Effizientes Vierwellenmischen durch Ausnutzen von Resonanzen in Quecksilber

In dieser Arbeit wird eine kohärente, kontinuierliche Strahlungsquelle im vakuum-ultravioletten (VUV) Spektrum vorgestellt. Sie basiert auf einem Vierwellenmischprozess in Quecksilberdampf mit Fundamentalstrahlen bei 253,7 nm, 407,9 nm und 545,5 nm Wellenlänge. Diese fundamentalen Strahlen werden durch frequenzverdoppelte bzw. frequenzvervierfachte Festkörperlasersysteme bereit gestellt. Durch das Ausnutzen der 6^1S-7^1S Zweiphotonenresonanz und zusätzlich der 6^1S-6^3P Einphotonenresonanz kann der Vierwellenmischprozess deutlich effizienter betrieben werden als zuvor. Eine nahe Einphotonenresonanz verringert die optimale Phasenanpassungstemperatur des Vierwellenmischprozesses, wodurch Druck- und Stoßverbreiterungen des Quecksilbers verkleinert und damit der nichtlineare Prozess effizienter wird. So können Leistungen bis zu 0,3 nW bei 121,56 nm, dem 1S-2P Lyman-alpha Übergang von Wasserstoff, erzeugt werden. Diese Lyman-alpha Quelle soll für die zukünftige Laserkühlung von Antiwasserstoff genutzt werden. rnrnNeben der Generierung von Strahlung bei Lyman-alpha kann, durch Veränderung der dritten Fundamentalwellenlänge, auch Strahlung in der Nähe zu einer Einphotonresonanz im VUV bei dem 6^1S-12^1P Übergang in Quecksilber durch Vierwellenmischen erzeugt werden. Durch diese weitere Einphotonresonanz kann die nichtlineare Suszeptibilität, verantwortlich für das Vierwellenmischen, stark vergrößert werden, ohne Einfluss auf die Phasenanpassung zu haben. Damit lässt sich der Mischprozess um drei Größenordnungen effizienter gestalten und Leistungen von 6 µW im VUV konnten realisiert werden. Dies entspricht einer Leistungsteigerung um einen Faktor 30 im Vergleich zu früheren Quellen. rnrnDarüberhinaus konnte die Zweiphotonenresonanz in Quecksilber ausführlich untersucht werden. Man erhält bei kleinen Rabifrequenzen der Fundamentalstrahlen eine geschwindigkeitsselektive Doppelresonanz, die den gleichen Ursprung wie Dunkelresonanzen in Lambda-Systemen hat. Bei hohen Rabifrequenzen kann die Anregung in das Zweiphotonenniveau so stark werden, dass auf dem 7^1S-6^1P Übergang ein Laserprozess initiiert wird. Dieser Prozess wurde hier zum ersten Mal mit kontinuierlichen Fundamentallasern nachgewiesen. Es wird gezeigt, dass der zusätzliche Laserprozess das Vierwellenmischen nicht beeinträchtigt.

Erzeugung vakuumultravioletter Strahlung durch Vierwellenmischen in einer Hohlfaser

In dieser Arbeit wird die Entwicklung und experimentelle Umsetzung einer kontinuierlichen, kohärenten Lichtquelle im vakuumultravioletten Wellenlängenbereich um 122 nm präsentiert. Diese basiert auf der nichtlinearen optischen Summenfrequenzmischung dreier Fundamentallaserstrahlen in einer mit Quecksilberdampf gefüllten Hohlfaser. Die Wellenlängen der fundamentalen Laser sind dabei an der Niveaustruktur des Quecksilbers orientiert, um eine mehrfach resonante Überhöhung der nichtlinearen Suszeptibilität zu erreichen. Der transversale Einschluss der Lichtfelder in der Faser verlängert die Wechselwirkungszone mit dem nichtlinearen Medium um mehrere Größenordnungen gegenüber dem Regime fokussierter Strahlen und erlaubt so signifikante Steigerungen der Mischeffizienz.rnrnIm Zuge dieser Arbeit wurde neben einer umfassenden mathematischen Analyse des nichtlinearen Mischprozesses unter Einfluss der Fasercharakteristika eine Apparatur zur Erzeugung und Detektion vakuumultravioletter Strahlung entwickelt. Die Generierung ausreichend hoher Dampfdichten innerhalb des 50 µm durchmessenden Faserkerns konnten spektroskopisch nachgewiesen werden.rnrnDas erste erfolgreiche Summenfrequenzmischen zu 121,26 nm in der Faser wurde demonstriert. Die erzielten Mischeffizienzen sind bereits mit denen vergleichbar, welche unter Verwendung fokussierter Strahlen erreicht werden, obwohl eine Phasenanpassung in der Faser bisher nicht möglich war. Die Ergebnisse dieser Arbeit markieren damit einen wichtigen Schritt hin zu Leistungssteigerungen kohärenter, kontinuierlicher vakuumultravioletter Lichtquellen.rnrnEine solche Quelle wird für zukünftige Laserkühlung von magnetisch gefangenem Antiwasserstoff auf dem Lyman-Alpha Übergang, sowie die Rydberganregung von Calciumionen in einer Paulfalle zur Implementierung quantenlogischer Operationen benötigt.rnrnFerner hat eine Untersuchung der, für eine effiziente Konversion essentiellen, 6^1S_0 - 7^1S_0 Zwei-Photonen Resonanz in Quecksilber Hinweise auf eine bis dato experimentell nicht beobachtete, auf einer Mehr-Photonen Anregung beruhende Licht-induzierte Drift ergeben.

A multi-tracer study of groundwater origin and transit-time in the aquifers of the Venice region (Italy)

Located in the northeastern region of Italy, the Venetian Plain (VP) is a sedimentary basin containing an extensively exploited groundwater system. The northern part is characterised by a large undifferentiated phreatic aquifer constituted by coarse grain alluvial deposits and recharged by local rainfalls and discharges from the rivers Brenta and Piave. The southern plain is characterised by a series of aquitards and sandy aquifers forming a well-defined artesian multi-aquifer system. In order to determine origins, transit times and mixing proportions of different components in groundwater (GW), a multi tracer study (H, He/He, C, CFC, SF, Kr, Ar, Sr/Sr, O, H, cations, and anions) has been carried out in VP between the rivers Brenta and Piave. The geochemical pattern of GW allows a distinction of the different water origins in the system, in particular based on View the MathML source HCO3-,SO42-,Ca/Mg,NO3-, O, H. A radiogenic Sr signature clearly marks GW originated from the Brenta and Tertiary catchments. End-member analysis and geochemical modelling highlight the existence of a mixing process involving waters recharged from the Brenta and Piave rivers, from the phreatic aquifer and from another GW reservoirs characterised by very low mineralization. Noble gas excesses in respect to atmospheric equilibrium occur in all samples, particularly in the deeper aquifers of the Piave river, but also in phreatic water of the undifferentiated aquifers. He–H ages in the phreatic aquifer and in the shallower level of the multi-aquifer system indicate recharge times in the years 1970–2008. The progression of H–He ages with the distance from the recharge areas together with initial tritium concentration (H + Hetrit) imply an infiltration rate of about 1 km/y and the absence of older components in these GW. SF and Kr data corroborate these conclusions. H − He ages in the deeper artesian aquifers suggest a dilution process with older, tritium free waters. C Fontes–Garnier model ages of the old GW components range from 1 to 12 ka, yielding an apparent GW velocity of about 1–10 m/y. Increase of radiogenic He follows the progression of C ages. Ar, radiogenic He and C tracers yield model-dependent age-ranges in overall good agreement once diffusion of C from aquitards, GW dispersion, lithogenic Ar production, and He production-rate heterogeneities are taken into account. The rate of radiogenic He increase with time, deduced by comparison with C model ages, is however very low compared to other studies. Comparison with C and C data obtained 40 years ago on the same aquifer system shows that exploitation of GW caused a significant loss of the old groundwater reservoir during this time.

Isotopic effects of nitrate photochemistry in snow: a field study at Dome C, Antarctica

Stable isotope ratios of nitrate preserved in deep ice cores are expected to provide unique and valuable information regarding paleoatmospheric processes. However, due to the post-depositional loss of nitrate in snow, this information may be erased or significantly modified by physical or photochemical processes before preservation in ice. We investigated the role of solar UV photolysis in the post-depositional modification of nitrate mass and stable isotoperatios at Dome C, Antarctica, during the austral summer of 2011/2012. Two 30 cm snow pits were filled with homogenized drifted snow from the vicinity of the base. One of these pits was covered with a plexiglass plate that transmits solar UV radiation, while the other was covered with a different plexiglass plate having a low UV transmittance. Samples were then collected from each pit at a 2–5 cm depth resolution and a 10-day frequency. At the end of the season, acomparable nitrate mass loss was observed in both pits for the top-level samples (0–7 cm) attributed to mixing with the surrounding snow. After excluding samples impacted by the mixing process, we derived an average apparent nitrogen isotopic fractionation (15" app/of role in driving the isotopic fractionation of nitrate in snow.We have estimated a purely photolytic nitrogen isotopic fractionation (15"photo) of -55.8 12.0 ‰ from the difference in the derived apparent isotopic ractionations of the two experimental fields, as both pits were exposed to similar physical processes except exposure to solar UV. This value is in close agreement with the 15" photo value of -47.9 6.8 ‰ derived in a laboratory experiment simulated for Dome C conditions (Berhanu et al., 2014). We have also observed an insensitivity of 15" with depth in the snowpack under the given experimental setup. This is due to the uniform attenuation of incoming solar UV by snow, as 15" is strongly dependent on the spectral distribution of the incoming light flux. Together with earlier work, the results presented here represent a strong body of evidence that solar UV photolysis is the most relevant post-depositional process modifying the stable isotope ratios of snow nitrate at low-accumulation sites, where many deep ice cores are drilled. Nevertheless, modeling the loss of nitrate in snow is still required before a robust interpretation of ice core records can be provided.

Geochemistry and petrology of ODP Leg 121 basalts

Basement lavas from Sites 756, 757, and 758 on Ninetyeast Ridge are tholeiitic basalts. Lavas from Sites 756 and 757 appear to be subaerial eruptives, but the lowermost flows from Hole 758A are pillow lavas. In contrast to the compositional variation during the waning stages of Hawaiian volcanism, no alkalic lavas have been recovered from Ninetyeast Ridge and highly evolved lavas were recovered from only one of seven drill sites (DSDP Site 214). All lavas from Site 758 have relatively high MgO contents (8-10 wt%), and they are less evolved than lavas from Sites 756 and 757. Although abundances of alkali metals in these Ninetyeast Ridge basalts were significantly modified by postmagmatic alteration, abundances of other elements reflect magmatic processes. At Site 757 most of the lavas are Plagioclase cumulates, but lava compositions require two compositionally distinct, AhCb-rich parental magmas, perhaps segregated at relatively low mantle pressures. In addition, at both Sites 756 and 758 more than one compositionally distinct parental magma is required. The compositions of these Ninetyeast Ridge lavas, especially those from Site 758, require a source component with a depleted composition; specifically, the abundance ratios Th/Ta, Th/La, Ba/Nb, Ba/La, and La/Ce in these lavas are generally less than the ratios inferred for primitive mantle. Lavas from Ninetyeast Ridge and the Kerguelen Archipelago have very different chondrite-normalized REE patterns, with lower light REE/heavy REE (LREE/HREE) ratios in lavas from Ninetyeast Ridge. However, lavas from Sites 757 and 758 have Pb isotope ratios that overlap with the field defined by lavas from the Kerguelen Archipelago (Weis and Frey, this volume). Therefore, these Ninetyeast Ridge lavas contain more of a component that is relatively depleted in LREE and other highly incompatible elements, but have similar amounts of the component that controls radiogenic Pb isotopes. A model involving mixing between components related to a depleted source and an enriched plume source has been proposed for the oldest Kerguelen Archipelago basalts and Ninetyeast Ridge lavas. Although the incompatible element characteristics of the Ninetyeast Ridge lavas are intermediate between depleted MORB and Kerguelen Archipelago basalts, these data are not consistent with a simple two-component mixing process. A more complex model is required.

Hexachlorocyclohexanes concentration in air and ocean water

Hexachlorocyclohexanes (HCHs) are ubiquitous organic pollutants derived from pesticide application. They are subject to long-range transport, persistent in the environment, and capable of accumulation in biota. Shipboard measurements of HCH isomers (a-, b- and g-HCH) in surface seawater and boundary layer atmospheric samples were conducted in the Atlantic and the Southern Ocean in October to December of 2008. SumHCHs concentrations (the sum of a-, g- and b-HCH) in the lower atmosphere ranged from 12 to 37 pg/m**3 (mean: 27 ± 11 pg/m**3) in the Northern Hemisphere (NH), and from 1.5 to 4.0 pg/m**3 (mean: 2.8 ± 1.1 pg/m**3) in the Southern Hemisphere (SH), respectively. Water concentrations were: a-HCH 0.33-47 pg/l, g-HCH 0.02-33 pg/l and b-HCH 0.11-9.5 pg/l. Dissolved HCH concentrations decreased from the North Atlantic to the Southern Ocean, indicating historical use of HCHs in the NH. Spatial distribution showed increasing concentrations from the equator towards North and South latitudes illustrating the concept of cold trapping in high latitudes and less interhemispheric mixing process. In comparison to concentrations measured in 1987-1999/2000, gaseous HCHs were slightly lower, while dissolved HCHs decreased by factor of 2-3 orders of magnitude. Air-water exchange gradients suggested net deposition for a-HCH (mean: 3800 pg/m**2/day) and g-HCH (mean: 2000 pg/m**2/day), whereas b-HCH varied between equilibrium (volatilization: <0-12 pg/m**2/day) and net deposition (range: 6-690 pg/m**2/day). Climate change may significantly accelerate the release of "old" HCHs from continental storage (e.g. soil, vegetation and high mountains) and drive long-range transport from sources to deposition in the open oceans. Biological productivities may interfere with the air-water exchange process as well. Consequently, further investigation is necessary to elucidate the long term trends and the biogeochemical turnover of HCHs in the oceanic environment.

Geochemistry of rare earth elements in basalts from Walvis Ridge

Selected basalts from a suite of dredged and drilled samples (IPOD sites 525, 527, 528 and 530) from the Walvis Ridge have been analysed to determine their rare earth element (REE) contents in order to investigate the origin and evolution of this major structural feature in the South Atlantic Ocean. All of the samples show a high degree of light rare earth element (LREE) enrichment, quite unlike the flat or depleted patterns normally observed for normal mid-ocean ridge basalts (MORBs). Basalts from Sites 527, 528 and 530 show REE patterns characterised by an arcuate shape and relatively low (Ce/Yb)N ratios (1.46-5.22), and the ratios show a positive linear relationship to Nb content. A different trend is exhibited by the dredged basalts and the basalts from Site 525, and their REE patterns have a fairly constant slope, and higher (Ce/Yb)N ratios (4.31-8.50). These differences are further reflected in the ratios of incompatible trace elements, which also indicate considerable variations within the groups. Mixing hyperbolae for these ratios suggest that simple magma mixing between a 'hot spot' type of magma, similar to present-day volcanics of Tristan da Cunha, and a depleted source, possibly similar to that for magmas being erupted at the Mid-Atlantic Ridge, was an important process in the origin of parts of the Walvis Ridge, as exemplified by Sites 527, 528 and 530. Site 525 and dredged basalts cannot be explained by this mixing process, and their incompatible element ratios suggest either a mantle source of a different composition or some complexity to the mixing process. In addition, the occurrence of different types of basalt at the same location suggests there is vertical zonation within the volcanic pile, with the later erupted basalts becoming more alkaline arid more enriched in incompatible elements. The model proposed for the origin and evolution of the Walvis Ridge involves an initial stage of eruption in which the magma was essentially a mixture of enriched and depleted end-member sources, with the N-MORB component being small. The dredged basalts and Site 525, which represent either later-stage eruptives or those close to the hot spot plume, probably result from mixing of the enriched mantle source with variable amounts and variable low degrees of partial melting of the depleted mantle source. As the volcano leaves the hot spot, these late-stage eruptives continue for some time. The change from tholeiitic to alkalic volcanism is probably related either to evolution in the plumbing system and magma chamber of the individual volcano, or to changes in the depth of origin of the enriched mantle source melt, similar to processes in Hawaiian volcanoes.

Time Evolution of the Fractal Dimension in Turbulent Plumes

Turbulent mixing is a very important issue in the study of geophysical phenomena because most fluxes arising in geophysics fluids are turbulent. We study turbulent mixing due to convection using a laboratory experimental model with two miscible fluids of different density with an initial top heavy density distribution. The fluids that form the initial unstable stratification are miscible and the turbulence will produce molecular mixing. The denser fluid comes into the lighter fluid layer and it generates several forced plumes which are gravitationally unstable. As the turbulent plumes develop, the denser fluid comes into contact with the lighter fluid layer and the mixing process grows. Their development is caused by the lateral interaction between these plumes at the complex fractal surface between the dense and light fluids

Estudio microestructural y de los procesos de hidratación de cementos con adiciones

En los últimos años, las sociedades industrializadas han tomado una mayor conciencia sobre el problema que suponen las emisiones indiscriminadas de gases de efecto invernadero a la atmósfera. El hormigón, cuyo principal componente es el cemento, es probablemente el material más utilizado en construcción. En la actualidad, las emisiones globales de CO2 debidas a la combustión del CaCO3 del cemento Pórtland representan entre el 5% y el 10% respecto del total. Estos valores son de gran interés si se considera que el compromiso aceptado al firmar el Protocolo de Kioto es de una reducción del 5% antes del año 2020, sobre el total de gases producidos. El principal objetivo del presente trabajo es el estudio microestructural y de los procesos de hidratación de los cementos con adiciones. Para ello se propone contribuir a la investigación sobre nuevos productos cementicios basados en micropartículas esféricas vítreas que pueden adicionarse al cemento antes del proceso de amasado. Los resultados obtenidos se han contrastado con las adiciones convencionales de más uso en la actualidad. El nuevo material basa su composición en la química del aluminio y el silicio. Al disminuir la cantidad de CaCO3, se contribuye al desarrollo sostenible y a la reducción de emisiones de CO2. La patente creada por el Grupo Cementos Pórtland Valderrivas (GCPV), describe el proceso de producción de las cemesferas (WO 2009/007470, 2010). Los productos que forman la materia prima para la elaboración de las cemesferas son arcillas, calizas, margas o productos o subproductos industriales, que tras su molienda, son fundidos mediante un fluido gaseoso a elevada temperatura (entre 1250ºC y 1600ºC). Este proceso permite obtener un producto final en forma esférica maciza o microesfera, que tras estabilizarse mediante un enfriamiento rápido, consigue una alta vitrificación idónea para su reactividad química, con una mínima superficie específica en relación a su masa. El producto final obtenido presenta prácticamente la finura requerida y no precisa ser molido, lo que reduce las emisiones de CO2 por el ahorro de combustible durante el proceso de molienda. El proceso descrito permite obtener un amplio abanico de materiales cementantes que, no solo pueden dar respuesta a los problemas generados por las emisiones de CO2, sino también a la disponibilidad de materiales en países donde hasta el momento no se puede fabricar cemento debido a la falta de calizas. Complementariamente se ha optimizado el método de cálculo del grado de hidratación a partir de los resultados del ensayo de ATD-TG en base a los modelos de cálculo de Bhatty y Pane. El método propuesto permite interpretar el comportamiento futuro del material a partir de la interpolación numérica de la cantidad de agua químicamente enlazada. La evolución del grado de hidratación tiene una relación directa con el desarrollo de la resistencia mecánica del material. Con el fin de caracterizar los materiales de base cemento, se ha llevado a cabo una amplia campaña experimental en pasta de cemento, mortero y hormigón. La investigación abarca tres niveles: caracterización microestructural, macroestructural y caracterización del comportamiento a largo plazo, fundamentalmente durabilidad. En total se han evaluado ocho adiciones diferentes: cuatro adiciones convencionales y cuatro tipos de cemesferas con diferente composición química. Los ensayos a escala microscópica comprenden la caracterización química, granulométrica y de la superficie específica BET de los materiales anhidros, análisis térmico diferencial y termogravimétrico en pasta de cemento y mortero, resonancia magnética de silicio en pasta de cemento, difracción de rayos X de los materiales anhidros y de las probetas de pasta, microscopía electrónica de barrido con analizador de energía dispersiva por rayos X en pasta y mortero, y porosimetría por intrusión de mercurio en mortero. La caracterización macroscópica del material comprende ensayos de determinación del agua de consistencia normal y de los tiempos de inicio y fin de fraguado en pasta de cemento, ensayos de resistencia mecánica a flexión y compresión en probetas prismáticas de mortero, y ensayos de resistencia a compresión en probetas de hormigón. Para caracterizar la durabilidad se han desarrollado ensayos de determinación del coeficiente de migración de cloruros y ensayos de resistividad eléctrica en probetas de mortero. Todos los ensayos enumerados permiten clarificar el comportamiento de las cemesferas y compararlo con las distintas adiciones de uso convencional. Los resultados reflejan un buen comportamiento resistente y durable de los materiales con adición de cemesferas. La caracterización microscópica refleja su relación con las propiedades mesoscópicas y permite comprender mejor la evolución en los procesos de hidratación de las cemesferas. In recent years industrialised societies have become increasingly aware of the problem posed by indiscriminate emission of greenhouse gases into the atmosphere. Concrete, with a main component being cement, is arguably the most widely used construction material. At present, global emissions of CO2 due to the combustion of CaCO3 from Portland cement represent between 5% and 10% of the total. If the requirement of the Kyoto Protocol of a reduction of 5% of the total gas produced before 2020 is considered, then such values are of significant interest. The main objective of this work is the assessment of the microstructure and the hydration processes of cements with additions. Such an examination proposes research into new cementitious products based on vitreous spherical microparticles that may be added to the cement before the mixing process. The results are compared with the most commonly used conventional additions. The new material bases its composition on the chemistry of aluminium and silicates. By decreasing the amount of CaCO3, it is possible both to contribute to sustainable development and reduce CO2 emissions. The patent created by Grupo Cementos Portland Valderrivas (GCPV) describes the production process of microspheres (WO 2009/007470, 2010). The products that form the raw material for manufacture are clays, lime-stone, marl and industrial products or by-products that melt after being ground and fed into a gaseous fluid at high temperatures (1250°C and 1600°C). This process allows the obtaining of a product with a solid-spherical or micro-spherical shape and which, after being stabilised in a solid state by rapid cooling, obtains a high vitrification suitable for chemical reactivity, having a minimal surface in relation to its mass. Given that the final product has the fineness required, it prevents grinding that reduces CO2 emissions by saving fuel during this process. The process, which allows a wide range of cementitious materials to be obtained, not only addresses the problems caused by CO2 emissions but also enhances the availability of materials in countries that until the time of writing have not produced cement due to a lack of limestone. In addition, the calculation of the degree of hydration from the test results of DTA-TG is optimised and based on Bhatty and Pane calculation models. The proposed method allows prediction of the performance of the material from numerical interpolation of the amount of chemically bound water. The degree of hydration has a direct relationship with the development of material mechanical strength. In order to characterise the cement-based materials, an extensive experimental campaign in cement paste, concrete and mortar is conducted. The research comprises three levels: micro-structural characterisation, macro-structural and long-term behaviour (mainly durability). In total, eight additions are assessed: four conventional additions and four types of microspheres with different chemical compositions. The micro-scale tests include characterisation of chemical composition, particle size distribution and the BET specific surface area of anhydrous material, differential thermal and thermogravimetric analysis in cement paste and mortar, silicon-29 nuclear magnetic resonance in cement paste, X-ray diffraction of the anhydrous materials and paste specimens, scanning of electron microscopy with energy dispersive X-ray analyser in cement paste and mortar, and mercury intrusion porosimetry in mortar. The macroscopic material characterisation entails determination of water demand for normal consistency, and initial and final setting times of cement paste, flexural and compressive mechanical strength tests in prismatic mortar specimens, and compressive strength tests in concrete specimens. Tests for determining the chloride migration coefficient are performed to characterise durability, together with electrical resistivity tests in mortar specimens. All the tests listed allow clarification of the behaviour of the microspheres and comparison with the various additions of conventional use. The results show good resistance and durable behaviour of materials with a microsphere addition. Microscopic characterisation reflects their relationship with mesoscopic properties and provides insights into the hydration processes of the microspheres.

Determinación de propiedades de inflamabilidad de mezclas para co-combustión

La recuperación de energía a partir de biomasa y residuos no reciclables por la combustión está cobrando una notable importancia actualmente. Una de las técnicas más utilizadas para esta propuesta es la co-combustión de mezclas de residuos y biomasa. Con esta nueva tecnología, mezclas de diferentes materiales han aparecido en las instalaciones industriales y tienen que ser reconocidas como nuevos combustibles, debido a que a sus propiedades son aún desconocidas. Estas propiedades incluyen las energéticas, que son el objetivo del proceso de mezcla, y también las propiedades de inflamabilidad. Residuos y biomasa en forma de polvos tienen propiedades de ignición que se han de tener en cuenta a la hora de diseñar las medidas de prevención y protección en una instalación industrial. El objetivo principal de este estudio es determinar el riesgo de ignición de las mezclas de residuos / biomasa en capas y cómo, mediante la adición de diferentes cantidades de estos materiales, este riesgo puede cambiar. Para desarrollar este estudio, se utiliza la temperatura mínima de ignición en la capa. Tres muestras diferentes han sido analizadas, lodos con secado térmico de depuradora, paja de trigo y virutas de madera, Abstract Energy recovery from biomass and non-recyclable waste products by combustion has become important. One of the most used techniques for this proposal is the co-firing of waste and biomass mixtures, With this new technology, mixtures of different materials have appeared in the industrial facilities and they have to be treated as new fuels because their properties are unknown. Among this properties we include energetic properties that are the objective of the mixing process, and also the ignitability properties. Waste and biomass dusts have ignition properties that have to be taken into account in the design but also in the, prevention and protection process of an industrial facility.. The main objective of this research is to determine the risk of ignition of waste / biomass mixtures layers and how, by adding different quantities of these materials, this risk may vary. To develop this, the minimum ignition temperature on layer is used. Three different samples have been analysed, thermally dried sewage sludge, wheat straw and wood chips.