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21.
O. Adriani  G. A. Bazilevskaya  G. C. Barbarino  R. Bellotti  M. Boezio  E. A. Bogomolov  L. Bonechi  M. Bongi  V. Bonvicini  S. V. Borisov  S. Bottai  A. Bruno  F. Cafagna  D. Campana  P. Carlson  M. Casolino  G. Castellini  M. P. De Pascale  G. De Rosa  D. Fedele  V. Di Felice  A. M. Galper  L. A. Grishantseva  P. Hofverberg  A. A. Leonov  S. V. Koldashov  S. Yu. Krutkov  A. N. Kvashnin  V. Malvezzi  L. Marcelli  W. Menn  V. V. Mikhailov  M. Minori  E. Mocchiutti  S. Orsi  G. Osteria  P. Papini  M. Pearce  P. Picozza  M. Ricci  S. B. Ricciarini  M. Simon  N. De Simone  R. Sparvoli  P. Spillantini  Yu. I. Stozhkov  E. Taddei  A. Vacchi  E. Vannuccini  G. V. Vasil’ev  S. A. Voronov  Yu. T. Yurkin  G. Zampa  N. Zampa  V. G. Zverev 《Bulletin of the Russian Academy of Sciences: Physics》2009,73(5):568-570
The PAMELA experiment is being carried out on board the Russian satellite Resurs DK1 placed in the near-earth near-polar orbit on June 15, 2006. The apparatus comprising a silicon-strip magnetic spectrometer and an electromagnetic calorimeter allows measurement of electron and positron fluxes in cosmic rays in a wide energy interval from ~100 MeV to hundreds of GeV. The high-energy electron and positron separation technique is discussed and the data on positron-to-electron ratio in primary cosmic rays up to E ≈ 10 GeV from the 2006–2007 measurements are reported in this work.  相似文献   
22.
Marrocchesi  P. S.  Adriani  O.  Akaike  Y.  Asaoka  Y.  Berti  E.  Bigongiari  G.  Bongi  M.  Brogi  P.  Bruno  A.  Cannady  N.  Checchia  C.  Cherry  M. L.  Collazuol  G.  Ficklin  A. W.  Guzik  T. G.  Ichimura  M.  Israel  M. H.  Kasahara  K.  Kawakubo  Y.  Krizmanic  J. F.  Messineo  A. M.  Mitchell  J. W.  Miyake  S.  Mori  M.  Mori  N.  Motz  H. M.  Munakata  K.  Pacini  L.  Palma  F.  Papini  P.  Rauch  B. F.  Ricciarini  S. B.  Sakamoto  T.  Sasaki  M.  Stolzi  F.  Sulaj  A.  Tamura  T.  Torii  S.  Wefel  J. P.  Yoshida  K.  Zober  W. V. 《Physics of Atomic Nuclei》2021,84(6):985-994
Physics of Atomic Nuclei - The CALorimetric Electron Telescope CALET is collecting science data on the International Space Station since October 2015 with excellent and continuous performance....  相似文献   
23.
A previously proposed model for representing the retention factor (k) of an analyte in mixed solvent mobile phases was extended to calculate the k of different analytes with respect to the nature of analyte, organic modifier, its concentration and type of the stationary phase. The accuracy of the proposed method was evaluated by calculating mean percentage deviation (MPD) as accuracy criterion. The predicted vs. observed plots were also provided as goodness of fit criteria. The developed model prediction capability compared with a number of previous models (i.e. LSER, general LSER and Oscik equation) through MPD and fitting plots. The proposed method provided acceptable predictions with the advantage of modeling the effects of organic modifiers, mobile phase compositions, columns and analytes using a single equation. The accuracy of developed model was checked using the one column and one analyte out cross validation analyses and the results showed that the developed model was able to predict the unknown analyte retention and the analytes retentions on unknown column accurately.  相似文献   
24.
25.
The development and application of new separation mechanisms such as hydrophilic interaction chromatography (HILIC) is of high importance for the simultaneous analysis of polar molecules such as primary metabolites. However the retention mechanism in HILIC is not fully understood and as a result retention prediction tools are not at hand for this chromatographic approach. In the present report we study the utility of a simple algorithm, based on a simple linear and/or a simple logarithmic retention model, for retention prediction in HILIC gradient separation of a mixture of 23 selected compounds including (poly)amines, amino acids, saccharides, and other molecules. Utilizing two types of gradient elution programs with or without an isocratic part, retention data were collected in order to build prediction models. Starting from at least three gradient runs the prediction of analyte retention was very satisfactory for all gradient programs tested, providing useful evidence of the value of such retention time prediction methodologies.  相似文献   
26.
V. V. Mikhailov  O. Adriani  G. A. Bazilevskaya  G. C. Barbarino  R. Bellotti  E. A. Bogomolov  M. Boezio  V. Bonvicini  M. Bongi  S. Bottai  A. Bruno  A. Vacchi  E. Vannuccini  G. I. Vasilyev  S. A. Voronov  A. M. Galper  C. De Santis  V. Di Felice  G. Zampa  N. Zampa  M. Casolino  D. Campana  A. V. Karelin  P. Carlson  G. Castellini  F. Cafagna  A. A. Kvashnin  A. N. Kvashnin  S. V. Koldashov  S. A. Koldobskiy  S. Y. Krutkov  A. A. Leonov  A. G. Mayorov  V. V. Malakhov  M. Martucci  L. Marcelli  W. Menn  M. Merge  E. Mocchiutti  A. Monaco  N. Mori  R. Munini  G. Osteria  B. Panico  P. Papini  P. Picozza  M. Pearce  M. Ricci  S. B. Ricciarini  M. F. Runtso  M. Simon  R. Sparvoli  P. Spillantini  Y. I. Stozhkov  Y. T. Yurkin 《Bulletin of the Russian Academy of Sciences: Physics》2017,81(2):154-156
The PAMELA magnetic spectrometer was launched aboard the Resurs DK-1 satellite into a nearpolar circumterrestrial orbit with an altitude of 350–600 km to study fluxes of the particles and antiparticles of cosmic rays in the wide energy range of ~80 MeV to several hundred gigaelectronvolts. The results from observations of temporal variations in electron and positron fluxes in 2006–2015 are presented. The ratio of electron and positron fluxes measured in this time interval reveals a dependence on the rigidity of particles, the solar activity, and the polarity of the solar magnetic field.  相似文献   
27.
E. A. Bogomolov  O. Adriani  G. A. Bazilevskaya  G. C. Barbarino  R. Bellotti  M. Boezio  V. Bonvicini  M. Bongi  S. Bottai  A. Bruno  A. Vacchi  E. Vannuccini  G. I. Vasilyev  S. A. Voronov  A. M. Galper  C. De Santis  V. Di Felice  G. Zampa  N. Zampa  M. Casolino  D. Campana  A. V. Karelin  P. Carlson  G. Castellini  F. Cafagna  A. A. Kvashnin  A. N. Kvashnin  S. V. Koldashov  S. A. Koldobskiy  S. Y. Krutkov  A. A. Leonov  A. G. Mayorov  V. V. Malakhov  M. Martucci  L. Marcelli  W. Menn  M. Merge  V. V. Mikhailov  E. Mocchiutti  A. Monaco  N. Mori  R. Munini  G. Osteria  B. Panico  P. Papini  P. Picozza  M. Pearce  M. Ricci  S. B. Ricciarini  M. F. Runtso  M. Simon  R. Sparvoli  P. Spillantini  Y. I. Stozhkov  Y. T. Yurkin 《Bulletin of the Russian Academy of Sciences: Physics》2017,81(2):132-135
The first results from measuring the spectra of solar neutrons with energies of ~10–1000 MeV in the solar flares of 2006–2015 observed by the PAMELA international space experiment are presented. The PAMELA neutron detector with 3He counters and a moderator with an area of 0.18 m2 allows us to estimate the flux of solar neutrons during solar flares. Solar neutrons with energies of ~10–1000 MeV likely occurred in 21 out of the 24 analyzed flares of 2006–2015.  相似文献   
28.
Summary The occurrence of a springtime ozone depletion over Antarctica appears to be the result of a chain of processes leading to catalitic destruction of the gas by the action of halogen radicals, in particular chlorine oxide. High abundances of ClO in the stratosphere are determined by abnormally low concentrations of nitrogen compounds; such denitrification is likely to be caused by heterogeneous reactions and transport carried out by the clouds present in the polar stratosphere. Stratospheric clouds form during most of the winter and the beginning of spring over the polar regions. Due to scarce accessibility, knowledge of their properties is still poor. Information on extent, particles shape and size distributions is, however, fundamental for the understanding of the magnitude of their contribution to the destruction chain. A balloon-borne experiment, aimed at thein situ observation of cloud particles from 2 to 200 microns in radius, is presented. This would be the first system to provide on-line TV images of cloud particles. The first measurement campaign in Antarctica is planned for the period August–October 1990.  相似文献   
29.
The analysis of amino acids presents significant challenges to contemporary analytical separations. The present paper investigates the possibility of retention prediction in hydrophilic interaction chromatography (HILIC) gradient elution based on the analytical solution of the fundamental equation of the multilinear gradient elution derived for reversed‐phase systems. A simple linear dependence of the logarithm of the solute retention (ln k) upon the volume fraction of organic modifier (φ) in a binary aqueous‐organic mobile is adopted. Utility of the developed methodology was tested on the separation of a mixture of 21 amino acids carried out with 14 different gradient elution programs (from simple linear to multilinear and curved shaped) using ternary eluents in which a mixture of methanol and water (1:1, v/v) was the strong eluting member and acetonitrile was the weak solvent. Starting from at least two gradient runs, the prediction of solute retention obtained under all the rest gradients was excellent, even when curved gradient profiles were used. Development of such methodologies can be of great interest for a wide range of applications.  相似文献   
30.
In an effort to gain enhancement of selectivity in reversed-phase liquid chromatography, retention was tuned in this study by introducing short and medium straight-chained-length alkanol additives (methanol (MeOH), ethanol, 1-propanol, 1-butanol, 1-pentanol, 1-hexanol or 1-heptanol) at low concentrations in mobile phases containing MeOH as the main organic solvent. A six-parameter retention model considering simultaneously the contents of the main organic modifier and of the alcohol additive as well as of the number of alkyl chain of additive was developed by a direct combination of equations expressing separately a linear dependence of the retention upon each of these factors. The effectiveness of the above model was tested in the retention prediction of a mixture of six alkylbenzenes under isocratic conditions with mobile phases containing as an additive any member of the homologues series of alkanols (with 1-7 carbon atoms) at different low concentrations in a wide range of MeOH-water mixtures. The prediction was excellent in all cases even when the alkanol additives used in experiments for the fitting procedure are different than those used in chromatographic runs done for testing the prediction ability of the proposed model.  相似文献   
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