symbols

•Download as DOCX, PDF•

0 likes•168 views

Kavi Kuyil

symbols

Science

Viewers also liked

Adab keluarga

sitinadiahihsan

ev75y.odt

Jeff Smith

Day one

Anthony Michael Loveday

Pauta para la producción de la exposición lectora, 8º Quiroz

Lissette Mella H.

fsnqj.pdf

Jeff Smith

Latihan Adab Bergaul Dengan Keluarga

Nik Faeez

Sílabo tarea 2 parte inicial Dr. iván pimienta

Universidad de los Andes

Tuesday assure

DB_Francisco

thjo2.pdf

Jeff Smith

Viewers also liked (9)

Adab keluarga

ev75y.odt

Day one

Pauta para la producción de la exposición lectora, 8º Quiroz

fsnqj.pdf

Latihan Adab Bergaul Dengan Keluarga

Sílabo tarea 2 parte inicial Dr. iván pimienta

Tuesday assure

thjo2.pdf

Recently uploaded

low price Call me 7857803690 100%genuine sexy VIP call girl safe service WhatsApp chat. 785780369 Normal call kijiye 7857803690 100% genuine young college girl and housewife Full enjoy open minded girl provide 24hour full cooperative model and full satisfactions☎️*78578//03690*⭐Escorts service █▬█⓿▀█▀ call girls and bhabhi available for room Sex and video call service A-1 HIGH CLASS CALL GIRLS TOP MODEL 24X7 HOME/HOTEL Call Girls Safe & Secure High Class Sm Affordable Rate 100% Satisfaction, Unlimited Enjoyment. Any Time for Model/Escort in High class luxury and premium

SAMASTIPUR CALL GIRL 7857803690 LOW PRICE ESCORT SERVICE

ayushi9330

(Vivek)Call Us, 8448380779,Call girls in Delhi NCr – We Offer best in class call girls. escort Service At Affordable Price At low Rate with Space Night 8000 We Are One Of The Oldest Escort and Call girls Agencies in Delhi. You Will Find That Our Female Escorts Are Full Of Fun, Sexy And They Would Love Enjoy Your Company. We Have A Fantastic Selection Of Escort Ladies Available For In-Calls As Well As Out-Calls. Our Escorts Are Not Only Beautiful But All Have Great Personalities Making Them The Perfect Companion For Any Occasion. In-Call:- You Can Come At Our Place in Delhi Our place Which Is Very Clean Hygienic 100% safe Accommodation. Out-Call:- You have To Come Pick The Girl From My Place We Are Also Provide Door Step Services (Delhi Ncr, Noida, Gurgaon, Faridabad, Ghaziabad Note:- Pic Collectors Time Passers Bargainers Stay Away As We Respect The Value For Your Money Time And Expect The Same From You Hygienic:- Full Ac room And Clean Rooms Available In Hotel 24 * 7 Hourly In Delhi NCR More Details, With WhatsApp Number, +91-8448380779

Connaught Place, Delhi Call girls :8448380779 Model Escorts | 100% verified

Delhi Call girls

American Type Culture Collection (ATCC).pptx

abhishekdhamu51

Clean In Place(CIP).pptx .

Poonam Aher Patil

Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency

Sheetal Arora

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

PirithiRaju

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

PirithiRaju

Seismic Method Estimate velocity from seismic data.pptx

AlMamun560346

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

Sérgio Sacani

GBSN - Microbiology (Unit 3)

Areesha Ahmad

Site Acceptance Test .

Poonam Aher Patil

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

Sumit Kumar yadav

Understanding circumstellar disks is of prime importance in astrophysics, however, their birth process remains poorly constrained due to observational and numerical challenges. Recent numerical works have shown that the small-scale physics, often wrapped into a sub-grid model, play a crucial role in disk formation and evolution. This calls for a combined approach in which both the protostar and circumstellar disk are studied in concert. Aims. We aim to elucidate the small scale physics and constrain sub-grid parameters commonly chosen in the literature by resolving the star-disk interaction. Methods. We carry out a set of very high resolution 3D radiative-hydrodynamics simulations that self-consistently describe the collapse of a turbulent dense molecular cloud core to stellar densities. We study the birth of the protostar, the circumstellar disk, and its early evolution (< 6 yr after protostellar formation). Results. Following the second gravitational collapse, the nascent protostar quickly reaches breakup velocity and sheds its surface material, thus forming a hot (∼ 103 K), dense, and highly flared circumstellar disk. The protostar is embedded within the disk, such that material can flow without crossing any shock fronts. The circumstellar disk mass quickly exceeds that of the protostar, and its kinematics are dominated by self-gravity. Accretion onto the disk is highly anisotropic, and accretion onto the protostar mainly occurs through material that slides on the disk surface. The polar mass flux is negligible in comparison. The radiative behavior also displays a strong anisotropy, as the polar accretion shock is shown to be supercritical whereas its equatorial counterpart is subcritical. We also f ind a remarkable convergence of our results with respect to initial conditions. Conclusions. These results reveal the structure and kinematics in the smallest spatial scales relevant to protostellar and circumstellar disk evolution. They can be used to describe accretion onto regions commonly described by sub-grid models in simulations studying larger scale physics.

Formation of low mass protostars and their circumstellar disks

Sérgio Sacani

99992-vip-66834 📞Noida Sector 22 Noida Low price 100% genuine sexy VIP call girls are provided safe and secure service .call 📞,,24 hours 🕰️-- ✅100% gesnuine young RIYA SERVICE COMPANY ✔✔✔ ★ A-Level (5 star ) ★ Strip-tease ★ BBBJ (Bareback Blowjob) Receive advanced sexual techniques in different mode make their life more pleasurable. ★ Spending time in hotel rooms ★ BJ (Blowjob Without a Condom) ★ Completion (Oral to completion) ★ Covered (Covered blowjob Without a Condom) ★ DATING (Dinner At Night) ★ DSL (Dick Sucking Lips) ★ DT (Dining at the Toes English Spanking) ★ Doggie (Sex style from behind) ★ Duo (shot with two escorts; Threesome with the client) ★ S-GFE (Special Girl Friend Experience) ★ HJ (Hand Job) ★ Special Massage ★ O-Level (Oral sex) ★ Tour (International) ★ 69 (69 sex) ★ BJ (Blowjob With Condom) ★ GFE (Girl Friend Experience) ★ CBJ (Covered Blow Job; Oral sex with a condom _ LOW PRICE V I P MODEL FULL SAFE AND SECURE CALL MExxxs CALL ME

9999266834 Call Girls In Noida Sector 22 (Delhi) Call Girl Service

nishacall1

Proteomics: types, protein profiling steps etc.

Silpa

Call Girls In Safdarung Enclave Arjun Nagar Whatsapp +91 9654467111 Delhi ⛟ Open 24 Hrs, ☎ Booking Short 2000 Night 6000 ALL HOME/HOTEL SERVICE DOORSTEP SERVICE IN/CALL & OUT/CALL SERVICE WITH MANY OPTIONS AVAILABLE DELHI GURGAON & NOIDA SERVICE IN REASONABLE RATES FROM LOW TO HIGH PROFILE STAFF’S. Call Girl Number~24X7~Call Girl Services, New Delhi, Delhi OutCall Rate Call Girl Mahipalpur,Call Girl Connaught Place,Call Girl Nehru Place,Call Girl Chanakyapuri,Call Girl Paharganj,Call Girl Dhaula Kuan,Call Girl Moti Bagh,Call Girl Karol Bagh,Call Girl Greater Kailash,Call Girl Naraina, Call Girl Katwaria Sarai,Call Girl Janakpuri,Call Girl Kalkaji,Call Girl Lajpat Nagar,Call Girl Palam,Call Girl Malviya Nagar,Call Girl Mehrauli,Call Girl Govindpuri,Call Girl Sarojini Nagar ,Call Girl Neb Sarai,Call Girl South Ex,Call Girl Munirka,Call Girl Saket,Call Girl Chattarpur

9654467111 Call Girls In Raj Nagar Delhi Short 1500 Night 6000

Sapana Sha

Conjugation, transduction and transformation

Areesha Ahmad

Justdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts Service Best High Class call girls Service Escorts Service in Home Hotel in Delhi NCR 24 Hours Available Service. We provide Super Class Hot and Sexy Indian Female Escorts Service, A to Z Body and Mind Satisfaction by Top Class Female Models in Delhi Gurgaon Noida NCR in Hotel 24hrs In Call and Out Call Service At Lowest Price. We Have Indian Punjabi Kashmiri Northeast Every Type Sexy Bold Beautiful Young Soft Cute Charming Female Escorts Available. Hygienic Full AC Neat and Clean Rooms Avail. In Hotel 24hrs in Delhi NCR

Justdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts Service

monikaservice1

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

Sérgio Sacani

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

Sumit Kumar yadav

Recently uploaded (20)

SAMASTIPUR CALL GIRL 7857803690 LOW PRICE ESCORT SERVICE

Connaught Place, Delhi Call girls :8448380779 Model Escorts | 100% verified

American Type Culture Collection (ATCC).pptx

Clean In Place(CIP).pptx .

Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency

Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf

Pests of mustard_Identification_Management_Dr.UPR.pdf

Seismic Method Estimate velocity from seismic data.pptx

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

GBSN - Microbiology (Unit 3)

Site Acceptance Test .

Botany 4th semester series (krishna).pdf

Formation of low mass protostars and their circumstellar disks

9999266834 Call Girls In Noida Sector 22 (Delhi) Call Girl Service

Proteomics: types, protein profiling steps etc.

9654467111 Call Girls In Raj Nagar Delhi Short 1500 Night 6000

Conjugation, transduction and transformation

Justdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts Service

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

Botany 4th semester file By Sumit Kumar yadav.pdf

symbols

Recommended

Recommended

More Related Content

Viewers also liked

Viewers also liked (9)

More from Kavi Kuyil

More from Kavi Kuyil (10)

Recently uploaded

Recently uploaded (20)