Radio - Orchestra and String Quartet

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Radio - Orchestra and String Quartet

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Radio - Orchestra and String Quartet

Val Coffey, Frederick Broeder, and Karl Chase

Radio - Orchestra and String Quartet

Maurice Warner, Frederick Broeder, and Val Coffey,

Radio - Orchestra and String Quartet

Maurice Warner, Karl Chase, Frederick Broeder, and Ray Hancock

Radio - Orchestra and String Quartet

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Radio - Orchestra and String Quartet

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Guerra-Peixe: arranjador de orquestras de rádio

Revisão biográfica sobre o músico brasileiro Guerra-Peixe e sua carreira como arranjador de orquestras de rádio. Objetiva-se compreender como compositores clássicos, como Guerra-Peixe, encontraram na esfera popular um meio de vida. Inclui dados biográficos pouco conhecidos sobre o compositor.

Arranjos de Guerra-Peixe para a orquestra da Rádio Nacional do Rio de Janeiro

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Radio - Birthday Party - 12th Anniversary

Note attached: In background are members of the orchestra, and in the foreground are some of those who had individual parts in the performance. Jefferson B. Webb, station manager, is in the center, with Reta Alcock, child actress, seated on his knee. Others seated from left to right, are Wynn Wright, actor in the sketch "The Night Express"; Ole Foersch, director of the orchestra; Miss Alcock, Mr. Webb. Mr. Webb and Marion Martin, pianist. Standing directly back of them are Frances Harris, soprano; B.D. Welling, actor in the sketch; Kathryn Young, Soprano soloist; Ty Tyson, announcer; Helen Kennedy Snyder, contralto; Rex White, station dramatist; Arnold Tieman, announcer; Wilfred Engelman, Baritone soloist. Among these in center background are Herschell Hart, announcer, and C.C. Bradner, who gave News Bulletins founded on Page One events of twelve years ago. 12th Anniversary: Aug. 20, 1932

Sintonizando emoções : o futebol e o radio : uma viagem nas ondas da midia radiofonica

Universidade Estadual de Campinas . Faculdade de Educação Física

Populations III.1 and III.2 gamma-ray bursts: constraints on the event rate for future radio and X-ray surveys

Aims. We calculate the theoretical event rate of gamma-ray bursts (GRBs) from the collapse of massive first-generation (Population III; Pop III) stars. The Pop III GRBs could be super-energetic with the isotropic energy up to E(iso) greater than or similar to 10(55-57) erg, providing a unique probe of the high-redshift Universe. Methods. We consider both the so-called Pop III.1 stars (primordial) and Pop III.2 stars (primordial but affected by radiation from other stars). We employ a semi-analytical approach that considers inhomogeneous hydrogen reionization and chemical evolution of the intergalactic medium. Results. We show that Pop III.2 GRBs occur more than 100 times more frequently than Pop III.1 GRBs, and thus should be suitable targets for future GRB missions. Interestingly, our optimistic model predicts an event rate that is already constrained by the current radio transient searches. We expect similar to 10-10(4) radio afterglows above similar to 0.3 mJy on the sky with similar to 1 year variability and mostly without GRBs (orphans), which are detectable by ALMA, EVLA, LOFAR, and SKA, while we expect to observe maximum of N < 20 GRBs per year integrated over at z > 6 for Pop III.2 and N < 0.08 per year integrated over at z > 10 for Pop III.1 with EXIST, and N < 0.2 for Pop III.2 GRBs per year integrated over at z > 6 with Swift.

Radio-frequency spectroscopy of (6)Li p-wave molecules: Towards photoemission spectroscopy of a p-wave superfluid

We study rf spectroscopy of a lithium gas with the goal to explore the possibilities for photoemission spectroscopy of a strongly interacting p-wave Fermi gas. Radio-frequency spectra of quasibound p-wave molecules and of free atoms in the vicinity of the p-wave Feshbach resonance located at 159.15G are presented. The spectra are free of detrimental final-state effects. The observed relative magnetic-field shifts of the molecular and atomic resonances confirm earlier measurements realized with direct rf association. Furthermore, evidence of molecule production by adiabatically ramping the magnetic field is observed. Finally, we propose the use of a one-dimensional optical lattice to study anisotropic superfluid gaps as most direct proof of p-wave superfluidity.

Calculating current densities and fields due to shielded bi-planar radio-frequency coils

A method for the accurate computation of the current densities produced in a wide-runged bi-planar radio-frequency coil is presented. The device has applications in magnetic resonance imaging. There is a set of opposing primary rungs, symmetrically placed on parallel planes and a similar arrangement of rungs on two parallel planes surrounding the primary serves as a shield. Current densities induced in these primary and shielding rungs are calculated to a high degree of accuracy using an integral-equation approach, combined with the inverse finite Hilbert transform. Once these densities are known, accurate electrical and magnetic fields are then computed without difficulty. Some test results are shown. The method is so rapid that it can be incorporated into optimization software. Some preliminary fields produced from optimized coils are presented.