The blackbody is a hollow enclosure with a pinhole to emit its radiations. The secure covering of the blackbody prevents the absorbed light from escaping.
A blackbody is a solid closed unreal body that is inexistent. But lamp black, platinum black, and graphite-coated surfaces are non-ideal black bodies for laboratory purposes. An object with above 0.95 emissivities is an approximate blackbody. Besides, the hotter bodies emitting electromagnetic radiation under thermal equilibrium conditions are also considered partial black bodies.
It is a PowerPoint presentation of Kirchhoff's law of thermal radiation. And it gives a brief idea of Kirchhoff's law, its applications, and examples. Moreover, it explains the terms absorptivity, emissive power, thermal equilibrium, and emissivity.
It discusses Kirchhoff's law and its examples. It explains blackbody emissions in thermal equilibrium conditions.
We are sorry to inform you about a small error in Kirchhoff's formula section of the above infographic. Kirchhoff's formula states that the absorptivity and emissivity of the body are equal in thermal equilibrium conditions. 'a' is the absorbing power of the body at a wavelength λ. And 'e' is the emissivity of the body at the same wavelength. So, we will write aλ=e but not aλ=eλ. We request you read it correctly while going through the PDF.
An ideal black body is an imaginary perception of Gustav Kirchhoff that played a significant role in the development of quantum mechanics. Every object in the universe absorbs and emits electromagnetic energy to a certain extent under favorable conditions. But a black body absorbs all the electromagnetic radiation falling on it without limit from all directions. Consequently, it is black.
It is a PowerPoint presentation of Kirchhoff's law of thermal radiation. And it gives a brief idea of Kirchhoff's law, its applications, and examples. Moreover, it explains the terms absorptivity, emissive power, thermal equilibrium, and emissivity.
It discusses Kirchhoff's law and its examples. It explains blackbody emissions in thermal equilibrium conditions.
We are sorry to inform you about a small error in Kirchhoff's formula section of the above infographic. Kirchhoff's formula states that the absorptivity and emissivity of the body are equal in thermal equilibrium conditions. 'a' is the absorbing power of the body at a wavelength λ. And 'e' is the emissivity of the body at the same wavelength. So, we will write aλ=e but not aλ=eλ. We request you read it correctly while going through the PDF.
An ideal black body is an imaginary perception of Gustav Kirchhoff that played a significant role in the development of quantum mechanics. Every object in the universe absorbs and emits electromagnetic energy to a certain extent under favorable conditions. But a black body absorbs all the electromagnetic radiation falling on it without limit from all directions. Consequently, it is black.
Here, Modern Physics is explained very shortly and simply to make people understand that Physics is a very interesting subject to learn and modern physics is more interesting.
Absorptivity
Reflectivity
Transmissivity
Emissivity
Grey Body
Black Body
Laws of black body radiation
Stefan-Boltzmann law
Planck’s Law
Wiens Displacement law
Conclusion
Heat transfer due to emission of electromagnetic waves is known as thermal radiation. Heat transfer through radiation takes place in form of electromagnetic waves mainly in the infrared region. Radiation emitted by a body is a consequence of thermal agitation of its composing molecules. The underlying mechanisms and the concepts involved are discussed in the ppt
Relation between a small body in a large enclosureSharath Kumar
Here in this presentation we will be discussing about Relation between a small body in a large enclosure, planks law, properties on a surface, absurdity, reflexivity, radiosity, intensity of radiation and emitted radiation
If everyone is thinking alike, we cannot solve the hurdles of a problem. It seems true if we observe these hypotheses' hierarchy once. Italian physicist Francesco Maria Grimaldi discovered the wave phenomenon of light in 1665. But the uncertainty about light's nature was finally solved by Einstein's explanation of the photoelectric effect. Similarly, Neil Bohr succeeded in describing the structure of an atom with quantized electron orbits. But his stipulation of allowed stationary orbits was only a supposition until the discovery of the de-Broglie equation.
Louis de-Broglie, a French physicist, presumed that moving microscopic and macroscopic objects are waves. He introduced a word called 'matter wave' to describe the waves of material objects in motion. As a result, matter exhibits a dual character of both particle and wave. Moreover, he derived an empirical formula to measure the wavelength of matter waves in 1923 called the de-Broglie equation.
It is a graphical explanation of a blackbody's emissive power and radiation wavelength at various temperatures. We know blackbody emissions are temperature specific. And a blackbody graph is an overall variation of a blackbody's emissive power as a function of wavelength measured at different temperatures. But the Wien displacement law graph focuses on spectral intensities of blackbody emissions as a function of wavelength at a peak wavelength state λmax at a specific temperature T.
Here, Modern Physics is explained very shortly and simply to make people understand that Physics is a very interesting subject to learn and modern physics is more interesting.
Absorptivity
Reflectivity
Transmissivity
Emissivity
Grey Body
Black Body
Laws of black body radiation
Stefan-Boltzmann law
Planck’s Law
Wiens Displacement law
Conclusion
Heat transfer due to emission of electromagnetic waves is known as thermal radiation. Heat transfer through radiation takes place in form of electromagnetic waves mainly in the infrared region. Radiation emitted by a body is a consequence of thermal agitation of its composing molecules. The underlying mechanisms and the concepts involved are discussed in the ppt
Relation between a small body in a large enclosureSharath Kumar
Here in this presentation we will be discussing about Relation between a small body in a large enclosure, planks law, properties on a surface, absurdity, reflexivity, radiosity, intensity of radiation and emitted radiation
If everyone is thinking alike, we cannot solve the hurdles of a problem. It seems true if we observe these hypotheses' hierarchy once. Italian physicist Francesco Maria Grimaldi discovered the wave phenomenon of light in 1665. But the uncertainty about light's nature was finally solved by Einstein's explanation of the photoelectric effect. Similarly, Neil Bohr succeeded in describing the structure of an atom with quantized electron orbits. But his stipulation of allowed stationary orbits was only a supposition until the discovery of the de-Broglie equation.
Louis de-Broglie, a French physicist, presumed that moving microscopic and macroscopic objects are waves. He introduced a word called 'matter wave' to describe the waves of material objects in motion. As a result, matter exhibits a dual character of both particle and wave. Moreover, he derived an empirical formula to measure the wavelength of matter waves in 1923 called the de-Broglie equation.
It is a graphical explanation of a blackbody's emissive power and radiation wavelength at various temperatures. We know blackbody emissions are temperature specific. And a blackbody graph is an overall variation of a blackbody's emissive power as a function of wavelength measured at different temperatures. But the Wien displacement law graph focuses on spectral intensities of blackbody emissions as a function of wavelength at a peak wavelength state λmax at a specific temperature T.
MCQs of blackbody & its radiation .pdfSaiKalyani11
It is an e-book of MCQs & answers on blackbody. It is in PowerPoint format with 40 questions and detailed answer explanation that makes you clear every single point of blackbody and its radiation. The e-book has 54 beautifully designed slides. The contents of the e-book are below.
Multiple choice questions and answers - 20 no.s
True or false questions-10 no.s
Reasoning questions - 10 no.s
To disclose all the contents of the e-book, visit this link.
https://kameswariservices201831.myinstamojo.com/product/3556812/mcqs-answers-of-blackbody-and-its-radiation
It discusses Wien displacement law. To go through the numerical problems of the Wien displacement law topic, visit our e-book at;
https://kameswariservices201831.myinstamojo.com/product/3493453/numerical-problems-on-wien-displacement-law-
MCQs of blackbody & Kirchhoff's law.pdfSaiKalyani11
It is a PowerPoint presentation on multiple choice questions and answers on Blackbody & Kirchhoff's law topics. It discusses all practical examples and numerical problems of the said concepts.
This PowerPoint presentation explains Planck's quantum theory and Planck's constant topics briefly. It is now available on Instamojo for just Rs.10/-. Save a personalized copy of this presentation by visiting Instamojo. The link is below.
https://kameswariservices201831.myinstamojo.com/product/3439450/planck-quantum-theory-postulates
Kirchhoff's law formula and its derivation. Numerical problems.pdfSaiKalyani11
It discusses Kirchhoff's formula and its derivation. And it includes numerical problems of Kirchhoff's law. For a colorful e-book for only 10/- rupees on Kirchhoff's law, visit our store at;
https://kameswariservices201831.myinstamojo.com/product/3467221/kirchhoffs-law-of-thermal-radiations
It describes the definition of Planck's constant. Planck constant helps compute the discrete energy changes of a body by relating to the frequency of the photon. Planck constant explains the proportionality relationship between the photon's energy and the frequency.
For more information on this topic, kindly visit our blog article at;
https://jayamchemistrylearners.blogspot.com/2022/08/plancks-constant-chemistry-learners.html
Numerical problems of Planck's quantum theory.pdfSaiKalyani11
It is a PowerPoint presentation on numerical problems of Planck quantum theory topic.
It includes 12 numerical problems with solved answers. Besides, this PowerPoint presentation has a mind map to remember all formulas of Planck quantum law.
The Rydberg formula helps to determine the wavenumber or wavelengths of hydrogen spectral lines obtained in the hydrogen spectrum. Previously, Johann Jakob Balmer discovered an empirical formula to determine the wavelengths of hydrogen spectral lines obtained in the visible region of the hydrogen spectrum. As we all know, the hydrogen spectrum is not limited to the visible zone only. It occupies the ultraviolet and infrared parts of the electromagnetic spectrum also. Hence, the scientists' quests to determine the spectral positions of various spectral lines of the hydrogen spectrum finally came to an end with the Rydberg formula.
Some important points of Rydberg formula.pdfSaiKalyani11
Rydberg formula calculates the wavenumber of spectral lines obtained in the spectra of single electron hydrogen-like atoms. Rydberg's envision to measure the wavenumber of spectral energies instead of wavelengths had brought a distinguishing variation in the spectral evaluations.
The applications of spectral studies.pdfSaiKalyani11
It discusses the importance of spectral studies. The Rydberg-Ritz combination principle deals with the identification of unknown spectral lines of the atomic spectrum. Besides, spectral studies have much significance in the analysis of the composition of astronomical matter. The study of emission and absorption spectra of the substance provides information on its structure. In particular, astronomers use this spectroscopic data to determine the constituents of stars and interstellar matter.
The Rydberg formula helps to determine the wavenumber or wavelengths of hydrogen spectral lines obtained in the hydrogen spectrum. Previously, Johann Jakob Balmer discovered an empirical formula to determine the wavelengths of hydrogen spectral lines obtained in the visible region of the hydrogen spectrum. As we all know, the hydrogen spectrum is not limited to the visible zone only. It occupies the ultraviolet and infrared parts of the electromagnetic spectrum also. Hence, the scientists' quests to determine the spectral positions of various spectral lines of the hydrogen spectrum finally came to an end with the Rydberg formula.
For more information on this topic, kindly visit our blog at;
https://jayamchemistrylearners.blogspot.com/2022/05/rydberg-ritz-combination-principle.html
The Rydberg formula helps to determine the wavenumber or wavelengths of hydrogen spectral lines obtained in the hydrogen spectrum. Previously, Johann Jakob Balmer discovered an empirical formula to determine the wavelengths of hydrogen spectral lines obtained in the visible region of the hydrogen spectrum. As we all know, the hydrogen spectrum is not limited to the visible zone only. It occupies the ultraviolet and infrared parts of the electromagnetic spectrum also. Hence, the scientists' quests to determine the spectral positions of various spectral lines of the hydrogen spectrum finally came to an end with the Rydberg formula.
For more information on this topic, kindly visit our blog article at;
https://jayamchemistrylearners.blogspot.com/2022/06/rydberg-formula-chemistry-learners.html
Biological screening of herbal drugs: Introduction and Need for
Phyto-Pharmacological Screening, New Strategies for evaluating
Natural Products, In vitro evaluation techniques for Antioxidants, Antimicrobial and Anticancer drugs. In vivo evaluation techniques
for Anti-inflammatory, Antiulcer, Anticancer, Wound healing, Antidiabetic, Hepatoprotective, Cardio protective, Diuretics and
Antifertility, Toxicity studies as per OECD guidelines
Embracing GenAI - A Strategic ImperativePeter Windle
Artificial Intelligence (AI) technologies such as Generative AI, Image Generators and Large Language Models have had a dramatic impact on teaching, learning and assessment over the past 18 months. The most immediate threat AI posed was to Academic Integrity with Higher Education Institutes (HEIs) focusing their efforts on combating the use of GenAI in assessment. Guidelines were developed for staff and students, policies put in place too. Innovative educators have forged paths in the use of Generative AI for teaching, learning and assessments leading to pockets of transformation springing up across HEIs, often with little or no top-down guidance, support or direction.
This Gasta posits a strategic approach to integrating AI into HEIs to prepare staff, students and the curriculum for an evolving world and workplace. We will highlight the advantages of working with these technologies beyond the realm of teaching, learning and assessment by considering prompt engineering skills, industry impact, curriculum changes, and the need for staff upskilling. In contrast, not engaging strategically with Generative AI poses risks, including falling behind peers, missed opportunities and failing to ensure our graduates remain employable. The rapid evolution of AI technologies necessitates a proactive and strategic approach if we are to remain relevant.
Operation “Blue Star” is the only event in the history of Independent India where the state went into war with its own people. Even after about 40 years it is not clear if it was culmination of states anger over people of the region, a political game of power or start of dictatorial chapter in the democratic setup.
The people of Punjab felt alienated from main stream due to denial of their just demands during a long democratic struggle since independence. As it happen all over the word, it led to militant struggle with great loss of lives of military, police and civilian personnel. Killing of Indira Gandhi and massacre of innocent Sikhs in Delhi and other India cities was also associated with this movement.
Palestine last event orientationfvgnh .pptxRaedMohamed3
An EFL lesson about the current events in Palestine. It is intended to be for intermediate students who wish to increase their listening skills through a short lesson in power point.
Macroeconomics- Movie Location
This will be used as part of your Personal Professional Portfolio once graded.
Objective:
Prepare a presentation or a paper using research, basic comparative analysis, data organization and application of economic information. You will make an informed assessment of an economic climate outside of the United States to accomplish an entertainment industry objective.
A Strategic Approach: GenAI in EducationPeter Windle
Artificial Intelligence (AI) technologies such as Generative AI, Image Generators and Large Language Models have had a dramatic impact on teaching, learning and assessment over the past 18 months. The most immediate threat AI posed was to Academic Integrity with Higher Education Institutes (HEIs) focusing their efforts on combating the use of GenAI in assessment. Guidelines were developed for staff and students, policies put in place too. Innovative educators have forged paths in the use of Generative AI for teaching, learning and assessments leading to pockets of transformation springing up across HEIs, often with little or no top-down guidance, support or direction.
This Gasta posits a strategic approach to integrating AI into HEIs to prepare staff, students and the curriculum for an evolving world and workplace. We will highlight the advantages of working with these technologies beyond the realm of teaching, learning and assessment by considering prompt engineering skills, industry impact, curriculum changes, and the need for staff upskilling. In contrast, not engaging strategically with Generative AI poses risks, including falling behind peers, missed opportunities and failing to ensure our graduates remain employable. The rapid evolution of AI technologies necessitates a proactive and strategic approach if we are to remain relevant.
Welcome to TechSoup New Member Orientation and Q&A (May 2024).pdfTechSoup
In this webinar you will learn how your organization can access TechSoup's wide variety of product discount and donation programs. From hardware to software, we'll give you a tour of the tools available to help your nonprofit with productivity, collaboration, financial management, donor tracking, security, and more.
The Roman Empire A Historical Colossus.pdfkaushalkr1407
The Roman Empire, a vast and enduring power, stands as one of history's most remarkable civilizations, leaving an indelible imprint on the world. It emerged from the Roman Republic, transitioning into an imperial powerhouse under the leadership of Augustus Caesar in 27 BCE. This transformation marked the beginning of an era defined by unprecedented territorial expansion, architectural marvels, and profound cultural influence.
The empire's roots lie in the city of Rome, founded, according to legend, by Romulus in 753 BCE. Over centuries, Rome evolved from a small settlement to a formidable republic, characterized by a complex political system with elected officials and checks on power. However, internal strife, class conflicts, and military ambitions paved the way for the end of the Republic. Julius Caesar’s dictatorship and subsequent assassination in 44 BCE created a power vacuum, leading to a civil war. Octavian, later Augustus, emerged victorious, heralding the Roman Empire’s birth.
Under Augustus, the empire experienced the Pax Romana, a 200-year period of relative peace and stability. Augustus reformed the military, established efficient administrative systems, and initiated grand construction projects. The empire's borders expanded, encompassing territories from Britain to Egypt and from Spain to the Euphrates. Roman legions, renowned for their discipline and engineering prowess, secured and maintained these vast territories, building roads, fortifications, and cities that facilitated control and integration.
The Roman Empire’s society was hierarchical, with a rigid class system. At the top were the patricians, wealthy elites who held significant political power. Below them were the plebeians, free citizens with limited political influence, and the vast numbers of slaves who formed the backbone of the economy. The family unit was central, governed by the paterfamilias, the male head who held absolute authority.
Culturally, the Romans were eclectic, absorbing and adapting elements from the civilizations they encountered, particularly the Greeks. Roman art, literature, and philosophy reflected this synthesis, creating a rich cultural tapestry. Latin, the Roman language, became the lingua franca of the Western world, influencing numerous modern languages.
Roman architecture and engineering achievements were monumental. They perfected the arch, vault, and dome, constructing enduring structures like the Colosseum, Pantheon, and aqueducts. These engineering marvels not only showcased Roman ingenuity but also served practical purposes, from public entertainment to water supply.
1. Blackbody
Hot blackbody emissions
A blackbody is a rigid, closed
unreal body that can absorb all
electromagnetic radiation that
falls on it regardless of its
frequencies, but it reflects
none.
It is a perfect
emitter and
absorber of
thermal
radiations
following
Kirchhoff's law.
On heating, the blackbody releases all thermal
electromagnetic radiation that it absorbed
previously. These are blackbody radiations. A
blackbody radiates heat energies without affecting
the intervening medium. It has the highest emissive
power of all other bodies at that particular
temperature and wavelength conditions.
An ideal black body is an imaginary
perception of Gustav Kirchhoff.
The blackbody is inexistent.
An object with above 0.95
emissivities is an
approximate blackbody.
A graph between emissive power
and radiation wavelength at a
fixed temperature T is known as a
blackbody curve. At different
source temperatures, we observe
different black body curves.
Blog:https://jayamchemistrylearners.blogspot.com/
The black body spectrum depends only
on the temperature. And it is
independent of the shape, structure, and
composition of blackbody enclosure.
Factors affecting
blackbody emission
Temperature
Emissivity
Surface area
Laws governing
blackbody emission
Planck quantum law
Wien displacement law
Stefan-Boltzmann law
