Ernest Meissonier: Master In His Genre

This study documents the career of one of the most widely known French artists of the nineteenth century. The embodiment of mainstream taste, Jean-Louis-Ernest Meissonier was scorned by the avant-garde, but his jewellike genre paintings were highly regarded by his middle-class audience. Examining his art in detail, Constance Cain Hungerford follows Meissonier from his formation as a wood engraving designer to his virtuous production of small scale genre scenes, his larger battlefield paintings, and his several images of modern revolution and war. Also analyzed are the state administered exhibition system, which Meissonier worked to his advantage, and developments in the marketing of art, both in Europe and in the United States

Protons in near earth orbit

The proton spectrum in the kinetic energy range 0.1 to 200 GeV was measured by the Alpha Magnetic Spectrometer (AMS) during space shuttle flight STS-91 at an altitude of 380 km. Above the geomagnetic cutoff the observed spectrum is parameterized by a power law. Below the geomagnetic cutoff a substantial second spectrum was observed concentrated at equatorial latitudes with a flux ~ 70 m^-2 sec^-1 sr^-1. Most of these second spectrum protons follow a complicated trajectory and originate from a restricted geographic region.Comment: 19 pages, Latex, 7 .eps figure

Search for antihelium in cosmic rays

The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 in a 51.7 degree orbit at altitudes between 320 and 390 km. A total of 2.86 * 10^6 helium nuclei were observed in the rigidity range 1 to 140 GV. No antihelium nuclei were detected at any rigidity. An upper limit on the flux ratio of antihelium to helium of < 1.1 * 10^-6 is obtained.Comment: 18 pages, Latex, 9 .eps figure

A Study of Cosmic Ray Secondaries Induced by the Mir Space Station Using AMS-01

The Alpha Magnetic Spectrometer (AMS-02) is a high energy particle physics experiment that will study cosmic rays in the $\sim 100 \mathrm{MeV}$ to $1 \mathrm{TeV}$ range and will be installed on the International Space Station (ISS) for at least 3 years. A first version of AMS-02, AMS-01, flew aboard the space shuttle \emph{Discovery} from June 2 to June 12, 1998, and collected $10^8$ cosmic ray triggers. Part of the \emph{Mir} space station was within the AMS-01 field of view during the four day \emph{Mir} docking phase of this flight. We have reconstructed an image of this part of the \emph{Mir} space station using secondary $\pi^-$ and $\mu^-$ emissions from primary cosmic rays interacting with \emph{Mir}. This is the first time this reconstruction was performed in AMS-01, and it is important for understanding potential backgrounds during the 3 year AMS-02 mission.Comment: To be submitted to NIM B Added material requested by referee. Minor stylistic and grammer change

Cosmic-ray positron fraction measurement from 1 to 30 GeV with AMS-01

A measurement of the cosmic ray positron fraction e+/(e+ + e-) in the energy range of 1-30 GeV is presented. The measurement is based on data taken by the AMS-01 experiment during its 10 day Space Shuttle flight in June 1998. A proton background suppression on the order of 10^6 is reached by identifying converted bremsstrahlung photons emitted from positrons

The biology of micrometastases from uveal melanoma

Background The aim of this study was to investigate the possible causes of tumour latency in uveal melanoma primarily through the analysis of micrometastases in tissue obtained from donors postmortem. Various explanations have been proposed but there is no clear answer from animal studies and few human data. The main hypotheses may be divided into several areas-immunological control of metastatic cells, lack of angiogenesis within micrometastases and reduced cell turnover. Methods 196 patients were recruited to the study between 2003 and 2007. Patients were invited to take part and their relatives agreed to postmortem examination of their liver and lungs in the event of their death, including tissue sampling to assess the presence of micrometastases and their biology. Metastatic cells were detected by immunohistochemistry using a pan-melanoma antibody reagent, and by quantitative reverse transcriptase (qRT)-PCR for three melanoma-associated genes (tyrosinase Melan-A, and gp100) and a housekeeping gene (HMBS/PBGD) in samples stored in RNAlater or as formalin-fixed paraffin-embedded tissue. Results 22 deaths were investigated at autopsy as part of the study. Sixteen patients died with large deposits of metastatic melanoma, while six patients died of other causes. In addition, a liver resection for hepatic adenoma provided further tissue from a case without clinical evidence of metastasis. Metastatic melanoma cells were identified by immunohistochemistry of the liver samples in one case and by qRT-PCR in two further cases without macrometastases. There was no evidence of multicellular micrometastases sufficiently large to require angiogenesis and no associated inflammation was observed. Conclusion The most likely explanation for latency in this setting is the inability of uveal melanoma cells in metastatic sites to grow.Ophthalmic researc