Inkluderande teaterverksamhet. Nya möjligheter för socialt arbete

I denna pro gradu-avhandling granskas teaterns möjligheter att främja social inklusion. Genom att analysera vad drama och teater kan ge ungdomar och hur social inklusion bland unga i ett samfund kan främjas, belyses även frågan om hur socialt arbete och teater ömsesidigt kan berika varandra. Avhandlingen är en fallstudie av Half Moon Young People’s Theatre, en barn- och ungdomsteater i Tower Hamlets i östra London. Teatern arbetar med barn och unga med ett särskilt fokus på att engagera grupper som ofta marginaliserats, exempelvis på grund av sin kulturella bakgrund eller till följd av funktionshinder. I denna studie är fokus på Half Moons projekt riktade till tonåringar: Careers in Theatre, Speak Up och ungdomsteatergrupperna Lunar och Solar. Studien är kvalitativ och studiens empiriska data har främst samlats in genom deltagande observation, intervjuer och granskning av dokument. Det empiriska materialet visar på Half Moons aktiva arbete för mångfald och för att göra verksamheten och deltagandet tillgängligt för alla barn och unga. Teatern blir en mötesplats genom vilken ungdomarna kan lära sig acceptera och uppskatta mångfalden i samfundet. Teaterarbetet bidrar till en ökad känsla för samfundet och till tolerans och förståelse för andra. Det är en glädjefylld, trygg och meningsfull fritidsverksamhet där nya vänskapskontakter kan knytas och många färdigheter övas inför framtiden. Teaterarbetet ger deltagarna bekräftelse vilket bidrar till att självförtroendet växer. Personalens engagemang och osjälviska arbete för inklusion genomsyrar verksamheten. Möjligheten att ge alla en ny chans och ett jämlikt bemötande är centralt i teaterns arbete. Forskningsresultaten pekar på teaterns potential inom socialt arbete och för att främja inklusion. Teaterns möjligheter att öka klientens delaktighet och utveckla förhållandet mellan socialarbetare och klient visar på betydelsen av etablera dylik verksamhet inom socialt arbete. Att inte låta sig begränsas, utan förutsättningslöst samarbeta över sektorer ökar chanserna att finna nya kreativa idéer och verksamhetsformer.

Silicon isotopes: from cosmos to benthos

Silicon is the second most abundant element on the Earth and one of the more abundant elements in our Solar System. Variations in the relative abundance of the stable isotopes of Si (Si isotope fractionation) in different natural reservoirs, both terrestrial (surface and deep Earth) as well as extra-terrestrial (e.g. meteorites, lunar samples), are a powerful tracer of present and past processes involving abiotic as well as biotic systems. The versatility of the Si isotope tracer is reflected in its wide-ranging applications from understanding the origin of early Solar System objects, planetary differentiation, Moon formation, mantle melting and magma differentiation on the Earth, ancient sea-water composition, to modern-day weathering, clay formation and biological fractionation on land as well as in the oceans. The application of Si isotopes as tracers of natural processes started over six decades ago and its usage has seen a sudden increase over the last decade due to improvements in mass spectrometry, particularly the advent of multi-collector inductively coupled plasma mass spectrometers, which has made Si isotope measurements safe and relatively easy while simultaneously improving the accuracy and precision of measurements.

Evaluación del crecimiento y rendimiento del cultivo de Rábano (Raphanus sativus L.) en diferentes fases lunares en la unidad de producción Las Mercedes, UNA, Managua 2010

Con el propósito de generar información científica sobre el cultivo de Rábano ( Raphanus sativus, L ) en diferentes fases lunares , se llevo a cabo el ensayo e ntre octubre 2010 y febrero 20 1 1, utilizando un Diseño de Bloques Completo al Azar (BCA) con cuatros tratamientos y cuatro repeticiones. El ensayo se realizó e n el Campus Las Mercedes propiedad de la Universidad Nacional Agraria. Teniendo su ubicación geográfica con las siguientes coordenadas: 12º10’14” a 12º08’05” en latitud norte y 86º10’22” a 86º09’44” Longitud oeste. Durante la fase de crecimiento se midi er on las siguientes variables: D iámetro del tallo, altura de la planta, numero de hojas y du rante la cosecha: Diámetro del bulbo , Longitud de la raíz, Peso fresco y rendimiento las cuales fueron sometidas a un análisis de varianza, analizando las diferencias entre medias por la prueba de comparaciones múltiples de Tukey . Los diferentes tratamientos no mostraron diferencias significativas en las variables evaluadas . Por lo tanto en luna llena se obtuvo ( 52143.6 kg ha - 1 ) , en cuarto creciente ( 49485.6 kg ha - 1 ) , en luna nueva (43365.6 kg ha - 1 ) y en cuarto menguante ( 42669.6 kg ha - 1 ) . Los mejores resultados se obtuvieron en luna llena porque en es t a fase la humedad es mayor lo que es favo rable para el cultivo . En esta fase de luna llena en el subsuelo se producen, entre otras cosas, grandes movimientos de agua que afectan directamente las actividades agrícolas, la disponibilidad de luz lunar va en aumento y las plantas tienen un crecimiento balanceado, en el que se favorece el crecimient o de follaje y raíz

Analyses of planetary atmospheres across the spectrum : from Titan to exoplanets

Planetary atmospheres exist in a seemingly endless variety of physical and chemical environments. There are an equally diverse number of methods by which we can study and characterize atmospheric composition. In order to better understand the fundamental chemistry and physical processes underlying all planetary atmospheres, my research of the past four years has focused on two distinct topics. First, I focused on the data analysis and spectral retrieval of observations obtained by the Ultraviolet Imaging Spectrograph (UVIS) instrument onboard the Cassini spacecraft while in orbit around Saturn. These observations consisted of stellar occultation measurements of Titan's upper atmosphere, probing the chemical composition in the region 300 to 1500 km above Titan's surface. I examined the relative abundances of Titan's two most prevalent chemical species, nitrogen and methane. I also focused on the aerosols that are formed through chemistry involving these two major species, and determined the vertical profiles of aerosol particles as a function of time and latitude. Moving beyond our own solar system, my second topic of investigation involved analysis of infra-red light curves from the Spitzer space telescope, obtained as it measured the light from stars hosting planets of their own. I focused on both transit and eclipse modeling during Spitzer data reduction and analysis. In my initial work, I utilized the data to search for transits of planets a few Earth masses in size. In more recent research, I analyzed secondary eclipses of three exoplanets and constrained the range of possible temperatures and compositions of their atmospheres.

Toward Understanding Astrophysical Phenomena

Fast radio bursts (FRBs), a novel type of radio pulse, whose physics is not yet understood at all. Only a handful of FRBs had been detected when we started this project. Taking account of the scant observations, we put physical constraints on FRBs. We excluded proposals of a galactic origin for their extraordinarily high dispersion measures (DM), in particular stellar coronas and HII regions. Therefore our work supports an extragalactic origin for FRBs. We show that the resolved scattering tail of FRB 110220 is unlikely to be due to propagation through the intergalactic plasma. Instead the scattering is probably caused by the interstellar medium in the FRB's host galaxy, and indicates that this burst sits in the central region of that galaxy. Pulse durations of order $\ms$ constrain source sizes of FRBs implying enormous brightness temperatures and thus coherent emission. Electric fields near FRBs at cosmological distances would be so strong that they could accelerate free electrons from rest to relativistic energies in a single wave period. When we worked on FRBs, it was unclear whether they were genuine astronomical signals as distinct from `perytons', clearly terrestrial radio bursts, sharing some common properties with FRBs. Recently, in April 2015, astronomers discovered that perytons were emitted by microwave ovens. Radio chirps similar to FRBs were emitted when their doors opened while they were still heating. Evidence for the astronomical nature of FRBs has strengthened since our paper was published. Some bursts have been found to show linear and circular polarizations and Faraday rotation of the linear polarization has also been detected. I hope to resume working on FRBs in the near future. But after we completed our FRB paper, I decided to pause this project because of the lack of observational constraints.

The pulsar triple system, J0733+1715, has its orbital parameters fitted to high accuracy owing to the precise timing of the central $\ms$ pulsar. The two orbits are highly hierarchical, namely $P_{\mathrm{orb,1}}\ll P_{\mathrm{orb,2}}$, where 1 and 2 label the inner and outer white dwarf (WD) companions respectively. Moreover, their orbital planes almost coincide, providing a unique opportunity to study secular interaction associated purely with eccentricity beyond the solar system. Secular interaction only involves effect averaged over many orbits. Thus each companion can be represented by an elliptical wire with its mass distributed inversely proportional to its local orbital speed. Generally there exists a mutual torque, which vanishes only when their apsidal lines are parallel or anti-parallel. To maintain either mode, the eccentricity ratio, $e_1/e_2$, must be of the proper value, so that both apsidal lines precess together. For J0733+1715, $e_1\ll e_2$ for the parallel mode, while $e_1\gg e_2$ for the anti-parallel one. We show that the former precesses $\sim 10$ times slower than the latter. Currently the system is dominated by the parallel mode. Although only a little anti-parallel mode survives, both eccentricities especially $e_1$ oscillate on $\sim 10^3\yr$ timescale. Detectable changes would occur within $\sim 1\yr$. We demonstrate that the anti-parallel mode gets damped $\sim 10^4$ times faster than its parallel brother by any dissipative process diminishing $e_1$. If it is the tidal damping in the inner WD, we proceed to estimate its tidal quantity parameter ($Q$) to be $\sim 10^6$, which was poorly constrained by observations. However, tidal damping may also happen during the preceding low-mass X-ray binary (LMXB) phase or hydrogen thermal nuclear flashes. But, in both cases, the inner companion fills its Roche lobe and probably suffers mass/angular momentum loss, which might cause $e_1$ to grow rather than decay.

Several pairs of solar system satellites occupy mean motion resonances (MMRs). We divide these into two groups according to their proximity to exact resonance. Proximity is measured by the existence of a separatrix in phase space. MMRs between Io-Europa, Europa-Ganymede and Enceladus-Dione are too distant from exact resonance for a separatrix to appear. A separatrix is present only in the phase spaces of the Mimas-Tethys and Titan-Hyperion MMRs and their resonant arguments are the only ones to exhibit substantial librations. When a separatrix is present, tidal damping of eccentricity or inclination excites overstable librations that can lead to passage through resonance on the damping timescale. However, after investigation, we conclude that the librations in the Mimas-Tethys and Titan-Hyperion MMRs are fossils and do not result from overstability.

Rubble piles are common in the solar system. Monolithic elements touch their neighbors in small localized areas. Voids occupy a significant fraction of the volume. In a fluid-free environment, heat cannot conduct through voids; only radiation can transfer energy across them. We model the effective thermal conductivity of a rubble pile and show that it is proportional the square root of the pressure, $P$, for $P\leq \epsy^3\mu$ where $\epsy$ is the material's yield strain and $\mu$ its shear modulus. Our model provides an excellent fit to the depth dependence of the thermal conductivity in the top $140\,\mathrm{cm}$ of the lunar regolith. It also offers an explanation for the low thermal inertias of rocky asteroids and icy satellites. Lastly, we discuss how rubble piles slow down the cooling of small bodies such as asteroids.

Electromagnetic (EM) follow-up observations of gravitational wave (GW) events will help shed light on the nature of the sources, and more can be learned if the EM follow-ups can start as soon as the GW event becomes observable. In this paper, we propose a computationally efficient time-domain algorithm capable of detecting gravitational waves (GWs) from coalescing binaries of compact objects with nearly zero time delay. In case when the signal is strong enough, our algorithm also has the flexibility to trigger EM observation {\it before} the merger. The key to the efficiency of our algorithm arises from the use of chains of so-called Infinite Impulse Response (IIR) filters, which filter time-series data recursively. Computational cost is further reduced by a template interpolation technique that requires filtering to be done only for a much coarser template bank than otherwise required to sufficiently recover optimal signal-to-noise ratio. Towards future detectors with sensitivity extending to lower frequencies, our algorithm's computational cost is shown to increase rather insignificantly compared to the conventional time-domain correlation method. Moreover, at latencies of less than hundreds to thousands of seconds, this method is expected to be computationally more efficient than the straightforward frequency-domain method.

A pedra da lua: contos de Machado de Assis reunidos em Papéis avulsos e Várias histórias

Machado de Assis, nas coletâneas de contos intituladas Papéis avulsos e Várias histórias, faz repetidas alusões à ficção e ao fazer ficcional, o que leva a pensar na possibilidade da escolha intencional de um eixo temático que percorra as narrativas, permitindo que sejam lidas na compreensão dessa intencionalidade, o que confere ao conjunto uma característica autorreferencial. As evocações de Diderot, Merimée e Edgar Allan Poe nessas famílias de contos situam literariamente um entendimento da ficção que a distingue do engano e da fraude, ao mesmo tempo em que não nega sua força e variedade de usos, enquanto supõe futuros e por vezes obscuros caminhos para os prazeres da sensação estética. No decorrer desta Tese procuro provar que o autor escolhe a narrativa curta para discorrer sobre o fazer ficcional, sendo esse tema um a mais dentre outros, apuradamente ordenados em camadas que não apenas se superpõem, mas interpenetram e reafirmam variadas vertentes de fios narrativos. Machado conta histórias, enquanto trata do próprio ato de contar, dos efeitos e da necessidade da ficção enquanto isso, reafirma-a como instrumento para a intelectualidade, num mundo onde a objetividade cartesiana já não supõe os olhos como fiéis receptores da realidade, mas precisa de outras maneiras de ver e de sentir

Conservação de morcegos no estado do Rio de Janeiro: como e onde já foram amostrados e que locais merecem atenção

A demarcação de Unidades de Conservação é uma forma supostamente eficaz para a conservação da biodiversidade. A Mata Atlântica é caracterizada por apresentar uma elevada biodiversidade e altos níveis de ameaça. O estado do Rio de Janeiro encontra-se totalmente inserido nesse bioma e seus remanescentes florestais são considerados um hotspot dentro de outro hotspot. O Rio de Janeiro pode ser considerado um dos estados melhor amostrados, porém ainda existem lacunas de conhecimentos geográficos sobre a ocorrência de morcegos. Esta tese foi desenvolvida em três capítulos com o objetivo de contribuir com conservação de morcegos no estado do Rio de Janeiro, focando em como e onde eles já foram amostrados e que locais ainda carecem de atenção. Para este estudo foram utilizados dados referentes a buscas bibliográficas e dados de amostragens do Laboratório de Diversidade de Morcegos da Universidade Federal Rural do Rio de Janeiro. No primeiro capítulo pode-se observar que as localidades com mais de 30 espécies de morcegos são resultado de grande esforço de captura e amostragens usando diversas metodologias. Para uma melhor amostragem da riqueza local, devem-se armar redes não somente em trilhas e próximas a árvores em frutificação, mas também sobre corpos de água. Fazer busca em refúgios diurnos também é aconselhável. Devem ser realizadas amostragens durante a noite toda e variar a fase do ciclo lunar, não restringindo a apenas uma ou partes das fases do ciclo lunar. No segundo capítulo observou-se que 43% das Unidades de Conservação aqui estudadas apresentam 20 ou mais espécies. Localidades que apresentam de 20 a 40 espécies de morcegos na Mata Atlântica podem ser consideradas bem amostradas. Isso demonstra que mais da metade das Unidades de Conservação não podem ser consideradas bem inventariadas. Muitos projetos de pesquisas dão prioridade para a localidade estudada ser uma Unidade de Conservação, porém existem poucos trabalhos de longa duração. No Rio de Janeiro ainda existem diversas Unidades de Conservação não amostradas, principalmente aquelas de difícil acesso e em altitudes elevadas. No terceiro capítulo foi possível observar que há uma maior proporção de espécies que apresentam distribuição geográfica restrita. Esse padrão constitui uma informação importante em termos de conservação, visto que indiretamente poderia indicar uma menor capacidade de dispersão desses animais em médias e grandes distâncias. Entretanto existem lacunas de conhecimento em decorrência da falta de amostragem em algumas regiões, sendo imperativos maiores esforços de captura. Importantes municípios para a conservação e/ou preservação de morcegos como Varre-Sai, Cambuci, Miracema, Carmo, Cantagalo, Valença, Barra do Piraí e Piraí não estão sob proteção legal, mesmo constituindo possíveis corredores entre Unidades de Conservação ou mesmo fragmentos importantes que ainda detém espécies que não estão representadas em Unidades de Conservação já estabelecidas. É imperativo que mais estudos e esforços de conservação sejam direcionados para essas áreas

Emigration dynamics of three species of penaeid prawn from backwaters and tidal ponds of Cochin, India

Emigration of three species of penaeid prawn from backwaters and tidal ponds were studied. Considerable diel, tidal, lunar and seasonal fluctuations were observed in emigration process, which was almost nocturnal. Rate of emigration and composition of emigrants varied with time of migration. Large pulses of emigration always coincided with spring tides with major peak during new moon. Seasonal variation was observed with peak emigration of Penaeus indicus during monsoon months and that of Metapenaeus dobsoni and Metapenaeus monoceros during pre-monsoon. Rate of emigration was relatively large from shallow tidal ponds. It correlated directly with the prevailing environmental conditions and juvenile density. Instantaneous rate of emigration was also large in seasonal ponds. The basic stimulus for emigration is the urge for sexual maturation. Coupled with it ecological changes in the habitat have been causing various patterns in migration.

A simple method of tagging prawns

The recognition of individual animals is crucial to many aspects of research. Prawns (Penaeus monodon) present unique difficulties in this respect since they molt regularly. Thus, almost all tagging and marking methods developed for prawns so far have proven inadequate. Some tags or marks are lost during molting; others cause injury to the prawns. A new and efficient method has been developed at the Igang Seafarming Station of the Aquaculture Department. Rectangular brass tags measuring 5 mm by 20 mm and numbered consecutively are used. The prawn is held gently but firmly at the base of the carapace with the left hand while the right hand slips the brass tag around the stalk of the unablated eye and presses the tag gently. All tagging must be made under water to avoid stress. From May 29 to September 7 1977 to a total of 348 unilaterally-ablated adult female prawns were tagged on the unablated eyestalk in 5 batches to enable individual observations on gonadal maturation, molting, and growth. Periodic examinations were made four times a month to coincide with the different phases of the lunar cycle. On each examination, survival and recovery rates were recorded. The data included death due to immediate mortality during ablation and loss to cannibalism for the duration of the experiments. In all five tagging experiments, most of the prawns recovered had their tags intact. These included even dead and molting animals. The eyestalk tagging method is suitable for prawns because the tags can be attached without causing injury and has no effect on the rate of growth, maturity, molting and behavior of the animal. The tags are identifiable and permanent; they remain attached to the animal even after death.

Spawning periodicity of milkfish, Chanos chanos

Daily samplings were conducted in the waters of Batbatan Island from April 17 to June 11, 1977 in order to collect milkfish (Chanos chanos ) eggs. The numbers of eggs collected is tabulated by lunar period. Milkfish fry are more abundant during the new and full moon periods, and periodicity does exist, during the first and last quarter periods.

Ingression, abundance and settlement dynamics of Penaeid chrimp postlarvae in backwaters and adjacent tidal ponds in Cochin, India

Dynamics of penaeid postlarval ingression and settlement in the backwaters of Cochin were studied. Postlarval recruits were constituted by Metapenaeus dobsoni (70.8-78.4%), Penaeus indicus (17.5-24.6%), M. monoceros (3.8-4.6%) and P. monodon (0.3-0.4%). Their composition varied with location and season. Postlarval abundance and ingression were influenced by diel, tidal, lunar and seasonal factors. Ingression is mainly nocturnal in all species with nearly 84% of the activity during night hours. Abundance and ingression peaked up during high tides at night with major peaks coinciding with spring tides of full and new moon. It also followed a generalized seasonal pattern with two well-defined peaks for all species. It was pre-monsoon followed by post-monsoon for P. indicus and M. monoceros and post-monsoon followed by pre-monsoon for M. dobsoni. Sizes of the recruits were relatively small during pre-monsoon and post-monsoon and large during monsoon.

The study of maturational progress in the whitespotted rabbitfish (Siganus sutor) under different photoperiod and light intensity conditions

The rule of light on the timing of maturation and spawning in tropical and subtropical regions is not clear well, because the reproductive cycle in these systems is lunar synchronized. In this study, thus, the effects of different light regimes were investigated on maturational progress of whitespotted rabbitfish, Siganus sutor, the commercial species in Persian Gulf and Oman Sea. During prespawning season, 50 adult fish were randomly divided into ten 300-l tanks (n=5). The fish in control tank received indoor light condition and the fish in each other tanks were exposed to nine different combinations of photoperiod (8L: 16D, 12L: 12D, 16L: 8D) and light intensity (1000, 2000, 3000 lux). After 60 days, GSI and HSI values, serum levels of estradiol (E2), testosterone (T), 17-α hydroxyprogestrone (OHP), calcium (Ca2+) and gonad histology were evaluated for females and males. In females the GSI mean values of exposed fish increased in comparison with control except for fish were kept under 8L, 2000 lux (tank 8). These differences were significant only for fishes in tank 7 (8L, 3000 lux). In the cases of HSI, the results were converse, so that, the most of thanks showed significant decreasing than fishes reared under indoor condition. Morphology and histology study of Ovaries showed three developmental phases including 3, 4 and chiefly 5 that were parallel with GSI values. Fortheremore the serum levels of E2 was recorded between 0.54-15.8 ng/ml in different fish and their mean values were lower than control in all treatmants (P> 0.05). In males, the similar results were obtained. The GSI and HSI mean values in experimental regimes compared with control were upper and lower, respectively, except for fishes were reared in tank 1 (16L, 3000 lux). Testes histology of fishes were reared under different regimes showed signs of stage 5, since no blood vessels observed and thick milt exuded on slight pressure. The mean values of testosterone consentration in fishes were kept in tanks 1 and 6 (12L, 1000 lux) were higher and in other ones were lower than control group. It is also noted that the OHP and Ca2+ had diverse results including increasing and decreasing mean values than control. So, these factors contrary to E2 and T were not suitable to evaluation of maturity in both sexes. On the basis of ovarian structure in stage 5, oocyte development pattern in this species was group synchronous. So, increased mean of GSI versus decreased values of HSI, E2 and perhaps Ca2+ were the signs of improved maturation. But in males, reduced levels of T and similarity of testes morphology in all samples caused that GSI mean value was the only indicator for differentiating among treatments. These findings suggest that alternations were used in light regimes have been the reason of improved maturity in all treatments except fishes reared in tank 8. The ١٠٧ rule of light intensity on induction of maturity was cleared by comparision between fishes in tanks 4, 5, 6 and control group. Because day length was the same whereas fishes in tanks 4, 5 and 6 were exposed to increased light intensity compared with control. This fact verified by results was obtained from fishes in tanks 9 and especially 7, since photoperiod in this group was lower than control. So, higher intensity was considered as the reason of alternations. Contrasting with indoor condition, Induced maturity was also cleared for fishes were kept in tanks 1, 2 and 3, where both of light duration and intensity were increased. But, the rule of photoperiod was individually demonstrated when obtained results were compared with similar light intensities in other treatments. In conclusion, with comparison among different light regimes it is declared that siganids were kept under light condition of tank 2 including 16h light duration combined with 2000 lux intensity showed the best signs of sexual maturation in both sexes. On the basis of this study, setting up the spring light condition during prespawning season induces maturation in withspotted rabbitfish. This improvement not only by influence of photoperiod or light intensity, separately, but obtained through interaction between them. Thus, determination of threshold and resistance to light be recommended before exposure, although using proper regime during suitable time are necessary to achieve purposes considerably.

East African Freshwater Fisheries Research Organization Annual Report 1973

The Annual report presents activities carried out by the Organization during the period 1973. It presents scientific work of the Organization which include: Tissue specificity of malate dehydrogenase in Astatoreochromis and two species of haplochromis, report on LaKe Babati Fishery, Observations on Engraulicypris orgenteus (PELLEGRIN) 1904 from Lake Victoria, Commercial trawl fishing on Lake Victoria: Fisheries development and conservation, Lunar periodicity and the breeding of Tilapia nilotica in the Northern part of Lake Victoria.

Otolith characteristics and age determination of an endemic Ptychobarbus dipogon (Regan, 1905) (Cyprinidae: Schizothoracinae) in the Yarlung Tsangpo River, Tibet

We describe the microincrements, checks and annuli in the lapilli of the schizothoracine Ptychobarbus dipogon, an endemic species of the Tibetan plateau. We collected samples in the Yarlung Tsangpo River and its tributaries on a monthly basis (from April 2004 to August 2006). We describe the shape features of the three pairs of otoliths and document the full trajectory of lapillus development. We found that five to seven checks were clearly visible in the opaque zone of the first annulus. The pattern of 21-23 daily growth increments within each check might be explained as a lunar-induced deposition. We counted between 137 and 154 increments within the first annulus. Annuli appeared as a sequence of gradually declining increment widths, whereas false rings were characterized by abrupt checks. Our oldest estimates were 23(+)years for males and 44(+) for females. The time of annulus completion was clearly between March and April each year using monthly marginal increments analysis. We consider the factors responsible for daily increment formation as an endogenous circadian rhythm. Environmental information, such as strong sunlight and cold water temperatures in the Tibetan Plateau, could reinforce the endogenous daily cycle. Our results provided important data addressing the ecology and population dynamics of P. dipogon.

Daily timing of emersion and elevated atmospheric CO2 concentration affect photosynthetic performance of the intertidal macroalga Ulva lactuca (Chlorophyta) in sunlight

The lunar day differs in length from the solar day so that times of low tide vary from day to day. Thus, aerial exposure of intertidal seaweeds may be during the day or during the night. We measured photosynthetic CO, assimilation rates of the intertidal green macroalga Ulva lactuca during exposures of varied daily timings during sunny days of summer to establish how photosynthetic performance responds to emersion timing under varied CO2 levels [at ambient (360 ppmv) and 2x ambient (720 ppmv) atmospheric CO2 concentrations]. There was an increase in net photosynthetic rates following some duration of exposure when the initial timing of exposure occurred during early morning (06.30 h) and late afternoon (17.15 h). In contrast, net rates exhibited a sharp decline with exposure duration when the initial timing of exposure occurred at 09.30 h, 15.30 h and especially at noon (12.30 h), implying the occurrence of a severe photoinhibition resulting from mid-day insolation. Doubled atmospheric CO2 concentration significantly enhanced the emersed photosynthetic rates, indicating that the emersed photosynthesis is CO2-limited at ambient CO2 levels. However, increasing CO2 barely stimulates the emersed photosynthetic rates during mid-day insolation.