Galactic cosmic rays consist of protons, electrons and ions, most of which are believed to be accelerated to relativistic speeds in supernova remnants. All components of the cosmic rays show an intensity that decreases as a power law with increasing energy (for example as E(-2.7)). Electrons in particular lose energy rapidly through synchrotron and inverse Compton processes, resulting in a relatively short lifetime (about 10(5) years) and a rapidly falling intensity, which raises the possibility of seeing the contribution from individual nearby sources (less than one kiloparsec away). Here we report an excess of galactic cosmic-ray electrons at energies of approximately 300-800 GeV, which indicates a nearby source of energetic electrons. Such a source could be an unseen astrophysical object (such as a pulsar or micro-quasar) that accelerates electrons to those energies, or the electrons could arise from the annihilation of dark matter particles (such as a Kaluza-Klein particle with a mass of about 620 GeV).

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-The final results of processing the data from the balloon-born experiment ATIC-2 (Antarctica, 2002(Antarctica, -2003 for the energy spectra of protons and He, C, O, Ne, Mg, Si, and Fe nuclei, the spectrum of all particles, and the mean logarithm of atomic weight of primary cosmic rays as a function of energy are presented. The final results are based on improvement of the methods used earlier, in particular, considerably increased resolution of the charge spectrum. The preliminary conclusions on the significant difference in the spectra of protons and helium nuclei (the proton spectrum is steeper) and the non-power character of the spectra of protons and heavier nuclei (flattening of carbon spectrum at energies above 10 TeV) are confirmed. A complex structure of the energy dependence of the mean logarithm of atomic weight is found.

A 67-nucleotide portion of the non-coding, 5'-leader sequence of tobacco mosaic virus RNA [defined as omega' (Gr. omega prime)] has been shown to enhance the translation of contiguous foreign gene transcripts both in vitro and in vivo. Chemically-synthesized omega', containing convenient linker sequences, was inserted into derivatives of an in vitro transcription plasmid (pSP64) between the bacteriophage-SP6 promoter and sequences coding for either chloramphenicol acetyltransferase (CAT) or neomycin phosphotransferase (NPTII). Run-off in vitro transcripts, with or without a 5'-cap structure (G(5')ppp(5')G) and/or the omega' sequence, were tested in mRNA-dependent cell-free translation systems derived from rabbit reticulocyte lysate, wheat germ extract or Escherichia coli (MRE 600). In all cases, the presence of omega' increased the translational expression of both reporter genes, typically between 2- to 10-fold. Electroporation of isolated mesophyll protoplasts from Nicotiana tabacum cv. Xanthi, or microinjection of oocytes from Xenopus laevis, with SP6-transcripts containing the CAT-coding region confirmed and extended the value of omega' as a potential translational enhancer of gene expression in vivo.

Measurements of the cosmic-ray hydrogen and helium spectra at energies from 20 to 800 TeV are presented. The experiments were performed on a series of twelve balloon Ñights, including several long duration Australia to South America and Antarctic circumpolar Ñights. No clear evidence is seen for a spectral break. Both the hydrogen and the helium spectra are consistent with power laws over the entire energy range, with integral spectral indices 1.80^0.04 and for the protons and helium, respec-1.68~0 .06 0.04 tively. The results are fully consistent with expectations based on supernova shock acceleration coupled with a "" leaky box ÏÏ model of propagation through the Galaxy.