Short-lived solar burst spectral component at f approximately 100 GHz

A new kind of burst emission component was discovered, exhibiting fast and distinct pulses (approx. 60 ms durations), with spectral peak emission at f approx. 100 GHz, and onset time coincident to hard X-rays to within approx. 128 ms. These features pose serious constraints for the interpretation using current models. One suggestion assumes the f approx. 100 GHz pulses emission by synchrotron mechanism of electrons accelerated to ultrarelativistic energies. The hard X-rays originate from inverse Compton scattering of the electrons on the synchrotron photons. Several crucial observational tests are needed for the understanding of the phenomenon, requiring high sensitivity and high time resolution (approx. 1 ms) simultaneous to high spatial resolution (0.1 arcsec) at f approx. 110 GHz and hard X-rays

The possible importance of synchrotron/inverse Compton losses to explain fast MM-wave and hard X-ray emission of a solar event

The solar burst of 21 May 1984 presented a number of unique features. The time profile consisted of seven major structures (seconds), with a turnover frequency or approx. 90 GHz, well correlated in time to hard X-ray emission. Each structure consisted of multiple fast pulses (.1 seconds), which were analyzed in detail. A proportionality between the repetition rate of the pulses and the burst fluxes at 90 GHz and or approx. 100 keV hard X-rays, and an inverse proportionality between repetition rates and hard X-rays power law indices have been found. A synchrotron/inverse Compton model has been applied to explain the emission of the fast burst structures, which appear to be possible for the first three or four structures

Pelidnota filippiniae Soula, 2009 (Coleoptera: Melolonthidae: Rutelinae): um novo desfolhador de acácia-australiana, Racosperma mangium (Willd.) Pedley (Fabaceae), na Amazônia Oriental, Brasil.

Plantios de acácia-australiana, Racosperma mangium (Willd.) Pedley (Fabaceae), são opção para reflorestamentos comerciais na Amazônia. O trabalho objetiva, pela primeira vez, reportar e descrever injúrias causadas por Pelidnota filippiniae Soula, 2009 (Coleoptera: Melolonthidae: Rutelinae) em plantio experimental em Dom Eliseu, Pará. Observações mensais foram feitas de 2006 a 2009. A maior incidência ocorreu no início do período chuvoso, em outubro e novembro, nos primeiros anos do plantio, quando diferentes intensidades de desfolha foram observadas. Embora danos significativos não tenham sido constatados, P. filippiniae tem potencial para causar prejuízos à cultura. Recomendam-se monitoramentos mensais nesse período e a catação manual do inseto para evitar maiores danos

A new class of solar burst with MM-wave emission but only at the highest frequency (90 GHz)

High sensitivity and high time resolution solar observations at 90 GHz (lambda = 3.3 mm) have identified a unique impulsive burst on May 21, 1984 with emission that was more intense at this frequency than at lower frequencies. The first major time structure of the burst was over 10 times more intense at 90 GHz than at 30 GHz, 7 GHz, or 2.8 GHz.Only 6 seconds later, the 30 GHz impulsive structures started to be observed but still with lower intensity than at 90 GHz. Hard X-ray time structures at energies above 25 keV were almost identical to the 90 GHZ structures (to better than one second). All 90 GHz major time structures consisted of trains of multiple subsecond pulses with rise times as short as 0.03 sec and amplitudes large compared to the mean flux. When detectable, the 30 GHz subsecond pulses had smaller relative amplitude and were in phase with the corresponding 90 GHz pulses

Young's modulus of (Ti,Si)N films by surface acoustic waves and indentation techniques

Ti1yxSixNy films with Si contents up to 17.5 at.% and N contents close to 50 at.% were prepared by r.f. reactive magnetron sputtering. Film densities are within the range 3.4–5.1 gycm3.X-Ray diffraction patterns indicated the formation of two crystalline phases.In the case of low surface mobility, a metastable (Ti, Si)N phase was formed, where Si atoms occupied Ti positions. With increasing surface mobility, a crystalline TiN phase was observed.This behaviour may be explained by the occurrence of Si3N4 segregation, leading to the formation of a nanocomposite film of the type nc-TiNync-(Ti,Si)Nya-Si3N4, although the presence of Si3N4 phase is difficult to prove.In some of the films, a mixture of the (Ti,Si)N metastable phase with the TiN phase was observed, which indicates that the segregation of both TiN and Si3N4 phases is not complete.The Young’s modulus, Ef, of each coating was evaluated using both indentation tests and the surface acoustic waves (SAW) method.For most samples, the results obtained by these two methods are in good agreement.Some differences were observed in films prepared with a bias voltage of y50 V and Si contents higher than 5.9 at.%. For these samples, indentation values of approximately 10–20% higher than those obtained from SAW were found.This discrepancy is related to the nanostructure of these coatings, and it should be pointed out that the SAW results are strongly correlated with the density of the material.Fundação para a Ciência e Tecnologia (FCT)European Community Fund (FEDER)German/Portuguese DAAD/ICCTI Institution

A MPCC approach on a Stackelberg game in an electric power market : changing the leadership

An electric power market is studied as a Stackelberg game where two firms, A and B, produce energy. It is analyzed two distinct situations, according to the firm who plays the leader role: the first one, when the firm A is the leader and the other firm is the follower, and the second that is the reverse of the players roles. The main goal is to understand the behavior of the various agents that compose the electric power network, such as transmissions capacity, quantities of power generated and demanded, when changing leadership. The problem is formulated as a Mathematical Program with Complementarity Constraints (MPCC) and reformulated into a Nonlinear Program (NLP), allowing the use of robust NLP solvers. Numerical results are presented and some final considerations are carried out.Universidade do Minho. Centro AlgoritmiFundação para a Ciência e a Tecnologia (FCT

Dinâmica de Scarabaeoidea (Insecta: Coleoptera) no sistema sucessional milho/pastagem em Teresina, Piauí.

Autoria: QUERINO [i.e. SILVA], R. B. Q. da. RANYSE BARBOSA QUERINO DA SILVA

Z_2-gradings of Clifford algebras and multivector structures

Let Cl(V,g) be the real Clifford algebra associated to the real vector space V, endowed with a nondegenerate metric g. In this paper, we study the class of Z_2-gradings of Cl(V,g) which are somehow compatible with the multivector structure of the Grassmann algebra over V. A complete characterization for such Z_2-gradings is obtained by classifying all the even subalgebras coming from them. An expression relating such subalgebras to the usual even part of Cl(V,g) is also obtained. Finally, we employ this framework to define spinor spaces, and to parametrize all the possible signature changes on Cl(V,g) by Z_2-gradings of this algebra.Comment: 10 pages, LaTeX; v2 accepted for publication in J. Phys.