The Brown algae Sargassum muticum in the Atlantic coast of Morocco: new record in Africa and risks of its potential expansion to nearby areas

Centro de Biodiversidad y Gestión Ambiental, Facultad de Ciencias del Mar, Universidad de Las Palmas de Gran Canaria, Las Palmas, Spain

Effects of ocean acidification on the brown alga "Padina pavonica": decalcification due to acute and chronic events

[EN] Since the industrial revolution, anthropogenic CO2 emissions have caused ocean acidification, which particularly affects calcified organisms. Given the fan-like calcified fronds of the brown alga Padina pavonica, we evaluated the acute (shortterm) effects of a sudden pH drop due to a submarine volcanic eruption (October 2011–early March 2012) affecting offshore waters around El Hierro Island (Canary Islands, Spain). We further studied the chronic (long-term) effects of the continuous decrease in pH in the last decades around the Canarian waters. In both the observational and retrospective studies (using herbarium collections of P. pavonica thalli from the overall Canarian Archipelago), the percent of surface calcium carbonate coverage of P. pavonica thalli were contrasted with oceanographic data collected either in situ (volcanic eruption event) or from the ESTOC marine observatory data series (herbarium study). Results showed that this calcified alga is sensitive to acute and chronic environmental pH changes. In both cases, pH changes predicted surface thallus calcification, including a progressive decalcification over the last three decades. This result concurs with previous studies where calcareous organisms decalcify under more acidic conditions. Hence, Padina pavonica can be implemented as a bio-indicator of ocean acidification (at short and long time scales) for monitoring purposes over wide geographic ranges, as this macroalga is affected and thrives (unlike strict calcifiers) under more acidic conditions

GC/MS-Meßsystem für Nicht-Methan-Kohlenwasserstoffe

Im Rahmen der Projekte CARIBIC ('Civil Aircraft for the Regular Investigation of the atmosphere Based on an Instrument Container') und INDOEX ('Indian Ocean Experi-ment') wurde ein Gaschromatograph mit Massenspektrometer zur Analyse von Luftproben auf Nicht-Methan-Kohlenwasserstoffe (NMKW) im ppb- und ppt-Bereich entwickelt. Während INDOEX erfolgte die Probennahme auf dem Forschungsschiff Ronald Brown, während CARIBIC mit einem automatischen Probensammler an Bord eines Passagierflugzeuges (Boeing 767-ER, LTU). Die NMKW-Meßergebnisse wurden zusammen mit Ergebnissen von Mes-sungen von Kohlenmonoxid (CO, einschließlich Isotopenzusam-mensetzung), Ozon (O3), Methan (CH4), Kohlendioxid (CO2), Distickstoffmonoxid (N2O), Schwefelhexafluorid (SF6) und Aerosoleigenschaften sowie meteorologischen Daten inter-pretiert. Während INDOEX (Februar / März 1999) wurde in der maritimen Grenzschicht (MBL) des Indischen Ozeans (IO) eine starke Variabilität diverser Spurengase beobachtet, die teilweise durch regionale Emissionen hervorgerufen wurde, die stärkste Variabilität war jedoch durch Langstrecken-transport aus mittleren Breiten der Nordhemisphäre bedingt. Aufgrund der Abweichungen vom klimatologischen Mittel, sollten regionale Quellen die MBL des IO im allgemeinen stärker beeinflussen. Die Einteilung des IO in meteorologi-sche Luftmassenregime wurde bestätigt. Starke Spurengasgra-dienten an der innertropischen Konvergenzzone (ITCZ) zeigen, daß die ITCZ in erster Linie den Austausch von Luftmassen zwischen den Hemisphären behindert. Bei CARIBIC werden Messungen von Spurengasen (ein-(schließlich NMKW) und Aerosoleigenschaften auf Flügen in der oberen Troposphäre / unteren Stratosphäre durchgeführt. Während eines Flug über Afrika wurden der Einfluß von durch Konvektion in die obere Troposphäre eingebrachten, frischen Abgasen aus Biomassenverbrennung nachgewiesen. Andere Luft-massen wurden durch Emissionen von Erdgas bzw. durch die Stratosphäre beeinflußt.

Brown band disease: valutazione della distribuzione e prevalenza in relazione a diversi gradi di antropizzazione nella Repubblica delle Maldive

Nonostante lo sforzo sempre crescente mirato allo studio delle malattie che colpiscono le sclerattinie, ancora poco si sa circa distribuzione, prevalenza, host range e fattori che concorrono alla comparsa di queste patologie, soprattutto nell’area indopacifica. Questo studio si propone quindi lo scopo di documentare la presenza della Brown Band Disease all’interno delle scogliere madreporiche dell’Arcipelago delle Maldive. Nell’arco di tempo tra Novembre e Dicembre 2013 è stata effettuata una valutazione di tipo quantitativo di tale patologia su tre isole appartenenti l’Atollo di Faafu, rispettivamente Magoodhoo, Filitheyo e Adangau. Queste tre isole sono caratterizzate da un diverso sfruttamento da parte dell’uomo: la prima isola è abitata da locali, la seconda caratterizzata dalla presenza di un resort e l’ultima, un’isola deserta. Al fine di valutare prevalenza, distribuzione e host range della BrBD sono stati effettuati belt transect (25x2 m), point intercept transect e analisi chimico fisiche delle acque. La Brown Band Disease è risultata essere diffusa tra le isole con prevalenze inferiori al 0,50%. Queste non hanno mostrato differenze significative tra le isole, facendo quindi ipotizzare che i diversi valori osservati potrebbero essere imputati a variazioni casuali e naturali. In tutta l’area investigata, le stazioni più profonde hanno mostrato valori di prevalenza maggiori. La patologia è stata registrata infestare soprattutto il genere Acropora (con prevalenza media totale inferiore all’1%) e in un solo caso il genere Isopora. È stato dimostrato come sia presente una correlazione negativa tra densità totale delle sclerattinie e la prevalenza della Brown Band sul genere Acropora. É stato inoltre notato come vi fosse una correlazione positiva tra la prevalenza della BrBD e la presenza del gasteropode Drupella sulle colonie già malate. Poiché il principale ospite della patologia è anche il più abbondante nelle scogliere madreporiche maldiviane, si rendono necessari ulteriori accertamenti e monitoraggi futuri della BrBD.

John Ronald Reuel Tolkien fra critica e traduzione: Il caso della history of Middle-Earth

Il progetto si propone di tradurre parti di un’opera di John Ronald Reuel Tolkien inedita in Italia. Si tratta dell'introduzione e di un capitolo del settimo volume della History of Middle-Earth, che raccoglie l’intero corpus degli scritti tolkeniani e ne ricostruisce l’evoluzione narrativa. La tesi, oltre al capitolo dedicato alla traduzione dall'inglese all'italiano e alla discussione delle scelte traduttive, include: alcune notizie biografiche su Tolkien, con particolare riferimento agli anni giovanili; una discussione sulla legittimità di un suo eventuale inserimento all'interno dei canoni letterari; una discussione sulle differenti interpretazioni de Il Signore degli Anelli; una discussione sui contenuti di tutti i volumi della History e sulle difficoltà che sorgono nella traduzione delle opere di Tolkien.

Brown Dwarf Binaries

Nearly 500 brown dwarfs have been discovered in recent years. The majority of these brown dwarfs exist in the solar neighborhood, yet determining their fundamental properties (mass, age, temperature & metallicity) has proved to be quite difficult, with current estimates relying heavily on theoretical models. Binary brown dwarfs provide a unique opportunity to empirically determine fundamental properties, which can then be used to test model predictions. In addition, the observed binary fractions, separations, mass ratios, & orbital eccentricities can provide insight into the formation mechanism of these low-mass objects. I will review the results of various brown dwarf multiplicity studies, and will discuss what we have learned about the formation and evolution of brown dwarfs by examining their binary properties as a function of age and mass.

Characterization of Halyomorpha halys (brown marmorated stink bug) biogenic volatile organic compound emissions and their role in secondary organic aerosol formation.

The formation of aerosols is a key component in understanding cloud formation in the context of radiative forcings and global climate modeling. Biogenic volatile organic compounds (BVOCs) are a significant source of aerosols, yet there is still much to be learned about their structures, sources, and interactions. The aims of this project were to identify the BVOCs found in the defense chemicals of the brown marmorated stink bug Halymorpha halys and quantify them using gas chromatography-mass spectrometry (GC/MS) and test whether oxidation of these compounds by ozone-promoted aerosol and cloud seed formation. The bugs were tested under two conditions: agitation by asphyxiation and direct glandular exposure. Tridecane, 2(5H)-furanone 5-ethyl, and (E)-2-decenal were identified as the three most abundant compounds. H. halys were also tested in the agitated condition in a smog chamber. It was found that in the presence of 100-180 ppm ozone, secondary aerosols do form. A scanning mobility particle sizer (SMPS) and a cloud condensation nuclei counter (CCNC) were used to characterize the secondary aerosols that formed. This reaction resulted in 0.23 microg/ bug of particulate mass. It was also found that these secondary organic aerosol particles could act as cloud condensation nuclei. At a supersaturation of 1%, we found a kappa value of 0.09. Once regional populations of these stink bugs stabilize and the populations estimates can be made, the additional impacts of their contribution to regional air quality can be calculated.

White-Nose Syndrome-Affected Litttle Brown Myotis (Myotis Lucifugus) Increase Grooming and Other Active Behaviors During Arousals from Hibernation

White-nose syndrome (WNS) is an emerging infectious disease of hibernating bats linked to the death of an estimated 5.7 million or more bats in the northeastern United States and Canada. White-nose syndrome is caused by the cold-loving fungus Pseudogymnoascus destructans (Pd), which invades the skin of the muzzles, ears, and wings of hibernating bats. Previous work has shown that WNS-affected bats arouse to euthermic or near euthermic temperatures during hibernation significantly more frequently than normal and that these too-frequent arousals are tied to severity of infection and death date. We quantified the behavior of bats during these arousal bouts to understand better the causes and consequences of these arousals. We hypothesized that WNS-affected bats would display increased levels of activity (especially grooming) during their arousal bouts from hibernation compared to WNS-unaffected bats. Behavior of both affected and unaffected hibernating bats in captivity was monitored from December 2010 to March 2011 using temperature-sensitive dataloggers attached to the backs of bats and infrared motion-sensitive cameras. The WNS-affected bats exhibited significantly higher rates of grooming, relative to unaffected bats, at the expense of time that would otherwise be spent inactive. Increased self-grooming may be related to the presence of the fungus. Elevated activity levels in affected bats likely increase energetic stress, whereas the loss of rest (inactive periods when aroused from torpor) may jeopardize the ability of a bat to reestablish homeostasis in a number of physiologic systems.

Infrared Parallaxes of Young Field Brown Dwarfs and Connections to Directly Imaged Gas-Giant Exoplanets

We have measured high-precision infrared parallaxes with the Canada-France-Hawaii Telescope for a large sample of candidate young (approximate to 10-100 Myr) and intermediate-age (approximate to 100-600 Myr) ultracool dwarfs, with spectral types ranging from M8 to T2.5. These objects are compelling benchmarks for substellar evolution and ultracool atmospheres at lower surface gravities (i.e., masses) than most of the field population. We find that the absolute magnitudes of our young sample can be systematically offset from ordinary (older) field dwarfs, with the young late-M objects being brighter and the young/dusty mid-L (L3-L6.5) objects being fainter, especially at J band. Thus, we conclude the "underluminosity" of the young planetary-mass companions HR 8799b and 2MASS J1207-39b compared to field dwarfs is also manifested in young free-floating brown dwarfs, though the effect is not as extreme. At the same time, some young objects over the full spectral type range of our sample are similar to field objects, and thus a simple correspondence between youth and magnitude offset relative to the field population appears to be lacking. Comparing the kinematics of our sample to nearby stellar associations and moving groups, we identify several new moving group members, including the first free-floating L dwarf in the AB Dor moving group, 2MASS J0355+11. Altogether, the effects of surface gravity (age) and dust content on the magnitudes and colors of substellar objects appear to be degenerate. (C) 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim