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Radiation belt particles of the inner magnetosphere precipitate into the atmosphere in the subauroral regions when they are pitch-angle scattered into the loss cone by wave-particle interactions. Such particle precipitations are known to be especially enhanced during space storms, though they can also occur during quiet times. The observed characteristics of precipitating electrons can be distinctively different, in their time series as well as in their spectra, depending on the waves involved. The present paper describes the High Energy Particle Detector (HEPD) on board the Next Generation Small Satellite-1 (NEXTSat-1), which will measure these radiation belt electrons from a low-Earth polar orbit satellite to study the mechanisms related to electron precipitation in the sub-auroral regions. The HEPD is based on silicon barrier detectors and consists of three telescopes that are mounted on the satellite to have angles of 0 ◦, 45 ◦, and 90 ◦, respectively with the local geomagnetic field during observations. With a high time resolution of 32 Hz and a high spectral resolution of 11 channels over the energy range from ~ 350 keV to ~ 2 MeV, together with the pitch angle information provided by the three telescopes, HEPD is capable of identifying physical processes, such as microbursts and dust-side relativistic electron precipitation (DREP) events associated with electron precipitations. NextSat-1 is scheduled for launch in early 2018.

Chicken is one of the most popular domesticated species worldwide, as it can serve an important role in agricultural as well as biomedical research fields. Because it inhabits almost every continent and presents diverse morphology and traits, the need of genetic markers for distinguishing each breed for various purposes has increased. The whole genome sequencing of three different breeds (White Leghorn, Korean domestic, and Araucana) that show similar coloring patterns, with the exception of the White Leghorn breed, have confirmed previously reported genomic alterations and identified many novel variants. Additionally, the Whole Genome Re-Sequencing (WGRS) approach identified an approximately 4 kb insert within SLCO1B3 responsible for blue egg shell color. Targeted investigation of pigment-related genes corroborated previously reported non-synonymous mutations, and provided deeper insight into chicken coloring, where not a single but a combination of non-synonymous mutations in the MC1R gene is likely to be responsible for altered feather coloring. [ABSTRACT FROM AUTHOR]