PPT-  DETERMINATION OF METHANOL PHOTOLYSIS BRANCHING RATIOS VIA ROTATIONAL SPECTROSCOPY

Carson Powers Morgan N McCabe Susanna L Widicus Weaver Department of Chemistry Emory University Wednesday June 21 2017 Garrod R T Widicus Weaver S L amp Herbst E Astrophys J. Terra Alta/East Preston School. Rotational Symmetry. If, when you rotate a shape, it looks exactly the same as it did in its original position, then we say that the shape has . rotational symmetry. .. Dr . Babak. . masoumi. . Assistant Professor of Emergency Medicine, . Emergency Department, . Alzahra. General Hospital,. Isfahan University Of Medical Sciences. Methanol. . . . Bright young things, lasers and alcohol. Spitzer mid-IR image of the DR21 region in the Cygnus-X molecular complex. Image Credit: . NASA, Spitzer Space Telescope.. Aims of the project. To test our best models of methanol masers. in . the global chemical . transport model (GEOS-. Chem. ) . Cui . Ge. , Jun Wang. Department of Earth & Atmospheric Sciences. Joseph Francisco. Department of Chemistry. 4 May 2015. 7. th. GEOS-. Dr. Elijah I. Ohimain. Biological Sciences Department . Niger Delta University. Wilberforce Island, Nigeria. Food Safety & Regulatory Measures International conference . 17 -19 August 2015 Birmingham, UK. 4. Photolysis and Reactions of the Resulting Radicals. Robin Shannon, Mark Blitz, Mike Pilling, Dwayne Heard, . Paul Seakins. University of Leeds, UK. Background to Leeds. Leeds has long background in . © 2015 Pearson Education, Inc.. This lecture will help you understand:. Circular Motion . Rotational Inertia. Torque. Center of Mass and Center of Gravity. Centripetal Force. Centrifugal Force. Rotating Reference Frames. Vikram Rao . Research Triangle Energy Consortium. June 13, 2017. DISTRIBUTED PRODUCTION OF FUELS. MAKES SENSE IF. Raw material is highly distributed. OR. Fuel use points are highly distributed. DISTRIBUTED RAW MATERIAL. in . a room temperature . flow reactor . . Daniel . zaleski. ,. . lawrence. . Harding, . stephen. . klippenstein. , . branko. . ruscic. , . Kirill prozument. Argonne National Laboratory. Chemical Sciences & Engineering Division. Houston Smith, AJ Mesko, and Susanna L. Widicus Weaver. Department of Chemistry, Emory University. Stefanie Milam. NASA GSFC. Interstellar medium (ISM) is abundant in chemical species in star-forming regions. 2. C. DANIEL WITSCH, VOLKER LUTTER, GUIDO W. FUCHS, . THOMAS GIESEN. Institute of Physics, University of Kassel, Germany. JÜRGEN GAUSS,. Institut. . für. . Physikalische. . Chemie. , Universität Mainz, Germany. Infrared (Vibrational). Raman (Rotational & Vibrational) . Texts. “Physical Chemistry”, 6th edition, . Atkins. “Fundamentals of Molecular Spectroscopy”, 4th edition, . Banwell & McCash. 2. UV Spectroscopy. Introduction. UV radiation and Electronic Excitations. The difference in energy between molecular bonding, non-bonding and anti-bonding orbitals ranges from 125-650 kJ/mole. This energy corresponds to EM radiation in the ultraviolet (UV) region, 100-350 nm, and visible (VIS) regions 350-700 nm of the spectrum. 2. Nuclear Magnetic Resonance Spectroscopy. After hydrogen, the most useful atom providing information is carbon-13.. The . overall intensity of a . 13. C signal is about 6400 . times . less than the intensity of an .