Research and development of magnesium/aluminum electroforming process for solar concentrators Final report, 13 May 1966 - 10 May 1967

Magnesium and aluminum electroforming process for solar concentrator

Distinct Scaling Regimes of Energy Release Dynamics in the Nighttime Magnetosphere

Based on a spatiotemporal analysis of POLAR UVI images, we show that the auroral emission events that initiate equatorward of the isotropic boundary (IB) obtained from a time-dependent empirical model, have systematically steeper power-law slopes of energy, power, area and lifetime probability distributions compared to the events that initiate poleward of the IB. The low-latitude group of events contains a distinct subpopulation of substorm-scale disturbances violating the power-law behavior, while the high latitude group is described by nearly perfect power-law statistics over the entire range of scales studied. The results obtained indicate that the inner and outer portions of the plasma sheet are characterized by substantially different scaling regimes of bursty energy dissipation suggestive of different physics in these regions.Comment: 11 pages, 2 figures, 2 table

Radial distribution of the inner magnetosphere plasma pressure using low-altitude satellite data during geomagnetic storm: the March 1-8, 1982 Event

Plasma pressure distribution in the inner magnetosphere is one of the key parameters for understanding the main magnetospheric processes including geomagnetic storms and substorms. However, the pressure profiles obtained from in-situ particle measurements by the high-altitude satellites do not allow tracking the pressure variations related to the storms and substorms, because a time interval needed to do this generally exceeds the characteristic times of them. On contrary, fast movement of low-altitude satellites makes it possible to retrieve quasi-instantaneous profiles of plasma pressure along the satellite trajectory, using the fluxes of precipitating particles. For this study, we used the Aureol-3 satellite data for plasma pressure estimation, and the IGRF, Tsyganenko 2001 and Tsyganenko 2004 storm time geomagnetic field models for the pressure mapping into the equatorial plane. It was found that during quiet geomagnetic condition the radial pressure profiles obtained coincide with the profiles, obtained previously from the high-altitude measurements. On the contrary, it was found that during geomagnetic storm the plasma pressure profiles became sharper; the position of the maximum of plasma pressure corresponds to expected one for given Dst minimum; the maximum value of inner magnetosphere static pressure correlates with the solar wind dynamic pressure. Increase in the plasma pressure profiles indicates the possibility to consider the interchange instability as one of important factors for the development of the main phase of geomagnetic storm.Comment: Accepted in Advances in Space Researc

Pisum Sativum L. cultivars : characterization and identification by electrophoresis of total seed proteins

Se realizó el estudio electroforético de proteínas seminales totales de 13 cultivares de arveja (Pisum sativum L.) en geles de poliacrilamida con Sodio Dodecil Sulfato. Se logró fraccionar 53 bandas proteicas, de las cuales 36 mostraron diferencias en sus movilidades. De esta manera se obtuvieron modelos electroforéticos diferentes para cada cultivar y mediante análisis de conglomerados (método UPGMA) se obtuvo un dendrograma que mostró la distinción entre cultivares en dicho carácter, permitiendo expresar las diferencias entre ellos.Electrophoretic study of reduced total seed proteins of 13 pea cultivars has been carried on polyacrylamide gels in the presence of Sodium Dodecyl Sulphate. The pea seed storage proteins were electrophoretically separated in 53 bands; 36 of them showed qualitative differences and allowed the characterization of the cultivars. Standard reference patterns of each cultivar were obtained on this basis. UPGMA analysis was performed on the gels and in the resulting dendrogram 12 clusters of different orders have been determined. Intervarietal differences were clearly expressed.Fil: Cevedo, Alicia M. L..Fil: Galussi, Alberto A..Fil: Lui, Lino M.