lecture 3/2023-Respiratory Physiology - compliance I.pdf

Overview: In this lecture, we will discuss the physiology of the respiratory system. We intend this lecture to students who are studying physiology, PS 141 at the medical school university of Tripoli. We will begin by defining respiration and discussing its stages. Then, we will examine the structure of the respiratory system, including the conducting part and respiratory part. Finally, we will explore the function of the respiratory system and how it relates to gas exchange and maintaining homeostasis. By the end of this lecture, you will have a solid understanding of the physiology of the respiratory system, including the role of respiration in maintaining homeostasis and the structure and function of the respiratory system. Recommended Readings: • Department: Lecture Notes in Medical Physiology • Mohd Noor, Noriah (2015) Illustrated human physiology. Pearson Malaysia Sdn. Bhd., Kuala Lumpur. ISBN 9789673496426 • Guyton & Hall, Textbook of Medical Physiology, 13rd Edition, 2016 • William F. Ganong, Review of Medical physiology, 26th Edition, 2019

10th Marksheet

CA Kishan Vaidya

Physiology of Respiratory System: Introduction

Asma Ben Hameid

Para 05 (Misbah Ul Quran)

Adeel Ahmad Munir Ahmad

PEADIATRICS (DIMS NOTES).pdf

7-LIVER_AND_GIT (DIMS NOTES).pdf

Caller To Islam / الداعية الإسلامي

Quran with Tajwid Surah 88 ﴾القرآن سورۃ الغاشية﴿ Al-Ghashiya 🙪 PDF

Quran with Tajwid Surah 21 ﴾القرآن سورۃ الأنبياء﴿ Al-Anbiya' 🙪 PDF

Caller To Islam / الداعية الإسلامي

lecture 3/2022 Special senses - Vision 3- Physiology of vision- Photo transd...

MICROBIOLOGY (DIMS NOTES).pdf

Afferent impulses to respiratory center from higher centers. Afferent impulses to respiratory center from non-chemical receptors Pulmonary stretch receptors (Hering–Breuer inflation reflex) J-receptors Irritant receptors in respiratory tract – a. Cough reflex b. Sneezing reflex c. Hering–Breuer deflation reflex d. Deglutition reflex Proprioceptors Chest wall stretch receptors Baroreceptors Thermoreceptors Coronary chemoreceptor

Voluntary control of respiration, respiratory reflexes

3-CARDIOLOGY (DIMS NOTES).pdf

Lecture 3 / 2022 General Physiology II- Inter cellular junctions

SURGICAL ANATOMY (DIMS NOTES).pdf

ENDOCRINE SYSTEM (DIMS NOTES).pdf

Zagor ZS KA COL 113 - Poslednji Viking

Broj Jedan

Respiratory System Review Questions for 1 st year MBBS

BIOCHEMISTRY Notes (DIMS).pdf

Surah al Jinn

Azaakhaana

Frank Starling

Richin Koshy

Tendances (20)

HISTOLOGY, EMBRYOLOGY (DIMS NOTES).pdf

10th Marksheet

Physiology of Respiratory System: Introduction

Para 05 (Misbah Ul Quran)

PEADIATRICS (DIMS NOTES).pdf

7-LIVER_AND_GIT (DIMS NOTES).pdf

Quran with Tajwid Surah 88 ﴾القرآن سورۃ الغاشية﴿ Al-Ghashiya 🙪 PDF

Quran with Tajwid Surah 21 ﴾القرآن سورۃ الأنبياء﴿ Al-Anbiya' 🙪 PDF

lecture 3/2022 Special senses - Vision 3- Physiology of vision- Photo transd...

MICROBIOLOGY (DIMS NOTES).pdf

Voluntary control of respiration, respiratory reflexes

3-CARDIOLOGY (DIMS NOTES).pdf

Lecture 3 / 2022 General Physiology II- Inter cellular junctions

SURGICAL ANATOMY (DIMS NOTES).pdf

ENDOCRINE SYSTEM (DIMS NOTES).pdf

Zagor ZS KA COL 113 - Poslednji Viking

Respiratory System Review Questions for 1 st year MBBS

BIOCHEMISTRY Notes (DIMS).pdf

Surah al Jinn

Frank Starling

Plus de Charushila Rukadikar

Lecture 10/2023 Respiratory Physiology : transport of oxygen II.pdf

lecture 9/ 2023 -Respiratory Physiology - transport of oxygen I.pdf

lecture 4/2023 -Respiratory Physiology - compliance II.pdf

Lecture 1/2022 General physiology I -Cell - nucleus and cytoplasm-

Lecture 2/2022 General Physiology II - Cell membrane

Lecture 6/2022 Special senses -Vision 6 - Physiology of vision -Visual cort...

Lecture 7/2022 , Special senses -Vision 7 -Physiology of vision -Visual perc...

Lecture 5/2022 Special senses -Vision 5 -Physiology of vision - Visual pathway

Lecture 4/2022 Special senses -Vision 4 -Physiology of vision - Processing o...

Lecture 2/2022 Special senses -Vision 2 -Physiology of vision – Retina, Photo...

Lecture 1/2022 Special senses , Vision 1- Basics of vision, Optics of the eye...

Lecture 8 /2022 Special senses: Taste

Lecture 9 /2022 , Special senses- Smell

Lecture 10 /2022 pecial sences Ear - Auditory pathway

Pain

Descending tracts- Central Nervous System

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 .

Ascending tracts- Central Nervous System

Receptor II

Receptor 1

Reflex

Plus de Charushila Rukadikar (20)

Lecture 10/2023 Respiratory Physiology : transport of oxygen II.pdf

lecture 9/ 2023 -Respiratory Physiology - transport of oxygen I.pdf

lecture 4/2023 -Respiratory Physiology - compliance II.pdf

Lecture 1/2022 General physiology I -Cell - nucleus and cytoplasm-

Lecture 2/2022 General Physiology II - Cell membrane

Lecture 6/2022 Special senses -Vision 6 - Physiology of vision -Visual cort...

Lecture 7/2022 , Special senses -Vision 7 -Physiology of vision -Visual perc...

Lecture 5/2022 Special senses -Vision 5 -Physiology of vision - Visual pathway

Lecture 4/2022 Special senses -Vision 4 -Physiology of vision - Processing o...

Lecture 2/2022 Special senses -Vision 2 -Physiology of vision – Retina, Photo...

Lecture 1/2022 Special senses , Vision 1- Basics of vision, Optics of the eye...

Lecture 8 /2022 Special senses: Taste

Lecture 9 /2022 , Special senses- Smell

Lecture 10 /2022 pecial sences Ear - Auditory pathway

Pain

Descending tracts- Central Nervous System

Ascending tracts- Central Nervous System

Receptor II

Receptor 1

Reflex

Dernier

Animal Communication- Auditory and Visual.pptx

UmerFayaz5

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

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.

Zoology 4th semester series (krishna).pdf

Sumit Kumar yadav

Botany 4th semester file By Sumit Kumar yadav.pdf

Sumit Kumar yadav

Chemical Tests; flame test, positive and negative ions test Edexcel Internati...

ssuser79fe74

Bacterial Identification and Classifications

Areesha Ahmad

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

GBSN - Microbiology (Unit 2)

Areesha Ahmad

Small size (20-300 nm) / bacteria (size measured in μm) Viral genome – single type of nucleic acid: DNA – dezoxyriboviruses RNA - riboviruses Totally dependant on living cells for all metabolic processes May infect humans, animals, plants, bacteria, fungi,parasites, insects Virion = viral corpuscle = elementary, infectious unit. Only visible by electron microscopy. Laboratory diagnosis of viral infections Methods: • Cytology • Electron microscopy • Cultivation • Detection of viral proteins • Serology • Molecular diagnosis (detection of genetic material i.e. nucleic acids) PPT prepared by Dr. Prince C P

VIRUSES structure and classification ppt by Dr.Prince C P

PRINCE C P

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

ssifa0344

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

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Monika Rani

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...

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

Sumit Kumar yadav

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