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Managing heat in the desert dairy global
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This method is limited to the numbers that have 5 in its unit’s place. With the help of these methods you will be able to find the square of any number that ends in 5 within a fraction of seconds.
Square of Numbers that end in 5
Square of Numbers that end in 5
rmathemagica
3ª PARTE Reunião que culminou com a criação da Comissão de Desenvolvimento de Políticas Tributárias para o setor de Revendedores de Veículos do Estado de Mato Grosso realizado, para o ano de 2016, na sede da secretaria da fazenda, (dia 14 de dezembro de 2015) com a presença do então Secretário de fazenda Paulo Brustolin.
REUNIÃO COM SECRETÁRIO DE FAZENDA DE MATO GROSSO, PAULO BRUSTOLIN - 3º PARTE
REUNIÃO COM SECRETÁRIO DE FAZENDA DE MATO GROSSO, PAULO BRUSTOLIN - 3º PARTE
AGENCIAUTO/MT - Associação dos Revendedores de Veículos do Estado de Mato Grosso
HANS Spring 2015, Confessions of a Baby Boomer
HANS Spring 2015, Confessions of a Baby Boomer
Ron Gale
Eng. Mohammad Zamil _MEP Engineer
Eng. Mohammad Zamil _MEP Engineer
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Dr. N. KARUNAKARAN (INTERNATIONAL OUTSTANDING FACULTY AWARD) 2015
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ServiceControl - PPT Template
ServiceControl - PPT Template
Rachel Rowling
வெற்றி = பணம் என்று வாதத்திற்கு ஒப்புக் கொண்டால் அந்த பணத்தை அடைய CASH என்பதிற்கு பதிலாக KASH என்பதை நீங்கள் வளர்த்தல் வேண்டும். அது என்ன KASH ? K = KNOWLEDGE = அறிவு A = ATTITUDE = மனப்பான்மை S = SKILL = திறமை H = HABIT = பழக்கம் இவை தான் உங்கள் வெற்றியை தீர்மானிக்கும் . ஏன்? எதற்கு? எங்கே? எப்பொழுது? ஏன்? உங்கள் வியாபார வளர்சிக்கு தேவையான தொழில் வளக்கலை. எதற்கு? 1.விற்பனை அதிகரிக்க..... 2.மார்க்கெட்டிங் துறை சார்ந்த அனைத்து பிரச்சனைகளுக்கும் சரியான வழிகாட்டுதல். 3.புதிய தயாரிப்புகளை சந்தைபடுத்த தேவையான ட்ரைனிங் ....... 4.உங்கள் தயாரிப்புகளுக்கு தனி ப்ரண்ட் அங்கிகாரம் பெற தேவையான ட்ரைனிங் .... 5.ஸ்டார்ட் அப் தொழில் அமைப்புகளுக்கு தங்கள் தயாரிப்புகள் மார்க்கெட்டிங் செய்ய தேவையான அனைத்து மார்க்கெட்டிங் ட்ரைனிங் நாங்கள் உங்களுக்கு தருகிறோம். மனிதவளத்துறை சார்ந்த வழிகாட்டுதல். செயல் திறன் மேம்பாடு ஒன்று மட்டுமே உங்கள் தொழில் வெற்றிக்கு வழிவகுக்கும். 1. நீங்கள் யார் உங்களுக்குள் இருக்கும் பிரச்சனைகளுக்கு சரியானவழிகாட்டுதல். 2.உங்கள் முடிவு எடுக்கும் முறை ஒழுங்குபடுத்த 3.உங்கள் தாழ்வு மனப்பான்மை மாற 4.உங்கள் வியாபார வெற்றிக்கு தேவையான அனைத்து ட்ரைனிங் எங்களிடம் உள்ளது. எங்கே? உங்களுக்கா உங்களிடத்தில். எப்பொழுது? உங்கள் வெற்றிக்கான நாளை நீங்களே தீர்மானியுங்கள். நாளைய அறிவு இன்றய வெற்றி. அணுகவும் கௌசிகா கன்சல்டண்சி ர.ராஜாராம் - 9865118262 kowshikaa2009@gmail.com
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Managing heat in the desert dairy global
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Dr.Rami Hamad
This method is limited to the numbers that have 5 in its unit’s place. With the help of these methods you will be able to find the square of any number that ends in 5 within a fraction of seconds.
Square of Numbers that end in 5
Square of Numbers that end in 5
rmathemagica
3ª PARTE Reunião que culminou com a criação da Comissão de Desenvolvimento de Políticas Tributárias para o setor de Revendedores de Veículos do Estado de Mato Grosso realizado, para o ano de 2016, na sede da secretaria da fazenda, (dia 14 de dezembro de 2015) com a presença do então Secretário de fazenda Paulo Brustolin.
REUNIÃO COM SECRETÁRIO DE FAZENDA DE MATO GROSSO, PAULO BRUSTOLIN - 3º PARTE
REUNIÃO COM SECRETÁRIO DE FAZENDA DE MATO GROSSO, PAULO BRUSTOLIN - 3º PARTE
AGENCIAUTO/MT - Associação dos Revendedores de Veículos do Estado de Mato Grosso
HANS Spring 2015, Confessions of a Baby Boomer
HANS Spring 2015, Confessions of a Baby Boomer
Ron Gale
Eng. Mohammad Zamil _MEP Engineer
Eng. Mohammad Zamil _MEP Engineer
Mohammad Zamil
Dr. N. KARUNAKARAN (INTERNATIONAL OUTSTANDING FACULTY AWARD) 2015
Dr. N. KARUNAKARAN (INTERNATIONAL OUTSTANDING FACULTY AWARD) 2015
Dr. N. KARUNAKARAN .
ServiceControl - PPT Template
ServiceControl - PPT Template
Rachel Rowling
வெற்றி = பணம் என்று வாதத்திற்கு ஒப்புக் கொண்டால் அந்த பணத்தை அடைய CASH என்பதிற்கு பதிலாக KASH என்பதை நீங்கள் வளர்த்தல் வேண்டும். அது என்ன KASH ? K = KNOWLEDGE = அறிவு A = ATTITUDE = மனப்பான்மை S = SKILL = திறமை H = HABIT = பழக்கம் இவை தான் உங்கள் வெற்றியை தீர்மானிக்கும் . ஏன்? எதற்கு? எங்கே? எப்பொழுது? ஏன்? உங்கள் வியாபார வளர்சிக்கு தேவையான தொழில் வளக்கலை. எதற்கு? 1.விற்பனை அதிகரிக்க..... 2.மார்க்கெட்டிங் துறை சார்ந்த அனைத்து பிரச்சனைகளுக்கும் சரியான வழிகாட்டுதல். 3.புதிய தயாரிப்புகளை சந்தைபடுத்த தேவையான ட்ரைனிங் ....... 4.உங்கள் தயாரிப்புகளுக்கு தனி ப்ரண்ட் அங்கிகாரம் பெற தேவையான ட்ரைனிங் .... 5.ஸ்டார்ட் அப் தொழில் அமைப்புகளுக்கு தங்கள் தயாரிப்புகள் மார்க்கெட்டிங் செய்ய தேவையான அனைத்து மார்க்கெட்டிங் ட்ரைனிங் நாங்கள் உங்களுக்கு தருகிறோம். மனிதவளத்துறை சார்ந்த வழிகாட்டுதல். செயல் திறன் மேம்பாடு ஒன்று மட்டுமே உங்கள் தொழில் வெற்றிக்கு வழிவகுக்கும். 1. நீங்கள் யார் உங்களுக்குள் இருக்கும் பிரச்சனைகளுக்கு சரியானவழிகாட்டுதல். 2.உங்கள் முடிவு எடுக்கும் முறை ஒழுங்குபடுத்த 3.உங்கள் தாழ்வு மனப்பான்மை மாற 4.உங்கள் வியாபார வெற்றிக்கு தேவையான அனைத்து ட்ரைனிங் எங்களிடம் உள்ளது. எங்கே? உங்களுக்கா உங்களிடத்தில். எப்பொழுது? உங்கள் வெற்றிக்கான நாளை நீங்களே தீர்மானியுங்கள். நாளைய அறிவு இன்றய வெற்றி. அணுகவும் கௌசிகா கன்சல்டண்சி ர.ராஜாராம் - 9865118262 kowshikaa2009@gmail.com
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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
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Sérgio Sacani
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This presentation offers the bird's eye view of the cell as the basic structural and functional unit of life. It also addresses the origin of eukaryotic cells from the prokaryotic cell by the endosymbiotic theory.
CELL -Structural and Functional unit of life.pdf
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Control of Microorganisms
GBSN - Microbiology (Unit 2)
GBSN - Microbiology (Unit 2)
Areesha Ahmad
Defense Mechanism of the body
GBSN - Microbiology (Unit 3)
GBSN - Microbiology (Unit 3)
Areesha Ahmad
Theoretical predictions and observational data indicate a class of sub-Neptune exoplanets may have water-rich interiors covered by hydrogen-dominated atmospheres. Provided suitable climate conditions, such planets could host surface liquid oceans. Motivated by recent JWST observations of K2-18 b, we self-consistently model the photochemistry and potential detectability of biogenic sulfur gases in the atmospheres of temperate sub-Neptune waterworlds for the first time. On Earth today, organic sulfur compounds produced by marine biota are rapidly destroyed by photochemical processes before they can accumulate to significant levels. Domagal-Goldman et al. suggest that detectable biogenic sulfur signatures could emerge in Archean-like atmospheres with higher biological production or low UV flux. In this study, we explore biogenic sulfur across a wide range of biological fluxes and stellar UV environments. Critically, the main photochemical sinks are absent on the nightside of tidally locked planets. To address this, we further perform experiments with a 3D general circulation model and a 2D photochemical model (VULCAN 2D) to simulate the global distribution of biogenic gases to investigate their terminator concentrations as seen via transmission spectroscopy. Our models indicate that biogenic sulfur gases can rise to potentially detectable levels on hydrogen-rich water worlds, but only for enhanced global biosulfur flux (20 times modern Earth’s flux). We find that it is challenging to identify DMS at 3.4 μm where it strongly overlaps with CH4, whereas it is more plausible to detect DMS and companion byproducts, ethylene (C2H4) and ethane (C2H6), in the mid-infrared between 9 and 13 μm. Unified Astronomy Thesaurus concepts: Exoplanet atmospheres (487); Exoplanet
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
Sérgio Sacani
Presentation from the "Opening up Research" conference organised by the University of Manchester's Office for Open Research. 24 April 2024 https://www.openresearch.manchester.ac.uk/ https://fairspectra.net https://alexhenderson.info
FAIRSpectra - Enabling the FAIRification of Spectroscopy and Spectrometry
FAIRSpectra - Enabling the FAIRification of Spectroscopy and Spectrometry
Alex Henderson
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
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
PirithiRaju
Microbiology
Bacterial Identification and Classifications
Bacterial Identification and Classifications
Areesha Ahmad
Botany is the branch of biology that deals with the scientific study of plants, including their structure, growth, reproduction, metabolism, development, and classification. It encompasses a wide range of topics, from the molecular biology of plant cells to the ecological relationships between plants and their environments. Botany is essential for understanding plant diversity, ecology, evolution, and the roles plants play in ecosystems and human societies.
Botany 4th semester series (krishna).pdf
Botany 4th semester series (krishna).pdf
Sumit Kumar yadav
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
Pests of mustard_Identification_Management_Dr.UPR.pdf
PirithiRaju
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Research Methodology
COST ESTIMATION FOR A RESEARCH PROJECT.pptx
COST ESTIMATION FOR A RESEARCH PROJECT.pptx
FarihaAbdulRasheed
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kantirani197
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).
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Sérgio Sacani
Seismic Method
Seismic Method Estimate velocity from seismic data.pptx
Seismic Method Estimate velocity from seismic data.pptx
AlMamun560346
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Basic concept of chemistry
GBSN - Biochemistry (Unit 1)
GBSN - Biochemistry (Unit 1)
Areesha Ahmad
Último
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Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
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CELL -Structural and Functional unit of life.pdf
CELL -Structural and Functional unit of life.pdf
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GBSN - Microbiology (Unit 2)
GBSN - Microbiology (Unit 2)
GBSN - Microbiology (Unit 3)
GBSN - Microbiology (Unit 3)
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
FAIRSpectra - Enabling the FAIRification of Spectroscopy and Spectrometry
FAIRSpectra - Enabling the FAIRification of Spectroscopy and Spectrometry
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
Bacterial Identification and Classifications
Bacterial Identification and Classifications
Botany 4th semester series (krishna).pdf
Botany 4th semester series (krishna).pdf
Pests of mustard_Identification_Management_Dr.UPR.pdf
Pests of mustard_Identification_Management_Dr.UPR.pdf
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COST ESTIMATION FOR A RESEARCH PROJECT.pptx
COST ESTIMATION FOR A RESEARCH PROJECT.pptx
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Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Seismic Method Estimate velocity from seismic data.pptx
Seismic Method Estimate velocity from seismic data.pptx
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GBSN - Biochemistry (Unit 1)
GBSN - Biochemistry (Unit 1)
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