181,628 research outputs found

    Group portrait / Perry, J.B.; Rosner, R. / 240 Robert; ABC-TV / 1963

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    Producer is Lehigh grad (rosner r;) (News release attached

    Group portrait / Perry, J.B.; Rosner, R. / 240 Robert; ABC-TV / 1963

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    Producer is Lehigh grad (rosner r;) (News release attached

    Box 56, Neg. No. 51522: Clarence Rosner

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    This black and white photograph features a portrait of Clarence Rosner - he is standing next to a wooden chair and is wearing a suit. Clarence Rosner ordered the photograph. Mr. Gray\u27s ledger indicated this photo should be sent to Clarence Rosner in care of John Lindsay, Macksville, Kansas.https://scholars.fhsu.edu/stafford_county/7436/thumbnail.jp

    Behavioural state affects motion-sensitive neurones in the fly visual system

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    Rosner R, Egelhaaf M, Warzecha A-K. Behavioural state affects motion-sensitive neurones in the fly visual system. JOURNAL OF EXPERIMENTAL BIOLOGY. 2010;213(2):331-338

    Variability of blowfly head optomotor responses

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    Rosner R, Egelhaaf M, Grewe J, Warzecha A-K. Variability of blowfly head optomotor responses. Journal of Experimental Biology. 2009;212(8):1170-1184

    Appropriate Similarity Measures for Author Cocitation Analysis

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    We provide a number of new insights into the methodological discussion about author cocitation analysis. We first argue that the use of the Pearson correlation for measuring the similarity between authors’ cocitation profiles is not very satisfactory. We then discuss what kind of similarity measures may be used as an alternative to the Pearson correlation. We consider three similarity measures in particular. One is the well-known cosine. The other two similarity measures have not been used before in the bibliometric literature. Finally, we show by means of an example that our findings have a high practical relevance.information science;Pearson correlation;cosine;similarity measure;author cocitation analysis

    Sposób i układ do wykrywania nierówności ciągów prowadników naczyń wyciągowych opis patentowy nr 194002 /

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    Tyt. z ekranu tyt.Pozostali twórcy wynalazku: Zbigniew Łowkis, Witold Rataj, Zbigniew Rosner, Jerzy Tobys, Jerzy Stępień.Zgłoszono 16 czerwca 2000.Zgłoszenie ogłoszono 17 grudnia 2001 r. BUP 26/01.Opublikowano 30 kwietnia 2007 r. WUP 04/07.Dostępny również w wersji drukowanej.Tryb dostępu: Internet

    "Closing the R&D Gap, Evaluating the Sources of R&D Spending"

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    Both spending and tax policies have been implemented in the United States with the goal of stimulating private sector research and development (R&D). Karier questions whether current R&D policy, especially the research and experimentation tax credit, can contribute to closing the gap between nondefense expenditures on R&D in the United States and such expenditures in other countries, such as Japan and Germany. He also explores possible changes to our current R&D policy to make it more effective.

    X-rays from protostellar jets: emission from continuous flows

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    Context: Recently X-ray emission from protostellar jets has been detected with both XMM-Newton and Chandra satellites, but the physical mechanism which can give rise to this emission is still unclear. Aims: We performed an extensive exploration of the parameter space for the main parameters influencing the jet/ambient medium interaction. Aims include: 1) to constrain the jet/ambient medium interaction regimes leading to the X-ray emission observed in Herbig-Haro objects in terms of the emission by a shock forming at the interaction front between a continuous supersonic jet and the surrounding medium; 2) to derive detailed predictions to be compared with optical and X-ray observations of protostellar jets; 3) to get insight into the protostellar jet's physical conditions. Methods: We performed a set of two-dimensional hydrodynamic numerical simulations, in cylindrical coordinates, modeling supersonic jets ramming into a uniform ambient medium. The model takes into account the most relevant physical effects, namely thermal conduction and radiative losses. Results: Our model explains the observed X-ray emission from protostellar jets in a natural way. In particular, we find that a protostellar jet that is less dense than the ambient medium well reproduces the observations of the nearest Herbig-Haro object, HH 154, and allows us to make detailed predictions of a possible X-ray source proper motion (v_sh ≈500 km s-1) detectable with Chandra. Furthermore, our results suggest that the simulated protostellar jets which best reproduce the X-rays observations cannot drive molecular outflows
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