Optics is the branch of physics that deals with the behavior and properties of light, including its interactions with matter and the construction of instruments that use or detect light. Interference occurs when two light waves superpose to form a resultant wave of greater or lower amplitude. Interference effects can be observed with all types of waves, including light, radio, acoustic, and water waves. Polarization is the process by which light waves vibrating in different planes can be made to vibrate in a particular plane. Polarimeters are instruments used to measure the angle of rotation caused by passing polarized light through an optically active substance.
This presentation talks about the basic terms and terminologies related to Radiometry and Photometry. Their definitions.
This article also highlights the different theories about Light. It provides a rudimentary and comprehensive idea about light and its nature.
Introducation to optical properties and also relation with nano material. As most of the properties are similar for simple and nano material only some fundamental points are changed.
MAHARASHTRA STATE BOARD
CLASS XI AND XII
PHYSICS
CHAPTER 7
WAVE OPTICS
CONTENT:
Huygen's principle.
Huygen's principles & proof of laws of reflection/refraction.
Condition for construction & destruction of coherent waves.
Young's double slit experiment.
Modified Young's double slit experiment.
Intensity of light in Y.D.S.E.
Diffraction due to single slit.
Polarisation & doppler effect.
(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...Scintica Instrumentation
Intravital microscopy (IVM) is a powerful tool utilized to study cellular behavior over time and space in vivo. Much of our understanding of cell biology has been accomplished using various in vitro and ex vivo methods; however, these studies do not necessarily reflect the natural dynamics of biological processes. Unlike traditional cell culture or fixed tissue imaging, IVM allows for the ultra-fast high-resolution imaging of cellular processes over time and space and were studied in its natural environment. Real-time visualization of biological processes in the context of an intact organism helps maintain physiological relevance and provide insights into the progression of disease, response to treatments or developmental processes.
In this webinar we give an overview of advanced applications of the IVM system in preclinical research. IVIM technology is a provider of all-in-one intravital microscopy systems and solutions optimized for in vivo imaging of live animal models at sub-micron resolution. The system’s unique features and user-friendly software enables researchers to probe fast dynamic biological processes such as immune cell tracking, cell-cell interaction as well as vascularization and tumor metastasis with exceptional detail. This webinar will also give an overview of IVM being utilized in drug development, offering a view into the intricate interaction between drugs/nanoparticles and tissues in vivo and allows for the evaluation of therapeutic intervention in a variety of tissues and organs. This interdisciplinary collaboration continues to drive the advancements of novel therapeutic strategies.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
Seminar of U.V. Spectroscopy by SAMIR PANDASAMIR PANDA
Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
Ultraviolet-visible spectroscopy refers to absorption spectroscopy or reflect spectroscopy in the UV-VIS spectral region.
Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
Professional air quality monitoring systems provide immediate, on-site data for analysis, compliance, and decision-making.
Monitor common gases, weather parameters, particulates.
Richard's aventures in two entangled wonderlandsRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
Slide 1: Title Slide
Extrachromosomal Inheritance
Slide 2: Introduction to Extrachromosomal Inheritance
Definition: Extrachromosomal inheritance refers to the transmission of genetic material that is not found within the nucleus.
Key Components: Involves genes located in mitochondria, chloroplasts, and plasmids.
Slide 3: Mitochondrial Inheritance
Mitochondria: Organelles responsible for energy production.
Mitochondrial DNA (mtDNA): Circular DNA molecule found in mitochondria.
Inheritance Pattern: Maternally inherited, meaning it is passed from mothers to all their offspring.
Diseases: Examples include Leber’s hereditary optic neuropathy (LHON) and mitochondrial myopathy.
Slide 4: Chloroplast Inheritance
Chloroplasts: Organelles responsible for photosynthesis in plants.
Chloroplast DNA (cpDNA): Circular DNA molecule found in chloroplasts.
Inheritance Pattern: Often maternally inherited in most plants, but can vary in some species.
Examples: Variegation in plants, where leaf color patterns are determined by chloroplast DNA.
Slide 5: Plasmid Inheritance
Plasmids: Small, circular DNA molecules found in bacteria and some eukaryotes.
Features: Can carry antibiotic resistance genes and can be transferred between cells through processes like conjugation.
Significance: Important in biotechnology for gene cloning and genetic engineering.
Slide 6: Mechanisms of Extrachromosomal Inheritance
Non-Mendelian Patterns: Do not follow Mendel’s laws of inheritance.
Cytoplasmic Segregation: During cell division, organelles like mitochondria and chloroplasts are randomly distributed to daughter cells.
Heteroplasmy: Presence of more than one type of organellar genome within a cell, leading to variation in expression.
Slide 7: Examples of Extrachromosomal Inheritance
Four O’clock Plant (Mirabilis jalapa): Shows variegated leaves due to different cpDNA in leaf cells.
Petite Mutants in Yeast: Result from mutations in mitochondrial DNA affecting respiration.
Slide 8: Importance of Extrachromosomal Inheritance
Evolution: Provides insight into the evolution of eukaryotic cells.
Medicine: Understanding mitochondrial inheritance helps in diagnosing and treating mitochondrial diseases.
Agriculture: Chloroplast inheritance can be used in plant breeding and genetic modification.
Slide 9: Recent Research and Advances
Gene Editing: Techniques like CRISPR-Cas9 are being used to edit mitochondrial and chloroplast DNA.
Therapies: Development of mitochondrial replacement therapy (MRT) for preventing mitochondrial diseases.
Slide 10: Conclusion
Summary: Extrachromosomal inheritance involves the transmission of genetic material outside the nucleus and plays a crucial role in genetics, medicine, and biotechnology.
Future Directions: Continued research and technological advancements hold promise for new treatments and applications.
Slide 11: Questions and Discussion
Invite Audience: Open the floor for any questions or further discussion on the topic.
2. Optics is the branch of physics which involves the behavior and properties of light,
including its interactions with matter and the construction of instruments that use
or detect it.
Optics usually describes the behavior of visible, ultraviolet, and infrared light.
7. Interference of Light
In physics, interference is a phenomenon in which two waves superpose to form a resultant wave
of greater or lower amplitude.
When two light waves from different coherent sources meet together, then the distribution of
energy due to one wave is disturbed by the other. This modification in the distribution
of light energy due to super- position of two light waves is called "Interference of light“
Interference effects can be observed with all types of waves, for example, light, radio, acoustic,
surface water waves or matter waves.
https://www.youtube.com/watch?v=Iuv6hY6zsd0
10. Conditions of Interference
When waves come together, they can interfere
constructively or destructively. To set up a stable and clear
interference pattern, two conditions must be met:
1. The sources of the waves must be coherent.
2. The waves should be monochromatic - they should be
of a single wavelength.
Coherent Sources
Those sources of light which emit light waves
continuously of same wavelength, time period,
frequency, and amplitude and have zero phase
difference or constant phase difference are called
coherent sources.
11. Constructive Interference
When two light waves superpose with each other in such a way that the crest of one wave falls on
the crest of the second wave, and trough of one wave falls on the trough of the second wave, then
the resultant wave has larger amplitude and it is called constructive interference.
Destructive Interference
When two light waves superpose with each other in such a way that the crest of one wave coincides the
trough of the second wave, then the amplitude of resultant wave becomes zero and it is called
destructive interference.
12. Newton’s Rings
Newton's ring is a phenomenon in which an
interference pattern is created by the reflection
of light between two surfaces—a spherical
surface and an adjacent flat surface. It is named
after Isaac Newton.
13. What do you mean by diffraction of light?
Diffraction is the slight bending of light as it passes around the edge of an object.
The amount of bending depends on the relative size of the wavelength of light to the size of the opening.
14. What are the conditions of diffraction
of light?
There are two conditions
(1) In case of straight edge: The edge should be
very sharp and its width is to be equal to or is of
the order of the wavelength, λ of light.
(2) In case of thin hole: the diameter of the hole
should be extremely very small such that it is
equal to or is of the order of the wavelength λ of
light.
15. # Distinguish between interference and diffraction of light
1. Two separate wave fronts originating from two coherent sources produce
interference. Secondary wavelets originating from different parts of the same wave
front constitute diffraction.
2. The region of minimum intensity is perfectly dark in interference. In
diffraction they are not perfectly dark.
3. Width of the fringes is equal in interference. In diffraction they are never
equal.
4. The intensity of all positions of maxima are of the same intensity in
interference. In diffraction they do vary.
5. When we have two infinitely narrow slits separated by a distance apart
near the source, we get interference. But when we have a single slit of finite width
or rather an aperture near the source, we get diffraction.
16. What do you mean by Polarization?
In an electromagnetic wave, both the electric field and magnetic field are oscillating but in different
directions. The process by which light waves vibrating in different planes can be made to vibrate in a
particular plane is called polarization of light.
17. # State Brewster’s Law
In 1811 Brewster’s proposed it. The law states that the tangent of the angle at which polarization is
obtained by reflection is numerically equal to the refractive index of the medium.
If θp is the angle and μ is the refractive index of the medium, then
μ = tan 𝜃 𝑝
This is known as Brewster’s law.
18. # State Malus Law and explain it mathematically.
According to Malus, when completely plane polarized light is incident on the analyzer, the
intensity E1 of the light transmitted by the analyzer is directly proportional to the square of
the cosine of angle between the transmission axes of the analyzer and the polarizer.
If E1 is the intensity of the transmitted wave and θ is the angle between the planes of polarizer and the
analyser. Then,
𝐸1 ∝ 𝑐𝑜𝑠2 𝜃
𝐸1 = 𝐸 𝑐𝑜𝑠2
𝜃
Where E is the intensity of the incident polarized light.
This is known as Malus law of polarization.
19. # What do you mean by Polarimeters?
A polarimeter is a scientific instrument used to measure the angle of rotation caused by
passing polarized light through an optically active substance.
Some chemical substances are optically active, and polarized (uni-directional) light will rotate
either to the left (counter-clockwise) or right (clockwise) when passed through these substances.
The amount, by which the light is rotated, is known as the angle of rotation. The angle of rotation
is basically known as observed angle.
20. Assignment
1. Light of wavelength 550 nm from a narrow slit is incident on a double slit. The overall separation
of 5 fringes on a screen 200 cm away is 1 cm. Compute the slit separation.
2. A parallel beam of monochromatic source of light is allowed to incident normally on a plane
transmission grating having 5000 lines per cm. A second order spectral line is found to be diffracted at
an angle 300
. Find the wavelength of the light.
21. QUESTIONS
1.Interference is a phenomenon where two waves superpose to form a resultant wave and
alternately bright and dark parallel fringes are formed. From the condition for bright fringes
and dark fringes, show that the distances between any two successive bright and dark
fringes are same.
2. From the theory of plane diffraction grating deduce the expression 𝑎 + 𝑏 sin 𝜃 = 𝑚 𝜆
where, the symbols have their usual meanings.
3. Evaluate the mathematical expression for Brewster’s law with statement.