Yamada bachelor thesis

•

0 likes•2,594 views

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

Yamada bachelor thesis

More Related Content

More from pflab

Tomoya Sato Master Thesis

Tomoya Sato Master Thesis

Tomoya Sato Master Thesis

Miyoshi Bachelor Thesis

Miyoshi Bachelor Thesis

Miyoshi Bachelor Thesis

Ikarashi Bachelor Thesis

Ikarashi Bachelor Thesis

Ikarashi Bachelor Thesis

Akihiro Sakurai Bachelor Thesis

Akihiro Sakurai Bachelor Thesis

Akihiro Sakurai Bachelor Thesis

Yuto Mochizuki bachelor thesis

Yuto Mochizuki bachelor thesis

Yuto Mochizuki bachelor thesis

Yoshio Kato Bachelor Thesis

Yoshio Kato Bachelor Thesis

Yoshio Kato Bachelor Thesis

Junnosuke Mizutani Bachelor Thesis

Junnosuke Mizutani Bachelor Thesis

Junnosuke Mizutani Bachelor Thesis

Cho Bachelor Thesis

Cho Bachelor Thesis

Cho Bachelor Thesis

Tatsuya Sueki Bachelor Thesis

Tatsuya Sueki Bachelor Thesis

Tatsuya Sueki Bachelor Thesis

Shusaku Taniguchi Bachelor Thesis

Shusaku Taniguchi Bachelor Thesis

Shusaku Taniguchi Bachelor Thesis

Shogo Yamazaki Bachelor Thesis

Shogo Yamazaki Bachelor Thesis

Shogo Yamazaki Bachelor Thesis

Hidehito Yabuuchi Bachelor Thesis

Hidehito Yabuuchi Bachelor Thesis

Hidehito Yabuuchi Bachelor Thesis

Yu Sasaki Bachelor Thesis

Yu Sasaki Bachelor Thesis

Yu Sasaki Bachelor Thesis

Tomoya Sato Bachelor Thesis

Tomoya Sato Bachelor Thesis

Tomoya Sato Bachelor Thesis

Kazumasa Sakiyama Bachelor Thesis

Kazumasa Sakiyama Bachelor Thesis

Kazumasa Sakiyama Bachelor Thesis

Akihiro Aritoshi Bachelor Thesis

Akihiro Aritoshi Bachelor Thesis

Akihiro Aritoshi Bachelor Thesis

Shinichi Awamoto Bachelor Thesis

Shinichi Awamoto Bachelor Thesis

Shinichi Awamoto Bachelor Thesis

輪講発表資料です。 The Multikernel: A new OS architecture for scalable multicore systems Andrew Baumann, Paul Barham, Pierre-Evariste Dagand, Tim Harris, Rebecca Isaacs, Simon Peter, Timothy Roscoe, Adrian Schüpbach, and Akhilesh Singhania SoSP09 An Analysis of Linux Scalability to Many Cores Silas Boyd-Wickizer, Austin T. Clements, Yandong Mao, Aleksey Pesterev, M. Frans Kaashoek, Robert Morris, and Nickolai Zeldovich MIT CSAIL OSDI10

輪講_Awamoto_20170601

輪講_Awamoto_20170601

輪講_Awamoto_20170601

輪講_Sakiyama_20170601

輪講_Sakiyama_20170601

輪講_Sakiyama_20170601

More from pflab (19)

Tomoya Sato Master Thesis

Tomoya Sato Master Thesis

Tomoya Sato Master Thesis

Miyoshi Bachelor Thesis

Miyoshi Bachelor Thesis

Miyoshi Bachelor Thesis

Ikarashi Bachelor Thesis

Ikarashi Bachelor Thesis

Ikarashi Bachelor Thesis

Akihiro Sakurai Bachelor Thesis

Akihiro Sakurai Bachelor Thesis

Akihiro Sakurai Bachelor Thesis

Yuto Mochizuki bachelor thesis

Yuto Mochizuki bachelor thesis

Yuto Mochizuki bachelor thesis

Yoshio Kato Bachelor Thesis

Yoshio Kato Bachelor Thesis

Yoshio Kato Bachelor Thesis

Junnosuke Mizutani Bachelor Thesis

Junnosuke Mizutani Bachelor Thesis

Junnosuke Mizutani Bachelor Thesis

Cho Bachelor Thesis

Cho Bachelor Thesis

Cho Bachelor Thesis

Tatsuya Sueki Bachelor Thesis

Tatsuya Sueki Bachelor Thesis

Tatsuya Sueki Bachelor Thesis

Shusaku Taniguchi Bachelor Thesis

Shusaku Taniguchi Bachelor Thesis

Shusaku Taniguchi Bachelor Thesis

Shogo Yamazaki Bachelor Thesis

Shogo Yamazaki Bachelor Thesis

Shogo Yamazaki Bachelor Thesis

Hidehito Yabuuchi Bachelor Thesis

Hidehito Yabuuchi Bachelor Thesis

Hidehito Yabuuchi Bachelor Thesis

Yu Sasaki Bachelor Thesis

Yu Sasaki Bachelor Thesis

Yu Sasaki Bachelor Thesis

Tomoya Sato Bachelor Thesis

Tomoya Sato Bachelor Thesis

Tomoya Sato Bachelor Thesis

Kazumasa Sakiyama Bachelor Thesis

Kazumasa Sakiyama Bachelor Thesis

Kazumasa Sakiyama Bachelor Thesis

Akihiro Aritoshi Bachelor Thesis

Akihiro Aritoshi Bachelor Thesis

Akihiro Aritoshi Bachelor Thesis

Shinichi Awamoto Bachelor Thesis

Shinichi Awamoto Bachelor Thesis

Shinichi Awamoto Bachelor Thesis

輪講_Awamoto_20170601

輪講_Awamoto_20170601

輪講_Awamoto_20170601

輪講_Sakiyama_20170601

輪講_Sakiyama_20170601

輪講_Sakiyama_20170601

Recently uploaded

Green chemistry and Sustainable development.pptx

Green chemistry and Sustainable development.pptx

Green chemistry and Sustainable development.pptx

RajatChauhan518211

Creating and Analyzing Definitive Screening Designs

Creating and Analyzing Definitive Screening Designs

Creating and Analyzing Definitive Screening Designs

NurulAfiqah307317

We explore different scenarios to explain the chemical difference found in the remarkable giant-giant binary system HD138202+CD−3012303. For the first time, we suggest how to distinguish these scenarios by taking advantage of the extensive convective envelopes of giant stars. Methods. We carried out a high-precision determination of stellar parameters and abundances by applying a full line-by-line differential analysis on GHOST high-resolution spectra. We used the FUNDPAR program with ATLAS12 model atmospheres and specific opacities calculated for an arbitrary composition through a doubly iterated method. Physical parameters were estimated with the isochrones package and evolutionary tracks were calculated via MIST models. Results. We found a significant chemical difference between the two stars (∆[Fe/H]∼0.08dex), which is largely unexpected considering the insensitivity of giant stars to planetary ingestion and diffusion effects. We tested the possibility of engulfment events by using several different combinations of stellar mass, ingested mass, metallicity of the engulfed object and different convective envelopes. However, the planetary ingestion scenario does not seem to explain the observed differences. For the first time, we distinguished the source of chemical differences using a giant-giant binary system. By ruling out other possible scenarios such as planet formation and evolutionary effects between the two stars, we suggest that primordial inhomogeneities might explain the observed differences. This remarkable result implies that the metallicity differences that were observed in at least some main-sequence binary systems might be related to primordial inhomogeneities rather than engulfment events. We also discuss the important implications of finding primordial inhomogeneities, which affect chemical tagging and other fields such as planet formation. We strongly encourage the use of giantgiant pairs. They are a relevant complement to main-sequence pairs for determining the origin of the observed chemical differences in multiple systems.

Disentangling the origin of chemical differences using GHOST

Disentangling the origin of chemical differences using GHOST

Disentangling the origin of chemical differences using GHOST

High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...

High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...

High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...

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

Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b

Pulmonary drug delivery system M.pharm -2nd sem P'ceutics

Pulmonary drug delivery system M.pharm -2nd sem P'ceutics

Pulmonary drug delivery system M.pharm -2nd sem P'ceutics

TEST BANK For Radiologic Science for Technologists, 12th Edition by Stewart C...

TEST BANK For Radiologic Science for Technologists, 12th Edition by Stewart C...

TEST BANK For Radiologic Science for Technologists, 12th Edition by Stewart C...

Bollworms are among the most damaging pests in cotton cultivation, affecting the bolls where the cotton fibers are formed. There are several species of bollworms, each capable of causing significant yield loss and quality degradation if not effectively managed. Here’s a detailed look at the primary bollworm species affecting cotton: Cotton Bollworm (Helicoverpa armigera): Also known as the corn earworm or the Old World bollworm, this pest is found in many regions around the world. It is highly polyphagous (feeds on many different plants) and poses a threat not only to cotton but also to maize, tomatoes, and legumes. The larvae bore into the cotton bolls, feeding on the developing seeds and fibers, which can lead to boll rot. Pink Bollworm (Pectinophora gossypiella): A significant pest of cotton, the pink bollworm larvae infest the cotton bolls, feeding on the seeds and lint. This can severely damage or destroy the bolls. In regions where pink bollworms are prevalent, they have been a major driver for the adoption of genetically engineered Bt cotton, which expresses a bacterium gene toxic to certain insects. Tobacco Budworm (Heliothis virescens): Closely related to the cotton bollworm, the tobacco budworm primarily attacks tobacco but is also a common pest in cotton. It primarily damages the flowers and bolls of the cotton plant. Differentiating between the tobacco budworm and the cotton bollworm based on appearance can be challenging, but it is crucial for effective management. American Bollworm (Helicoverpa zea): Known in some regions as the corn earworm, it is similar in behavior to Helicoverpa armigera and poses a threat to a variety of crops, including cotton. The larvae attack the cotton bolls, leading to direct damage to the cotton lint and seeds. Management Strategies: Cultural Controls: Crop rotation, destruction of crop residues, and deep plowing can help break the pest’s life cycle. Timing of planting can also be adjusted to avoid peak pest infestation. Biological Controls: Natural enemies like Trichogramma wasps, which parasitize bollworm eggs, and predators such as lacewings and ladybugs can be encouraged. Bacillus thuringiensis (Bt) products can also be sprayed, which are particularly effective against young larvae. Chemical Controls: Insecticides may be required when infestation levels exceed economic thresholds. However, resistance management must be considered, alternating modes of action to avoid developing resistance. Genetic Approaches: Bt cotton, genetically modified to express Bacillus thuringiensis toxin, has been highly effective in controlling bollworms and has dramatically reduced the reliance on chemical insecticides. Monitoring and Scouting: Regular field scouting and using pheromone traps to monitor adult populations can help in timely and targeted application of control measures. The effective management of bollworms often requires an integrated approach

Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf

Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf

Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf

GBSN - Microbiology (Unit 1)

GBSN - Microbiology (Unit 1)

GBSN - Microbiology (Unit 1)

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.

Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...

Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...

Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...

Forensic Biology & Its biological significance.pdf

Forensic Biology & Its biological significance.pdf

Forensic Biology & Its biological significance.pdf

rohankumarsinghrore1

GUIDELINES ON SIMILAR BIOLOGICS Regulatory Requirements for Marketing Authori...

GUIDELINES ON SIMILAR BIOLOGICS Regulatory Requirements for Marketing Authori...

GUIDELINES ON SIMILAR BIOLOGICS Regulatory Requirements for Marketing Authori...

Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency

Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency

Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency

Chemistry is the scientific study of matter, its properties, composition, structure, and the changes it undergoes. It's often divided into various sub-disciplines such as organic chemistry, inorganic chemistry, physical chemistry, analytical chemistry, and biochemistry. Chemistry plays a crucial role in understanding the world around us and has applications in various fields such as medicine, materials science, environmental science, and industry.

Chemistry 4th semester series (krishna).pdf

Chemistry 4th semester series (krishna).pdf

Chemistry 4th semester series (krishna).pdf

Sumit Kumar yadav

Biological Classification BioHack (3).pdf

Biological Classification BioHack (3).pdf

Biological Classification BioHack (3).pdf

CELL -Structural and Functional unit of life.pdf

CELL -Structural and Functional unit of life.pdf

CELL -Structural and Functional unit of life.pdf

Nistarini College, Purulia (W.B) India

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

Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds

........................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................................

SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx

SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx

SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx

RizalinePalanog2

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

Pests of cotton_Sucking_Pests_Dr.UPR.pdf

Nanoparticles synthesis and characterization

Nanoparticles synthesis and characterization

Nanoparticles synthesis and characterization

kaibalyasahoo82800

Recently uploaded (20)

Green chemistry and Sustainable development.pptx

Green chemistry and Sustainable development.pptx

Green chemistry and Sustainable development.pptx

Creating and Analyzing Definitive Screening Designs

Creating and Analyzing Definitive Screening Designs

Creating and Analyzing Definitive Screening Designs

Disentangling the origin of chemical differences using GHOST

Disentangling the origin of chemical differences using GHOST

Disentangling the origin of chemical differences using GHOST

High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...

High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...

High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...

Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b

Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b

Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b

Pulmonary drug delivery system M.pharm -2nd sem P'ceutics

Pulmonary drug delivery system M.pharm -2nd sem P'ceutics

Pulmonary drug delivery system M.pharm -2nd sem P'ceutics

TEST BANK For Radiologic Science for Technologists, 12th Edition by Stewart C...

TEST BANK For Radiologic Science for Technologists, 12th Edition by Stewart C...

TEST BANK For Radiologic Science for Technologists, 12th Edition by Stewart C...

Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf

Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf

Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf

GBSN - Microbiology (Unit 1)

GBSN - Microbiology (Unit 1)

GBSN - Microbiology (Unit 1)

Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...

Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...

Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...

Forensic Biology & Its biological significance.pdf

Forensic Biology & Its biological significance.pdf

Forensic Biology & Its biological significance.pdf

GUIDELINES ON SIMILAR BIOLOGICS Regulatory Requirements for Marketing Authori...

GUIDELINES ON SIMILAR BIOLOGICS Regulatory Requirements for Marketing Authori...

GUIDELINES ON SIMILAR BIOLOGICS Regulatory Requirements for Marketing Authori...

Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency

Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency

Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency

Chemistry 4th semester series (krishna).pdf

Chemistry 4th semester series (krishna).pdf

Chemistry 4th semester series (krishna).pdf

Biological Classification BioHack (3).pdf

Biological Classification BioHack (3).pdf

Biological Classification BioHack (3).pdf

CELL -Structural and Functional unit of life.pdf

CELL -Structural and Functional unit of life.pdf

CELL -Structural and Functional unit of life.pdf

Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds

Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds

Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds

SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx

SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx

SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx

Pests of cotton_Sucking_Pests_Dr.UPR.pdf

Pests of cotton_Sucking_Pests_Dr.UPR.pdf

Pests of cotton_Sucking_Pests_Dr.UPR.pdf

Nanoparticles synthesis and characterization

Nanoparticles synthesis and characterization

Nanoparticles synthesis and characterization