Relations between coal petrology and gas content in the Upper Newlands Seam, central Queensland, Australia

The Upper Newlands Seam in the northern Bowen Basin, Queensland, Australia consists of six benches (A-F) that have different petrographic assemblages. Benches C and E contain relatively abundant inertodetrinite and mineral matter, as well as anomalously high reflectance values; these characteristics support a largely allochthonous, detrital origin for the C and E benches. Fractures and cleats in the seam show a consistent orientation of northeast- southwest for face cleats, and a wide range of orientations for fractures. Cleat systems are well developed in bright bands, with poor continuity in the dull coal. Both maceral content and cleat character are suggested to influence gas drainage in the Upper Newlands Seam. A pronounced positive correlation between vitrinite abundance and gas desorption data suggests more efficient drainage from benches with abundant vitrinite. Conversely, inertinite-rich benches are suggested to have less efficient drainage, and possibly retain gas within pore spaces, which could increase the outburst potential of the coal. (C) 2001 Elsevier Science BN. All rights reserved.

Random primordial magnetic fields and the gas content of dark matter haloes

We recently predicted the existence of random primordial magnetic fields (RPMFs) in the form of randomly oriented cells with dipole-like structure with a cell size L(0) and an average magnetic field B(0). Here, we investigate models for primordial magnetic field with a similar web-like structure, and other geometries, differing perhaps in L(0) and B(0). The effect of RPMF on the formation of the first galaxies is investigated. The filtering mass, M(F), is the halo mass below which baryon accretion is severely depressed. We show that these RPMF could influence the formation of galaxies by altering the filtering mass and the baryon gas fraction of a halo, f(g). The effect is particularly strong in small galaxies. We find, for example, for a comoving B(0) = 0.1 mu G, and a reionization epoch that starts at z(s) = 11 and ends at z(e) = 8, for L(0) = 100 pc at z = 12, the f(g) becomes severely depressed for M < 10(7) M(circle dot), whereas for B(0) = 0 the f(g) becomes severely depressed only for much smaller masses, M < 10(5) M(circle dot). We suggest that the observation of M(F) and f(g) at high redshifts can give information on the intensity and structure of primordial magnetic fields.

X-ray properties and evolution of high-redshift AGN, and the gas content of host galaxies

In this thesis, I have investigated the evolution of the high-redshift (z > 3) AGN population by collecting data from some of the major Chandra and XMM-Newton surveys. The final sample (141 sources) is one of the largest selected at z> 3 in the X- rays and it is characterised by a very high redshift completeness (98%). I derived the spectral slopes and obscurations through a spectral anaysis and I assessed the high-z evolution by deriving the luminosity function and the number counts of the sample. The best representation of the AGN evolution is a pure density evolution (PDE) model: the AGN space density is found to decrease by a factor of 10 from z=3 to z=5. I also found that about 50% of AGN are obscured by large column densities (logNH > 23). By comparing these data with those in the Local Universe, I found a positive evolution of the obscured AGN fraction with redshift, especially for luminous (logLx > 44) AGN. I also studied the gas content of z < 1 AGN-hosting galaxies and compared it with that of inactive galaxies. For the first time, I applied to AGN a method to derive the gas mass previously used for inactive galaxies only. AGN are found to live preferentially in gas-rich galaxies. This result on the one hand can help us in understanding the AGN triggering mechanisms, on the other hand explains why AGN are preferentially hosted by star-forming galaxies.

Gas content, composition of gas hydrate and volumetric gas/water ratios of ODP and DSDP sites

Gas hydrate samples were recovered from four sites (Sites 994, 995, 996, and 997) along the crest of the Blake Ridge during Ocean Drilling Program (ODP) Leg 164. At Site 996, an area of active gas venting, pockmarks, and chemosynthetic communities, vein-like gas hydrate was recovered from less than 1 meter below seafloor (mbsf) and intermittently through the maximum cored depth of 63 mbsf. In contrast, massive gas hydrate, probably fault filling and/or stratigraphically controlled, was recovered from depths of 260 mbsf at Site 994, and from 331 mbsf at Site 997. Downhole-logging data, along with geochemical and core temperature profiles, indicate that gas hydrate at Sites 994, 995, and 997 occurs from about 180 to 450 mbsf and is dispersed in sediment as 5- to 30-m-thick zones of up to about 15% bulk volume gas hydrate. Selected gas hydrate samples were placed in a sealed chamber and allowed to dissociate. Evolved gas to water volumetric ratios measured on seven samples from Site 996 ranged from 20 to 143 mL gas/mL water to 154 mL gas/mL water in one sample from Site 994, and to 139 mL gas/mL water in one sample from Site 997, which can be compared to the theoretical maximum gas to water ratio of 216. These ratios are minimum gas/water ratios for gas hydrate because of partial dissociation during core recovery and potential contamination with pore waters. Nonetheless, the maximum measured volumetric ratio indicates that at least 71% of the cages in this gas hydrate were filled with gas molecules. When corrections for pore-water contamination are made, these volumetric ratios range from 29 to 204, suggesting that cages in some natural gas hydrate are nearly filled. Methane comprises the bulk of the evolved gas from all sites (98.4%-99.9% methane and 0%-1.5% CO2). Site 996 hydrate contained little CO2 (0%-0.56%). Ethane concentrations differed significantly from Site 996, where they ranged from 720 to 1010 parts per million by volume (ppmv), to Sites 994 and 997, which contained much less ethane (up to 86 ppmv). Up to 19 ppmv propane and other higher homologues were noted; however, these gases are likely contaminants derived from sediment in some hydrate samples. CO2 concentrations are less in gas hydrate than in the surrounding sediment, likely an artifact of core depressurization, which released CO2 derived from dissolved organic carbon (DIC) into sediment. The isotopic composition of methane from gas hydrate ranges from d13C of -62.5 per mil to -70.7 per mil and dD of -175 per mil to -200 per mil and is identical to the isotopic composition of methane from surrounding sediment. Methane of this isotopic composition is mainly microbial in origin and likely produced by bacterial reduction of bicarbonate. The hydrocarbon gases here are likely the products of early microbial diagenesis. The isotopic composition of CO2 from gas hydrate ranges from d13C of -5.7 per mil to -6.9 per mil, about 15 per mil lighter than CO2 derived from nearby sediment.

The molecular gas content of star-forming galaxies in the ALPINE fields.

In this thesis, I aim to study the evolution with redshift of the gas mass fraction of a sample of 53 sources (from z ∼ 0.5 to z > 5) serendipitously detected in ALMA band 7 as part of the ALMA Large Program to INvestigate C II at Early Times (ALPINE). First, I used SED-fitting software CIGALE, which is able to implement energy balancing between the optical and the far infrared part, to produce a best-fit template of my sources and to have an estimate of some physical properties, such as the star formation rate (SFR), the total infrared luminosity and the total stellar mass. Then, using the tight correlation found by Scoville et al. (2014) between the ISM molecular gas mass and the rest-frame 850 μm luminosity, I used the latter, extrapolating it from the best-fit template using a code that I wrote in Python, as a tracer for the molecular gas. For my sample, I then derived the most important physical properties, such as molecular gas mass, gas mass fractions, specific star formation rate and depletion timescales, which allowed me to better categorize them and find them a place within the evolutionary history of the Universe. I also fitted our sources, via another code I wrote again in Python, with a general modified blackbody (MBB) model taken from the literature (Gilli et al. (2014), D’Amato et al. (2020)) to have a direct method of comparison with similar galaxies. What is evident at the end of the paper is that the methods used to derive the physical quantities of the sources are consistent with each other, and these in turn are in good agreement with what is found in the literature.

Instantaneous outbursts in underground coal mines: An overview and association with coal type

Instantaneous outbursts in underground coal mines have occurred in at least 16 countries, involving both methane (CH4) and carbon dioxide (CO2). The precise mechanisms of an instantaneous outburst are still unresolved but must consider the effects of stress, gas content and physico-mechanical properties of the coal. Other factors such as mining methods (e.g., development heading into the coal seam) and geological features (e.g., coal seam disruptions from faulting) can combine to exacerbate the problem. Prediction techniques continue to be unreliable and unexpected outburst incidents resulting in fatalities are a major concern for underground coal operations. Gas content thresholds of 9 m(3)/t for CH4 and 6 m(3)/t for CO2 are used in the Sydney Basin, to indicate outburst-prone conditions, but are reviewed on an individual mine basis and in mixed as situations. Data on the sorption behaviour of Bowen Basin coals from Australia have provided an explanation for the conflicting results obtained by coal face desorption indices used for outburst-proneness assessment. A key factor appears to be different desorption rates displayed by banded coals, which is supported by both laboratory and mine-site investigations. Dull coal bands with high fusinite and semifusinite contents tend to display rapid desorption from solid coal, for a given pressure drop. The opposite is true for bright coal bands with high vitrinite contents and dull coal bands with high inertodetrinite contents. Consequently, when face samples of dull, fusinite-or semifusinite-rich coal of small particle size are taken for desorption testing, much gas has already escaped and low readings result. The converse applies for samples taken from coal bands with high vitrinite and/or inertodetrinite contents. In terms of outburst potential, it is the bright, vitrinite-rich and the dull, inertodetrinite-rich sections of a coal seam that appear to be more outburst-prone. This is due to the ability of the solid coal to retain gas, even after pressure reduction, creating a gas content gradient across the coal face sufficient to initiate an outburst. Once the particle size of the coal is reduced, rapid gas desorption can then take place. (C) 1998 Elsevier Science.

Neue Erkenntnisse zum geologischen Bau des “Kleinen Berges” zwischen Bad Laer und Bad Rothenfelde (südwestliches Niedersachsen) aufgrund der Ergebnisse der Tiefbohrung ‘Bad Laer Z 1’

The 2108,0 m deep exploration well "Bad Laer Z 1" (1993) has been carried down in order to investigate the deeper ground lying beneath the "Kleiner Berg" anticline, concerning the existence of reservoir beds which was postulated according to preceeding seismic investigations. This aim of the borehole was not attained, because no formations have been drilled suitable for the construction of an artificial gas reservoir. On the other hand the bore hole revealed a great amount of new regional geologic, stratigraphic, mining, coalification and coal bed gas data. Therefore, from a scientific point of view the exploration well must be considered successful. After the drilling of a stratigraphic succession, mainly consisting of cretaceous "Pläner" limestones (from Albian to Turonian), surprisingly in a depth of only 439 m productive Upper Carboniferous rocks formed by the Lembeck beds of uppermost Westfalian C have been found. In addition to this discovery, nearly the whole Westfalian C and B reaching down to the coal bed "Katharina" at the Westfalian A boundary were drilled through revealing over 66 partly minable coal beds. Investigations of the coalification pattern showed a more or less continuous increase of the rank gradient with depth reaching from the step of gas flame coal down to 700 m over that of gas coal down to 1600 m to that of fat coal down to the bottom of the borehole. An additional surprising result of the exploration well was the observation, that immediately below the base of the Cretaceous the coal beds revealed a high gas content without the presence of a desorption zone. This result must also be considered as success of the drilling with respect to the strong interest in a potential utilization of coal bed methane nowadays.

Exploiting a prioritized MAC protocol to efficiently compute interpolations

Consider a network where all nodes share a single broadcast domain such as a wired broadcast network. Nodes take sensor readings but individual sensor readings are not the most important pieces of data in the system. Instead, we are interested in aggregated quantities of the sensor readings such as minimum and maximum values, the number of nodes and the median among a set of sensor readings on different nodes. In this paper we show that a prioritized medium access control (MAC) protocol may advantageously be exploited to efficiently compute aggregated quantities of sensor readings. In this context, we propose a distributed algorithm that has a very low time and message-complexity for computing certain aggregated quantities. Importantly, we show that if every sensor node knows its geographical location, then sensor data can be interpolated with our novel distributed algorithm, and the message-complexity of the algorithm is independent of the number of nodes. Such an interpolation of sensor data can be used to compute any desired function; for example the temperature gradient in a room (e.g., industrial plant) densely populated with sensor nodes, or the gas concentration gradient within a pipeline or traffic tunnel.

Kaasun jakauma paineellisissa sulpunkäsittelylaitteissa

Työn tarkoituksena oli tutkia kuinka kaasukuplat jakautuvat sellususpensioon, kun prosessiolosuhteita muutetaan. Kuplien kokojakauman avulla pyritään kartoittamaan kuinka kaasukuplat pilkkoutuvat ja onko olemassa raja-arvoa, milloin tehon lisäys ei enää pilko sellususpensiossa olevia kuplia pienemmiksi. Jakaumien avulla voidaan mahdollisesti kehittää kaasunpoistoa. Työssä selvitettiin voidaanko kameratekniikkaa käyttää kuplakokojen määrittämiseen sellusulpusta. Läpinäkymätön sellumassa tarjoaa kuvaukselle haasteellisen ympäristön. Myöskään kirjallisuudessa ei vastaavaa menetelmää aikaisemmin oltu käytetty. Kuvatusta materiaalista laskettiin kuplien halkaisijat, joita pyrittiin tarkastelemaan tilastollisesti. Tilastollinen tarkastelu toi eroja mittauspisteiden välille. Kuplien halkaisijoiden perusteella mallinnettiin kuplakokoon vaikuttavat prosessisuureet lineaarisella regressioanalyysillä. Mallinnuksen perusteella saatiinvasteisiin vaikuttavat riippumattomat muuttujat ja niiden matemaattiset malliyhtälöt. Tuloksina saatiin selville, että kuplien kokojakaumissa on eroja sekoitussäiliön eri puolilla. Sekoitussäiliössä suurten kuplien suhteellinen osuus kasvaa kaasupitoisuuden ja sakeuden noustessa. Mallinnuksen tärkeimpänä tuloksena voidaan todeta, että sakeus ja kaasutilavuus vaikuttavat kuplakokoon kasvattavasti. Kierrosnopeuden kasvattaminen pienentää kuplakokoa. Visuaalisen informaation avulla on helpompi ymmärtää kuinka kuplat käyttäytyvät.

Teollisuuden jäähdytysjärjestelmät. Case: Kaasunerotuslaitteiston evaluointi

Teollisuuden jäähdytysjärjestelmiä tarvitaan prosessien lämpötilan ja paineen hal-litsemiseen. Vesi on käytetyin lämmönsiirtoaine hyvän saatavuutensa, halvan hin-nan ja korkean lämmönsiirtokyvyn ansiosta. Jäähdytysjärjestelmät jaetaan kolmeen päätyyppiin, joita ovat läpivirtausjäähdytys, suljettu ja avoin kiertojäähdytys. Kullakin järjestelmätyypillä on tyypilliset alatyyppinsä. Avoimella kiertojär-jestelmällä on eniten alatyyppejä, joista yleisin on jäähdytystorni. Jäähdytystorneja on kolmea tyyppiä: märkä-, kuiva ja hybriditorni. Kullakin järjestelmätyypillä on ominaiset piirteensä käyttökohteiden, ympäristövaikutusten, ohjattavuuden, investointi- ja käyttökulujen suhteen, joita tässä työssä esitellään. Työssä tutkitaan teollisuuden jäähdytysjärjestelmien esittelyn lisäksi erään ali-painekaasunpoistimen soveltuvuutta suljetun kiertojäähdytysjärjestelmän kaasun-poistoon. Suljettuun kiertojäähdytysjärjestelmään jää ilmaa täyttövaiheessa ja kul-keutuu liuenneena käytettävän jäähdytysveden mukana. Muodostuva ylikylläinen seos synnyttää veden sekaan ilmakuplia, jotka aiheuttavat korroosiota kemiallisesti ja kuluttamalla. Lisäksi kaasukuplat vievät tilavuutta nesteeltä. Tämä pienentää järjestelmän jäähdytystehoa merkittävästi, koska kaasun lämmönsiirtokyky verrat-tuna veden lämmönsiirtokykyyn on pieni. Työssä esitellään myös muita mahdolli-sia suljetun järjestelmän kaasulähteitä ja niiden aiheuttamia ongelmia. Alipainekaasunpoistimen kaasunerotustehokkuutta mitattiin jäähdytysvesinäyttei-den selkeytymisnopeudella ja lämmönsiirtimien tehon paranemisella. Kahden viikon tarkastelujaksolla selkeytymisajat paranivat 36–60 % eri mittauspaikoissa ja lämmönsiirtimien tehot paranivat 6–29 %. Järjestelmään kuitenkin jäi merkittävä määrä kaasua, vaikka laitteen käyttöä jatkettiin tarkastelujakson jälkeen, joten tavoitteisiin ei päästy. Tutkitun alipainekaasunpoistolaitteen ei todettu soveltuvan tehdasympäristöön kestämättömyyden, hankalakäyttöisyyden ja tehottomuuden takia. Tulokset kuitenkin osoittavat, että kaasunerotuksella on merkittävä vaikutus suljetun jäähdytysjärjestelmän toimivuuteen ja saavutettavaan jäähdytystehoon.

GALAXY EVOLUTION IN A COMPLEX ENVIRONMENT: A MULTI-WAVELENGTH STUDY OF HCG 7

The environment where galaxies are found heavily influences their evolution. Close groupings, like the ones in the cores of galaxy clusters or compact groups, evolve in ways far more dramatic than their isolated counterparts. We have conducted a multi-wavelength study of Hickson Compact Group 7 (HCG 7), consisting of four giant galaxies: three spirals and one lenticular. We use Hubble Space Telescope (HST) imaging to identify and characterize the young and old star cluster populations. We find young massive clusters (YMCs) mostly in the three spirals, while the lenticular features a large, unimodal population of globular clusters (GCs) but no detectable clusters with ages less than a few Gyr. The spatial and approximate age distributions of the similar to 300 YMCs and similar to 150 GCs thus hint at a regular star formation history in the group over a Hubble time. While at first glance the HST data show the galaxies as undisturbed, our deep ground-based, wide-field imaging that extends the HST coverage reveals faint signatures of stellar material in the intragroup medium (IGM). We do not, however, detect the IGM in H I or Chandra X-ray observations, signatures that would be expected to arise from major mergers. Despite this fact, we find that the H I gas content of the individual galaxies and the group as a whole are a third of the expected abundance. The appearance of quiescence is challenged by spectroscopy that reveals an intense ionization continuum in one galaxy nucleus, and post-burst characteristics in another. Our spectroscopic survey of dwarf galaxy members yields a single dwarf elliptical galaxy in an apparent stellar tidal feature. Based on all this information, we suggest an evolutionary scenario for HCG 7, whereby the galaxies convert most of their available gas into stars without the influence of major mergers and ultimately result in a dry merger. As the conditions governing compact groups are reminiscent of galaxies at intermediate redshift, we propose that HCGs are appropriate for studying galaxy evolution at z similar to 1-2.

Políticas de conteúdo local: crescimento econômico e rule of law

As chamadas Políticas de Conteúdo Local (“PCLs”) fazem parte de um grupo de políticas desenvolvimentistas adotadas em todo o mundo com o objetivo de maximizar os benefícios sociais e econômicos decorrentes de determinadas atividades econômicas. Neste trabalho, analisaram-se, principalmente, as PCLs relativas à extração e produção de petróleo e gás. O instituto é juridicamente polêmico, uma vez que, além de ser difícil de definir, é instrumentalizado por diversos atos normativos diferentes. Tal situação agrava-se com o fato de que o desenho de cada PCL pode sugerir ou impor diversas medidas de implementação diferentes, com impactos nas diferentes áreas do Direito. Considerando este cenário, aponta-se que o principal objetivo deste trabalho é a análise de transplantes ao nosso ordenamento jurídico de PCLs bem-sucedidas em ordenamentos jurídicos estrangeiros. Para isso, demonstrou-se, em um primeiro momento, que o instituto das PCLs deve ser reinterpretado à luz da Constituição vigente. Isso porque as PCLs foram criadas em uma época em que a escola desenvolvimentista principal era a keynesiana, que foi substituída atualmente pela escola do Rule of Law. Embora nosso ordenamento jurídico tenha acompanhado essa evolução (através de Emendas Constitucionais e adoção de determinadas leis), as PCLs não acompanharam e, por isso, precisam sofrer essa releitura. Nesse sentido, extraíram-se da Lei quatro elementos principais que as PCLs devem preencher para estar em consonância com o Rule of Law: (A) Benefícios aos Consumidores Finais; (B) Sustentabilidade; (C) Transetorialidade; e (D) Ampliação do Mercado de Trabalho. Em sequência, classificaram-se as diversas PCLs mapeadas, exemplificando cada uma. Ao longo da classificação, apontaram-se três critérios que facilitam a identificação das maiores dificuldades jurídicas em cada transplante: (A) Canal; (B) Natureza; e (C) Instrumento. Por fim, quatro PCLs estrangeiras bem-sucedidas foram escolhidas para uma análise mais aprofundada: a Kazakhstan Contract Agency, no Cazaquistão, a Petro Arctic Supplier Asssociation, na Noruega, o Australian Industry Participation Plan na Austrália e o Nigerian Oil & Gas Content Industry Development Act, na Nigéria. Para cada uma, é dedicada uma análise especial. As análises são seguidas pela Conclusão.