Nucleonic intensities investigated during the Atlantic Expedition IQSY 1965 of RV "Meteor" (Appendix)

The nucleonic component of the cosmic rays has been measured by the German research vessel "Meteor" during the Atlantic Expedition IQSY 1965. The pressure corrected intensities fit well the rigidity calculations of Kondo and Kodamo. In this way we confirm the earth's magnetic field model used by these authors. Two positions of the cosmic ray equator have been determined at 29,7 °W (6,5 ± 1) °N and at 19 °W (7 ± 1) °N. These positions agree with the calculated values of Kondo and Kodamo. The total latitude effect of the nucleonic component amounts to 1.74 and 1.76. The measurements were carried out at solar minima activity. Using the values of latitude measurements at maxima solar activity the degree of modulation of the primary cosmic rays was determined in the rigidity range 2 - 13 GV. For rigidity values above 6 GV the modulation remains constant to 20 %.

Campi magnetici in astrofisica: determinazione dell'intensità minima e massima del campo magnetico delle pulsar

L’intento dell’elaborato è quello di ricavare i limiti teorici ai quali è soggetta l’intensità del campo magnetico delle pulsar. Troveremo due relazioni: una che esprime il valore massimo dell’intensità del campo magnetico per una pulsar, e una che ne esprime il valore minimo. Combineremo infine i nostri due risultati in una disequazione, nella quale l'intensità del campo magnetico di una pulsar è minorata e maggiorata dai due termini trovati. Il valore massimo che può assumere l’intensità del campo magnetico di una pulsar verrà derivato dalla condizione di stabilità espressa dal teorema del viriale per un sistema sferico rotante in presenza di un campo magnetico. Enunceremo inizialmente il teorema del viriale nella sua forma generale, dopodiché ne presenteremo l'espressione in un caso statico in presenza di un campo magnetico. Abbandoneremo poi il caso statico per includere l'effetto della rotazione, non trascurabile nel caso delle pulsar. Dopo aver adattato la condizione di stabilità derivante dal teorema del viriale al nostro modello di pulsar, ricaveremo il valore massimo dell'intensità del campo magnetico. Il valore minimo che può assumere l’intensità del campo magnetico di una pulsar verrà ricavato uguagliando la potenza emessa dalla pulsar mentre ruota (approssimata ad un dipolo rotante) con la perdita di energia rotazionale che si osserva normalmente per questi oggetti. Otterremo alla fine due termini che delimitano i valori che può assumere l’intensità del campo magnetico per una pulsar. Sostituendo alla relazione trovata i valori di raggio e massa tipici per una pulsar, saremo in grado di riscrivere tale relazione unicamente in funzione del periodo di rotazione della pulsar e della sua derivata rispetto al tempo. Sostituiremo i valori di periodo e derivata temporale del periodo di una pulsar esistente per avere un’idea del range di valori sotteso dai due termini trovati.

Identifying Robust Proxies of Gonad Maturation for the Protandrous Hermaphrodite Tridacna maxima (Röding, 1798, Bivalvia) from Individual to Population Scale

Monitoring gonadmaturation for protandrous and functional hermaphrodite species such as the giant clamTridacna maxima is difficult due to the juxtaposition and relative proportion ofmale and female tissues in the gonad [gonadal sex ratio (GSR)]. Here, the relevance of the widely used gonadosomatic index (GSI) as proxy of giant clam gonad maturation is tested with a large dataset (n = 265). Gonadosomatic index is compared with other indices, namely the proportion of the male part harboring spermatozoids, the proportion of empty oocyte follicles, the mean oocyte diameter, and the oocyte elongation. At gonad scale, high index variability highlighted partial spawning. At individual scale, male and female maturation proxies were contrasted, showing either asynchronous emissions of male and female gametes or contrasted spermatogenesis and oogenesis duration. The GSI was mostly driven by the number and diameter of oocytes and therefore it is recommended here as primary proxy for female maturity. Except for the oocyte elongation, all indices were affected by the GSR, which ruled out drawing conclusions at population scale. These results highlight the need for maturation stage proxies that are optimized for functional hermaphrodite species.

Utilización de espirulina (Spirulina maxima) en la alimentación de alevinos de trucha arco Iris (Oncorhynchus mikyss)

Tesis (Zootecnista). -- Universidad de La Salle. Facultad de Ciencias Agropecuarias. Programa de Zootecnia, 2014

Análise de modelos geológicos utilizando percolação dinâmica

In the present study we elaborated algorithms by using concepts from percolation theory which analyze the connectivity conditions in geological models of petroleum reservoirs. From the petrophysical parameters such as permeability, porosity, transmittivity and others, which may be generated by any statistical process, it is possible to determine the portion of the model with more connected cells, what the interconnected wells are, and the critical path between injector and source wells. This allows to classify the reservoir according to the modeled petrophysical parameters. This also make it possible to determine the percentage of the reservoir to which each well is connected. Generally, the connected regions and the respective minima and/or maxima in the occurrence of the petrophysical parameters studied constitute a good manner to characterize a reservoir volumetrically. Therefore, the algorithms allow to optimize the positioning of wells, offering a preview of the general conditions of the given model s connectivity. The intent is not to evaluate geological models, but to show how to interpret the deposits, how their petrophysical characteristics are spatially distributed, and how the connections between the several parts of the system are resolved, showing their critical paths and backbones. The execution of these algorithms allows us to know the properties of the model s connectivity before the work on reservoir flux simulation is started

Identificazione di nuove strategie per la valutazione della malattia minima residua nel Mieloma Multiplo: la Biopsia Liquida

Il Mieloma Multiplo (MM) è una patologia neoplastica delle cellule B caratterizzata dalla proliferazione di più cloni di plasmacellule portatrici di diverse anomalie genomiche. Il MM presenta tipicamente un’eterogeneità genomica spaziale e intraclonale, che rende l’aspirato midollare "a singolo sito", attualmente utilizzato per la valutazione della malattia residua (MRD) dopo trattamento, non realmente informativo sulla taglia di malattia e sul panorama genomico della malattia. In considerazione della crescente importanza che sta assumendo la valutazione della MRD, i test per monitorarla dovrebbero essere non invasivi, affidabili e in grado di rappresentare le eterogeneità che caratterizzano il MM. Il presente studio ha permesso di dimostrare la possibilità di utilizzare la biopsia liquida, una metodica innovativa e non invasiva, per caratterizzare i pazienti con MM attivo o con MM smoldering ad alto rischio di evoluzione (HR-SMM) e per determinale l’MRD nei pazienti sottoposti a terapia di prima linea, integrando le metodiche attualmente validate. Nei pazienti arruolati nel presente studio è stato possibile identificare la frazione tumorale di DNA libero circolante (cfDNA-TF) nel sangue periferico, ed è stato possibile caratterizzare la malattia da un punto di vista qualitativo, dimostrando un’elevata concordanza del profilo genomico tra DNA libero circolante e DNA midollare (100% nei pazienti con HR-SMM e 86% nei pazienti con MM attivo). L’esecuzione seriata di biopsie liquide in corso di terapia, con un follow-up mediano di 24 mesi, ha mostrato una rapida e netta riduzione della cfDNA-TF xdalle prime fasi di terapia, con una tendenza a mantenersi mediamente sotto la soglia di sensibilità della metodica anche nelle fasi successive, indipendentemente dall’eventuale persistenza di MRD individuabile a livello midollare o mediante PET-CT. Con un follow-up più lungo probabilmente sarà possibile valutare meglio la capacità di questa metodica di affiancare o eventualmente sostituire l’aspirato midollare.

Notas e descrições em Oemini, Dodecosini e Elaphidionini (Coleoptera: Cerambycidae: Cerambycinae)

Novas espécies são descritas em três tribos de Cerambycinae: em Oemini, Kalore minima sp. nov., do Brasil (Amazonas); em Dodecosini, Olexandrella rafaeli sp. nov., do Brasil (Rondônia); em Elaphidionini, Curtomerus lingafelteri sp. nov. da Bolívia, Mephritus apicepullus sp. nov., M. vescus sp. nov. e M. estoni sp. nov. as três do Brasil (Amazonas). Notas e novos registros são fornecidos para Macroeme vittipennis (Melzer, 1934), Dodecosis nigricornis Martins & Galileo, 1991 e Adiposphaerion rubrum Martins & Napp, 1992.

Multifractality in plasma edge electrostatic turbulence

Plasma edge turbulence in Tokamak Chauffage Alfven Bresilien (TCABR) [R. M. O. Galvao et al., Plasma Phys. Contr. Fusion 43, 1181 (2001)] is investigated for multifractal properties of the fluctuating floating electrostatic potential measured by Langmuir probes. The multifractality in this signal is characterized by the full multifractal spectra determined by applying the wavelet transform modulus maxima. In this work, the dependence of the multifractal spectrum with the radial position is presented. The multifractality degree inside the plasma increases with the radial position reaching a maximum near the plasma edge and becoming almost constant in the scrape-off layer. Comparisons between these results with those obtained for random test time series with the same Hurst exponents and data length statistically confirm the reported multifractal behavior. Moreover, the persistence of these signals, characterized by their Hurst exponent, present radial profile similar to the deterministic component estimated from analysis based on dynamical recurrences. (C) 2008 American Institute of Physics.

Time-frequency and time-scale analysis of Barkhausen noise signals

Carrying out information about the microstructure and stress behaviour of ferromagnetic steels, magnetic Barkhausen noise (MBN) has been used as a basis for effective non-destructive testing methods, opening new areas in industrial applications. One of the factors that determines the quality and reliability of the MBN analysis is the way information is extracted from the signal. Commonly, simple scalar parameters are used to characterize the information content, such as amplitude maxima and signal root mean square. This paper presents a new approach based on the time-frequency analysis. The experimental test case relates the use of MBN signals to characterize hardness gradients in a AISI4140 steel. To that purpose different time-frequency (TFR) and time-scale (TSR) representations such as the spectrogram, the Wigner-Ville distribution, the Capongram, the ARgram obtained from an AutoRegressive model, the scalogram, and the Mellingram obtained from a Mellin transform are assessed. It is shown that, due to nonstationary characteristics of the MBN, TFRs can provide a rich and new panorama of these signals. Extraction techniques of some time-frequency parameters are used to allow a diagnostic process. Comparison with results obtained by the classical method highlights the improvement on the diagnosis provided by the method proposed.

Liquid polymorphism, order-disorder transitions and anomalous behavior: A Monte Carlo study of the Bell-Lavis model for water

The Bell-Lavis model for liquid water is investigated through numerical simulations. The lattice-gas model on a triangular lattice presents orientational states and is known to present a highly bonded low density phase and a loosely bonded high density phase. We show that the model liquid-liquid transition is continuous, in contradiction with mean-field results on the Husimi cactus and from the cluster variational method. We define an order parameter which allows interpretation of the transition as an order-disorder transition of the bond network. Our results indicate that the order-disorder transition is in the Ising universality class. Previous proposal of an Ehrenfest second order transition is discarded. A detailed investigation of anomalous properties has also been undertaken. The line of density maxima in the HDL phase is stabilized by fluctuations, absent in the mean-field solution. (C) 2009 American Institute of Physics. [doi:10.1063/1.3253297]

Interlayer interference in double wells in a tilted magnetic field

Magnetotransport measurements on bilayer electron systems reveal repeated reentrance of the resistance minima at filling factors nu=4N+1 and nu=4N+3, where N is the Landau index number, in the tilted magnetic field. At high filling factors, the Shubnikov-de Haas oscillations exhibit beating effects at certain tilt angles. We attribute such behavior to oscillations of the tunneling gap due to Aharonov-Bohm interference effect between cyclotron orbits in different layers. The interplay between quantum and quasiclassical regimes is established.

Energy spectra for quantum wires and two-dimensional electron gases in magnetic fields with Rashba and Dresselhaus spin-orbit interactions

We introduce an analytical approximation scheme to diagonalize parabolically confined two-dimensional (2D) electron systems with both the Rashba and Dresselhaus spin-orbit interactions. The starting point of our perturbative expansion is a zeroth-order Hamiltonian for an electron confined in a quantum wire with an effective spin-orbit induced magnetic field along the wire, obtained by properly rotating the usual spin-orbit Hamiltonian. We find that the spin-orbit-related transverse coupling terms can be recast into two parts W and V, which couple crossing and noncrossing adjacent transverse modes, respectively. Interestingly, the zeroth-order Hamiltonian together with W can be solved exactly, as it maps onto the Jaynes-Cummings model of quantum optics. We treat the V coupling by performing a Schrieffer-Wolff transformation. This allows us to obtain an effective Hamiltonian to third order in the coupling strength k(R)l of V, which can be straightforwardly diagonalized via an additional unitary transformation. We also apply our approach to other types of effective parabolic confinement, e. g., 2D electrons in a perpendicular magnetic field. To demonstrate the usefulness of our approximate eigensolutions, we obtain analytical expressions for the nth Landau-level g(n) factors in the presence of both Rashba and Dresselhaus couplings. For small values of the bulk g factors, we find that spin-orbit effects cancel out entirely for particular values of the spin-orbit couplings. By solving simple transcendental equations we also obtain the band minima of a Rashba-coupled quantum wire as a function of an external magnetic field. These can be used to describe Shubnikov-de Haas oscillations. This procedure makes it easier to extract the strength of the spin-orbit interaction in these systems via proper fitting of the data.

gamma Cassiopeiae: an X-ray Be star with personality

An exciting unsolved problem in the study of high energy processes of early type stars concerns the physical mechanism for producing X-rays near the Be star gamma Cassiopeiae. By now we know that this source and several ""gamma Cas analogs"" exhibit an unusual hard thermal X-ray spectrum, compared both to normal massive stars and the non-thermal emission of known Be/X-ray binaries. Also, its light curve is variable on almost all conceivable timescales. In this study we reanalyze a high dispersion spectrum obtained by Chandra in 2001 and combine it with the analysis of a new (2004) spectrum and light curve obtained by XMM-Newton. We find that both spectra can be fit well with 3-4 optically thin, thermal components consisting of a hot component having a temperature kT(Q) similar to 12-14 keV, perhaps one with a value of similar to 2.4 keV, and two with well defined values near 0.6 keV and 0.11 keV. We argue that these components arise in discrete (almost monothermal) plasmas. Moreover, they cannot be produced within an integral gas structure or by the cooling of a dominant hot process. Consistent with earlier findings, we also find that the Fe abundance arising from K-shell ions is significantly subsolar and less than the Fe abundance from L-shell ions. We also find novel properties not present in the earlier Chandra spectrum, including a dramatic decrease in the local photoelectric absorption of soft X-rays, a decrease in the strength of the Fe and possibly of the Si K fluorescence features, underpredicted lines in two ions each of Ne and N (suggesting abundances that are similar to 1.5-3x and similar to 4x solar, respectively), and broadening of the strong NeXLy alpha and OVIII Ly alpha lines. In addition, we note certain traits in the gamma Cas spectrum that are different from those of the fairly well studied analog HD110432 - in this sense the stars have different ""personalities."" In particular, for gamma Cas the hot X-ray component remains nearly constant in temperature, and the photoelectric absorption of the X-ray plasmas can change dramatically. As found by previous investigators of gamma Cas, changes in flux, whether occurring slowly or in rapidly evolving flares, are only seldomly accompanied by variations in hardness. Moreover, the light curve can show a ""periodicity"" that is due to the presence of flux minima that recur semiregularly over a few hours, and which can appear again at different epochs.