2,667 research outputs found
Chertok (L.) et Michel-Wolfromm (H.). — La méthode de Balint et l’approche psychosomatique. Balint (M.). — Examen du malade par lui-même. Rev. Méd. Psychosomatique 1961, n° 2, pp. 17-29
No full textTurbiaux Marcel. Chertok (L.) et Michel-Wolfromm (H.). — La méthode de Balint et l’approche psychosomatique. Balint (M.). — Examen du malade par lui-même. Rev. Méd. Psychosomatique 1961, n° 2, pp. 17-29. In: Bulletin de psychologie, tome 20 n°252, 1967. p. 119
Software Design and Implementation of a UNIX Based Graphics System
No full textiv, 206 p.The author describes his internship as a Programmer/Analyst at u.s. Windpower Inc., the nation’s largest windmill producer and his work on the design, implementation, and testing of a UNIX-based graphics system named AUTOGRAPH.Power Plant Systems Development. U.S. Windpower, Inc. Burlington, Massachusetts.Analytic Studies. U.S. Windpower, Inc. Burlington, Massachusetts
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Searches for beyond the MSSM phenomena at CDF
No full textCDF searches for R{sub p} violation, extra quark generations, and long-lived charged massive particles are presented. These phenomena are not predicted by the Minimal Supersymmetric Standard Model (MSSM) and therefore complement the classic SUSY searches. Prospects for continuing these analyses during Run II of the Tevatron are outlined
Tests of discrete symmetries in the semileptonic decays of neutral kaons at CPLEAR
No full textThe semileptonic decays of neutral kaon beams, and , were measured in the CPLEAR experiment, and the parameters , Re(), Im(), and Re() were extracted using the time-dependent asymmetries in the rates of these two decay channels. Here, is the mass difference between the long and short lived components of the neutral kaons, Re() and Im() are proportional to the real and imaginary parts, repectively, of the = - amplitude in semileptonic decays, and Re() is the real part of the CP violating mixing parameter for the short lived neutral kaon
Measurement of the mass difference m(D-s(+))-m(D+) at CDF II
No full textWe present a measurement of the mass difference m(D-s(+))-m(D+), where both the D-s(+) and D+ are reconstructed in the phipi(+) decay channel. This measurement uses 11.6 pb(-1) of data collected by CDF II using the new displaced-track trigger. The mass difference is found to be m(D-s(+))-m(D+)=99.41+/-0.38(stat)+/-0.21(syst) MeV/c(2)
Correlation of near-Earth proton enhancements >100 MeV with parameters of solar microwave bursts
No full textWe analyze the relations between various combinations of peak fluxes and fluences of solar microwave bursts at 35 GHz recorded with the Nobeyama Radio Polarimeters during 1990–2015, and corresponding parameters of proton enhancements with E>100 MeV exceeding 0.1 pfu registered by GOES monitors in near-Earth environment. The highest correlation has been found between the microwave and proton fluences. This fact reflects a dependence of the total number of protons on the total duration of the acceleration process. In the events with strong flares, the correlation coefficients of proton fluences with microwave and soft X-ray fluences are higher than those with speeds of coronal mass ejections. The results indicate a statistically larger contribution of flare processes to acceleration of high-energy protons. Acceleration by shock waves seems to be less important at high energies in events associated with strong flares, although its contribution probably prevails in weaker events. The probability of a detectable proton enhancement was found to directly depend on the peak flux and duration of a microwave burst. This can be used for diagnostics of proton enhancements based on microwave observations
On some features of the solar proton event on 2021 October 28 (GLE73)
No full textIn addition to several recent articles devoted to the rare event of
ground-level enhancement of the solar relativistic proton flux observed on 2021
October 28 (GLE73), we study the 10-100 MeV solar energetic particle (SEP)
component of this event. Based on the GOES satellite data for 26 GLEs recorded
since 1986, we have formed a scatter plot displaying the ratio of the peak
fluxes of the >10 MeV (J10) and >100 MeV (J100) protons and their energy
spectra. Two extreme characteristics of the prompt component of the SEP-GLE73
event were revealed: (1) very small J10 and J100 proton fluxes and (2) a very
hard energetic spectrum in the 10-100 MeV range. There are only two events with
these characteristics similar to SEP-GLE73 namely, GLE40 (1989 July 25) and
GLE46 (1989 November 15). A correspondence was demonstrated between the hard
frequency spectrum of microwave radio bursts of initiating flares and the hard
SEP energy spectrum of these two and other GLEs. These results suggest that the
flare magnetic reconnection both in the impulsive and post-eruption phases
plays an important role in the acceleration of the SEP-GLE protons.Comment: 10 pages, 3 figures, 1 table. Accepted for publication in MNRA
Powerful Solar Flares of 2017 September: Correspondence between Parameters of Microwave Bursts and Proton Fluxes near Earth
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