Deposits of clastic carbonate-dominated (calciclastic) sedimentary slope systems in the rock record have been identified mostly as linearly-consistent carbonate apron deposits, even though most ancient clastic carbonate slope deposits fit the submarine fan systems better. Calciclastic submarine fans are consequently rarely described and are poorly understood. Subsequently, very little is known especially in mud-dominated calciclastic submarine fan systems. Presented in this study are a sedimentological core and petrographic characterisation of samples from eleven boreholes from the Lower Carboniferous of Bowland Basin (Northwest England) that reveals a >250 m thick calciturbidite complex deposited in a calciclastic submarine fan setting. Seven facies are recognised from core and thin section characterisation and are grouped into three carbonate turbidite sequences. They include: 1) Calciturbidites, comprising mostly of highto low-density, wavy-laminated bioclast-rich facies; 2) low-density densite mudstones which are characterised by planar laminated and unlaminated muddominated facies; and 3) Calcidebrites which are muddy or hyper-concentrated debrisflow deposits occurring as poorly-sorted, chaotic, mud-supported floatstones. These

Phd by thesis

There is a special reason for reviewing this book at this time: it is the 50th edition of a compendium that is known and used frequently in most chemical and physical laboratories in many parts of the world. Surely, a publication that has been published for 56 years, withstanding the vagaries of science in this century, must have had something to offer. There is another reason: while the book is a standard fixture in most chemical and physical laboratories, including those in medical centers, it is not as frequently seen in the laboratories of physician's offices (those either in solo or group practice). I believe that the Handbook can be useful in those laboratories. One of the reasons, among others, is that the various basic items of information it offers may be helpful in new tests, either physical or chemical, which are continuously being published. The basic information may relate

Handbook of Chemistry and Physics

We present the fifth release of the UMIST Database for Astrochemistry (UDfA). The new reaction network contains 6173 gas-phase reactions, involving 467 species, 47 of which are new to this release. We have updated rate coefficients across all reaction types. We have included 1171 new anion reactions and updated and reviewed all photorates. In addition to the usual reaction network, we also now include, for download, state-specific deuterated rate coefficients, deuterium exchange reactions and a list of surface binding energies for many neutral species. Where possible, we have referenced the original source of all new and existing data. We have tested the main reaction network using a dark cloud model and a carbon-rich circumstellar envelope model. We present and briefly discuss the results of these models.

The UMIST database for astrochemistry 2012

As brown dwarfs cool, a variety of species condense in their atmospheres, forming clouds. Iron and silicate clouds shape the emergent spectra of L dwarfs, but these clouds dissipate at the L/T transition. A variety of other condensates are expected to form in cooler T dwarf atmospheres. These include Cr, MnS, Na2S, ZnS, and KCl, but the opacity of these optically thinner clouds has not been included in previous atmosphere models. Here, we examine their effect on model T and Y dwarf atmospheres. The cloud structures and opacities are calculated using the Ackerman & Marley (2001) cloud model, which is coupled to an atmosphere model to produce atmospheric pressure-temperature profiles in radi ative-convective equilibrium. We generate a suite of models between Teff = 400 and 1300 K, log g=4.0 and 5.5, and condensate sedimentation efficiencies fro m fsed=2 to 5. Model spectra are compared to two red T dwarfs, Ross 458C and UGPS 0722‐05; models that include clouds are found to match observed spectra significa ntly better than cloudless models. The emergence of sulfide clouds in cool atmospheres, particularly Na 2S, may be a more natural explanation for the “cloudy” spectra of these objects, rather than the re-emergence of si licate clouds that wane at the L-to-T transition. We find that sulfide clouds provide a mechanism to match the near- and mid-infrared colors of observed T dwarfs. Our results indicate that including the opacity of condensa tes in T dwarf atmospheres is necessary to accurately determine the physical characteristics of many of the obser ved objects. Subject headings:brown dwarfs — stars: atmospheres

Neglected Clouds in T and Y Dwarf Atmospheres

The ExoMol database: Molecular line lists for exoplanet and other hot atmospheres

/pdf/erratum-new-investigation-of-the-n3-c-h-stretching-region-of-56zu9nlq2s.pdf

Erratum: "New investigation of the ν3 C-H stretching region of 12CH4 through the analysis of high temperature infrared emission spectra" [J. Chem. Phys. 148, 134306 (2018)].

http://manuscript.elsevier.com/S0022285222000261/pdf/S0022285222000261.pdf

Analytical expression of tensorial rotational operators for semi-classical interpretation of molecular spectra. Relations between molecular Hamiltonian parameters in different formalisms

High-Resolution spectroscopy and analysis of the fundamental modes of 28SiF4. Accurate experimental determination of the Si−F bond length

Line Positions and Intensities for the ν_3 Band of 5 Isotopologues of Germane for Planetary Applications

A metal sputtering source suitable for laboratory production of metal hydrides is described. Sputtering from pure nickel or iron in an Ar/H2 discharge is analyzed at low resolution. High resolution laser excitation and dispersed fluorescence spectra of NiH have also been recorded. The source has been designed to operate with a ferromagnetic circuit for Zeeman spectroscopy. Signals from the source are strong enough to record dispersed fluorescence from NiH by Fourier transform interferometry in magnetic fields up to 1 T. We establish that FeH can also be formed in this source.

Cyril Richard

Papers

Erratum: "New investigation of the ν3 C-H stretching region of 12CH4 through the analysis of high temperature infrared emission spectra" [J. Chem. Phys. 148, 134306 (2018)].

Analytical expression of tensorial rotational operators for semi-classical interpretation of molecular spectra. Relations between molecular Hamiltonian parameters in different formalisms

High-Resolution spectroscopy and analysis of the fundamental modes of 28SiF4. Accurate experimental determination of the Si−F bond length

Line Positions and Intensities for the ν_3 Band of 5 Isotopologues of Germane for Planetary Applications

Room-Temperature Metal—Hydride Discharge Source, with Observations on NiH and FeH.