4,466 research outputs found

    Radio signals from very large showers

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    Radio signals from air showers with electron sizes in the range 1 x 10 to the 7th power to 2 x 10 to the 9th power were detected at 50kHz, 170kHz, and 1,647kHz at large core distances in the Akeno square kilometers air-shower array. The field strength is higher than that expected from any mechanisms hitherto proposed

    Altitude variations of cosmic-ray soft and hard components observed by airborne detectors

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    The altitude variations of cosmic-ray total and hard components were measured up to 12,000 m on board a jet liner over Japan island on December, 1981. Observed results together with soft component are presented comparing with the model calculations through the atmosphere by applying the hadronic cascade

    Arrival time distributions of electrons in air showers with primary energies above 10 (18)eV observed at 900m above sea level

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    Detection of air showers with primary energies above 10 to the 19th power eV with sufficient statistics is extremely important in an astrophysical aspect related to the Greisen cut off and the origin of such high energy cosmic rays. Recently, a method is proposed to observe such giant air showers by measuring the arrival time distributions of air-shower particles at large core distances with a mini array. Experiments to measure the arrival time distributions of muons were started in 1981 and those of electrons in early 1983 in the Akeno air-shower array (930 gcm cm squared atmospheric depth, 900m above sea level). During the time of observation, the detection area of the Akeno array was expanded from 1 sq km to sq km in 1982 and to 20 sq km in 1984. Now the arrival time distribution of electrons and muons can be measured for showers with primary energies above 1019eV at large core distances

    Longitudinal development of muons in large air showers studies from the arrival time distributions measured at 900m above sea level

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    The arrival time distributions of muons with energies above 1.0GeV and 0.5GeV have been measured in the Akeno air-shower array to study the longitudinal development of muons in air showers with primary energies in the range 10 to the 17th power to 10 to the 18th power ev. The average rise times of muons with energies above 1.0GeV at large core distances are consistent with those expected from very high multiplicity models and, on the contrary, with those expected from the low multiplicity models at small core distances. This implies that the longitudinal development at atmospheric depth smaller than 500 cm square is very fast and that at larger atmospheric depths is rather slow

    Preparation and in vitro evaluation of primaquine-conjugated gum arabic microspheres

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    Gum arabic, a branched polysaccharide, was oxidized using periodate to generate reactive aldehyde groups on the biopolymer. Primaquine, an 8-aminoquinoline, was covalently coupled onto oxidized gum arabic via an imine bond and simultaneously fabricated into microspheres of less than 2 μm in size by heat denaturation in a reverse emulsion of 1:1 light paraffin oil and toluene stabilized by sorbitan sesquioleate as the surfactant. The covalent binding of primaquine to the polysaccharide using the clinically used water-soluble form of the drug primaquine phosphate was achieved in the presence of borate buffer of pH 11. Up to 35% of the drug could be bound to the polymer backbone depending on the concentration of the drug employed initially and the degree of oxidation of the polysaccharide. Interestingly, both the aliphatic and the hindered aromatic amino groups of primaquine were found to react with the aldehyde functions through Schiff base formation leading to cross-linking of the polysaccharide with the drug itself. In vitro release of the drug from microspheres into phosphate buffered saline (PBS, pH 7.4, 0.1 M) at 37 °C showed that the release of primaquine from the matrix was slow, although gradually increased with time. The maximum released was below 50% of the drug payload even after 10 days. Release into simulated gastric and intestinal fluids was faster compared to the release in PBS due to rapid hydrolysis of the Schiff's linkage in the gastric fluid. A possible reason for the poor hydrolytic susceptibility of the Schiff's linkage is suggested based on the unequal reactivity of the amino groups on primaquine and its relevance in possible therapeutic application of this polymer-drug conjugate discussed
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