Discarge compilation from The Global River Discharge (RivDIS) Project

The Global River Discharge (RivDIS) data set contains monthly discharge measurements for 1018 stations located throughout the world. The period of record varies widely from station to station, with a mean of 21.5 years. These data were digitized from published UNESCO archives by Charles Voromarty, Balaze Fekete, and B.A. Tucker of the Complex Systems Research Center (CSRC) at the University of New Hampshire. River discharge is typically measured through the use of a rating curve that relates local water level height to discharge. This rating curve is used to estimate discharge from the observed water level. The rating curves are periodically rechecked and recalibrated through on-site measurement of discharge and river stage.

Innovating global value chains : creation of the netbook market by Taiwanese firms

This paper explores the process of creation of the netbook market by Taiwanese firms as an example of a disruptive innovation by latecomer firms. As an analytical framework, I employ the global value chain perspective to capture the dynamics of vertical inter-firm relationships that drive some firms in the chain to change the status quo of the industry. I then divide the process of the emergence of the netbook market into three consecutive stages, i.e. (1) the launch of the first-generation netbook by a Taiwanese firm named ASUSTeK, (2) the response of the two powerful platform leaders of the industry, Intel and Microsoft Intel, to ASUSTeK’s innovation, and (3) the market entry by another powerful Taiwanese firm, Acer, and explain how Taiwanese firms broke the Intel-centric market and tapped into the market-creating innovation opportunities that had been suppressed by the two powerful platform leaders. I also show that the creation of the netbook industry was an evolutionary process in which a series of responses by different industry players led to changes in the status quo of the industry.

Potenciación de la respuesta productiva en rumiantes mediante el empleo de proteínas protegidas

El principal objetivo de esta tesis fue incrementar la eficiencia proteica en las dietas de rumiantes mediante el uso de proteínas protegidas (harina de girasol y guisante de primavera), así como mejorar la predicción de los aportes de proteína microbiana. Una partida de harinas comerciales de girasol (HG) y de guisante de primavera (GP) fueron tratadas con soluciones 4 N de ácido málico (268,2 g/L) o ácido ortofosfórico (130,6 g/L). Para cada harina, ácido y día de tratamiento, dos fracciones de 12,5 kg fueron pulverizadas sucesivamente en una hormigonera con la solución de ácido correspondiente mediante un pulverizador de campo. Las dos fracciones fueron mezcladas posteriormente y se dejaron reposar durante 1 h a temperatura ambiente. La mezcla fue luego secada en una estufa de aire forzado a 120 ºC durante 1 h. La estufa fue apagada inmediatamente después y el material tratado se mantuvo dentro de ésta hasta la mañana siguiente. El material fue removido durante el proceso de secado cada 30 min durante las primeras 2 h y cada 60 min durante las 5 h posteriores. Este proceso se repitió hasta conseguir las cantidades de harinas tratadas necesarias en los distintos ensayos. En el primer experimento (capitulo 3) se llevaron a cabo estudios de digestión ruminal e intestinal para evaluar los efectos de la aplicación de las soluciones ácidas indicadas y calor a fin de proteger las proteínas de HG y GP contra la degradación ruminal. Estos estudios se realizaron con tres corderos canulados en el rumen y en el duodeno. El estudio de digestión ruminal fue realizado en tres periodos experimentales en los que los corderos fueron alimentados sucesivamente con tres dietas isoproteicas que incluían HG y GP, sin tratar o tratadas con ácidos málico u ortofosfórico. Cada periodo experimental de 21 días incluyó sucesivamente: 10 días de adaptación a las dietas, un estudio del tránsito ruminal de las partículas de HG y GP (días 11 a 14), y la incubación de las muestras de ambos alimentos en bolsas de nailon (días 15–21). Las harinas incubadas en cada periodo experimental correspondieron a las que fueron incluidas en las dietas. Las bacterias ruminales fueron marcadas desde el día 11 hasta el día 21 del periodo experimental mediante infusión intra-ruminal continua con una fuente de 15N. Tras finalizar las incubaciones in situ el día 21 el rumen fue vaciado en cada periodo para aislar las bacterias asociadas a la fase sólida y liquida del rumen. El estudio de digestión intestinal fue realizado veinte días después del final del estudio ruminal a fin de eliminar el enriquecimiento en 15N de la digesta. En este estudio se incubaron muestras compuestas obtenidas mediante la combinación de los diferentes residuos no degradados en el rumen de forma que fuesen representativas de la composición química de la fracción no degradada en el rumen (RU). En esta fase los corderos fueron alimentados con la dieta sin tratar para determinar la digestibilidad de las harinas tanto tratadas como sin tratar mediante la técnica de las bolsas móviles. Además, las proteínas contenidas en las harinas tratadas y sin tratar, así como en las muestras correspondientes a los residuos a 0 h, las muestras compuestas anteriormente indicadas y las muestras no digeridas intestinalmente fueron extraídas y sometidas a electroforesis para determinar el sitio de digestión de las diferentes fracciones proteicas. Las estimaciones de la RU y la digestibilidad intestinal de la materia seca, la materia orgánica (solamente para RU), la proteína bruta (PB) y el almidón (solamente en GP) fueron obtenidos considerando la contaminación microbiana y las tasas de conminución y salida de partículas. Las estimaciones de RU y de la digestibilidad intestinal disminuyeron en todas las fracciones evaluadas de ambos alimentos al corregir por la contaminación microbiana acaecida en el rumen. Todas las estimaciones de RU aumentaron con los tratamientos de protección, incrementándose también la digestibilidad intestinal de la materia seca en la HG. Los bajos valores de la digestibilidad de la proteína de GP tratado y sin tratar sugieren la presencia de algún factor antitripsico no termolábil es esta harina. Los tratamientos de protección incrementaron consistentemente la fracción de materia seca y PB digerida intestinalmente en los dos alimentos, mientras que la fracción de almidón en la muestra de GP solamente aumentó numéricamente (60,5% de media). Sin embargo, los tratamientos también redujeron la fermentación de la materia orgánica, lo cual podría disminuir la síntesis de proteína microbiana. Los estudios de electroforesis muestran la práctica desaparición de la albumina por la degradación ruminal en ambos alimentos, así como que los cambios en otras proteínas de la muestra RU fueron más pronunciados en GP que en HG. La composición de las bacterias asociadas con las fases de digesta ruminal sólida (BAS) y líquida (BAL) fue estudiada para revisar la precisión de un sistema de predicción previo que determinaba la infravaloración del aporte de nutrientes correspondiente a las BAS cuando de usa 15N como marcador y las BAL como referencia microbiana (capitulo 4). Al comparar con BAS, BAL mostraron menores contenidos en materia orgánica, polisacáridos de glucosa y lípidos totales y un mayor contenido en PB, así como un mayor enriquecimiento en 15N. Los datos obtenidos en el estudio actual se ajustan bien a la ecuación previa que predice el enriquecimiento en 15N de las BAS a partir del mismo valor en BAL. Esta nueva ecuación permite establecer que se produce una infravaloración de un 22% en el aporte de PB al animal a partir de las BAS sintetizadas si las BAL son usadas como muestras de referencia. Una segunda relación calculada utilizando los valores medios por dieta expuestos en numerosos trabajos encontrados en la literatura confirma la magnitud de este error. Esta infravaloración asociada al uso de BAL como referencia fue mayor para el aporte de glucosa (43,1%) y todavía mayor para el aporte de lípidos (59,9%), como consecuencia de los menores contenidos de ambas fracciones en BAL frente a SAB. Estos errores deberían ser considerados para obtener mayor precisión en la estimación del aporte de nutrientes microbianos y mejorar la nutrición de los rumiantes. En el experimento 2 se realizó un estudio de producción (capitulo 5) para evaluar los efectos del tratamiento de las harinas HG y GP con soluciones de ácido málico o ácido ortofosfórico sobre el crecimiento, el consumo de concentrado y el rendimiento y engrasamiento de las canales de corderos de engorde. Noventa corderos machos de cruce entrefino procedentes de tres granjas comerciales (peso inicial medio = 14,6, 15,3 y 13,3 kg, respectivamente) fueron asignados aleatoriamente a cinco dietas con diferentes niveles de proteína y diferentes tratamientos con ácidos y engordados hasta un peso medio al sacrificio de 25 kg. Las fuentes de proteína en el pienso control (C; PB=18,0%) fueron harina de soja, HG y GP sin tratar. En tres de los piensos experimentales, las harinas tratadas con ácido ortofosfórico sustituyeron a las de HG y GP sin tratar (Control Ortofosfórico, PC; PB=18,0% sobre materia seca), sustituyéndose, además, la harina de soja parcialmente (Sustitución Media Ortofosfórico, MSP; PB=16,7%) o totalmente (Sustitución Total Ortofosfórico, TSP; PB=15,6%). Finalmente, en uno de los piensos el ácido ortofosfórico fue reemplazo por acido málico para proteger ambas harinas (Sustitución Media Málico, MSM; PB= 16,7%). La paja de trigo (fuente de forraje) y el concentrado fueron ofrecidos ad libitum. Dieciocho corderos fueron distribuidos en seis cubículos con tres animales para cada dieta. Los datos fueron analizados según un análisis factorial considerando el peso inicial como covariable y la granja de procedencia como bloque. Los datos de consumo de concentrado y eficiencia de conversión fueron analizados usando el cubículo como unidad experimental, mientras que los datos sobre ganancia media diaria, rendimiento a la canal, grasa dorsal y grasa pélvico renal fueron analizados usando el cordero como unidad experimental. No se encontró ningún efecto asociado con el nivel de PB sobre ninguna variable estudiada. Esto sugiere que usando proteínas protegidas es posible utilizar concentrados con 15,6% de PB (sobre materia seca) disminuyendo así la cantidad de concentrados de proteína vegetal a incluir en los piensos y la calidad de los concentrados proteicos. Los corderos alimentados con la dieta MSM tuvieron mayores ganancias medias diarias (15,2%; P= 0,042), y mejores rendimiento a la canal en caliente (1,3 unidades porcentuales; P= 0,037) que los corderos alimentados con el concentrado MSP. Esto podría ser explicado por los efectos benéficos ruminales del malato o por el mayor efecto de protección conseguido con el ácido málico. ABSTRACT The main objective of this thesis project was to increase the protein efficiency in ruminant diets by using protected protein (sunflower meal and spring pea), and improving the prediction of microbial protein supply. Commercial sunflower meal (SFM) and spring pea (SP) were treated with 4 N solutions (200 mL/kg) of malic acid (268.2 g/L) or orthophosphoric acid (130.6 g/L). Daily, two fractions of 12.5 kg of one of these meals were successively sprayed with the tested acid solution in a concrete mixer using a sprayer. Both fractions were then mixed and allowed to rest for 1 h at room temperature. The blend was then dried in a forced air oven at 120 ºC for 1 h. Then the oven was turned off and the treated material was left in the oven overnight. During the drying process, the material was stirred every 30 min during the first 2 h and then every 60 min for the subsequent 5 h. This process was repeated until the amounts of treated flour needed for the different trials performed. In the first experiment (chapter 3), ruminal and intestinal digestion trials were conducted to study the effects of the application of these acid solutions and heat to protect proteins of SFM and SP against ruminal degradation using three wethers fitted with rumen and duodenum cannulae. The ruminal digestion study was carried out in three experimental periods in which the wethers were successively fed three isoproteic diets including SFM and SP, untreated or treated with malic or orthophosphoric acids. The experimental periods of 21 days included successively: 10 days of diet adaptation, SFM and SP particle ruminal transit study (days 11–14) and ruminal nylon-bag incubations (days 15–21). The meals incubated in each experimental period were those corresponding to the associated diet. Rumen bacteria were labelled from days 11 to 21 by continuous intra-ruminal infusion of a 15N source and the rumen was emptied at the end of in situ incubations in each period to isolate solid adherent bacteria and liquid associate bacteria. The intestinal digestion trial was conducted twenty days after the end of the ruminal studies to eliminate the 15N enrichment in the digesta. The tested samples were composite samples obtained pooling the different ruminally undegraded residues to be representative of the chemical composition of the ruminally undegraded fraction (RU). Wethers were fed the untreated diet to determine the intestinal digestibility of untreated and treated meals using the mobile nylon bag technique. In addition, protein in untreated and treated meals and their 0 h, composite and intestinally undigested samples were extracted and subjected to electrophoresis to determine the digestion site of the different protein fractions. Estimates of the RU and its intestinal digestibility of dry matter, organic matter (only for RU), crude protein (CP) and starch (only in SP) were obtained considering ruminal microbial contamination and particle comminution and outflow rates. When corrected for the microbial contamination taking place in the rumen, estimates of RU and intestinal digestibility decreased in all tested fractions for both feeds. All RU estimates increased with the protective treatments, whereas intestinal digestibility-dry matter also increased in SFM. Low intestinal digestibility-CP values in untreated and treated samples suggested the presence of non-heat labile antitrypsin factors in SP. Protective treatments of both feeds led to consistent increases in the intestinal digested fraction of dry matter and CP, being only numerically different for SP-starch (60.5% as average). However, treatments also reduced the organic matter fermentation, which may decrease ruminal microbial protein synthesis. Electrophoretic studies showed albumin disappearance in both SFM and SP, whereas changes in other RU proteins were more pronounced in SP than SFM. The chemical composition of bacteria associated with solid (SAB) and liquid (LAB) rumen-digesta phases was studied to examine the accuracy of a previous regression system determining the underevaluation of SAB-nutrient supply using 15N as marker and LAB as microbial reference (chapter 4). Compared with SAB, LAB showed lower contents of organic matter, polysaccharide-glucose and total lipids and the opposite for the CP content and the 15N enrichment. Present data fitted well to the previous relationship predicting the 15N enrichment of SAB from the same value in LAB. This new equation allows establishing an underevaluation in the supply of CP from the synthesized SAB in 22.0% if LAB is used as reference. Another relationship calculated using mean diet values from the literature confirmed the magnitude of this error. This underevaluation was higher for the supply of glucose (43.1%) and still higher for the lipid supply (59.9%) as a consequence of the lower contents of these both fractions in LAB than in SAB. These errors should be considered to obtain more accurate estimates of the microbial nutrient supply and to improve ruminant nutrition. A production study was performed in experiment 2 (chapter 5) to examine the effects of treating SFM and SP meals with orthophosphoric or malic acid solutions on growth performance, concentrate intake, and carcass yield and fatness of growing-fattening lambs. Ninety "Entrefino" cross male lambs from three commercial farms (average initial body weights (BW) = 14.6, 15.3 and 13.3 kg) were randomly assigned to five diets with different acid treatment and protein levels, and fattened to an average slaughter weight of 25 kg. Protein sources in the control concentrate (C; CP=18%) were soybean meal and untreated SFM and SP. In three of the experimental concentrates, orthophosphoric acid-treated meals substituted untreated SFM and SP (Orthophosphoric Control, PC; CP=18% dry matter basis), and soybean meal was partially (Medium Substitution Orthophosphoric, MSP; CP=16.7%) or totally removed (Total Substitution Orthophosphoric, TSP; CP=15.6%). In addition, in one concentrate orthophosphoric acid was replaced by malic acid to protect these meals (Medium Substitution Malic, MSM; CP= 16.7%). Wheat straw (roughage source) and concentrate were offered ad libitum. Eighteen lambs were allocated to six pens of three animals on each diet. Data were analyzed using a factorial analysis with initial body weight BW as covariate and farm of origin as block. Data on concentrate intake and feed conversion efficiency were analyzed using pen as experimental unit, while data on average daily gain, carcass yield, dorsal fat, and kidney-pelvic-fat were analyzed with lamb as experimental unit. No effect associated with the CP level was observed on any parameter. This suggests that with protected proteins it is possible to feed concentrates with 15.6% CP (dry matter basis) reducing the quantity of vegetable protein meals to include in the concentrate as well as the quality of the protein concentrates. Lambs feed MSM had higher average daily gains (15.2%; P= 0.042), and better hot carcass yields (1.3 percentage points; P= 0.037) than lambs feed MSP. This probably can be explained by ruminal malate actions and by greater protection effects obtained with malic acid.

The Mice at play in the CALIFA survey. A case study of a gas-rich major merger between first passage and coalescence

We present optical integral field spectroscopy (IFS) observations of the Mice, a major merger between two massive (≳10^11 M_⊙) gas-rich spirals NGC 4676A and B, observed between first passage and final coalescence. The spectra provide stellar and gas kinematics, ionised gas properties, and stellar population diagnostics, over the full optical extent of both galaxies with ~1.6 kpc spatial resolution. The Mice galaxies provide a perfect case study that highlights the importance of IFS data for improving our understanding of local galaxies. The impact of first passage on the kinematics of the stars and gas has been significant, with strong bars most likely induced in both galaxies. The barred spiral NGC 4676B exhibits a strong twist in both its stellar and ionised gas disk. The edge-on disk galaxy NGC 4676A appears to be bulge free, with a strong bar causing its “boxy” light profile. On the other hand, the impact of the merger on the stellar populations has been minimal thus far. By combining the IFS data with archival multiwavelength observations we show that star formation induced by the recent close passage has not contributed significantly to the total star formation rate or stellar mass of the galaxies. Both galaxies show bicones of high ionisation gas extending along their minor axes. In NGC 4676A the high gas velocity dispersion and Seyfert-like line ratios at large scaleheight indicate a powerful outflow. Fast shocks (vs ~ 350 km s^-1) extend to ~6.6 kpc above the disk plane. The measured ram pressure (P/k = 4.8 × 10^6 K cm^-3) and mass outflow rate (~8−20 M_⊙ yr^-1) are similar to superwinds from local ultra-luminous infrared galaxies, although NGC 4676A only has a moderate infrared luminosity of 3 × 10^10 L_⊙. Energy beyond what is provided by the mechanical energy of the starburst appears to be required to drive the outflow. Finally, we compare the observations to mock kinematic and stellar population maps extracted from a hydrodynamical merger simulation. The models show little enhancement in star formation during and following first passage, in agreement with the observations. We highlight areas where IFS data could help further constrain the models.

The nature of LINER galaxies: Ubiquitous hot old stars and rare accreting black holes

Context. Galaxies, which often contain ionised gas, sometimes also exhibit a so-called low-ionisation nuclear emission line region (LINER). For 30 years, this was attributed to a central mass-accreting supermassive black hole (more commonly known as active galactic nucleus, AGN) of low luminosity, making LINER galaxies the largest AGN sub-population, which dominate in numbers over higher luminosity Seyfert galaxies and quasars. This, however, poses a serious problem. While the inferred energy balance is plausible, many LINERs clearly do not contain any other independent signatures of an AGN. Aims. Using integral field spectroscopic data from the CALIFA survey, we compare the observed radial surface brightness profiles with what is expected from illumination by an AGN. Methods. Essential for this analysis is a proper extraction of emission lines, especially weak lines, such as Balmer H beta lines, which are superposed on an absorption trough. To accomplish this, we use the GANDALF code, which simultaneously fits the underlying stellar continuum and emission lines. Results. For 48 galaxies with LINER-like emission, we show that the radial emission-line surface brightness profiles are inconsistent with ionisation by a central point-source and hence cannot be due to an AGN alone. Conclusions. The most probable explanation for the excess LINER-like emission is ionisation by evolved stars during the short but very hot and energetic phase known as post-AGB. This leads us to an entirely new interpretation. Post-AGB stars are ubiquitous and their ionising effect should be potentially observable in every galaxy with the gas present and with stars older than ~1 Gyr unless a stronger radiation field from young hot stars or an AGN outshines them. This means that galaxies with LINER-like emission are not a class defined by a property but rather by the absence of a property. It also explains why LINER emission is observed mostly in massive galaxies with old stars and little star formation.