during the last decade as 6 Gl (6·106 m3) per month for the lake below the western cauldron and 9 Gl per month for the eastern caul- dron. Data on water accumulation and lake water composition in the western cauldron were used to estimate the power of the underlying geothermal area as ∼550 MW. For a jökulhlaup from the Western Skaftá cauldron in September 2006, the low- ering of the ice cover overlying the subglacial lake, the discharge in Skaftá and the temperature of the flood water close to the glacier margin were measured. The dis- charge from the subglacial lake during the jökulhlaup was calculated using a hypso- metric curve for the subglacial lake, estimated from the form of the surface cauldron after jökulhlaups. The maximum outflow from the lake during the jökulhlaup is esti- mated as 123 m3 s−1 while the maximum discharge of jökulhlaup water at the glacier terminus is estimated as 97 m3 s−1. -
Computational Investigation of Surface Freezing in a Molecular Model Of
Computational investigation of surface freezing in a molecular model of water Amir Haji-Akbari ( )a,1 and Pablo G. Debenedettia,2 aDepartment of Chemical and Biological Engineering, Princeton University, Princeton, NJ 08544 Contributed by Pablo G. Debenedetti, February 17, 2017 (sent for review December 21, 2016; reviewed by Christoph Dellago and Angelos Michaelides) Water freezes in a wide variety of low-temperature environ- is therefore one of the major open challenges of atmospheric ments, from meteors and atmospheric clouds to soil and bio- sciences. logical cells. In nature, ice usually nucleates at or near inter- One major difficulty in constructing such predictive frame- faces, because homogenous nucleation in the bulk can only be works is the inability to determine the proper scaling of observed at deep supercoolings. Although the effect of proximal volumetric nucleation rates with the size of microdroplets and surfaces on freezing has been extensively studied, major gaps in nanodroplets that constitute clouds. This is practically impor- understanding remain regarding freezing near vapor–liquid inter- tant because atmospheric clouds are composed of droplets of faces, with earlier experimental studies being mostly inconclu- different sizes. This scaling is determined by whether freezing is sive. The question of how a vapor–liquid interface affects freez- enhanced or suppressed near vapor–liquid interfaces. If freezing ing in its vicinity is therefore still a major open question in ice is suppressed at a free interface, the effective volumetric nucle- physics. Here, we address this question computationally by using ation rate will be independent of r, the droplet radius, and bulk the forward-flux sampling algorithm to compute the nucleation freezing will be dominant at all sizes. -
Case Study: Water and Ice
Case Study: Water and Ice Timothy A. Isgro, Marcos Sotomayor, and Eduardo Cruz-Chu 1 The Universal Solvent Water is essential for sustaining life on Earth. Almost 75% of the Earth’s surface is covered by it. It composes roughly 70% of the human body by mass [1]. It is the medium associated with nearly all microscopic life pro- cesses. Much of the reason that water can sustain life is due to its unique properties. Among the most essential and extreme properties of water is its capabil- ity to absorb large amounts of heat. The heat capacity of water, which is the highest for compounds of its type in the liquid state, measures the amount of heat which needs to be added to water to change its temperature by a given amount. Water, thus, is able to effectively maintain its temperature even 1 when disturbed by great amounts of heat. This property serves to main- tain ocean temperatures, as well as the atmospheric temperature around the oceans. For example, when the sun rises in the morning and a large amount of heat strikes the surface of the Earth, the vast majority of it is absorbed by the ocean. The ocean water, however, does not exhibit a drastic increase in temperature that could make it inhospitable to life. In constrast, when the sun sets in the evening and that heat is taken away, the oceans do not become too cold to harbor life. Water also has high latent heats of vapor- ization and melting, which measure the amount of heat needed to change a certain amount of liquid water to vapor and ice to liquid, respectively. -
First International Conference on Mars Polar Science and Exploration
FIRST INTERNATIONAL CONFERENCE ON MARS POLAR SCIENCE AND EXPLORATION Held at The Episcopal Conference Center at Carnp Allen, Texas Sponsored by Geological Survey of Canada International Glaciological Society Lunar and Planetary Institute National Aeronautics and Space Administration Organizers Stephen Clifford, Lunar and Planetary Institute David Fisher, Geological Survey of Canada James Rice, NASA Ames Research Center LPI Contribution No. 953 Compiled in 1998 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the Universities Space Research Association under Contract No. NASW-4574 with the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. Abstracts in this volume may be cited as Author A. B. (1998) Title of abstract. In First International Conference on Mars Polar Science and Exploration, p. xx. LPI Contribution No. 953, Lunar and Planetary Institute, Houston. This report is distributed by ORDER DEPARTMENT Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1 113 Mail order requestors will be invoiced for the cost of shipping and handling. LPI Contribution No. 953 iii Preface This volume contains abstracts that have been accepted for presentation at the First International Conference on Mars Polar Science and Exploration, October 18-22? 1998. The Scientific Organizing Committee consisted of Terrestrial Members E. Blake (Icefield Instruments), G. Clow (U.S. Geologi- cal Survey, Denver), D. Dahl-Jensen (University of Copenhagen), K. Kuivinen (University of Nebraska), J. -
11Th International Conference on the Physics and Chemistry of Ice, PCI
11th International Conference on the Physics and Chemistry of Ice (PCI-2006) Bremerhaven, Germany, 23-28 July 2006 Abstracts _______________________________________________ Edited by Frank Wilhelms and Werner F. Kuhs Ber. Polarforsch. Meeresforsch. 549 (2007) ISSN 1618-3193 Frank Wilhelms, Alfred-Wegener-Institut für Polar- und Meeresforschung, Columbusstrasse, D-27568 Bremerhaven, Germany Werner F. Kuhs, Universität Göttingen, GZG, Abt. Kristallographie Goldschmidtstr. 1, D-37077 Göttingen, Germany Preface The 11th International Conference on the Physics and Chemistry of Ice (PCI- 2006) took place in Bremerhaven, Germany, 23-28 July 2006. It was jointly organized by the University of Göttingen and the Alfred-Wegener-Institute (AWI), the main German institution for polar research. The attendance was higher than ever with 157 scientists from 20 nations highlighting the ever increasing interest in the various frozen forms of water. As the preceding conferences PCI-2006 was organized under the auspices of an International Scientific Committee. This committee was led for many years by John W. Glen and is chaired since 2002 by Stephen H. Kirby. Professor John W. Glen was honoured during PCI-2006 for his seminal contributions to the field of ice physics and his four decades of dedicated leadership of the International Conferences on the Physics and Chemistry of Ice. The members of the International Scientific Committee preparing PCI-2006 were J.Paul Devlin, John W. Glen, Takeo Hondoh, Stephen H. Kirby, Werner F. Kuhs, Norikazu Maeno, Victor F. Petrenko, Patricia L.M. Plummer, and John S. Tse; the final program was the responsibility of Werner F. Kuhs. The oral presentations were given in the premises of the Deutsches Schiffahrtsmuseum (DSM) a few meters away from the Alfred-Wegener-Institute. -
Hydrated Sulfate Clusters SO4^2
Article Cite This: J. Phys. Chem. B 2019, 123, 4065−4069 pubs.acs.org/JPCB 2− n − Hydrated Sulfate Clusters SO4 (H2O)n ( =1 40): Charge Distribution Through Solvation Shells and Stabilization Maksim Kulichenko,† Nikita Fedik,† Konstantin V. Bozhenko,‡,§ and Alexander I. Boldyrev*,† † Department of Chemistry and Biochemistry, Utah State University, 0300 Old Main Hill, Logan, Utah 84322-0300, United States ‡ Department of Physical and Colloid Chemistry, Peoples’ Friendship University of Russia (RUDN University), 6 Miklukho-Maklaya St, Moscow 117198, Russian Federation § Institute of Problems of Chemical Physics, Russian Academy of Sciences, Chernogolovka 142432, Moscow Region, Russian Federation *S Supporting Information 2− ABSTRACT: Investigations of inorganic anion SO4 interactions with water are crucial 2− for understanding the chemistry of its aqueous solutions. It is known that the isolated SO4 dianion is unstable, and three H2O molecules are required for its stabilization. In the 2− current work, we report our computational study of hydrated sulfate clusters SO4 (H2O)n (n =1−40) in order to understand the nature of stabilization of this important anion by fi 2− water molecules. We showed that the most signi cant charge transfer from dianion SO4 ≤ 2− to H2O takes place at a number of H2O molecules n 7. The SO4 directly donates its charge only to the first solvation shell and surprisingly, a small amount of electron density of 0.15|e| is enough to be transferred in order to stabilize the dianion. Upon further addition of ff ≤ H2O molecules, we found that the cage e ect played an essential role at n 12, where the fi 2− | | rst solvation shell closes. -
Electromagnetism Based Atmospheric Ice Sensing Technique - a Conceptual Review
Int. Jnl. of Multiphysics Volume 6 · Number 4 · 2012 341 Electromagnetism based atmospheric ice sensing technique - A conceptual review Umair N. Mughal*, Muhammad S. Virk and M. Y. Mustafa High North Technology Center Department of Technology, Narvik University College, Narvik, Norway ABSTRACT Electromagnetic and vibrational properties of ice can be used to measure certain parameters such as ice thickness, type and icing rate. In this paper we present a review of the dielectric based measurement techniques for matter and the dielectric/spectroscopic properties of ice. Atmospheric Ice is a complex material with a variable dielectric constant, but precise calculation of this constant may form the basis for measurement of its other properties such as thickness and strength using some electromagnetic methods. Using time domain or frequency domain spectroscopic techniques, by measuring both the reflection and transmission characteristics of atmospheric ice in a particular frequency range, the desired parameters can be determined. Keywords: Atmospheric Ice, Sensor, Polar Molecule, Quantum Excitation, Spectroscopy, Dielectric 1. INTRODUCTION 1.1. ATMOSPHERIC ICING Atmospheric icing is the term used to describe the accretion of ice on structures or objects under certain conditions. This accretion can take place either due to freezing precipitation or freezing fog. It is primarily freezing fog that causes this accumulation which occurs mainly on mountaintops [16]. It depends mainly on the shape of the object, wind speed, temperature, liquid water content (amount of liquid water in a given volume of air) and droplet size distribution (conventionally known as the median volume diameter). The major effects of atmospheric icing on structure are the static ice loads, wind action on iced structure and dynamic effects. -
Ice Molecular Model Kit © Copyright 2015 Ryler Enterprises, Inc
Super Models Ice Molecular Model Kit © Copyright 2015 Ryler Enterprises, Inc. Recommended for ages 10-adult ! Caution: Atom centers and vinyl tubing are a choking hazard. Do not eat or chew model parts. Kit Contents: 50 red 4-peg oxygen atom centers (2 spares) 100 white hydrogen 2-peg atom centers (2 spares) 74 clear, .87”hydrogen bonds (2 spares) 100 white, .87” covalent bonds (2 spares) Related Kits Available: Chemistry of Water Phone: 806-438-6865 E-mail: [email protected] Website: www.rylerenterprises.com Address: 5701 1st Street, Lubbock, TX 79416 The contents of this instruction manual may be reprinted for personal use only. Any and all of the material in this PDF is the sole property of Ryler Enterprises, Inc. Permission to reprint any or all of the contents of this manual for resale must be submitted to Ryler Enterprises, Inc. General Information Ice, of course, ordinarily refers to water in the solid phase. In the terminology of astronomy, an ice can be the solid form of any element or compound which is usually a liquid or gas. This kit is designed to investigate the structure of ice formed by water. Fig. 1 Two water molecules bonded by a hydrogen bond. Water ice is very common throughout the universe. According to NASA, within our solar system ice is The symbol δ means partial, so when a plus sign is found in comets, asteroids, and several moons of added, the combination means partial positive the outer planets, and it has been located in charge. The opposite obtains when a negative sign interstellar space as well.