Interim report on the progress of an inventory of artesian wells in Florida: leading to the enforcement of sections 370.051 - 370.54, Florida statues

One of the causes of lower artesian pressure, water waste and aquifer contamination is the misuse and insufficient care of artesian wells. In 1953, Senate Bill No. 57, entitled "An Act to Protect and Control the Artesian Waters of the State" (see Appendix) became a law. This law was passed through the efforts exerted by leading members of the Senate and the House of Representatives, who understood the need for a wise and controlled expenditure of our most valuable natural resource. The State Geologist and his authorized representatives were designated by this law to enforce this conservation measure; however, no financial provision was included for the 1953-55 biennium. The proposed program of the Florida Geological Survey for this biennium did not include the funds nor provide any full-time personnel for the enforcement of this statute. As a result, little actual work was accomplished during these two years, although much time was given to planning and discussion of the problem. Realizing that this program could provide additional basic data needed in the analysis of the water-supply problem, the State Geologist sought and was granted by the 1955 Legislature adequate funds with which to activate the first phase of the enforcement of Florida Statute No. 370.051-054. Enumerated below is a summary of the progress made on this investigation as outlined previously: 1. Data have been collected on 967 wildly flowing wells in 22 counties. 2. Chloride determinations have been run on 850 of the 967 wells. 3. Of the 967 wells, 554 have chlorides in excess of the 250 ppm, the upper limit assigned by the State Board of Health for public consumption. 4. Water escapes at the rate of 37, 762 gallons per minute from these 967 wells. This amounts to 54, 377, 280 gallons per day. The investigation is incomplete at this time; therefore, no final conclusions can be reached. However, from data already collected, the following recommendations are proposed: 1. That the present inventory of wildly flowing wells be completed for the entire State. 2. That the current inventory of wildly flowing wells be expanded at the conclusion of the present inventory to include all flowing wells. 3. That a complete statewide inventory program be established and conducted in cooperation with the Ground Water Branchof the U.S. Geological Survey. 4. That the enforcement functions as set down in Sections 370.051/.054, Florida Statutes, be separated from the program to collect water-resource data and that these functions be given to the Water Resources Department, if such is created (to be recommended by the Water Resources Study Commission in a water policy law presented to the 1957 Legislature). 5. That the research phase (well inventory) of the program remain under the direction of the Florida Geological Survey. (PDF contains 204 pages.)

An adaptive sliding mode control law for the power maximization of the wind turbine system

POWERENG 2011

Boiling heat transfer enhancement by using micro-pin-finned surface for electronics cooling

For efficiently cooling electronic components with high heat flux, experiments were conducted to study the flow boiling heat transfer performance of FC-72 over square silicon chips with the dimensions of 10 × 10 × 0.5 mm3. Four kinds of micro-pin-fins with the dimensions of 30 × 60, 30 × 120, 50 × 60, 50 × 120 μm2 (thickness, t × height, h) were fabricated on the chip surfaces by the dry etching technique for enhancing boiling heat transfer. A smooth surface was also tested for comparison. The experiments were made at three different fluid velocities (0.5, 1 and 2 m/s) and three different liquid subcoolings (15, 25 and 35 K). The results were compared with the previous published data of pool boiling. All micro-pin-fined surfaces show a considerable heat transfer enhancement compared with a smooth surface. Flow boiling can remarkably decrease wall superheat compared with pool boiling. At the velocities lower than 1 m/s, the micro-pin-finned surfaces show a sharp increase in heat flux with increasing wall superheat. For all surfaces, the maximum allowable heat flux, qmax, for the normal operation of LSI chips increases with fluid velocity and subcooling. For all micro-pin-finned surfaces, the wall temperature at the critical heat flux (CHF) is less than the upper limit for the reliable operation of LSI chips, 85◦C. The largest value of qmax can reach nearly 148 W/cm2 for micro-pin-finned chips with the fin height of 120 μm at the fluid velocity of 2 m/s and the liquid subcooling of 35 K. The perspectives for the boiling heat transfer experiment of the prospective micro-pin-finned sur- faces, which has been planned to be made in the Drop Tower Beijing/NMLC in the future, are also presented.

Sea-level rise in Hawaii: Implications for future shoreline locations and Hawaii coastal management

Management of coastal development in Hawaii is based on the location of the certified shoreline, which is representative of the upper limit of marine inundation within the last several years. Though the certified shoreline location is significantly more variable than long-term erosion indicators, its migration will still follow the coastline's general trend. The long-term migration of Hawaii’s coasts will be significantly controlled by rising sea level. However, land use decisions adjacent to the shoreline and the shape and nature of the nearshore environment are also important controls to coastal migration. Though each of the islands has experienced local sea-level rise over the course of the last century, there are still locations across the islands of Kauai, Oahu, and Maui, which show long- term accretion or anomalously high erosion rates relative to their regions. As a result, engineering rules of thumb such as the Brunn rule do not always predict coastal migration and beach profile equilibrium in Hawaii. With coastlines facing all points of the compass rose, anthropogenic alteration of the coasts, complex coastal environments such as coral reefs, and the limited capacity to predict coastal change, Hawaii will require a more robust suite of proactive coastal management policies to weather future changes to its coastline. Continuing to use the current certified shoreline, adopting more stringent coastal setback rules similar to Kauai County, adding realistic sea-level rise components for all types of coastal planning, and developing regional beach management plans are some of the recommended adaptation strategies for Hawaii. (PDF contains 4 pages)

Capturing protein dynamics with time-resolved luminescence spectroscopy

The presented doctoral research utilizes time-resolved spectroscopy to characterize protein dynamics and folding mechanisms. We resolve millisecond-timescale folding by coupling time-resolved fluorescence energy transfer (trFRET) to a continuous flow microfluidic mixer to obtain intramolecular distance distributions throughout the folding process. We have elucidated the folding mechanisms of two cytochromes---one that exhibits two-state folding (cytochrome cb₅₆₂) and one that has both a kinetic refolding intermediate ensemble and a distinct equilibrium unfolding intermediate (cytochrome c₅₅₂). Our data reveal that the distinct structural features of cytochrome c₅₅₂ contribute to its thermostability.

We have also investigated intrachain contact dynamics in unfolded cytochrome cb₅₆₂ by monitoring electron transfer, which occurs as the heme collides with a ruthenium photosensitizer, covalently bound to residues along the polypeptide. Intrachain diffusion for chemically denatured proteins proceeds on the microsecond timescale with an upper limit of 0.1 microseconds. The power-law dependence (slope = -1.5) of the rate constants on the number of peptide bonds between the heme and Ru complex indicate that cytochrome cb₅₆₂ is minimally frustrated.

In addition, we have explored the pathway dependence of electron tunneling rates between metal sites in proteins. Our research group has converted cytochrome b₅₆₂ to a c-type cytochrome with the porphyrin covalently bound to cysteine sidechains. We have investigated the effects of the changes to the protein structure (i.e., increased rigidity and potential new equatorial tunneling pathways) on the electron transfer rates, measured by transient absorption, in a series of ruthenium photosensitizer-modified proteins.

Search for heavy neutral resonances in the dielectron channel with the CMS detector at the LHC

A search for dielectron decays of heavy neutral resonances has been performed using proton-proton collision data collected at √s = 7 TeV by the Compact Muon Solenoid (CMS) experiment at the Large Hadron Collider (LHC) in 2011. The data sample corresponds to an integrated luminosity of 5 fb⁻¹. The dielectron mass distribution is consistent with Standard Model (SM) predictions. An upper limit on the ratio of the cross section times branching fraction of new bosons, normalized to the cross section times branching fraction of the Z boson, is set at the 95 % confidence level. This result is translated into limits on the mass of new neutral particles at the level of 2120 GeV for the Z′ in the Sequential Standard Model, 1810 GeV for the superstring-inspired Z′_ψ resonance, and 1940 (1640) GeV for Kaluza-Klein gravitons with the coupling parameter k/M_Pl of 0.10 (0.05).

Rational design of zinc phosphide heterojunction photovoltaics

The prospect of terawatt-scale electricity generation using a photovoltaic (PV) device places strict requirements on the active semiconductor optoelectronic properties and elemental abundance. After reviewing the constraints placed on an "earth-abundant" solar absorber, we find zinc phosphide (α-Zn₃P₂) to be an ideal candidate. In addition to its near-optimal direct band gap of 1.5 eV, high visible-light absorption coefficient (>10⁴ cm^-1), and long minority-carrier diffusion length (>5 μm), Zn₃P₂ is composed of abundant Zn and P elements and has excellent physical properties for scalable thin-film deposition. However, to date, a Zn₃P₂ device of sufficient efficiency for commercial applications has not been demonstrated. Record efficiencies of 6.0% for multicrystalline and 4.3% for thin-film cells have been reported, respectively. Performance has been limited by the intrinsic p-type conductivity of Zn₃P₂ which restricts us to Schottky and heterojunction device designs. Due to our poor understanding of Zn₃P₂ interfaces, an ideal heterojunction partner has not yet been found.

The goal of this thesis is to explore the upper limit of solar conversion efficiency achievable with a Zn₃P₂ absorber through the design of an optimal heterojunction PV device. To do so, we investigate three key aspects of material growth, interface energetics, and device design. First, the growth of Zn₃P₂ on GaAs(001) is studied using compound-source molecular-beam epitaxy (MBE). We successfully demonstrate the pseudomorphic growth of Zn₃P₂ epilayers of controlled orientation and optoelectronic properties. Next, the energy-band alignments of epitaxial Zn₃P₂ and II-VI and III-V semiconductor interfaces are measured via high-resolution x-ray photoelectron spectroscopy in order to determine the most appropriate heterojunction partner. From this work, we identify ZnSe as a nearly ideal n-type emitter for a Zn₃P₂ PV device. Finally, various II-VI/Zn₃P₂ heterojunction solar cells designs are fabricated, including substrate and superstrate architectures, and evaluated based on their solar conversion efficiency.

Observations of hydrogen and helium isotopes in solar cosmic rays

The isotopic composition of hydrogen and helium in solar cosmic rays provides a means of studying solar flare particle acceleration mechanisms since the enhanced relative abundance of rare isotopes, such as ²H, ³H and ³He, is due to their production by inelastic nuclear collisions in the solar atmosphere during the flare. In this work the Caltech Electron/Isotope Spectrometer on the IMP-7 spacecraft has been used to measure this isotopic composition. The response of the dE/dx-E particle telescope is discussed and alpha particle channeling in thin detectors is identified as an important background source affecting measurement of low values of (³He/⁴He).

The following flare-averaged results are obtained for the period, October, 1972 - November, 1973: (²H/¹H) = 7⁺¹⁰_-6 X 10^-6 (1.6 - 8.6 MeV/nuc), (³H/¹H) less than 3.4 x 10^-6 (1.2 - 6.8 MeV/nuc), (³He/⁴He) = (9 ± 4) x 10^-3, (³He/¹H) = (1.7 ± 0.7) x 10^-4 (3.1 - 15.0 MeV/nuc). The deuterium and tritium ratios are significantly lower than the same ratios at higher energies, suggesting that the deuterium and tritium spectra are harder than that of the protons. They are, however, consistent with the same thin target model relativistic path length of ~ 1 g/cm² (or equivalently ~ 0.3 g/cm² at 30 MeV/nuc) which is implied by the higher energy results. The ³He results, consistent with previous observations, would imply a path length at least 3 times as long, but the observations may be contaminated by small ³He rich solar events.

During 1973 three "³He rich events," containing much more ³He than ²H or ³H were observed on 14 February, 29 June and 5 September. Although the total production cross sections for ²H,³H and ³He are comparable, an upper limit to (²H/³He) and (³H/³He) was 0.053 (2.9-6.8 MeV/nuc), summing over the three events. This upper limit is marginally consistent with Ramaty and Kozlovsky's thick target model which accounts for such events by the nuclear reaction kinematics and directional properties of the flare acceleration process. The 5 September event was particularly significant in that much more ³He was observed than ⁴He and the fluxes of ³He and ¹H were about equal. The range of (³He/⁴He) for such events reported to date is 0.2 to ~ 6 while (³He/¹H) extends from 10^-3 to ~ 1. The role of backscattered and mirroring protons and alphas in accounting for such variations is discussed.

Neutron-neutron scattering parameters from the ^3He(d,t)2p and ^3H(d,^3He)2n reactions

The energy spectra of tritons and Helium-3 nuclei from the reactions ³He(d,t)2p, ³H(d,³He)2n, ³He(d,³He)pn, and ³H(d,t)pn were measured between 6° and 20° at a bombarding energy of 10.9 MeV. An upper limit of 5 μb/sr. was obtained for producing a bound di-neutron at 6° and 7.5°. The ³He(d,t)2p and ³H(d,³He)2n data, together with previous measurements at higher energies, have been used to investigate whether one can unambiguously extract information on the two-nucleon system from these three-body final state reactions. As an aid to these theoretical investigations, Born approximation calculations were made employing realistic nucleon-nucleon potentials and an antisymmetrized final state wave function for the five-particle system. These calculations reproduce many of the features observed in the experimental data and indicate that the role of exchange processes cannot be ignored. The results show that previous attempts to obtain information on the neutron-neutron scattering length from the ³H(d,³He)2n reaction may have seriously overestimated the precision that could be attained.

Electromagnetic decay of the 1.7- and 2.43-MeV levels in ^9Be

The 1.7- and 2.43-MeV levels in ⁹Be were populated with the reaction ¹¹B(d, α)⁹Be* by bombarding thin boron on carbon foils with 1.7-MeV deuterons. The alpha particles were analyzed in energy with a surface-barrier counter set at the unique kinematically determined angle and the recoiling ⁹Be nuclei at 90^o were analyzed in rigidity with a magnetic spectrometer, in energy by a surface-barrier counter at the spectrometer focus, and in velocity by the time delay between an alpha and a ⁹Be count. When a pulse from the spectrometer counter was in the appropriate delayed coincidence with a pulse from the alpha counter, the two pulses were recorded in a two-dimensional pulse height analyzer. Most of the ⁹Be* decay by particle breakup. Only those that gamma decay are detected by the spectrometer counter. Thus the experiment provides a direct measurement of Γ_rad/Γ. Analysis of 384 observed events gives Γ_rad/Γ = (1.16 ± 0.14) X 10^-4 for the 2.43-MeV level. Combining this ratio with the value of Γ_rad = 0.122 ± 0.015 eV found from inelastic electron scattering gives Γ = (1.05 ± 0.18) keV. For the 1.7-MeV level, an upper limit, Γ_rad/Γ ≤ 2.4 = 10^-5, was determined.

A Multiwavelength Study of the Intracluster Medium and the Characterization of the Multiwavelength Sub/millimeter Inductance Camera

The first part of this thesis combines Bolocam observations of the thermal Sunyaev-Zel’dovich (SZ) effect at 140 GHz with X-ray observations from Chandra, strong lensing data from the Hubble Space Telescope (HST), and weak lensing data from HST and Subaru to constrain parametric models for the distribution of dark and baryonic matter in a sample of six massive, dynamically relaxed galaxy clusters. For five of the six clusters, the full multiwavelength dataset is well described by a relatively simple model that assumes spherical symmetry, hydrostatic equilibrium, and entirely thermal pressure support. The multiwavelength analysis yields considerably better constraints on the total mass and concentration compared to analysis of any one dataset individually. The subsample of five galaxy clusters is used to place an upper limit on the fraction of pressure support in the intracluster medium (ICM) due to nonthermal processes, such as turbulent and bulk flow of the gas. We constrain the nonthermal pressure fraction at r500c to be less than 0.11 at 95% confidence, where r500c refers to radius at which the average enclosed density is 500 times the critical density of the Universe. This is in tension with state-of-the-art hydrodynamical simulations, which predict a nonthermal pressure fraction of approximately 0.25 at r500c for the clusters in this sample.

The second part of this thesis focuses on the characterization of the Multiwavelength Sub/millimeter Inductance Camera (MUSIC), a photometric imaging camera that was commissioned at the Caltech Submillimeter Observatory (CSO) in 2012. MUSIC is designed to have a 14 arcminute, diffraction-limited field of view populated with 576 spatial pixels that are simultaneously sensitive to four bands at 150, 220, 290, and 350 GHz. It is well-suited for studies of dusty star forming galaxies, galaxy clusters via the SZ Effect, and galactic star formation. MUSIC employs a number of novel detector technologies: broadband phased-arrays of slot dipole antennas for beam formation, on-chip lumped element filters for band definition, and Microwave Kinetic Inductance Detectors (MKIDs) for transduction of incoming light to electric signal. MKIDs are superconducting micro-resonators coupled to a feedline. Incoming light breaks apart Cooper pairs in the superconductor, causing a change in the quality factor and frequency of the resonator. This is read out as amplitude and phase modulation of a microwave probe signal centered on the resonant frequency. By tuning each resonator to a slightly different frequency and sending out a superposition of probe signals, hundreds of detectors can be read out on a single feedline. This natural capability for large scale, frequency domain multiplexing combined with relatively simple fabrication makes MKIDs a promising low temperature detector for future kilopixel sub/millimeter instruments. There is also considerable interest in using MKIDs for optical through near-infrared spectrophotometry due to their fast microsecond response time and modest energy resolution. In order to optimize the MKID design to obtain suitable performance for any particular application, it is critical to have a well-understood physical model for the detectors and the sources of noise to which they are susceptible. MUSIC has collected many hours of on-sky data with over 1000 MKIDs. This work studies the performance of the detectors in the context of one such physical model. Chapter 2 describes the theoretical model for the responsivity and noise of MKIDs. Chapter 3 outlines the set of measurements used to calibrate this model for the MUSIC detectors. Chapter 4 presents the resulting estimates of the spectral response, optical efficiency, and on-sky loading. The measured detector response to Uranus is compared to the calibrated model prediction in order to determine how well the model describes the propagation of signal through the full instrument. Chapter 5 examines the noise present in the detector timestreams during recent science observations. Noise due to fluctuations in atmospheric emission dominate at long timescales (less than 0.5 Hz). Fluctuations in the amplitude and phase of the microwave probe signal due to the readout electronics contribute significant 1/f and drift-type noise at shorter timescales. The atmospheric noise is removed by creating a template for the fluctuations in atmospheric emission from weighted averages of the detector timestreams. The electronics noise is removed by using probe signals centered off-resonance to construct templates for the amplitude and phase fluctuations. The algorithms that perform the atmospheric and electronic noise removal are described. After removal, we find good agreement between the observed residual noise and our expectation for intrinsic detector noise over a significant fraction of the signal bandwidth.

星载激光对水下目标通信可行性研究

The characteristics of media in communication channel are analyzed briefly and the reasonable optical parameters of media are adopted. With certain communication system parameters the temporal and spatial distributions of the received signal from submerged platform are simulated using Monte Carlo method. The upper limit of the ratio of Monte Carlo estimated error to averaged value is about 0.3%. From the simulated results, the optimized sampling timing of receiver and field of view of telescope are obtained. Also the signal-to-noise ratio of the receiver is calculated. Based on this, the error probability of the communication system is deduced from laser pulse position modulation and maximum likelihood detection. The results show that under severe environment robust laser communication from a satellite to a submerged platform can be achieved.

Estresse ocupacional segundo o modelo demanda-controle e suas repercussões na saúde do trabalhador de enfermagem: análise das variações de cortisol salivar

O objeto de estudo foi o estresse no trabalho e os níveis de cortisol salivar. O objetivo geral foi avaliar a associação entre estresse no trabalho e variações de cortisol salivar de trabalhadores de Enfermagem inseridos na assistência hospitalar no Rio de Janeiro. A hipótese do estudo foi que existe associação entre trabalhadores expostos à alta exigência no trabalho e as variações de cortisol salivar. Trata-se de estudo epidemiológico observacional analítico seccional, realizado em hospital estadual localizado no Rio de Janeiro com amostra de 103 trabalhadores. Para avaliação dos aspectos psicossociais do trabalho, utilizou-se o questionário Job Content Questionnaire. O cortisol salivar foi medido através da coleta de 04 amostras de cada participante em um dia do plantão: ao acordar, 30 minutos depois, às 12h e 18 h. A coleta de dados foi realizada entre março e abril de 2012. Utilizou-se o programa SPSS 18.0 para análise dos dados. As dimensões demanda psicológica e controle e a subtração foram utilizadas sob a forma contínua nas análises de correlação com as covariáveis e desfecho. Os níveis de cortisol foram quantificados por meio de cinco índices: o cálculo da área sob a curva em relação ao zero ou base (AUCg), área sob a curva em relação ao aumento (AUCi), o aumento médio (MnInc), a excreção do cortisol no período pós acordar (AUCtrab) e a área sob a curva em relação ao zero ou base do ciclo diurno (AUCCD). Para avaliar a associação entre as covariáveis e exposição e desfecho utilizou-se os testes de Mann Whitney e Kruskall-Wallis. As covariáveis associadas à exposição ou ao desfecho com nível de significância de 20% (p≤0,20) foram testadas no modelo de regressão linear. Realizada análise de correlação utilizando-se o coeficiente de correlação de Spearmans. Como resultado encontrou-se que os trabalhadores de Enfermagem obtiveram médias para demanda psicológica e controle que tendem para o limite superior, bem como para a subtração, caracterizando alta demanda e alto controle, ou seja, trabalho ativo. O valor médio de cortisol observado ao acordar, 30 minutos após, 12h e 18h foi de 5,82 nmol/L) (4,86), 16,60 nmol/L ( 8,31), 7,49 nmol/L ( 6,97) e 3,93 nmol/L ( 3,15), respectivamente. O aumento do cortisol entre o acordar e 30 minutos após foi em média de 64%. Já para os índices de cortisol adotados observa-se o valor médio da MnInc, AUCg, AUCi, AUCtrab e AUCCD foi de 10,78 nmol/L (6,99), 5,61 nmol/L ( 2,92) 2,69 nmol/L ( 1,75), 32,51 nmol/L ( 21,99) e 107,99 nmol/L ( 61,63), respectivamente. Este estudo demonstrou que os níveis de cortisol salivar livre não estão associados à alta exigência no trabalho, mesmo quando ajustadas pelas possíveis variáveis de confusão ou modificadoras de efeito. A hipótese do estudo não foi confirmada. Os dados obtidos neste estudo revelaram aspectos importantes dos riscos psicossociais a que estão expostos os trabalhadores de Enfermagem durante o processo de trabalho, oferecendo subsídios para que sejam implementados programas de orientação e promoção à saúde do trabalhador e fornecem um contributo para entender os caminhos biológicos pelos quais o estresse no trabalho influencia a saúde.

Assobios do boto-cinza, Sotalia guianensis, (Cetacea, Delphinidae) em três áreas de concentração na costa do Rio de Janeiro

A espécie Sotalia guianensis apresenta um variado repertório de assobios que estão ligados a interação social e a diferentes contextos de comportamento. As variações intraespecíficas nas estruturas dos assobios podem indicar diferenças entre populações dessa espécie. O presente estudo caracterizou e comparou o repertório dos assobios de Sotalia guianensis, em três baías do estado do Rio de Janeiro: Baía de Guanabara (BG), Baía de Sepetiba (BS) e Baía da Ilha Grande (BI), utilizando um sistema de gravação com limite superior de frequência de 48 kHz e através da aplicação das análises quantitativas e qualitativas dos parâmetros acústicos. As gravações dos assobios foram realizadas com embarcações de 5,5 e 7m e sistema de gravação composto por um hidrofone High Tech, modelo HTI-96-MIN, e um gravador digital modelo PMD 671 Marantz, com limite superior de frequência de 48 kHz. As análises dos espectrogramas foram realizadas com os softwares Adobe Audition 1.5 e Raven 1.3. Os assobios foram classificados em seis categorias de forma de contorno e 11 parâmetros acústicos foram medidos para cada assobio. Para comparar os parâmetros acústicos de mesma forma de contorno entre as três baías, foram aplicados a análise descritiva e testes estatísticos de comparação de média. Um total de 1800 assobios foi selecionado e 61,38% (N=1105) dos assobios apresentaram forma de contorno ascendente. Assobios com zero ou um ponto de inflexão foram mais frequentes (N=1476), correspondendo a 82%. A amplitude de frequência encontrada variou de 1,03 a 46,87 kHz, maior alcance registrado para essa espécie no Brasil. A média de duração dos assobios da BG foi menor do que as médias encontradas na BS e na BI. Os resultados de todas as comparações realizadas demonstraram que os parâmetros de frequência (FI, FF, FMAX e F3/4) foram os que mais apresentaram diferenças significativas entre as três áreas. A variação encontrada nos assobios de S. guianensis entre as três áreas estudadas pode também estar ligada aos tipos de assobios mais comuns em cada área, representados pelos assobios ascendentes, que apesar de apresentarem a mesma forma de contorno, possuem diferenças em seus parâmetros acústicos, possivelmente ligados a informações individuais. A utilização de um sistema de gravação com limite superior de 48 kHz possibilitou a análise de muitos assobios. Com isso, foi possível verificar a importância do limite de frequência aplicado para caracterizar o repertório acústico dessa espécie, juntamente com as análises qualitativas das formas de contorno e as análises quantitativas dos parâmetros acústicos dos assobios. A aplicação dessa metodologia foi eficaz na comparação intraespecífica dos assobios, e futuramente, estudos mais detalhados da classificação dos assobios, poderá acrescentar informações relevantes sobre a variação desse tipo de emissão sonora no repertório acústico S. guianensis

Populações de Chthamalus spp. em costões rochosos da baía da ilha Grande (RJ) e suas relações com o clima entre 2002 e 2012

Poucos organismos são aptos a suportar o alto estresse provocado pelas variações de temperatura e alta dessecação na faixa superior da região entremarés de costões rochosos, sendo um deles o cirripédio Chthamalus. Apesar da sua resistência, vivem constantemente próximos ao seu limite de tolerância fisiológica, o que pode influenciar suas populações. O objetivo deste estudo foi caracterizar as flutuações das populações de Chthamalus spp. na faixa superior da região entremarés em quatro costões rochosos na Baía da Ilha Grande entre 2002 e 2012, relacionando estas variações com os fatores ambientais temperatura do ar, temperatura superficial marinha e precipitação, verificando o potencial destes organismos como indicadores de variações climáticas. Para isso foram investigadas a temperatura do ar e precipitação a partir de dados da estação meteorológica de Angra dos Reis e temperatura da superfície do mar a partir de imagens de satélite (MODIS/AQUA), além das porcentagens de cobertura de Chthamalus spp. a partir de amostragens sazonais. Em geral o estudo indica que as populações foram influenciadas pelas variáveis biológicas recrutamento e competição intraespecífica. Foram verificadas grandes diferenças entre as populações nos costões rochosos estudados. A estação C1, apresentou altas coberturas de cirripédios jovens e adultos ao longo de praticamente todo o período de estudo. Na estação C2 ocorreram as maiores variações, enquanto nas estações C3 e C4 ocorreram coberturas menores e variações menos proeminentes. Estas diferenças provavelmente estiveram ligadas às características físicas de cada costão rochoso. Os anos de 2003 e 2010 foram caracterizados como de altas temperaturas (temperaturas do mar e do ar) quando comparados com os demais anos de estudo. Estes anos foram ainda caracterizados pela ocorrência do fenômeno El Niño, com altas anomalias térmicas, o que indica que este fenômeno climático influenciou as temperaturas da região. Nestes mesmos anos as coberturas de Chthamalus spp. foram relativamente baixas, o que indica que o estresse térmico afetou as populações deste cirripédio. Pode-se inferir através deste estudo que as populações de Chthamalus spp. sofrem influência direta dos fatores ambientais investigados, sendo com isso um potencial indicador de mudanças climáticas.