5th International Conference on Aquaculture and Marine Biology.pdf

•

0 likes•3 views

Expand research Globally by attending the 5th International Conference on Aquaculture and Marine Biology is scheduled during April 28-29, 2023 https://conferencemind.com/conference/aquacultureandmarinebiology

Science

5TH INTERNATIONAL
CONFERENCE ON AQUACULTURE
AND MARINE BIOLOGY
+91-7735912022 contact@conferencemind.com
https://conferencemind.com/conference/aquacultureandmarinebiology
Kurcheti Pani Prasad
Principal Scientist
ICAR-Central Institute of
Fisheries Education, India
Keerthi Thalakattil Raghavan
Professor
Mahatma Gandhi University,
India
Rakesh Rahul Jadhav
Assistant Professor
Dr. B.S. Konkan Krishi
Vidyapeeth, India
Sandesh Vitthal Patil
Assistant Professor
College of Fisheries Ratnagiri,
Maharashtra, India
Suja Aarattuthodi
Research Professor
Delta Research and Extension Center,
Mississippi State University
USA
Mahadevan Ramanan
Director
Banaras Hindu University
Kanchipuram Campus, India
Phibi Philip Naduvathu
Assistant Professor
Tamil Nadu Dr J Jayalalithaa
Fisheries University, India
A. Devivaraprasad Reddy
Scientist
Dr YSR Horticultural University
Venkataramannagudem, India
Binay Kumar Chakraborty
Project Director
Project Director Department of
Fisheries, Bangladesh
Pavanasam Natarajan
Professor
Hawassa University, Ethiopia
G. Vidya Sagar Reddy
Professor & Head
Centurion University of Technology
and Management, India
C. Greg Lutz
Professor
Louisiana State University
United States
Jyoti Saroj
Assistant Professor
College of Fisheries, Acharya
Narendra Deva University of
Agriculture and Technology,
Ayodhya, Uttar Pradesh, India
Dr. Sumit Kumar
Research Associate
ICAR-Directorate of Coldwater Fisheries
Research, Bhimtal, Uttarakhand
India
Bhaskar Gaikwad
Scientist
National Institute of Abiotics
StressManagement
India
April 28-29, 2023
Renowned Speakers

Similar to 5th International Conference on Aquaculture and Marine Biology.pdf

The International Journal of Scientific & Innovative Research (IJSIR) is a bi-annual published on line/ offline journal which publishes innovative research papers, reviews, mini reviews, short communications and notes dealing with all branches of science, technology, engineering health and agriculture. All manuscripts are subject to rapid peer review, those of high quality (not previously published and not under consideration for publication in another journal) contributing significantly to further the scientific knowledge in science, technology, engineering, health and agriculture will be published without delay. The subjects will cover all the disciplines and branches of science, technology, engineering, health and agriculture.

International journal of scientific and innovative research 2015; 3(1)p issn ...

Sanjay Dixit

Curriculum Vitae

Ashok kumar sekar

05. research awards vdgood

Manu Mitra

Recent Advances in Biological Sciences

Dr. K. P. Senthilkumar Naidu

Dr KVS AD

kvvvorg

International journal of scientific and innovative research 2014; 2(2)p issn ...

Sanjay Dixit

Geriatric Care Clinic (GCC) is a pioneering attempt in SRMC to address the problems unique to the older adults, be it physical, psychological, or social, associated with aging. It is as a one-stop center for comprehensive care for individuals above the age of 50 in a multi-disciplinary setting. Any person above the age of 50 years can walk-in for the GCC expert consultation and opinion in an outpatient settingGCC has special focus on memory disorders like Alzheimer’s Dementia & other types of dementias, as well as Neuro-psychiatric manifestations of disorders like Parkinson’s Disease, Epilepsy, Stroke, Traumatic Brain Injury etc.

Elderly Depression Treatment | Old Age Neurological Problems | Functional Dif...

SRI RAMACHANDRA UNIVERSITY

2015 CV of Prof. BVV doc

Dr.Vidya Vardhini

2015 cv of prof. bvv doc

Dr.Vidya Vardhini

IJSIR Vol.5 Issue (ii)

Sanjay Dixit

International journal of scientific and innovative research 2015; 3(2)p issn ...

Sanjay Dixit

Academic Strength- PSN.pdf

Navaraj4

National Conference on Faunal Diversity

Dr.Ravindra Kshirsagar P.G Department of Zoology Modern College Ganeshkhind Pune

cv for job

2.Profile

20150107150528762

C V of Dr GLH

Akash Verma CV

Editorial board of journal of global innovations in agricultural and social s...

Jiban Shrestha

Applications of Statistics in Biological Sciences

RajaKrishnan M

Similar to 5th International Conference on Aquaculture and Marine Biology.pdf (20)

International journal of scientific and innovative research 2015; 3(1)p issn ...

Curriculum Vitae

05. research awards vdgood

Recent Advances in Biological Sciences

Dr KVS AD

International journal of scientific and innovative research 2014; 2(2)p issn ...

Elderly Depression Treatment | Old Age Neurological Problems | Functional Dif...

2015 CV of Prof. BVV doc

2015 cv of prof. bvv doc

IJSIR Vol.5 Issue (ii)

International journal of scientific and innovative research 2015; 3(2)p issn ...

Academic Strength- PSN.pdf

National Conference on Faunal Diversity

cv for job

2.Profile

20150107150528762

C V of Dr GLH

Akash Verma CV

Editorial board of journal of global innovations in agricultural and social s...

Applications of Statistics in Biological Sciences

Recently uploaded

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

On 26 January 2023, a military pilot reported four potential unidentified anomalous phenomena (UAP) while operating in the Eglin Air Force Base training range off the coast of Florida. Through the onboard radar system, the pilot initially observed that the four objects were aloft between 16,000 – 18,000 feet and appeared to be flying in formation. However the pilot observed only one of the four objects visually and captured two images of the single object via the aircraft’s electro-optical/infrared (EO/IR) sensor (see Figures 1A and 1B). The pilot could not record video of the event because the aircraft’s video recording equipment was inoperable prior to and during the aircraft’s flight. The pilot observed this single object aloft at 16,000 feet. The following case information is based on the pilot’s initial report and a subsequent discussion that AARO held with the pilot to seek additional details about the pilot’s observation of the reported object.

All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...

Sérgio Sacani

👉 𝑾𝑰𝑳𝑳 𝑷𝑹𝑶𝑽𝑰𝑫𝑬 𝒀𝑶𝑼 𝑾𝑰𝑻𝑯 𝑺𝑬𝑿𝒀 𝑴𝑶𝑫𝑬𝑳𝑺 𝑾𝑯𝑶 𝑾𝑰𝑳𝑳 𝑫𝑨𝑵𝑪𝑬 & 𝑫𝑹𝑰𝑵𝑲 𝑾𝑰𝑻𝑯 𝒀𝑶𝑼 𝑨𝑵𝑫 𝑨𝑳𝑺𝑶 𝑷𝑹𝑶𝑽𝑰𝑫𝑬 𝒀𝑶𝑼 𝑺𝑬𝑿𝑼𝑨𝑳 𝑩𝑶𝑫𝒀 𝑻𝑶 𝑩𝑶𝑫𝒀 𝑴𝑨𝑺𝑺𝑨𝑮𝑬 𝑾𝑰𝑻𝑯 𝑺𝑬𝑿. 👉𝒀𝑶𝑼 𝑴𝑨𝒀 𝑻𝑨𝑲𝑬 𝑻𝑯𝑬𝑴 𝑶𝑼𝑻 𝑭𝑶𝑹 𝑨 𝑷𝑨𝑹𝑻𝒀 𝑶𝑹 𝑨𝑳𝑺𝑶 𝑭𝑶𝑹 𝑨𝑵𝒀 𝑷𝑹𝑰𝑽𝑨𝑻𝑬 𝑷𝑨𝑹𝑻𝑰𝑬𝑺. 👉𝑻𝑯𝑬𝑺𝑬 𝑮𝑰𝑹𝑳𝑺 𝑨𝑹𝑬 𝑰𝑵𝑻𝑬𝑹𝑬𝑺𝑻𝑬𝑫 𝑰𝑵 𝑯𝑨𝑽𝑰𝑵𝑮 𝑺𝑶𝑴𝑬 𝑭𝑼𝑵 𝑾𝑰𝑻𝑯 𝒀𝑶𝑼 𝑨𝑵𝑫 𝑾𝑰𝑳𝑳 𝑬𝑵𝑺𝑼𝑹𝑬 𝑻𝑯𝑨𝑻 𝒀𝑶𝑼 𝑯𝑨𝑽𝑬 𝑪𝑶𝑴𝑷𝑳𝑬𝑻𝑬 𝑭𝑼𝑵. 28/April/2024 {{🎗️SCH🎗️}} 8923113531 How to book call girls The Booking process is particularly time-saving and more comfortable for us. Below mentioned are the steps you need to follow to hire our call girl: Step 1 - Visit our Call Girls Service website Step 2 - check for the portfolios of our sexy and hot call girls Step 3 - check on the services provided by the specific call girls Step 4 - Once you have selected the call girls and respective services, go to the contact us page. Step 5 - on the contact page, you will get our phone number, WhatsApp number, and email address. You can choose any one of them to connect with us. Call Us – 8923113531 ✣ ✤ ✥ ✦ 𝑻𝑰𝑴𝑬 𝑾𝑨𝑺𝑻𝑬𝑹𝑺 𝑨𝑵𝑫 𝑩𝑨𝑹𝑮𝑨𝑰𝑵𝑬𝑹𝑺 𝑨𝑹𝑬 𝑷𝑳𝑬𝑨𝑺𝑬 𝑬𝑿𝑪𝑼𝑺𝑬, 𝑾𝑬 𝑹𝑬𝑺𝑷𝑬𝑪𝑻 𝒀𝑶𝑼𝑹 𝑺𝑨𝑭𝑬𝑻𝒀 𝑨𝑵𝑫 𝑷𝑹𝑰𝑽𝑨𝑪𝒀 𝑨𝑵𝑫 𝑬𝑿𝑷𝑬𝑪𝑻 𝑻𝑯𝑬 𝑺𝑨𝑴𝑬 𝑭𝑹𝑶𝑴 𝒀𝑶𝑼.✣ ✤ ✥ ✦ Duration Normal Girls Housewives High-Profile Models (Celebrities) 1 Shot ₹ 8,000 ₹ 10,000 ₹ 15,000 2 Shots ₹ 15,000 ₹ 15,000 ₹ 25,000 Full Day ₹ 35,000 ₹ 35,000 ₹ 40,000 Full Night ₹ 40,000 ₹ 40,000 ₹ 50,000 Weekend ₹ 45,000 ₹ 45,000 ₹ 50,000 Party Nights ₹ 50,000 ₹ 50,000 ₹ 60,000

CALL ON ➥8923113531 🔝Call Girls Kesar Bagh Lucknow best Night Fun service 🪡

anilsa9823

GBSN - Microbiology (Unit 2)

Areesha Ahmad

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

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

Spermiogenesis or Spermateleosis or metamorphosis of spermatid

Sarthak Sekhar Mondal

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

Sérgio Sacani

BooK Now Call us at +918448380779 to hire a gorgeous and seductive call girl for sex. Take a Delhi Escort Service. The help of our escort agency is mostly meant for men who want sexual Indian Escorts In Delhi NCR. It should be noted that any impersonator will get 100 attention from our Young Girls Escorts in Delhi. They will assume the position of reliable allies. VIP Call Girl With Original Photos Book Tonight +918448380779 Our Cheap Price 1 Hour not available 2 Hours 5000 Full Night 8000 TAG: Call Girls in Delhi, Noida, Gurgaon, Ghaziabad, Connaught Place, Greater Kailash Delhi, Lajpat Nagar Delhi, Mayur Vihar Delhi, Chanakyapuri Delhi, New Friends Colony Delhi, Majnu Ka Tilla, Karol Bagh, Malviya Nagar, Saket, Khan Market, Noida Sector 18, Noida Sector 76, Noida Sector 51, Gurgaon Mg Road, Iffco Chowk Gurgaon, Rajiv Chowk Gurgaon All Delhi Ncr Free Home Deliver

Stunning ➥8448380779▻ Call Girls In Panchshil Enclave Delhi NCR

Delhi Call girls

Raman spectroscopy.pptx M Pharm, M Sc, Advanced Spectral Analysis

Diwakar Mishra

RecoveringancientrecordsofEarth'smagneticfieldisessentialfordeterminingtheroleofthemagnetosphereinprotectingearlyEarthfromcosmicradiationandatmosphericescape.WepresentpaleomagneticfieldtestshintingthatarecordofEarth's3.7‐billion‐year(Ga)oldmagneticfieldmaybepreservedinthenortheasternIsuaSupracrustalBeltasachemicalremanentmagnetizationacquiredduringamphibolite‐grademetamorphisminthebandedironformation.MultiplepetrologicalandgeochronologicallinesofevidenceindicatethatthenorthernmostpartofIsuahasnotexperiencedmetamorphictemperaturesexceeding380°CsincetheEoarchean,suggestingtherockshavenotbeensignificantlyheatedsincemagnetizationwasacquired.Weuse“pseudo”bakedcontacttests(intrusionsemplaced3.26–3.5Gaago)andafoldtest(folding3.6Gaago)todemonstratethatsomesamplespreserveaca.3.7Garecordofthemagneticfield.Werecoverafieldstrengthof>15μT.ThissuggeststhatEarth'smagneticfieldmayhavebeenweakenoughtoenhanceatmosphericescapeduringtheArchean

PossibleEoarcheanRecordsoftheGeomagneticFieldPreservedintheIsuaSupracrustalBe...

Sérgio Sacani

Botany krishna series 2nd semester Only Mcq type questions

Sumit Kumar yadav

Physiochemical properties of nanomaterials and its nanotoxicity.pptx

AArockiyaNisha

Just Call Vip call girls Srinagar Jammu Kashmir Escorts ☎️ 8617697112 Starting From 5K to 15K High Profile Escorts In Srinagar Jammu Kashmir ❤Personal Whatsapp Number Jammu Kashmir Call Girls 8617697112 💦✅. There are a number of Srinagar Jammu Kashmir Escorts willing to meet you at an affordable rate, which also possesses high moral standards and humanitarian tendencies. These girls can help satisfy the sexual desires of clients without fail; it is therefore essential that clients select an established service. Our services feature various packages at competitive rates: One shot: ₹2000/in-call, ₹5000/out-call Two shots with one girl: ₹3500/in-call, ₹6000/out-call Body to body massage with sex: ₹3000/in-call Full night for one person: ₹7000/in-call, ₹10000/out-call

❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.

Nitya salvi

Biological Classification BioHack (3).pdf

muntazimhurra

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

Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Available Now New Year Offer Best Call Girl Site Lucknow Call Us – 8923113531 ★ *Doggie (Sex style from behind)* ★ *Duo (Sex with two *escorts; Threesome with the client)* ★ *S-GFE *(*Special Girl Friend Experience*)* ★ *HJ (*Hand Job*) ★ *Special Massage* ★ *O-Level* *(*Oral sex*)* ★ *Tour (Internationaly*) ★ *sex)* ★ *BJ (Blowjob With Condom*) ★ *GFE (Girl Friend Experience*) ★ *CBJ (Covered Blow Job; Oral sex with a condom) Full on escorts Service by High Profile 28/April/2024 {{🎗️SCH🎗️}} 8923113531

Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...

anilsa9823

Past civilisations have nurtured small populations of those trying to understand and manipulate nature to some advantage in materials, tools, weapons, food, and wealth. However, they never formed communities and lacked the means of recording, communicating, and sharing successes and failures. They also lacked a common framework/philosophy to qualify them as scientists, but that all began to change in the 16th Century. In this lecture we consider the progression to a philosophy of science, and the underlying principles and assumptions that now guide scientific inquiry.We also examines the nature of scientific knowledge, the methods of acquisition, evolution, and significance over past centuries, and reflect on the value to society. In the struggle to solve problems, deliver understanding, and reveal the truth about our universe, science had to suffer and survive: ignorance, bigotry, established superstitions, and the ‘diktats’ of religions and politics, and latterly, falling education standards mired by social media. We chart that ‘scientific’ journey emphasising the importance of observation, experimentation, and the search for universal laws. Ultimately, this essentially Aristotelian perspective was challenged and overtaken by the rise of empiricism, which emphasised the importance of sensory experience and the limitations of human knowledge. Science continues to evolve and provide us with the best truths attainable with our leading edge technologies of observation and experimentation. Today, it stands as the greatest and richest contributor to human knowledge, understanding, progress, and wellbeing. In turn, debates and controversies are ongoing, shaping the field and philosophy which remains essential for understanding the nature of scientific knowledge and the models it creates. But unlike any belief system, the answers and models furnishers by science are not certain and invariant, they tend to be stochastic and incomplete - ‘the best we can do’ at a given time.

The Philosophy of Science

University of Hertfordshire

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...

Sérgio Sacani

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

sakshisoni2385

Recently uploaded (20)

Formation of low mass protostars and their circumstellar disks

All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...

CALL ON ➥8923113531 🔝Call Girls Kesar Bagh Lucknow best Night Fun service 🪡

GBSN - Microbiology (Unit 2)

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

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

Spermiogenesis or Spermateleosis or metamorphosis of spermatid

Isotopic evidence of long-lived volcanism on Io

Stunning ➥8448380779▻ Call Girls In Panchshil Enclave Delhi NCR

Raman spectroscopy.pptx M Pharm, M Sc, Advanced Spectral Analysis

PossibleEoarcheanRecordsoftheGeomagneticFieldPreservedintheIsuaSupracrustalBe...

Botany krishna series 2nd semester Only Mcq type questions

Physiochemical properties of nanomaterials and its nanotoxicity.pptx

❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.

Biological Classification BioHack (3).pdf

Botany 4th semester file By Sumit Kumar yadav.pdf

Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...

The Philosophy of Science

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

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

5th International Conference on Aquaculture and Marine Biology.pdf

1. 5TH INTERNATIONAL CONFERENCE ON AQUACULTURE AND MARINE BIOLOGY +91-7735912022 contact@conferencemind.com https://conferencemind.com/conference/aquacultureandmarinebiology Kurcheti Pani Prasad Principal Scientist ICAR-Central Institute of Fisheries Education, India Keerthi Thalakattil Raghavan Professor Mahatma Gandhi University, India Rakesh Rahul Jadhav Assistant Professor Dr. B.S. Konkan Krishi Vidyapeeth, India Sandesh Vitthal Patil Assistant Professor College of Fisheries Ratnagiri, Maharashtra, India Suja Aarattuthodi Research Professor Delta Research and Extension Center, Mississippi State University USA Mahadevan Ramanan Director Banaras Hindu University Kanchipuram Campus, India Phibi Philip Naduvathu Assistant Professor Tamil Nadu Dr J Jayalalithaa Fisheries University, India A. Devivaraprasad Reddy Scientist Dr YSR Horticultural University Venkataramannagudem, India Binay Kumar Chakraborty Project Director Project Director Department of Fisheries, Bangladesh Pavanasam Natarajan Professor Hawassa University, Ethiopia G. Vidya Sagar Reddy Professor & Head Centurion University of Technology and Management, India C. Greg Lutz Professor Louisiana State University United States Jyoti Saroj Assistant Professor College of Fisheries, Acharya Narendra Deva University of Agriculture and Technology, Ayodhya, Uttar Pradesh, India Dr. Sumit Kumar Research Associate ICAR-Directorate of Coldwater Fisheries Research, Bhimtal, Uttarakhand India Bhaskar Gaikwad Scientist National Institute of Abiotics StressManagement India April 28-29, 2023 Renowned Speakers

5th International Conference on Aquaculture and Marine Biology.pdf

Recommended

Recommended

More Related Content

Similar to 5th International Conference on Aquaculture and Marine Biology.pdf

Similar to 5th International Conference on Aquaculture and Marine Biology.pdf (20)

Recently uploaded

Recently uploaded (20)

5th International Conference on Aquaculture and Marine Biology.pdf