Formation and Decomposition of Chemically Activated and Stabilized Hydrazine

Total Page:16

File Type:pdf, Size:1020Kb

Formation and Decomposition of Chemically Activated and Stabilized Hydrazine J. Phys. Chem. A 2010, 114, 6235–6249 6235 Formation and Decomposition of Chemically Activated and Stabilized Hydrazine Rubik Asatryan,*,† Joseph W. Bozzelli,†,* Gabriel da Silva,‡ Saartje Swinnen,§ and Minh Tho Nguyen§ Department of Chemistry and EnVironmental Science, New Jersey Institute of Technology, Newark, New Jersey 07102, USA, Department of Chemical and Biomolecular Engineering, The UniVersity of Melbourne, Victoria 3010, Australia, and Department of Chemistry, Katholieke UniVersiteit LeuVen, B-3001 LeuVen, Belgium ReceiVed: February 23, 2010; ReVised Manuscript ReceiVed: April 15, 2010 2 Recombination of two amidogen radicals, NH2 (X B1), is relevant to hydrazine formation, ammonia oxidation and pyrolysis, nitrogen reduction (fixation), and a variety of other N/H/X combustion, environmental, and interstellar processes. We have performed a comprehensive analysis of the N2H4 potential energy surface, using a variety of theoretical methods, with thermochemical kinetic analysis and master equation simulations used to treat branching to different product sets in the chemically activated NH2 + NH2 process. For the first time, iminoammonium ylide (NH3NH), the less stable isomer of hydrazine, is involved in the kinetic modeling of N2H4. A new, low-energy pathway is identified for the formation of NH3 plus triplet NH, via initial production of NH3NH followed by singlet-triplet intersystem crossing. This new reaction channel results in the formation of dissociated products at a relatively rapid rate at even moderate temperatures and above. A further novel pathway is described for the decomposition of activated N2H4, which eventually leads to the formation of the simple products N2 + 2H2, via H2 elimination to cis-N2H2. This process, termed as “dihydrogen catalysis”, may have significant implications in the formation and decomposition chemistry of hydrazine and ammonia in diverse environments. In this mechanism, stereoselective attack of cis-N2H2 by molecular hydrogen results in decomposition to N2 with a fairly low barrier. The reverse termolecular reaction leading to the gas-phase formation of cis-N2H2 + H2 achieves non-heterogeneous catalytic nitrogen fixation with a relatively low activation barrier (77 kcal mol-1), much lower than the 125 kcal mol-1 barrier recently reported for bimolecular addition of H2 to N2. This termolecular reaction is an entropically disfavored path, but it does describe a new means of activating the notoriously unreactive N2. We design heterogeneous analogues of this reaction using the model compound (CH3)2FeH2 as a source of the H2 catalyst and apply it to the decomposition of cis-diazene. The reaction is seen to proceed via a topologically similar transition state, suggesting that our newly described mechanism is general in nature. 1. Introduction Association and disproportionation reactions involving the NH2 radical have long been studied experimentally,4-28 and to a lesser Hydrazine (N2H4) is an important energetic material, the degree by theoretical methods.29-31 main component of diamine-based rocket fuels. Hydrazine and its methyl-substituted homologues are unique endother- The N2H4 potential energy surface (PES) involves several mic compounds forming the class of hypergolic propellants. important transformation pathways closely related to the This type of propellant ignites spontaneously on contact with storage of hydrogen and the fixation of nitrogen (i.e., 1 32-35 an oxidizer, typically nitrogen tetroxide. N2H4 can be reduction to NH3, HCN, etc). It is evident that the gas- stabilized as a flame without any oxidizer, and its decomposi- phase hydrogenation of nitrogen occurs without a catalyst tion can lead to self-ignition or detonation.2 Hydrazine, as only at extreme conditions, and we note that the degree of the simplest diamine, has been the subject of numerous this “extremity” and the corresponding energy paths of the investigations with the earlier literature reviewed compre- process are not well established. hensively in refs 3-9. The overall free energy change (∆G) for the reaction N At adequate pressures, self-reaction of two amidogen radicals 2 + T - -1 generates hydrazine: 3H2 2NH3 is about 8 kcal mol . However, the first step of activating the triple bond is extremely unfavorable, with bond dissociation energy at 225 kcal mol-1. According + + f + to the recent calculations of Hwang and Mebel,30 the lowest NH2 NH2 ( M) N2H4( M) (1) barrier associating H2 and N2 into diimide is about 125 kcal mol-1 at the G2M(MP2)//MP2/6-31G** level of theory. Such * To whom correspondence should be addressed. E-mail: bozzelli@ a high activation barrier results in little or no probability for njit.edu (J.W.B.), [email protected] (R.A.). unimolecular occurrence of this reaction in the gas-phase. † New Jersey Institute of Technology. ‡ University of Melbourne. Hence, chain reactions are considered by the authors as the § University of Leuven. dominant reaction channels for nitrogen hydrogenation:30 10.1021/jp101640p 2010 American Chemical Society Published on Web 05/12/2010 6236 J. Phys. Chem. A, Vol. 114, No. 21, 2010 Asatryan et al. + f N2 H N2H is made in some kinetic models between isomers of N2H2 and + f + they are often combined into one reaction by use of a single N2H H2 HNNH H + f average N2H2 species. Analysis of the principal energetic, HNNH H N2H3 + f + structural, and kinetic differences between trans-N2H2, cis-N2H2, N2H3 H2 H2NNH2 H + f + and NNH2 (also called iso-N2H2) show significant distinctions. H2NNH2 H NH2 NH3 Kinetic analysis in this study suggests that the specific isomer + f + NH2 H2 NH3 H that forms or dominates in a given process may well play a crucial role in the final integrated results. Dean et al. proposed10 + f that the recombination reaction NH + NH had two channels Net: N2 3H2 2NH3 2 2 to N2H3 + H and N2H4 to better explain their radical profile measurements in rich ammonia flames. Formation of an N2H4 Recent studies substantiate that N2H4 is an intermediate product appears to dominate at lower-temperatures in agreement reaction product in the thermal decomposition of ammonia (at with literature data8 with wide variation in the reported rate ° 38 800 C). Chain-mediated decomposition of hydrazine is known constants. Other reaction channels, however, are less consistent. f + + from classic literature: 2N2H4 2NH3 N2 H2 with chain Miller and Bowman suggested7 that the high-temperature 4 steps N2H4 f H + N2H3 f H + N2H2 f N2 + H2. 25 products are N2H2 + H2. The measurements by Stothard et al. There are a number of unresolved problems in the mechanism at room temperature and low pressures indicate that H2 of nitrogen fixation in biological media (reduction of N2 to NH3 production is the dominant channel. They deduced a rate by nitrogenase via bacterial enzymes, nitrogen metabolism in coefficient for the bimolecular channel of amidogen recombina- 33 archaea, etc.). Notably, hydrogen is always produced when 11 3 -1 -1 tion forming N2H2 as 7.8 × 10 cm mol s . However, the nitrogenase reduces N2 to NH3 (vide infra). Most N2 fixing mass-spectrometric method used by these authors did not allow bacteria contain hydrogenase to recycle hydrogen.34 There is for assigning an observed experimental value to one of the N2H2 an agreement that N2 binds end-on to the Fe[H]2 complex and coproduct isomers. Dean and Bozzelli have further examined releases H2, while the bound N2 is reduced to N2H2. Hydrazine this system6 to try to account for the observations of Stothard as an intermediate has been detected experimentally whereas et al.25 at ambient temperatures and have interpreted their results N2H2 is assumed to be a very unstable intermediate that tends 33 in terms of a new reaction channel to H2 and singlet H2NN. To to decompose back to N2 + H2. account for reactions of H2NN in nitrogen mechanisms, several It is also believed that the primary initiation step in the thermal rate constants for a series of related reactions have been de-NOx processes is the reaction of ammonia with hydroxyl to 6 8 6,36 proposed. Recent modeling of Konnov and De Ruyck dem- form amidogen (NH2). The temperature dependence of the onstrates that reactions forming N2H2, as well as their unimo- thermal de-NOx process depends on the behavior of NH2. lecular decomposition and bimolecular radical reactions, are Recombination and cross-reactions of NH2 radicals with simple important in hydrazine flames, since N2H2 is a crucial open and closed-shell species such as O2, NO, O3,SO2, and intermediate. CO, along with the oxidation of NH3, are also of principal importance in combustion media, environmental processes, and Decomposition of gaseous hydrazine behind a reflected shock 28,37 wave is found to be pressure dependent; the falloff behavior in atmospheric chemistry. 27 The amidogen radical self-reaction involves several dispro- depends on the nature of diluents. The main products of portionation channels hydrazine decomposition are ammonia, hydrogen, and nitrogen. Relative yields of the products in hydrazine decomposition flames closely correspond to the overall equation 2N2H4 f 2 + 2 f 2 ′ + NH2(X B1) NH2(X B1) N2H3(X A ) H (2) 2NH3 + N2 + H2, and their relative yields were found to be 11,39 f + unaffected by pressure. Notably, less ammonia is formed trans-N2H2 H2 in hydrazine decomposition at higher temperatures.40 An (3) inclusive review on the kinetic modeling of decomposition of f cis-N H + H (4) hydrazine using different estimated rate constants is contained 2 2 2 in the Konnov and De Ruyck article,8 while some early models f + 41 NNH2 H2 (5) are described by Adams. The overall recombination process of amidogen radicals have 3 - f + 28 NH3 NH(X Σ ) been considered quite recently by Bahng and Macdonald at (6) 293 ( 2 K over a pressure range from 2 to 10 Torr. The low pressure rate constant showed a linear dependence on pressure.
Recommended publications
  • A Photoionization Reflectron Time‐Of‐Flight Mass Spectrometric
    Articles ChemPhysChem doi.org/10.1002/cphc.202100064 A Photoionization Reflectron Time-of-Flight Mass Spectrometric Study on the Detection of Ethynamine (HCCNH2) and 2H-Azirine (c-H2CCHN) Andrew M. Turner,[a, b] Sankhabrata Chandra,[a, b] Ryan C. Fortenberry,*[c] and Ralf I. Kaiser*[a, b] Ices of acetylene (C2H2) and ammonia (NH3) were irradiated with 9.80 eV, and 10.49 eV were utilized to discriminate isomers energetic electrons to simulate interstellar ices processed by based on their known ionization energies. Results indicate the galactic cosmic rays in order to investigate the formation of formation of ethynamine (HCCNH2) and 2H-azirine (c-H2CCHN) C2H3N isomers. Supported by quantum chemical calculations, in the irradiated C2H2:NH3 ices, and the energetics of their experiments detected product molecules as they sublime from formation mechanisms are discussed. These findings suggest the ices using photoionization reflectron time-of-flight mass that these two isomers can form in interstellar ices and, upon spectrometry (PI-ReTOF-MS). Isotopically-labeled ices confirmed sublimation during the hot core phase, could be detected using the C2H3N assignments while photon energies of 8.81 eV, radio astronomy. 1. Introduction acetonitrile (CH3CN; 1) and methyl isocyanide (CH3NC; 2) ‘isomer doublet’ (Figure 2) – the methyl-substituted counterparts of For the last decade, the elucidation of the fundamental reaction hydrogen cyanide (HCN) and hydrogen isocyanide (HNC) – has pathways leading to structural isomers – molecules with the been detected toward the star-forming region SgrB2.[4,8–9] same molecular formula, but distinct connectivities of atoms – However, none of their higher energy isomers has ever been of complex organic molecules (COMs) in the interstellar identified in any astronomical environment: 2H-azirine (c- [10–14] [15–19] medium (ISM) has received considerable interest from the NCHCH2; 3), ethynamine (HCCNH2; 4), ketenimine [1–3] [20] [21] astrochemistry and physical chemistry communities.
    [Show full text]
  • Condensed-Phase Photochemistry in the Absence of Radiation Chemistry Ella Mullikin
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Wellesley College Wellesley College Wellesley College Digital Scholarship and Archive Faculty Research and Scholarship 6-27-2018 Condensed-Phase Photochemistry in the Absence of Radiation Chemistry Ella Mullikin Pierce van Mulbregt Jeniffer Perea Muhammad Kasule Jean Huang See next page for additional authors Follow this and additional works at: https://repository.wellesley.edu/scholarship Version: Post-print Recommended Citation E. Mullikin, P. van Mulbregt, J. Perea, M. Kasule, J. Huang, C. Buffo, J. Campbell, L. Gates, H. M. Cumberbatch, Z. Peeler, H. Schneider, J. Lukens, S. T. Bao, R. Tano-Menka, S. Baniya, K. Cui, M. Thompson, A. Hay, L. Widdup, A. Caldwell-Overdier, J. Huang, M. C. Boyer, M. Rajappan, G. Echebiri and C. R. Arumainayagam, ACS Earth and Space Chemistry, 2018, DOI: 10.1021/ acsearthspacechem.8b00027. This Article is brought to you for free and open access by Wellesley College Digital Scholarship and Archive. It has been accepted for inclusion in Faculty Research and Scholarship by an authorized administrator of Wellesley College Digital Scholarship and Archive. For more information, please contact [email protected]. Authors Ella Mullikin, Pierce van Mulbregt, Jeniffer Perea, Muhammad Kasule, Jean Huang, Christina Buffo, Jyoti Campbell, Leslie Gates, Helen M. Cumberbatch, Zoe Peeler, Hope Schneider, Julia Lukens, Si Tong Bao, Rhoda Tano-Menka, Subha Baniya, Kendra Cui, Mayla Thompson, Aury Hay, Lily Widdup, Anna Caldwell- Overier, Justine Huang, Michael C. Boyer, Mahesh Rajappan, Geraldine Echebiri, and Christopher R. Arumainayagam This article is available at Wellesley College Digital Scholarship and Archive: https://repository.wellesley.edu/scholarship/183 Condensed-Phase Photochemistry in the Absence of Radiation Chemistry Ella Mullikin,1 Pierce van Mulbregt,2 Jeniffer Perea,1 Muhammad Kasule,3 Jean Huang,1 Christina Buffo,1 Jyoti Campbell,1 Leslie Gates,1 Helen M.
    [Show full text]
  • Nitroxyl (Hno) and Carbonylnitrenes
    INVESTIGATION OF REACTIVE INTERMEDIATES: NITROXYL (HNO) AND CARBONYLNITRENES by Tyler A. Chavez A dissertation submitted to the Johns Hopkins University in conformity with the requirements for the degree of Doctor of Philosophy Baltimore, Maryland February 2016 © 2016 Tyler A. Chavez All rights reserved Abstract Membrane inlet mass spectrometry (MIMS) is a well-established method used to detect gases dissolved in solution through the use of a semipermeable hydrophobic membrane that allows the dissolved gases, but not the liquid phase, to enter a mass spectrometer. Interest in the unique biological activity of azanone (nitroxyl, HNO) has highlighted the need for new sensitive and direct detection methods. Recently, MIMS has been shown to be a viable method for HNO detection with nanomolar sensitivity under physiologically relevant conditions (Chapter 2). In addition, this technique has been used to explore potential biological pathways to HNO production (Chapter 3). Nitrenes are reactive intermediates containing neutral, monovalent nitrogen atoms. In contrast to alky- and arylnitrenes, carbonylnitrenes are typically ground state singlets. In joint synthesis, anion photoelectron spectroscopic, and computational work we studied the three nitrenes, benzoylnitrene, acetylnitrene, and trifluoroacetylnitrene, with the purpose of determining the singlet-triplet splitting (ΔEST = ES – ET) in each case (Chapter 7). Further, triplet ethoxycarbonylnitrene and triplet t-butyloxycarbonylnitrene have been observed following photolysis of sulfilimine precursors by time-resolved infrared (TRIR) spectroscopy (Chapter 6). The observed growth kinetics of nitrene products suggest a contribution from both the triplet and singlet nitrene, with the contribution from the singlet becoming more prevalent in polar solvents. Advisor: Professor John P. Toscano Readers: Professor Kenneth D.
    [Show full text]
  • Tables of Rate Constants for Gas Phase Chemical Reactions of Sulfur Compounds (1971-1980)
    A 11 ID 2 1 M t> 3 5 7 All 1021 46357 Weslley, Francis/Tables of rate constant QC100 .U573 V72;1982 C.2 NBS-PUB-C 1982 NSRDS-NBS 72 U.S. DEPARTMENT OF COMMERCE / National Bureau of Standards NATIONAL BUREAU OF STANDARDS The National Bureau of Standards' was established by an act of Congress on March 3, 1901. The Bureau’s overall goal is to strengthen and advance the Nation’s science and technology and facilitate their effective application for public benefit. To this end, the Bureau conducts research and provides: (1) a basis for the Nation’s physical measurement system, (2) scientific and technological services for industry and government, (3) a technical basis for equity in trade, and (4) technical services to promote public safety. The Bureau’s technical work is per- formed by the National Measurement Laboratory, the National Engineering Laboratory, and the Institute for Computer Sciences and Technology. THE NATIONAL MEASUREMENT LABORATORY provides the national system of physical and chemical and materials measurement; coordinates the system with measurement systems of other nations and furnishes essential services leading to accurate and uniform physical and chemical measurement throughout the Nation’s scientific community, industry, and commerce; conducts materials research leading to improved methods of measurement, standards, and data on the properties of materials needed by industry, commerce, educational institutions, and Government; provides advisory and research services to other Government agencies; develops, produces, and
    [Show full text]
  • The Role of State-Of-The-Art Quantum-Chemical Calculations in Astrochemistry: Formation Route and Spectroscopy of Ethanimine As a Paradigmatic Case
    Article The role of state-of-the-art quantum-chemical calculations in astrochemistry: formation route and spectroscopy of ethanimine as a paradigmatic case Carmen Baiano1 , Jacopo Lupi1 , Nicola Tasinato1 , Cristina Puzzarini2,∗ and Vincenzo Barone1,∗ 1 Scuola Normale Superiore, Piazza dei Cavalieri 7, I-56126 Pisa, Italy 2 Dipartimento di Chimica “Giacomo Ciamician”, Università di Bologna, Via F. Selmi 2, 40126 Bologna, Italy * Correspondence: [email protected]; [email protected] Received: date; Accepted: date; Published: date Abstract: The gas-phase formation and spectroscopic characteristics of ethanimine have been re-investigated as a paradigmatic case illustrating the accuracy of state-of-the-art quantum-chemical (QC) methodologies in the field of astrochemistry. According to our computations, the reaction between the amidogen, NH, and ethyl, C2H5, radicals is very fast, close to the gas-kinetics limit. Although the main product channel under conditions typical of the interstellar medium leads to methanimine and the methyl radical, the predicted amount of the two E,Z stereoisomers of ethanimine is around 10%. State-of-the-art QC and kinetic models lead to a [E-CH3CHNH]/[Z-CH3CHNH] ratio of ca. 1.4, slightly higher than the previous computations, but still far from the value determined from astronomical observations (ca. 3). An accurate computational characterization of the molecular structure, energetics, and spectroscopic properties of the E and Z isomers of ethanimine combined with millimeter-wave measurements up to 300 GHz, allows for predicting the rotational spectrum of both isomers up to 500 GHz, thus opening the way toward new astronomical observations. Keywords: quantum chemistry; spectroscopy; kinetics; ethanimine; prebiotic chemistry 1.
    [Show full text]
  • Compilation of Chemical Kinetic Data for Combustion Chemistry. Part 2. Non-Aromatic C, H, O, N, and S Containing Compounds
    v NBS PUBLICATIONS r A111D2 TBOmi NAT'L INST OF STANDARDS & TECH R.I.C. All 102730091 Westley, Francls/Compllatlon of chemical 2 QC100 .11573 NO. 73 V2;1987 C.2 NBS-PUB-C NSRDS-NBS 73, Part U.S. DEPARTMENT OF COMMERCE / National Bureau of Standards 1 BB he National Bureau of Standards was established by an act of Congress on March 3, 1901. The Bureau’s overall M goal is to strengthen and advance the nation’s science and technology and facilitate their effective application for public benefit. To this end, the Bureau conducts research to assure international competidveness and leadership of U.S. industry, science arid technology. NBS work involves development and transfer of measurements, standards and related science and technology, in support of continually improving U.S. productivity, product quality and reliability, innovation and underlying science and engineering. The Bureau’s technical work is performed by the National Measurement Laboratory, the National Engineering Laboratory, the Institute for Computer Sciences and Technology, and the Institute for Materials Science and Engineering. The National Measurement Laboratory Provides the national system of physical and chemical measurement; • Basic Standards 2 coordinates the system with measurement systems of other nations and • Radiation Research furnishes essential services leading to accurate and uniform physical and • Chemical Physics chemical measurement throughout the Nation’s scientific community, • Analytical Chemistry industry, and commerce; provides advisory and research
    [Show full text]
  • Electron-Induced Radiolysis of Astrochemically Relevant Ammonia Ices
    1 Electron-Induced Radiolysis of Astrochemically Relevant Ammonia Ices Katherine E. Shulenberger, Jane L. Zhu, Katherine Tran, Sebiha Abdullahi, Carina Belvin, Julia Lukens, Zoe Peeler, Ella Mullikin, Helen M. Cumberbatch, Jean Huang, Kathleen Regovich, Alice Zhou, Lauren Heller, Milica Markovic, Leslie Gates, Christina Buffo, Rhoda Tano-Menka, a and Christopher R. Arumainayagam Department of Chemistry, Wellesley College, Wellesley, MA 02481 Esther Böhler, Petra Swiderek, Institute of Applied and Physical Chemistry, University of Bremen, D-28334 Bremen, Germany Sasan Esmaili, Andrew D. Bass, Michael Huels, and Léon Sanche Department of Nuclear Medicine and Radiobiology, University of Sherbrooke, Sherbrooke, QC, Canada Abstract We elucidate mechanisms of electron-induced radiolysis in cosmic (interstellar, planetary, and cometary) ice analogs of ammonia (NH3), likely the most abundant nitrogen-containing compound in the interstellar medium (ISM). Astrochemical processes were simulated under ultrahigh vacuum conditions by high-energy (1 keV) and low-energy (7 eV) electron-irradiation of nanoscale thin films of ammonia deposited on cryogenically cooled metal substrates. Irradiated films were analyzed by temperature-programmed desorption (TPD). Experiments with ammonia isotopologues provide convincing evidence for the electron-induced formation of hydrazine (N2H4) and diazene (N2H2) from condensed NH3. To understand the dynamics of ammonia radiolysis, the dependence of hydrazine and diazene yields on incident electron energy, electron flux, electron fluence, film thickness, and ice temperature were investigated. Radiolysis yield measurements versus (1) irradiation time and (2) film thickness are semi-quantitatively consistent with a reaction mechanism that involves a bimolecular step for the formation of hydrazine and diazene from the dimerization of amidogen (NH2) and imine (NH) radicals, respectively.
    [Show full text]
  • Magnetic Trapping of Atomic Nitrogen and Cotrapping of NH
    Magnetic trapping of atomic nitrogen and cotrapping of NH A dissertation presented by Matthew Taylor Hummon to The Department of Physics in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the subject of Physics Harvard University Cambridge, Massachusetts March 2010 c 2010 - Matthew Taylor Hummon All rights reserved. Thesis advisor Author John M. Doyle Matthew Taylor Hummon Magnetic trapping of atomic nitrogen and cotrapping of NH Abstract We observe magnetic trapping of atomic nitrogen (14N) and cotrapping of ground- 14 3 state imidogen ( NH, X Σ−). Both are loaded directly from a room-temperature beam via buffer gas cooling. We trap approximately 1 1012 14N atoms at a peak × 12 3 density of 2 10 cm− at 600 mK. We also trap similar numbers of the isotope × 15N. Observation times of magnetically trapped 14N of over 100 s have been achieved. Utilizing a new pulsed cryogenic reservoir for introducing buffer gas into the cell, we are able to cotrap 14N and 14NH and subsequently rapidly remove most of the buffer gas. This allows for observation times of trapped NH of up to 10 s. This is sufficiently long to study N-NH collisions in the magnetic trap. From our observations, we estimate a ratio of elastic to inelastic N-NH collisions of γ 100 at a temperature ≈ of 570 mK. iii Contents TitlePage.................................... i Abstract..................................... iii TableofContents................................ iv ListofFigures.................................. vi ListofTables .................................. viii Citations to Previously Published Work . ix Acknowledgments................................ x Dedication.................................... xi 1 Introduction 1 1.1 Motivation................................. 1 1.1.1 Few-bodyphysics ......................... 2 1.1.2 Precision measurement .
    [Show full text]
  • ASA Conference a HARVARD-SMITHSONIAN CENTER for ASTROPHYSICS
    H I T R A N - A The Combined S 15th HITRAN & 14th ASA Conference A HARVARD-SMITHSONIAN CENTER FOR ASTROPHYSICS CAMBRIDGE MA, USA 2018 June 13 – June 15, 2018 The following companies contributed to The Combined 15th HITRAN & 14th ASA Conference: Gold Sponsor: Elsevier Radarweg 29 1043 NX Amsterdam The Netherlands Gold Sponsor: Aerodyne Research, Inc. 45 Manning Road Billerica MA 01821-3976 USA Cover image: Original HITRAN “Rosetta-stone” logo weaved by Dr. Marina Zivkovic-Rothman (https://www.mzrstudio.com/). Presented to the HITRAN group in May 2017. The HITRAN Project has been funded by grants from the National Aeronautics and Space Administration. DAY 1, Wednesday 13 June SESSION I: Databases and Tools 1 I-1. Brief Report on the Status and Future Directions of the HITRAN Database I. E. Gordon, L. S. Rothman, Y. Tan, R. V. Kochanov, R. J. Hargreaves, E. K. Conway 2 I-2. Considerations for Sharing and Preserving Research Software and Data D. Bouquin ...................................3 I-3. PNNL Databases for Atmospheric Monitoring T. J. Johnson, T. L. Myers, S. W. Sharpe, R. L. Sams, R. G. Tonkyn, M. S. Taubman, T. O. Danby, J. C. Birnbaum ...........................4 I-4. Spectroscopic Toolbox for HITRAN R. V. Kochanov, I. E. Gordon, L. S. Rothman, Y. Tan, C. Hill, J. Karns, W. Matt, J. Lamouroux ..................................5 I-5. Evaluation of the Spectroscopic Parameters of Current Spectroscopic Databases, such as GEISA-2015 and HITRAN-2016, in the Frame of the New 2018 Release of GEISA R. Armante, A. Perrin, N. Jacquinet, N. Scott, A. Ch´edin .............6 I-6.
    [Show full text]
  • Table of Recommended Rate Constants for Chemical Reactions Occurring in Combustion
    A111D2 14bB cn 0- NATL INST OF STANMffii.SSJ All 1021 46399 1964 ffiSWR***""" NBS-PUB-C « JC $ to NSRDS-NBS 67 \ %J 0* U.S. DEPARTMENT OF COMMERCE / National Bureau of Standards U, 2 NATIONAL BUREAU OF STANDARDS The National Bureau of Standards' was established by an act of Congress on March 3, 1901. The Bureau's overall goal is to strengthen and advance the Nation's science and technology and facilitate their effective application for public benefit. To this end, the Bureau conducts research and provides: (1) a basis for the Nation’s physical measurement system, (2) scientific and technological services for industry and government, (3) a technical basis for equity in trade, and (4) technical services to promote public safety. The Bureau’s technical work is per- formed by the National Measurement Laboratory, the National Engineering Laboratory, and the Institute for Computer Sciences and Technology. THE NATIONAL MEASUREMENT LABORATORY provides the national system of physical and chemical and materials measurement; coordinates the system with measurement systems of other nations and furnishes essential services leading to accurate and uniform physical and chemical measurement throughout the Nation’s scientific community, industry, and commerce; conducts materials research leading to improved methods of measurement, standards, and data on the properties of materials needed by industry, commerce, educational institutions, and Government; provides advisory and research services to other Government agencies; develops, produces, and distributes Standard Reference Materials; and provides calibration services. The Laboratory consists of the following centers: Absolute Physical Quantities 2 — Radiation Research — Thermodynamics and Molecular Science — Analytical Chemistry — Materials Science.
    [Show full text]
  • User's Guide for Estimating Methane and Nitrous Oxide Emissions From
    USER’S GUIDE FOR ESTIMATING METHANE AND NITROUS OXIDE EMISSIONS FROM MOBILE COMBUSTION USING THE STATE INVENTORY TOOL SEPTEMBER 2020 Prepared by: ICF Prepared for: State Energy and Environment Program, U.S. Environmental Protection Agency This section of the User’s Guide provides instruction on using the Mobile Combustion module of the State Inventory Tool (SIT), and describes the methodology used for estimating greenhouse gas (GHG) emissions from highway and non-highway vehicles at the state level. Module 3 – Mobile Combustion Module September 2020 TABLE OF CONTENTS 1.1 Getting Started .............................................................................................. 2 1.2 Module Overview ........................................................................................... 4 1.2.1 Data Requirements .................................................................................. 6 1.2.2 Tool Layout ............................................................................................. 7 1.3 Methodology.................................................................................................. 9 1.4 Uncertainty ................................................................................................. 20 1.5 Explanation of Mobile Combustion Module Updates ........................................... 21 1.6 References .................................................................................................. 22 State Greenhouse Gas Inventory Tool User’s Guide for the Mobile Combustion Module 1.1
    [Show full text]
  • Photochemistry Vs. Radiation Chemistry of Interstellar Ices Chris
    Extraterrestrial Prebiotic Molecules: Photochemistry vs. Radiation Chemistry of Interstellar Ices Chris R. Arumainayagam, Robin T. Garrod, Michael Boyer, Aurland Hay, Si Tong Bao, Jyoti Campbell, Amy Wang, Chris M. Nowak, Michael R. Arumainayagam, and Peter J. Hodge In 2016, unambiguous evidence for the presence of the amino acid glycine, an important prebiotic molecule, was deduced based on in situ mass-spectral studies of the coma surrounding cometary ice. This finding is significant because comets are thought to have preserved the icy grains originally found in the interstellar medium prior to solar system formation. Energetic processing of cosmic ices via photochemistry and radiation chemistry is thought to be the dominant mechanism for the extraterrestrial synthesis of prebiotic molecules. Radiation chemistry is defined as the “study of the chemical changes produced by the absorption of radiation of sufficiently high energy to produce ionization.” Ionizing radiation in cosmic chemistry includes high-energy particles (e.g., cosmic rays) and high-energy photons (e.g., extreme-UV). In contrast, photochemistry is defined as chemical processes initiated by photon-induced electronic excitation not involving ionization. Vacuum-UV (6.2 –12.4 eV) light may, in addition to photochemistry, initiate radiation chemistry because the threshold for producing secondary electrons is lower in the condensed phase than in the gas phase. Unique to radiation chemistry are four phenomena: (1) production of a cascade of low-energy (< 20 eV) secondary electrons which are thought to be the dominant driving force for radiation chemistry, (2) reactions initiated by cations, (3) non-uniform distribution of reaction intermediates, and (4) non-selective chemistry leading to the production of multiple reaction products.
    [Show full text]