Wordles_Flor B

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The document discusses various science concepts including cell division, the sun being the center of the universe, triple bonds, projectile motion, multiple genes, tissues, diffusion, sublimation, and wavelength. Many terms are repeated or written across multiple lines.

Science

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Mein spiritueller Weg Mein spiritueller Weg begann schon in meiner frühen Kindheit, was mir jedoch erst im Erwachsenenalter bewusst wurde. Geborgen und aufgewachsen in einer desolaten Familiensituation begann ich eine Ausbildung u.a. in der Psychologie und erweiterte mein Wissen durch Meditation und Karateübungen, was mir jedoch keinen wirklichen inneren Frieden brachte. In den Folgejahren besuchte ich dann nebenbei eine Ausbildung bei den Mönchen, die mir gezeigt haben, was es bedeutet in Demut und Liebe zu leben. Es war eine sehr lehrreiche und schöne Zeit für mich. Erst Jahre später entschloss ich mich meine bis dahin erkannten frühkindlichen Begabungen an die Menschen weiterzugeben und fing an mich für die Kunst des Kundalini Reiki zu interessieren. Nach meiner Ausbildung zum Kundalini-Meister folgten 6 Einweihungen von Booster 1 bis Booster 2. Anschließend habe ich eine Einweihung in das Engel-Ki erhalten. Das ist auch ein sehr schönes Erlebnis, wo man den Kontakt zu den Engeln schneller findet über die Regenbogenbrücke. Das ist wie bei einer ISDN Anlage - man wird schneller verbunden zu den Engeln. Das Kipper Karten legen habe ich in der Schweiz gelernt . Auch habe ich eine Ausbildung mit den Karten der Madame Lenormand. Im Juni 2010 habe ich meinen Ursprungs Namen erfahren aus der Kryonschule in Rosenheim von Sabine Sangitar. Mein Ursprungs Name heißt: Solvanias, der Krieger des Lichtes. Im Oktober 2011 habe ich meine 1. Ausbildung mit Quanten Heilung mit der 2-Punkte-Methode erlernt. Im November 2011 habe ich die 2. Ausbildung gemacht mit der Quanten Heilung. Das Ganze ist Heilen mit Herz, weil die Heilung aus dem Herzen geschieht. Meine Jenseits Kontakte habe ich schon immer gehabt, was schon zu sehr viel Erfolg beigetragen hat. Ich möchte höflich darauf hinweisen, dass ich keinen Arzt oder Heilpraktiker ersetze. Auch gebe ich keine Auskunft über Tod oder Rechtsfragen. Herzlichst, Euer Jürgen Weber

Ich bin bei meiner Berufung

Mein Spiritueller Weg

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cristianceronguerrero

Der abscheuliche Anschlag in Paris hat uns alle erschüttert. Den Opfern der feigen Anschläge und ihren Familien gilt in dieser schwierigen Zeit unser Mitgefühl und unsere Anteilnahme. Bei aller Trauer stimmen mich viele Reaktionen zuversichtlich, dass die Terroristen ihr eigentliches Ziel nicht erreichen werden: Furcht zu verbreiten, die unsere Werte lähmt und zerstört. Millionen von Menschen in Frankreich und weit darüber hinaus haben am Sonntag mit ihrem Protest den Wert der Freiheit in beeindruckender Weise zum Ausdruck gebracht. Sie zeigen ihre Solidarität mit genau den Werten, die die Terroristen bekämpfen. Die Berichte in allen Medien machen unmissverständlich klar, dass unsere Grundwerte wie Meinungsfreiheit, Glaubensfreiheit und Pressefreiheit stärker sind als jeder Terror. In Deutschland haben Vertreter aller großen Religionsgemeinschaften – Christen, Juden und Muslime – mit einem gemeinsamen Manifest gegen den Terror reagiert: Im Namen Gottes darf nicht getötet werden. Wir werden nicht zulassen, dass Fanatismus, Terror und Gewalt unsere gemeinsamen Werte zerstören. Innenminister de Maizière hat in Kreuth unterstrichen, dass wir bereits einiges im Kampf gegen den islamistischen Terror unternommen haben und diesen Weg konsequent fortsetzen. Wir werden weiterhin gegen islamistische Vereinigungen und Dschihadisten vorgehen, Strafbarkeitslücken schließen und unseren Behörden die rechtlichen und technischen Mittel zum Schutz der Bürger zur Verfügung stellen. Wer unsere freiheitlich-demokratische Ordnung bekämpft, dem werden wir gemeinsam mit aller Härte und Entschlossenheit begegnen. Die Terroristen können gegen uns und unsere Werte kämpfen. Den Kampf gewinnen können sie nicht!

Brief aus Berlin 01 // 2015

Hansjörg Durz

Die Publikation von wissenschaftlichen Ergebnissen in elektronischer Form ist heute gängige Praxis. Die Entwicklungen der letzten Jahre führten dabei zu einer Vielfalt an elektronischen Ressourcen und zusammen mit neuen Geschäfts- und Lizenzierungsmodellen zu immer komplexeren Geschäftsprozessen. Das Angebot an kommerzieller Bibliothekssoftware zur Abbildung dieser Prozesse (Electronic Resource Management, ERM) ist jedoch überschaubar. Auch eine tragfähige Open-Source-Lösung existiert nicht, obwohl für die Verwaltung von E-Medien ein offenes, flexibles System erforderlich ist, um auf die stetigen Veränderungen schnell reagieren zu können. Basis einer solchen ERM-Anwendung ist ein entsprechender Datenbestand, wobei die Nutzung hochwertiger Wissensdatenbanken (Knowledge bases), vorhandener Lokalsysteme und anderer Quellen eine Homogenisierung der Daten notwendig macht. Die Linked Data-Technologie bietet durch die Flexibilität der Datenmodelle, die Verlinkung zu externen Datenbeständen und die derzeitigen Bestrebungen zum Aufbau bibliothekarischer Vokabulare eine optimale Grundlage für die Integration dieser Daten. Die Universitätsbibliothek Leipzig stellt sich mit Unterstützung der Forschungsgruppe Agile Knowledge Engineering and Semantic Web (AKSW) den genannten Herausforderungen. Das Projekt ERM ist Teil des EFRE-geförderten Projekts Wissenschaftskommunikation im Semantischen Web und hat zum Ziel, ein offenes ERM-System auf Basis von Linked Data-Technologien zu entwickeln. Projektpartner ist die SLUB Dresden, die eine Datenmanagement-Plattform zur automatischen Verknüpfung von Bibliotheksdaten entwickeln wird. Im Rahmen des Vortrags sollen Anforderungen an ein ERM-System unter Berücksichtigung des Reports der ERM Initiative der Digital Library Federation sowie Lösungskonzepte dargestellt werden.

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Studien-Erfolg

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diticuptm

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Tomas Enrique Pita Gutierrez

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Carlos Arturo Quintanilla Matos

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Standortentscheidungen in einer globalen welt

Studien-Erfolg

GAMESPLANET.com

4P-Marco

Die Maut kommt – und sie kommt so, wie vor der Wahl versprochen. Für deutsche Autofahrer gibt es keine Mehrbelastung. Da Halter von in Deutschland zugelassenen PKW bereits über die Zahlung der Kraftfahrzeugsteuer zur Finanzierung des Bundesfernstraßennetzes beitragen, werden sie bei der Kraftfahrzeugsteuer entsprechend entlastet. Erstmals werden Halter von im Ausland zugelassenen PKW an den Infrastrukturkosten direkt beteiligt. Damit schließen wir eine Gerechtigkeitslücke. Ein Rechtsgutachten der Universität Bonn bestätigt die Vereinbarkeit der Maut mit EU-Recht: Die Einführung der Maut stellt keine Diskriminierung von Unionsbürgern aus Gründen der Staatsangehörigkeit dar. Die Maut ist mit dem amtlichen Kraftfahrzeugkennzeichen verknüpft. Die Datenerhebung erfolgt ausschließlich zu Zwecken der Mauterhebung, eine andere Nutzung ist nach dem Gesetz ausgeschlossen. Halter von nicht in Deutschland Kfz-steuerpflichtigen Fahrzeugen können zwischen Zehntages-, Zweimonats- und Jahresvignetten wählen und sie schnell und unkompliziert als elektronische Vignette über das Internet oder an Vertriebsstellen wie Tankstellen erwerben. Durch die Beschränkung auf Autobahnen werden mögliche Auswirkungen auf die Grenzregionen ausgeschlossen. Alexander Dobrindt hat eine wirklich gute Lösung gefunden. Die Maut bringt ab 2016 netto Mehreinnahmen von 500 Mio. Euro pro Jahr, etwa zehn Prozent des gesamten Straßenverkehrsetats, die zweckgebunden in die Verkehrsinfrastruktur fließen und so dringend benötigte Investitionen ermöglichen. Es gibt viel zu tun, wir packen es an!

Brief aus Berlin 18 // 2014

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Cotton crops are vulnerable to a variety of sucking pests, which can severely impact plant health, yield, and fiber quality. These pests primarily feed on plant sap, extracting nutrients directly from the plant's vascular system. Here's a breakdown of some of the most significant sucking pests in cotton cultivation: Aphids: Cotton aphids or melon aphids can cause direct damage by sucking sap and indirect damage by secreting honeydew, which encourages sooty mold growth. This can interfere with photosynthesis and weaken the plant. Aphids can also transmit viral diseases. Whiteflies: Two species, the silverleaf whitefly and the bandedwinged whitefly, are particularly troublesome. They not only suck sap from the underside of leaves, causing yellowing and leaf drop, but their honeydew excretion promotes sooty mold and they can transmit several plant viruses. Thrips: While thrips can chew on plants, their primary damage to cotton is through sucking. They attack the cotton plant during its seedling stage, which can stunt growth and reduce vigor. Thrips are also capable of transmitting the Cotton Bud disease. Spider Mites: These are not insects but arachnids. Spider mites, such as the two-spotted spider mite, suck cell contents from the leaves, leading to speckled discoloration and potentially significant leaf loss if infestations are severe. Leafhoppers: Including various species, leafhoppers can cause direct damage through feeding, which results in leaf curling and stunted growth. They can also be vectors for plant diseases. Mealybugs: These pests are less common but can be problematic, especially in clustered planting conditions. They suck sap and secrete honeydew, which leads to sooty mold. Mealybugs can also spread viruses. Stink Bugs: Although primarily known for their chewing mouthparts, certain stink bugs can cause damage similar to sucking pests by injecting saliva into the plant and sucking out nutrients, leading to boll damage and stained lint. Management Strategies: Cultural Controls: This includes practices such as crop rotation, using resistant varieties, and managing planting and harvesting times to avoid peak pest populations. Biological Controls: Beneficial insects like lady beetles, lacewings, and predatory mites can naturally control sucking pest populations. Parasitic wasps also play a role in controlling aphid and whitefly populations. Chemical Controls: Insecticides may be used but should be chosen carefully to minimize resistance development and preserve beneficial insects. Systemic insecticides can be particularly effective against sucking pests. Integrated Pest Management (IPM): Combining multiple control strategies based on monitoring and thresholds to apply the most effective and environmentally sensitive approach. Effective management of sucking pests in cotton requires a thorough understanding of the pest species present, their life cycles, and the ecological balance of the field environment.

Pests of cotton_Sucking_Pests_Dr.UPR.pdf

PirithiRaju

Context. WASP-76 b has been a recurrent subject of study since the detection of a signature in high-resolution transit spectroscopy data indicating an asymmetry between the two limbs of the planet. The existence of this asymmetric signature has been confirmed by multiple studies, but its physical origin is still under debate. In addition, it contrasts with the absence of asymmetry reported in the infrared (IR) phase curve. Aims. We provide a more comprehensive dataset of WASP-76 b with the goal of drawing a complete view of the physical processes at work in this atmosphere. In particular, we attempt to reconcile visible high-resolution transit spectroscopy data and IR broadband phase curves. Methods. We gathered 3 phase curves, 20 occultations, and 6 transits for WASP-76 b in the visible with the CHEOPS space telescope. We also report the analysis of three unpublished sectors observed by the TESS space telescope (also in the visible), which represents 34 phase curves. Results. WASP-76 b displays an occultation of 260±11 and 152±10 ppm in TESS and CHEOPS bandpasses respectively. Depending on the composition assumed for the atmosphere and the data reduction used for the IR data, we derived geometric albedo estimates that range from 0.05 ± 0.023 to 0.146 ± 0.013 and from <0.13 to 0.189 ± 0.017 in the CHEOPS and TESS bandpasses, respectively. As expected from the IR phase curves, a low-order model of the phase curves does not yield any detectable asymmetry in the visible either. However, an empirical model allowing for sharper phase curve variations offers a hint of a flux excess before the occultation, with an amplitude of ∼40 ppm, an orbital offset of ∼−30◦ , and a width of ∼20◦ . We also constrained the orbital eccentricity of WASP-76 b to a value lower than 0.0067, with a 99.7% confidence level. This result contradicts earlier proposed scenarios aimed at explaining the asymmetry observed in high-resolution transit spectroscopy. Conclusions. In light of these findings, we hypothesise that WASP-76 b could have night-side clouds that extend predominantly towards its eastern limb. At this limb, the clouds would be associated with spherical droplets or spherically shaped aerosols of an unknown species, which would be responsible for a glory effect in the visible phase curves.

Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b

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Wepresent Atacama Large Millimeter/submillimeter Array 12-m, 7-m, and Total Power Array observations of the FUOrionis outbursting system, covering spatial scales ranging from 160 to 25,000 au. The high-resolution interferometric data reveal an elongated 12CO(2–1) feature previously observed at lower resolution in 12CO(3–2). Kinematic modeling indicates that this feature can be interpreted as an accretion streamer feeding the binary system. The mass infall rate provided by the streamer is significantly lower than the typical stellar accretion rates (even in quiescent states), suggesting that this streamer alone is not massive enough to sustain the enhanced accretion rates characteristic of the outbursting class prototype. The observed streamer may not be directly linked to the current outburst, but rather a remnant of a previous, more massive streamer that may have contributed enough to the disk mass to render it unstable and trigger the FU Orionis outburst. The new data detect, for the first time, a vast, slow-moving carbon monoxide molecular outflow emerging from this object. To accurately assess the outflow properties (mass, momentum, and kinetic energy), we employ 13CO(2–1) data to correct for optical depth effects. The analysis indicates that the outflow corresponds to swept-up material not associated with the current outburst, similar to the slow molecular outflows observed around other FUor and Class I protostellar objects.

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A botany file is similar to a chemistry practical file but specifically focuses on experiments and observations related to plants. It typically includes detailed descriptions of plant-related experiments, such as germination studies, growth experiments, tissue culture techniques, plant anatomy investigations, and ecological surveys. The file may contain records of plant specimens collected, their classification, characteristics, and ecological significance. Additionally, it may include diagrams, photographs, drawings, tables, and data analysis related to plant research. Like a chemistry practical file, a botany file serves as a documentation of practical work conducted in the field of botany and is often used for assessment and educational purposes.

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Mustard, as a crop, is susceptible to a variety of pests that can affect its growth and yield. Here’s a rundown of some common pests that target mustard plants: Aphids: These small, sap-sucking insects can cause significant damage by feeding on the leaves and stems. Aphids also excrete a sticky substance known as honeydew, which can lead to the growth of sooty mold on the plants. Flea Beetles: These tiny beetles jump like fleas when disturbed and chew small holes in the leaves. They are particularly damaging in the early growth stages of the plant. Cabbage Loopers: The larvae of a type of moth, these caterpillars are known for their distinctive looping movement. They chew large holes in the leaves and can defoliate plants if present in large numbers. Diamondback Moth Larvae: Another caterpillar pest, these larvae chew small holes in the leaves and can cause extensive damage, especially when infestations are heavy. Whiteflies: These are tiny, winged insects that feed on plant sap and can quickly become a problem in greenhouse or close planting conditions. Like aphids, they also secrete honeydew. Cutworms: These are the larvae of certain types of moths and are known for cutting young plants at the stem base at ground level. They are most destructive during the night. Root Maggots: The larvae of root maggot flies, these pests attack the roots of mustard plants, causing wilting and potentially killing young plants. Harlequin Bugs: These are colorful stink bugs that suck the sap from mustard plant stems and leaves, causing the leaves to become stippled, wilt, and eventually die if the infestation is severe. Mustard Sawfly: The larvae of the mustard sawfly can cause considerable defoliation, as they feed voraciously on the leaves. Clubroot: Caused by a fungus-like organism, clubroot affects the roots, causing them to swell and distort. While technically a disease, it is often associated with pest management because controlling it involves similar preventative strategies. Control Measures: Managing pests in mustard involves a combination of cultural, biological, and chemical methods. Crop rotation, resistant varieties, timely sowing, maintaining plant health, and using natural predators like ladybugs and parasitic wasps can help keep pest populations under control. Chemical pesticides should be used as a last resort due to their potential impact on the environment and non-target species.

Pests of mustard_Identification_Management_Dr.UPR.pdf

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HotJupiters are amongthebest-studied exoplanets, but it is still poorly understood how their chemical composition and cloud properties vary with longitude. Theoretical models predict that clouds may condense on the nightside and that molecular abundances can be driven out of equilibrium by zonal winds. Here we report a phase-resolved emission spectrum of the hot Jupiter WASP-43b measured from 5–12µ 5–12µ 5–12µm with JWST’s Mid-Infrared Instrument (MIRI). 1524 ±35 1524 ±35 and 863±23 The spectra reveal a large day–night temperature contrast (with average brightness temperatures of 1524 ± 35 863 ±23 863 ±23Kelvin, respectively) and evidence for water absorption at all orbital phases. Comparisons with three-dimensional atmospheric models show that both the phase curve shape and emission spectra strongly suggest the presence of nightside clouds which become optically thick to thermal emission at pressures greater than ∼100mbar. The dayside is consistent with a cloudless atmosphere above the mid-infrared photosphere. Con3trary to expectations from equilibrium chemistry but consistent with disequilibrium kinetics models, methane is not detected on the nightside (2σ upper limit of 1–6 parts per million, depending on model assumptions).

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Wordles_Flor B

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