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First Successful Horizontal Completion in the Rogersville Shale. Holds the Kentucky record for deepest well (MD) at 16,108' Holds the Kentucky record for largest successful completion. The numbers are moderate with obviously dryer gas than what was rumored or anticipated. Numbers show a lot of promise, particularly within the slightly shallower "Rogersville Oil Window". History's first three Marcellus horizontal wells, 1st-20 mcfp/d, 2nd-250 mcfp/d, 3rd-600 mcfp/d

Cimarex Energy's Walbridge 1-H First Successful Rogersville Shale Horizontal ...

Cimarex Energy's Walbridge 1-H First Successful Rogersville Shale Horizontal ...

Cimarex Energy's Walbridge 1-H First Successful Rogersville Shale Horizontal ...

First Successful Horizontal Completion in the Rogersville Shale. The numbers are moderate with obviously dryer gas than what was rumored or anticipated. Numbers show a lot of promise, particularly within the Rogersville Oil Window. History's First three Marcellus horizontal wells, 1st-20 mcfp/d, 2nd-250 mcfp/d, 3rd-600 mcfp/d. It took Range a hundred and fifty million dollars and 5 wells including the first vertical to get to over a million cfd out of any of the wells, this first horizontal Rogersville wildcat is as good as Range's first 4 Marcellus wells combined.

Cimarex Energy's Bruin-Walbridge 1-H Horizontal Rogersville Shale Flow Back ...

Cimarex Energy's Bruin-Walbridge 1-H Horizontal Rogersville Shale Flow Back ...

Cimarex Energy's Bruin-Walbridge 1-H Horizontal Rogersville Shale Flow Back ...

Cimarex Energy's "Defined" Rogersville Shale Log Signature

Cimarex Energy's "Defined" Rogersville Shale Log Signature

Cimarex Energy's "Defined" Rogersville Shale Log Signature

Rogersville Shale Compostion Reading Between the Plates Maryville over Rome,...

Rogersville Shale Compostion Reading Between the Plates Maryville over Rome,...

Rogersville Shale Compostion Reading Between the Plates Maryville over Rome,...

New State Drilling Depth Record Reached in Lawrence County, Kentucky Geologic...

New State Drilling Depth Record Reached in Lawrence County, Kentucky Geologic...

New State Drilling Depth Record Reached in Lawrence County, Kentucky Geologic...

A reasonable explanation for the anomalous interval thickness of the Rutledge Limestone in the Chesapeake Energy Stephens Law-1 Vertical Rogersville Shale Well, based on proprietary geophysical data with matching signature. The geophysical logs run on this well are confidential through the Strat Test arrangements operator negotiated with the KY Dept of Oil & Gas so verification by examination of the well logs can only proceed when the confidentiality period expires. Modified from a cross section by the KGS flattened on the top of the Rogersville Shale

Evidence for a repeated section of the rutledge limestone in the chesapeake e...

Evidence for a repeated section of the rutledge limestone in the chesapeake e...

Evidence for a repeated section of the rutledge limestone in the chesapeake e...

Completions Report for the CHK Stephens Rogersville Shale Vertical Well less the important data still held confidential via the Confidentiality of the Stratigraphic Test phase of this well. Differences in adjacent control are noted on report. Thinking back on completions report where the PKV was so wet, noticed Chesapeake had pumped in 7660 bbl water and x link jel with 425 Klbs sand and only recovered 5700 bbl water just 8 days before the Pumpkin Valley completion where they pumped in 50 bbl water and got back 50 bo, 252 mcfg, 815 bbl water. These zones are 400' apart vert but directly on or adjacent to a small reverse fault, could be they recovered the Rome input water from the adjacent PKV treatment zone.

Chesapeake Energy Rogersville Shale completion report

Chesapeake Energy Rogersville Shale completion report

Chesapeake Energy Rogersville Shale completion report

November 7 2016 m 5.0 Earthquake - 2km w of cushing, oklahoma

November 7 2016 m 5.0 Earthquake - 2km w of cushing, oklahoma

November 7 2016 m 5.0 Earthquake - 2km w of cushing, oklahoma

Rogersville Shale Maryville LS & SS New Cores Relative to IEP and CHK Contr...

Rogersville Shale Maryville LS & SS New Cores Relative to IEP and CHK Contr...

Rogersville Shale Maryville LS & SS New Cores Relative to IEP and CHK Contr...

Second only Rogersville Shale Deep Horizontal Well Spudded to Date and should show up on Rig Counts Week of 10-14-2016. Permit app and revisions to location and amended Depth to 16,536' TMD. Mud and casing weights as well as ratings on BOP's infer an overpressured reservoir and Cimarex has data on the vertical wells previously drilled so they are not going into this one blind. Rig in Photo is Nomac Rig #79 Spud Date 10-10-2016. Permit Application & Data obtained through Open Records Request at KY DOG.

Cimarex Energy's First Rogersville Shale Horizontal Deep Well the Walbridge 1...

Cimarex Energy's First Rogersville Shale Horizontal Deep Well the Walbridge 1...

Cimarex Energy's First Rogersville Shale Horizontal Deep Well the Walbridge 1...

Modified from RI21_12_plate4_8, author Michael Solis NEKY Stacked Opportunities Near the Top, the Berea Sandstone, Kentucky's Best Oil Play for the Second Year in a row and near the bottom Kentucky's Newest the Rogersville Shale.. Originally created to show stacked Co2 disposal possibilities, it represents a more complete strat. column allowing highlighting of the numerous hydrocarbon producing zones stacked within the Rome Trough of NEKY in contrast to most publications.

NEKY Stacked Opportunities Rogersville Shale Berea Sandstone and More

NEKY Stacked Opportunities Rogersville Shale Berea Sandstone and More

NEKY Stacked Opportunities Rogersville Shale Berea Sandstone and More

The Emerging Rogersville Shale Play: Hurry up and Wait

The Emerging Rogersville Shale Play: Hurry up and Wait

The Emerging Rogersville Shale Play: Hurry up and Wait

Oklahoma Induced Earthquakes as seen from Northeastern Kentucky

Oklahoma Induced Earthquakes as seen from Northeastern Kentucky

Oklahoma Induced Earthquakes as seen from Northeastern Kentucky

Abstract structural and stratigraphic implications of the north bounding fau...

Abstract structural and stratigraphic implications of the north bounding fau...

Abstract structural and stratigraphic implications of the north bounding fau...

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Cimarex Energy's Walbridge 1-H First Successful Rogersville Shale Horizontal ...

Cimarex Energy's Walbridge 1-H First Successful Rogersville Shale Horizontal ...

Cimarex Energy's Walbridge 1-H First Successful Rogersville Shale Horizontal ...

Cimarex Energy's Bruin-Walbridge 1-H Horizontal Rogersville Shale Flow Back ...

Cimarex Energy's Bruin-Walbridge 1-H Horizontal Rogersville Shale Flow Back ...

Cimarex Energy's Bruin-Walbridge 1-H Horizontal Rogersville Shale Flow Back ...

Cimarex Energy's "Defined" Rogersville Shale Log Signature

Cimarex Energy's "Defined" Rogersville Shale Log Signature

Cimarex Energy's "Defined" Rogersville Shale Log Signature

Rogersville Shale Compostion Reading Between the Plates Maryville over Rome,...

Rogersville Shale Compostion Reading Between the Plates Maryville over Rome,...

Rogersville Shale Compostion Reading Between the Plates Maryville over Rome,...

New State Drilling Depth Record Reached in Lawrence County, Kentucky Geologic...

New State Drilling Depth Record Reached in Lawrence County, Kentucky Geologic...

New State Drilling Depth Record Reached in Lawrence County, Kentucky Geologic...

Evidence for a repeated section of the rutledge limestone in the chesapeake e...

Evidence for a repeated section of the rutledge limestone in the chesapeake e...

Evidence for a repeated section of the rutledge limestone in the chesapeake e...

Chesapeake Energy Rogersville Shale completion report

Chesapeake Energy Rogersville Shale completion report

Chesapeake Energy Rogersville Shale completion report

November 7 2016 m 5.0 Earthquake - 2km w of cushing, oklahoma

November 7 2016 m 5.0 Earthquake - 2km w of cushing, oklahoma

November 7 2016 m 5.0 Earthquake - 2km w of cushing, oklahoma

Rogersville Shale Maryville LS & SS New Cores Relative to IEP and CHK Contr...

Rogersville Shale Maryville LS & SS New Cores Relative to IEP and CHK Contr...

Rogersville Shale Maryville LS & SS New Cores Relative to IEP and CHK Contr...

Cimarex Energy's First Rogersville Shale Horizontal Deep Well the Walbridge 1...

Cimarex Energy's First Rogersville Shale Horizontal Deep Well the Walbridge 1...

Cimarex Energy's First Rogersville Shale Horizontal Deep Well the Walbridge 1...

NEKY Stacked Opportunities Rogersville Shale Berea Sandstone and More

NEKY Stacked Opportunities Rogersville Shale Berea Sandstone and More

NEKY Stacked Opportunities Rogersville Shale Berea Sandstone and More

The Emerging Rogersville Shale Play: Hurry up and Wait

The Emerging Rogersville Shale Play: Hurry up and Wait

The Emerging Rogersville Shale Play: Hurry up and Wait

Oklahoma Induced Earthquakes as seen from Northeastern Kentucky

Oklahoma Induced Earthquakes as seen from Northeastern Kentucky

Oklahoma Induced Earthquakes as seen from Northeastern Kentucky

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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

The presentation first gives the brief introduction about the animal communication covering the reasons for communication. It then describes the important types of animal communication emphasizing the important points regarding auditory and visual communication. With respect to auditory communication, it covers the uses of it and mechanisms of auditory communication along with examples. Later the presentation discusses the various forms of visual communication such as gestures, postures, facial expressions, color changes , bioluminescent communication. It then describes the visual communication in bees in the form of bee dance . In bee dance it gives a brief overview of round dance , sickle dance and waggle dance .

Animal Communication- Auditory and Visual.pptx

Animal Communication- Auditory and Visual.pptx

Animal Communication- Auditory and Visual.pptx

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Jupiter’s moon Io hosts extensive volcanism, driven by tidal heating. The isotopic composition of Io's inventory of volatile chemical elements, including sulfur and chlorine, reflects its outgassing and mass loss history, and thus records information about its evolution. We used millimeter observations of Io’s atmosphere to measure sulfur isotopes in gaseous SO2 and SO, and chlorine isotopes in gaseous NaCl and KCl. We find 34S/32S = 0.0595 ± 0.0038 (equivalent to δ34S = +347 ± 86‰), which is highly enriched compared to average Solar System values and indicates that Io has lost 94 to 99% of its available sulfur. Our measurement of 37Cl/35Cl = 0.403 ± 0.028 (δ37Cl = +263 ± 88‰) shows that chlorine is similarly enriched. These results indicate that Io has been volcanically active for most (or all) of its history, with potentially higher outgassing and mass-loss rates at earlier times.

Isotopic evidence of long-lived volcanism on Io

Isotopic evidence of long-lived volcanism on Io

Isotopic evidence of long-lived volcanism on Io

GBSN - Microbiology (Unit 1)

GBSN - Microbiology (Unit 1)

GBSN - Microbiology (Unit 1)

Green chemistry and Sustainable development.pptx

Green chemistry and Sustainable development.pptx

Green chemistry and Sustainable development.pptx

RajatChauhan518211

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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.

Botany 4th semester file By Sumit Kumar yadav.pdf

Botany 4th semester file By Sumit Kumar yadav.pdf

Botany 4th semester file By Sumit Kumar yadav.pdf

Sumit Kumar yadav

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

Biopesticide (2).pptx .This slides helps to know the different types of biop...

Biopesticide (2).pptx .This slides helps to know the different types of biop...

Biopesticide (2).pptx .This slides helps to know the different types of biop...

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Context. Determining the size distribution of asteroids is key to understanding the collisional history and evolution of the inner Solar System. Aims. We aim to improve our knowledge of the size distribution of small asteroids in the main belt by determining the parallaxes of newly detected asteroids in the Hubble Space Telescope (HST) archive and subsequently their absolute magnitudes and sizes. Methods. Asteroids appear as curved trails in HST images because of the parallax induced by the fast orbital motion of the spacecraft. Taking into account the trajectory of this latter, the parallax effect can be computed to obtain the distance to the asteroids by fitting simulated trajectories to the observed trails. Using distance, we can obtain the absolute magnitude of an object and an estimation of its size assuming an albedo value, along with some boundaries for its orbital parameters. Results. In this work, we analyse a set of 632 serendipitously imaged asteroids found in the ESA HST archive. Images were captured with the ACS/WFC and WFC3/UVIS instruments. A machine learning algorithm (trained with the results of a citizen science project) was used to detect objects in these images as part of a previous study. Our raw data consist of 1031 asteroid trails from unknown objects, not matching any entries in the Minor Planet Center (MPC) database using their coordinates and imaging time. We also found 670 trails from known objects (objects featuring matching entries in the MPC). After an accuracy assessment and filtering process, our analysed HST asteroid set consists of 454 unknown objects and 178 known objects. We obtain a sample dominated by potential main belt objects featuring absolute magnitudes (H) mostly between 15 and 22 mag. The absolute magnitude cumulative distribution logN(H > H0) ∝ αlog(H0) confirms the previously reported slope change for 15 < H < 18, from α ≈ 0.56 to α ≈ 0.26, maintained in our case down to absolute magnitudes of around H ≈ 20, and therefore expanding the previous result by approximately two magnitudes. Conclusions. HST archival observations can be used as an asteroid survey because the telescope pointings are statistically randomly oriented in the sky and cover long periods of time. They allow us to expand the current best samples of astronomical objects at no extra cost in regard to telescope time.

Hubble Asteroid Hunter III. Physical properties of newly found asteroids

Hubble Asteroid Hunter III. Physical properties of newly found asteroids

Hubble Asteroid Hunter III. Physical properties of newly found asteroids

Recombinant DNA technology (Immunological screening)

Recombinant DNA technology (Immunological screening)

Recombinant DNA technology (Immunological screening)

PraveenaKalaiselvan1

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

Botany 4th semester series (krishna).pdf

Sumit Kumar yadav

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

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

GBSN - Microbiology (Unit 2)

GBSN - Microbiology (Unit 2)

GBSN - Microbiology (Unit 2)

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

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

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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

Animal Communication- Auditory and Visual.pptx

Animal Communication- Auditory and Visual.pptx

Animal Communication- Auditory and Visual.pptx

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Isotopic evidence of long-lived volcanism on Io

Isotopic evidence of long-lived volcanism on Io

Isotopic evidence of long-lived volcanism on Io

GBSN - Microbiology (Unit 1)

GBSN - Microbiology (Unit 1)

GBSN - Microbiology (Unit 1)

Green chemistry and Sustainable development.pptx

Green chemistry and Sustainable development.pptx

Green chemistry and Sustainable development.pptx

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Botany 4th semester file By Sumit Kumar yadav.pdf

Botany 4th semester file By Sumit Kumar yadav.pdf

Botany 4th semester file By Sumit Kumar yadav.pdf

Pests of cotton_Sucking_Pests_Dr.UPR.pdf

Pests of cotton_Sucking_Pests_Dr.UPR.pdf

Pests of cotton_Sucking_Pests_Dr.UPR.pdf

Biopesticide (2).pptx .This slides helps to know the different types of biop...

Biopesticide (2).pptx .This slides helps to know the different types of biop...

Biopesticide (2).pptx .This slides helps to know the different types of biop...

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Hubble Asteroid Hunter III. Physical properties of newly found asteroids

Hubble Asteroid Hunter III. Physical properties of newly found asteroids

Hubble Asteroid Hunter III. Physical properties of newly found asteroids

Recombinant DNA technology (Immunological screening)

Recombinant DNA technology (Immunological screening)

Recombinant DNA technology (Immunological screening)

Botany 4th semester series (krishna).pdf

Botany 4th semester series (krishna).pdf

Botany 4th semester series (krishna).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

Disentangling the origin of chemical differences using GHOST

Disentangling the origin of chemical differences using GHOST

Disentangling the origin of chemical differences using GHOST

GBSN - Microbiology (Unit 2)

GBSN - Microbiology (Unit 2)

GBSN - Microbiology (Unit 2)

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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...

Southern California hit by 7.1 earthquake, as recorded by EK14 Microseismic station

1. Rush (EK14) < SAT 07/06/2019 > Go view HHN View HHE Back to Seismic Recordings RIGHT CLICK on the image to view a larger version * Select VIEW IMAGE from pop-up menu