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101. Methane and its isotopes - Current status and prospects for improvement

Author

Brown, L. R, Margolis, J. S, Champion, J. P, Hilico, J. C, Jouvard, J. M, Loete, M, Chackerian, C., Jr, Tarrago, G, and Benner, D. C

Subjects
Atomic And Molecular Physics
Abstract

Numerous changes made for the 1991 and 1992 versions of the HITRAN database in the 0-6185/cm region for molecular line parameters of methane are described. An assessment of deficiencies in the parameters is presented.

Published
1992
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103. Measurements of Lorentz-broadening coefficients and pressure-induced line shift coefficients in the nu2 band of D2(O-16)

Author

Rinsland, Curtis P, Smith, Mary A. H, Malathy Devi, V, and Benner, D. C

Subjects
Atomic And Molecular Physics
Abstract

Lorentz-broadening and pressure-induced line-shift coefficients are determined experimentally for 126 transitions in the nu2 band of D2(O-16) from laboratory spectra with a Fourier-transform spectrometer. A nonlinear least-squares fitting procedure is employed to measure transitions up to J double-prime = 12 in the buffer gases air, nitrogen, and oxygen. The N2-broadening/O2-broadening coefficient ratio is correlated with the magnitude of the O2-broadening coefficient, and the pressure coefficients are not correlated with line widths.

Published
1991
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106. Gaussian quadrature exponential sum modeling of near infrared methane laboratory spectra obtained at temperatures from 106 to 297 K

Author

Giver, Lawrence P, Benner, D. C, Tomasko, M. G, Fink, U, and Kerola, D

Subjects
Lunar And Planetary Exploration
Abstract

Transmission measurements made on near-infrared laboratory methane spectra have previously been fit using a Malkmus band model. The laboratory spectra were obtained in three groups at temperatures averaging 112, 188, and 295 K; band model fitting was done separately for each temperature group. These band model parameters cannot be used directly in scattering atmosphere model computations, so an exponential sum model is being developed which includes pressure and temperature fitting parameters. The goal is to obtain model parameters by least square fits at 10/cm intervals from 3800 to 9100/cm. These results will be useful in the interpretation of current planetary spectra and also NIMS spectra of Jupiter anticipated from the Galileo mission.

Published
1990

107. High resolution spectroscopy to support atmospheric measurements

Author

Smith, Mary Ann H, Devi, V. Malathy, Rinsland, Curtis P, Benner, D. Chris, and Harvey, Gale A

Subjects
Geophysics
Abstract

Detailed knowledge of the molecular spectra of ozone and other infrared-active atmospheric species is needed for accurate calculation of atmospheric heating and cooling rates in climate models. Remote sensing experiments on the Nimbus-7 satellites and the Spacelab-3 Space Shuttle Mission have shown that space-based measurements of infrared absorption or emission can be used to accurately determine the concentrations and distributions of stratospheric species on a global scale. The objective of this research task is to improve knowledge of the spectroscopic line parameters (positions, intensities, assignments, halfwidths, and pressure-induced shifts) of key atmospheric constituents through laboratory measurements.

Published
1990

108. Leistungsunterschiede von Schülerinnen und Schülern in Shanghai und Deutschland: Erklärungsansätze und deren Überprüfung

Author

Benner, Dietrich, Meyer, Hilbert, Peng, Zhengmei, Li, Zhengtao, Benner, D ( Dietrich ), Meyer, H ( Hilbert ), Peng, Z ( Zhengmei ), Li, Z ( Zhengtao ), Praetorius, Anna-Katharina; https://orcid.org/0000-0001-7581-367X, Kuger, Susanne, Qi, Li, Klieme, Eckhard, Benner, Dietrich, Meyer, Hilbert, Peng, Zhengmei, Li, Zhengtao, Benner, D ( Dietrich ), Meyer, H ( Hilbert ), Peng, Z ( Zhengmei ), Li, Z ( Zhengtao ), Praetorius, Anna-Katharina; https://orcid.org/0000-0001-7581-367X, Kuger, Susanne, Qi, Li, and Klieme, Eckhard

Published
2018

114. Erziehung

Author

Benner, D, Oelkers, J, Benner, D ( D ), Oelkers, J ( J ), Benner, D, Oelkers, J, Benner, D ( D ), and Oelkers, J ( J )

Published
2010

115. Aufklärung

Author

Benner, D, Oelkers, J, Benner, D ( D ), Oelkers, J ( J ), Benner, D, Oelkers, J, Benner, D ( D ), and Oelkers, J ( J )

Published
2010

116. Measured and Theoretical Self- and N₂-Broadened Line Parameters in the ν₆ Band of CH₃D

Author

Devi, V. Malathy, Benner, D. Chris, Sung, Keeyon, Predoi-Cross, Adriana, Smith, Mary Ann H., Mantz, Arlan W., Sinyakova, Tatyana, and Buldyreva, Jeanna

Subjects
Temperature variation, Poster Session, Methane, Spectroscopy
Abstract

Monodeuterated methane (CH3D) is a constituent trace species in several planetary atmospheres, and its spectrum is often used in determinations of atmosphericH/Dratios. Methane plays an important role in terrestrial atmospheric chemistry. It is the most abundant hydrocarbon in our atmosphere and as anIRactive gas makes an important contribution to the enhanced greenhouse effect. Methane is increasing in the Earth’s atmosphere at a rate of about 1% per year. The current knowledge of its sources and sinks are not sufficient to isolate the cause of the observed changes in the mixing ratio and global distribution. As a result, the infrared spectrum of methane and its isotopomers is continually being investigated in order to obtain improved spectroscopic line parameters needed to interpret remote sensing observations. Remote sensing instruments require laboratory data sets based on measurements of very high accuracy. The primary objective of this study is to enhance our spectroscopic knowledge of monodeuterated methane in theν6band located at 6.8 microns. We present measurement results for self- and N2-broadened line parameters from room temperature down to about 80K. A total of 23 high-resolution, highS/Nspectra recorded with two Fourier transform spectrometers: a) the McMath-Pierce FTS located on Kitt Peak and b) a Bruker IFS-125HR FTS at the Jet Propulsion Laboratory (JPL)1were fit simultaneously in a multispectrum approach. 2The set included both pure CH3D and dilute mixtures of CH3D in research grade nitrogen. The variations in the measured line parameters with the symmetry species, the rotational quantum numbers and with temperature are reported and discussed in comparison with earlier measurements. For the case of nitrogen-broadening, we also provide semi-classical calculations based on a rigorous treatment of the active molecule as a symmetric top, a model intermolecular potential comprising both short- and long-range interactions, and exact classical trajectories. These calculations are done for various temperatures and for wide ranges of rotational quantum numbers. The role of the various high-order multipoles in the line-broadening at low, middle and high values of the rotational quantum numberJis investigated. Main features of theK-dependences are also analyzed. These theoretical values are included in the general comparison of our new experimental and already available in the literature results.3

Published
2014
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117. Self- and Air-Broadened Line Shape Parameters of ¹²CH₄ : 4500-4620 cm⁻¹

Author

Devi, V. Malathy, Benner, D. Chris, Sung, K., Brown, L. R., Crawford, T. J., Smith, M. A. H., Mantz, A. W., and Predoi-Cross, A.

Subjects
Poster Session, Methane, Spectroscopy
Abstract

Accurate knowledge of spectral line shape parameters is important for infrared transmission and radiance calculations in the terrestrial atmosphere. We report the self and air-broadened Lorentz widths, shifts and line mixing coefficients along with their temperature dependencies for methane absorption lines in the 2.2 µm spectral region. For this, we obtained a series of high-resolution, high S/N spectra of 99.99% 12C-enriched samples of pure methane and its dilute mixtures in dry air at cold temperatures down to 150 K using the Bruker IFS 125HR Fourier transform spectrometer at JPL. The coolable absorption cell had an optical path of 20.38 cm and was specially built to reside inside the sample compartment of the Bruker FTS1. The 13 spectra used in the analysis consisted of seven pure 12CH4 spectra at pressures from 4.5 to 169 Torr and six air-broadened spectra with total sample pressures of 113-300 Torr and methane volume mixing ratios between 4 and 9.7%. These 13 spectra were fit simultaneously using the multispectrum least-squares fitting technique2. The results will be compared to existing values reported in the literature3.

Published
2014
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118. An Activity Model to Demonstrate Countercurrent Exchange.

Author

Benner, D. B.

Abstract

Discusses the scant coverage in high school textbooks of countercurrent exchange for the efficient movement of molecules across biological membranes. Argues that this is one of the most intriguing of the physiological adaptive mechanisms. (DDR)

Published
1998

120. SPECTRAL LINE SHAPES IN THE 2ν3 Q BRANCH OF 12CH4

Author

Devi, V., primary, Boudon, Vincent, additional, Mantz, Arlan, additional, Ismail, Syed, additional, Smith, Mary, additional, Yu, Shanshan, additional, Crawford, Timothy, additional, Brown, Linda, additional, Sung, Keeyoon, additional, and Benner, D., additional

Published
2016
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121. MULTISPECTRUM ANALYSIS OF THE OXYGEN A-BAND

Author

Drouin, Brian, primary, Wishnow, Edward, additional, Robichaud, David, additional, Mlawer, Eli, additional, Hodges, Joseph, additional, Devi, V., additional, Benner, D., additional, Yu, Shanshan, additional, Sung, Keeyoon, additional, Payne, Vivienne, additional, Oyafuso, Fabiano, additional, Guillaume, Alexander, additional, Crawford, Timothy, additional, Cich, Matthew, additional, and Brown, Linda, additional

Published
2016
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124. Anti-Inflammatory and Anti-Oxidative Nutrition in Hypoalbuminemic Dialysis Patients (AIONID) study: Results of the pilot-feasibility, double-blind, randomized, placebo-controlled trial

Author

Rattanasompattikul, M, Molnar, MZ, Lee, ML, Dukkipati, R, Bross, R, Jing, J, Kim, Y, Voss, AC, Benner, D, Feroze, U, MacDougall, IC, Tayek, JA, Norris, KC, Kopple, JD, Unruh, M, Kovesdy, CP, and Kalantar-Zadeh, K

Abstract

Background: Low serum albumin is common and associated with protein-energy wasting, inflammation, and poor outcomes in maintenance hemodialysis (MHD) patients. We hypothesized that in-center (in dialysis clinic) provision of high-protein oral nutrition supplements (ONS) tailored for MHD patients combined with anti-oxidants and anti-inflammatory ingredients with or without an anti-inflammatory appetite stimulator (pentoxifylline, PTX) is well tolerated and can improve serum albumin concentration. Methods: Between January 2008 and June 2010, 84 adult hypoalbuminemic (albumin

Published
2013
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126. Development of a 1.65 μm pulsed laser DIAL System to map atmospheric CH4 distributions

Author

Syed, Ismail, Crawford, James, Leifer, Ira, Hovis, Floyd, Burnham, Ralph, Hair, John, Refaat, Tamer, Notari, Anthony, Collins, James, Kooi, Susan, Hardesty, Michael, Devi, V. Malathy, Benner, D. Chris, Brown, Linda R., Sung, Keeyoon, Diskin, Glenn, Fix, Andreas, Abedin, Nurul, and Hostetler, Chris

Subjects
Methan, Lidar, DIAL
Published
2010

128. Spectral Line Parameters in the ν9 Band ofEthane

Author

Devi, V. Malathy, Benner, D. Chris, Rinsland, C. P., Smith, M. A. H., Sams, R. L., Blake, T. A., Flaud, J.-M., Sung, K., Brown, L. R., and Mantzf, A. W.

Subjects
HITRAN, Astronomical spectroscopy
Abstract

Spectral line parameters, including line center positions, absolute line intensities, self- and N2-broadened halfwidth coefficients, and the temperature dependences of these halfwidth coefficients, have been measured for more than 1330 transitions in the ν9 band of ethane (C2H6) by applying a multispectrum nonlinear least squares analysis technique.1 We analyzed a total of 43 high-resolution (0.00156-0.005 cm−1) infrared absorption spectra recorded with two different Bruker Fourier transform spectrometers (at PNNL and at JPL) at various sample path lengths, pressures and temperatures. The ν9 fundamental of C2H6 is the strongest band in the terrestrial spectral window, and it is often used for ethane identification and abundance determination in remote sensing of planetary atmospheres. Torsional splittings are fairly large (dependent upon J;K) and measurable in several rQ and pQ sub-band structures. However, in the case of the rQ0 sub-band the two split components are completely obscured because of the overlap of Doppler-broadened J transitions. The results from the present study2 will be compared with other published data.

Published
2010
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129. HIGH PRESSURE OXYGEN A-BAND SPECTRA

Author

Drouin, Brian, primary, Hoo, Jiajun, additional, Devi, V., additional, Benner, D., additional, Robichaud, David, additional, Hodges, Joseph, additional, Long, David, additional, Bray, Caitlin, additional, Rupasinghe, Priyanka, additional, Okumura, Mitchio, additional, Bui, Thinh, additional, Lunny, Elizabeth, additional, Yu, Shanshan, additional, and Sung, Keeyoon, additional

Published
2015
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133. The HITRAN 2008 molecular spectroscopic database

Author

Rothman, L.S., Gordon, I.E., Barbe, A., Benner, D. Chris, Bernath, P.F., Birk, Manfred, Brown, L.R., Campargue, A., Champion, J.-P., Chance, K., Coudert, L.H., Dana, V., Devi, V.M., Fally, S., Flaud, J.-M., Gamache, R.R., Goldman, A., Jacquemart, D., Kleiner, I., Lacome, N., Lafferty, W.J., Mandin, J.Y., Massie, S.T., Mikhailenko, S.N., Miller, C.E., Moazzen-Ahmadi, N., Naumenko, O.V., Nikitin, A.V., Orphal, J., Perevalov, V.I., Perrin, A., Predoi-Cross, A., Rinsland, C.P., Rotger, M., Simeckova, M., Smith, M.A.H., Sung, K., Tashkun, S.A., Tennyson, J., Toth, R.A., Vandaele, A.C., and Vander Auwera, J.

Subjects
Spectroscopic database, HITRAN, Molecular absorption, Molecular spectroscopy
Published
2009

137. THE OXYGEN A BAND

Author

Devi, V., primary, Rupasinghe, Priyanka, additional, Bui, Thinh, additional, Okumura, Mitchio, additional, Drouin, Brian, additional, Sung, Keeyoon, additional, Long, David, additional, Hodges, Joseph, additional, Hoo, Jiajun, additional, and Benner, D., additional

Published
2014
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142. The HITRAN2012 molecular spectroscopic database

Author

UCL - SST/IMCN/NAPS - Nanoscopic Physics, Rothman, L.S., Gordon, I.E., Babikov, Y., Barbe, A., Chris Benner, D., Bernath, P.F., Birk, M., Bizzocchi, L., Boudon, V., Brown, L.R., Campargue, A., Chance, K., Cohen, E.A., Coudert, L.H., Devi, V.M., Drouin, B.J., Fayt, André, Flaud, J.-M., Gamache, R.R., Harrison, J.J., Hartmann, J.-M., Hill, C., Hodges, J.T., Jacquemart, D., Jolly, A., Lamouroux, J., Le Roy, R.J., Li, G., Long, D.A., Lyulin, O.M., Mackie, C.J., Massie, S.T., Mikhailenko, S., Müller, H.S.P., Naumenko, O.V., Nikitin, A.V., Orphal, J., Perevalov, V., Perrin, A., Polovtseva, E.R., Richard, C., Smith, M.A.H., Starikova, E., Sung, K., Tashkun, S., Tennyson, J., Toon, G.C., Tyuterev, Vl.G., Wagner, G., UCL - SST/IMCN/NAPS - Nanoscopic Physics, Rothman, L.S., Gordon, I.E., Babikov, Y., Barbe, A., Chris Benner, D., Bernath, P.F., Birk, M., Bizzocchi, L., Boudon, V., Brown, L.R., Campargue, A., Chance, K., Cohen, E.A., Coudert, L.H., Devi, V.M., Drouin, B.J., Fayt, André, Flaud, J.-M., Gamache, R.R., Harrison, J.J., Hartmann, J.-M., Hill, C., Hodges, J.T., Jacquemart, D., Jolly, A., Lamouroux, J., Le Roy, R.J., Li, G., Long, D.A., Lyulin, O.M., Mackie, C.J., Massie, S.T., Mikhailenko, S., Müller, H.S.P., Naumenko, O.V., Nikitin, A.V., Orphal, J., Perevalov, V., Perrin, A., Polovtseva, E.R., Richard, C., Smith, M.A.H., Starikova, E., Sung, K., Tashkun, S., Tennyson, J., Toon, G.C., Tyuterev, Vl.G., and Wagner, G.

Abstract

This paper describes the status of the latest edition of the HITRAN molecular spectroscopic compilation. The new edition is meant to replace the previous HITRAN edition of 2008 and its updates during the intervening years. The HITRAN molecular absorption compilation is comprised of six major components structured into folders that are freely accessible on the internet. These folders consist of the traditional line-by-line spectroscopic parameters required for high-resolution radiative-transfer codes, infrared absorption cross-sections for molecules not yet amenable to representation in a line-by-line form, ultraviolet spectroscopic parameters, aerosol indices of refraction, collision-induced absorption data, and general tables such as partition sums that apply globally to the data. The new HITRAN is greatly extended in terms of accuracy, spectral coverage, additional absorption phenomena, and validity. Molecules and isotopologues have been added that address the issues of atmospheres beyond the Earth. Also discussed is a new initiative that casts HITRAN into a relational database format that offers many advantages over the long-standing sequential text-based structure that has existed since the initial release of HITRAN in the early 1970s.

Published
2013

143. The HITRAN2012 molecular spectroscopic database

Author

Rothman, L. S., Gordon, I. E., Babikov, Y., Barbe, A., Benner, D. Chris, Bernath, P. F., Birk, M., Bizzocchi, L., Boudon, V., Brown, L. R., Campargue, A., Chance, K., Cohen, E. A., Coudert, L. H., Devi, V. M., Drouin, B. J., Fayt, A., Flaud, J. -M., Gamache, R. R., Harrison, J. J., Hartmann, J. -M., Hill, C., Hodges, J. T., Jacquemart, D., Jolly, A., Lamouroux, J., Le Roy, R. J., Li, G., Long, D. A., Lyulin, O. M., Mackie, C. J., Massie, S. T., Mikhailenko, S., Mueller, H. S. P., Naumenko, O. V., Nikitin, A. V., Orphal, J., Perevalov, V., Perrin, A., Polovtseva, E. R., Richard, C., Smith, M. A. H., Starikova, E., Sung, K., Tashkun, S., Tennyson, J., Toon, G. C., Tyuterev, Vl. G., Wagner, G., Rothman, L. S., Gordon, I. E., Babikov, Y., Barbe, A., Benner, D. Chris, Bernath, P. F., Birk, M., Bizzocchi, L., Boudon, V., Brown, L. R., Campargue, A., Chance, K., Cohen, E. A., Coudert, L. H., Devi, V. M., Drouin, B. J., Fayt, A., Flaud, J. -M., Gamache, R. R., Harrison, J. J., Hartmann, J. -M., Hill, C., Hodges, J. T., Jacquemart, D., Jolly, A., Lamouroux, J., Le Roy, R. J., Li, G., Long, D. A., Lyulin, O. M., Mackie, C. J., Massie, S. T., Mikhailenko, S., Mueller, H. S. P., Naumenko, O. V., Nikitin, A. V., Orphal, J., Perevalov, V., Perrin, A., Polovtseva, E. R., Richard, C., Smith, M. A. H., Starikova, E., Sung, K., Tashkun, S., Tennyson, J., Toon, G. C., Tyuterev, Vl. G., and Wagner, G.

Abstract

This paper describes the status of the 2012 edition of the HITRAN molecular spectroscopic compilation. The new edition replaces the previous HITRAN edition of 2008 and its updates during the intervening years. The HITRAN molecular absorption compilation is comprised of six major components structured into folders that are freely accessible on the internet. These folders consist of the traditional line-by-line spectroscopic parameters required for high-resolution radiative-transfer codes, infrared absorption cross-sections for molecules not yet amenable to representation in a line-by-line form, ultraviolet spectroscopic parameters, aerosol indices of refraction, collision-induced absorption data, and general tables such as partition sums that apply globally to the data. The new HITRAN is greatly extended in terms of accuracy, spectral coverage, additional absorption phenomena, and validity. Molecules and isotopologues have been added that address the issues of atmospheres beyond the Earth. Also discussed is a new initiative that casts HITRAN into a relational database format that offers many advantages over the long-standing sequential text-based structure that has existed since the initial release of HITRAN in the early 1970s. (C) 2013 Elsevier Ltd. All rights reserved.

Published
2013

144. A day in the life

Author

Benner, D. Cristopher

Subjects
Health care industry
Abstract

In addition to practicing in emergency medicine, I am a Fellow of the Academy of Wilderness Medicine, Wilderness Medical Society, and I volunteer with a search and rescue (SAR) team [...]

Published
2009

145. The 2009 edition of the GEISA spectroscopic database

Author

Université Pierre et Marie Curie, Ecole Polytechnique - Laboratoire de Météorologie Dynamique, Université Pierre et Marie Curie - Institut Pierre Simon Laplace, Université de Reims-Champagne-Ardenne - Groupe de Spectrométrie Moléculaire et Atmosphérique, Université Grenoble 1 - Laboratoire de Spectrométrie Physique, The College of William and Mary - Department of Physics, Williamsburg, USA, Universités Paris Diderot (Paris 7) et Paris EST-Créteil (UPEC), - Laboratoire Inter-Universitaire des Systèmes Atmosphériques, Universités Pierre et Marie Curie et Denis Diderot - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Université de Bourgogne - Laboratoire Interdisciplinaire Carnot de Bourgogne, UCL - SST/IMCN/NAPS - Nanoscopic Physics, Jacquinet-Husson, N., Poulet-Crovisier, N., Barbe, A., Campargue, A., Chris Benner, D., Jolly, A., Bézard, B., Boudon, V., Fayt, André, Université Pierre et Marie Curie, Ecole Polytechnique - Laboratoire de Météorologie Dynamique, Université Pierre et Marie Curie - Institut Pierre Simon Laplace, Université de Reims-Champagne-Ardenne - Groupe de Spectrométrie Moléculaire et Atmosphérique, Université Grenoble 1 - Laboratoire de Spectrométrie Physique, The College of William and Mary - Department of Physics, Williamsburg, USA, Universités Paris Diderot (Paris 7) et Paris EST-Créteil (UPEC), - Laboratoire Inter-Universitaire des Systèmes Atmosphériques, Universités Pierre et Marie Curie et Denis Diderot - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Université de Bourgogne - Laboratoire Interdisciplinaire Carnot de Bourgogne, UCL - SST/IMCN/NAPS - Nanoscopic Physics, Jacquinet-Husson, N., Poulet-Crovisier, N., Barbe, A., Campargue, A., Chris Benner, D., Jolly, A., Bézard, B., Boudon, V., and Fayt, André

Abstract

The updated 2009 edition of the spectroscopic database GEISA (Gestion et Etude des Informations Spectroscopiques Atmosphériques; Management and Study of Atmospheric Spectroscopic Information) is described in this paper. GEISA is a computer-accessible system comprising three independent sub-databases devoted, respectively, to: line parameters, infrared and ultraviolet/visible absorption cross-sections, microphysical and optical properties of atmospheric aerosols. In this edition, 50 molecules are involved in the line parameters sub-database, including 111 isotopologues, for a total of 3,807,997 entries, in the spectral range from 10−6 to 35,877.031 cm−1. The successful performances of the new generation of hyperspectral sounders depend ultimately on the accuracy to which the spectroscopic parameters of the optically active atmospheric gases are known, since they constitute an essential input to the forward radiative transfer models that are used to interpret their observations. Currently, GEISA is involved in activities related to the assessment of the capabilities of IASI (Infrared Atmospheric Sounding Interferometer; http://smsc.cnes.fr/IASI/index.htm) on board the METOP European satellite through the GEISA/IASI database derived from GEISA. Since the Metop-A (http://www.eumetsat.int) launch (19 October 2006), GEISA is the reference spectroscopic database for the validation of the level-1 IASI data. Also, GEISA is involved in planetary research, i.e., modeling of Titan's atmosphere, in the comparison with observations performed by Voyager, or by ground-based telescopes, and by the instruments on board the Cassini–Huygens mission. GEISA, continuously developed and maintained at LMD (Laboratoire de Météorologie Dynamique, France) since 1976, is implemented on the IPSL/CNRS (France) “Ether” Products and Services Centre WEB site (http://ether.ipsl.jussieu.fr), where all archived spectroscopic data can be handled through general and user friendly associated management so

Published
2011

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