The document discusses refraction rules for converging and diverging lenses. It states that for a converging lens, any ray parallel to the principal axis will pass through the focal point on the opposite side, and any ray through the focal point will exit parallel to the principal axis. For a diverging lens, any ray parallel to the principal axis will pass through the focal point, and any ray toward the focal point will exit parallel to the principal axis. Additionally, any ray passing through the center of either lens will continue in the same direction.
Reflection of light in spherical mirrorMUBASHIRA M
this slide contains laws and terms of reflection of light. especially the image formation and ray diagrams of spherical mirror that are mainly useful for science students
When light travelling in one medium falls on the surface of second medium the following three effect may occur.
1:- A part of incident light is reflected back into the same medium. This is called Reflection of light.
2:- A part of light is passes through the medium.This Is known as Refraction of light.
3:- And remaining part of the light is absorbed by the surface on which the light fall. This is known as Absorption of light.
Reflection of light in spherical mirrorMUBASHIRA M
this slide contains laws and terms of reflection of light. especially the image formation and ray diagrams of spherical mirror that are mainly useful for science students
When light travelling in one medium falls on the surface of second medium the following three effect may occur.
1:- A part of incident light is reflected back into the same medium. This is called Reflection of light.
2:- A part of light is passes through the medium.This Is known as Refraction of light.
3:- And remaining part of the light is absorbed by the surface on which the light fall. This is known as Absorption of light.
Light - Reflection and Refraction, Class X, CBSE, ScienceDevesh Saini
PowerPoint Presentation covering all the concepts and topics of the chapter : Light- Reflection and Refraction of class X (CBSE).
This is exactly what you are looking for.
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Light is a transverse, electromagnetic wave that can be seen by humans. The wave nature of light was first illustrated through experiments on diffraction and interference. Like all electromagnetic waves, light can travel through a vacuum. The transverse nature of light can be demonstrated through polarization.
Light - Reflection and Refraction, Class X, CBSE, ScienceDevesh Saini
PowerPoint Presentation covering all the concepts and topics of the chapter : Light- Reflection and Refraction of class X (CBSE).
This is exactly what you are looking for.
Don't forget to comment and give feedback.
Light is a transverse, electromagnetic wave that can be seen by humans. The wave nature of light was first illustrated through experiments on diffraction and interference. Like all electromagnetic waves, light can travel through a vacuum. The transverse nature of light can be demonstrated through polarization.
Optics History, part I, until 1850.
Please send comments and suggestions for improvements to solo.hermelin@gmail.com.
More presentations in Optics and other subjects can be found in my website on http://www.solohermelin.com.
Reference books for the preparation of IIT JAM physics entrance examination 2016. Recommended books of Mathematical Methods, Mechanics, Optics, Thermodynamics, Kinetic Theory and Electricity and Magnetism.
Describes human eye optics.
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For more presentations on different subjects please visit my website at http://www.solohermelin.com.
Presentation on Various ideologies and concepts of Light.
Assessment for class X students for 2nd term.
With highly elaborated information on Light and it's properties.
100% Most Accurate Presentation on Light chapter Class X CBSE..
With Transitions and animations..
The Indian Dental Academy is the Leader in continuing dental education , training dentists in all aspects of dentistry and
offering a wide range of dental certified courses in different formats.for more details please visit
www.indiandentalacademy.com
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INVENTION AND INNOVATION DUE TO INDUSTRIAL REVOLUTIONAbhishek Sharma
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THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
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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.
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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
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optics at visible wavelengths.
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The ambient solar wind that flls the heliosphere originates from multiple
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2022 is driven by spatio-temporal changes in the magnetic connectivity to
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a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
Introduction:
RNA interference (RNAi) or Post-Transcriptional Gene Silencing (PTGS) is an important biological process for modulating eukaryotic gene expression.
It is highly conserved process of posttranscriptional gene silencing by which double stranded RNA (dsRNA) causes sequence-specific degradation of mRNA sequences.
dsRNA-induced gene silencing (RNAi) is reported in a wide range of eukaryotes ranging from worms, insects, mammals and plants.
This process mediates resistance to both endogenous parasitic and exogenous pathogenic nucleic acids, and regulates the expression of protein-coding genes.
What are small ncRNAs?
micro RNA (miRNA)
short interfering RNA (siRNA)
Properties of small non-coding RNA:
Involved in silencing mRNA transcripts.
Called “small” because they are usually only about 21-24 nucleotides long.
Synthesized by first cutting up longer precursor sequences (like the 61nt one that Lee discovered).
Silence an mRNA by base pairing with some sequence on the mRNA.
Discovery of siRNA?
The first small RNA:
In 1993 Rosalind Lee (Victor Ambros lab) was studying a non- coding gene in C. elegans, lin-4, that was involved in silencing of another gene, lin-14, at the appropriate time in the
development of the worm C. elegans.
Two small transcripts of lin-4 (22nt and 61nt) were found to be complementary to a sequence in the 3' UTR of lin-14.
Because lin-4 encoded no protein, she deduced that it must be these transcripts that are causing the silencing by RNA-RNA interactions.
Types of RNAi ( non coding RNA)
MiRNA
Length (23-25 nt)
Trans acting
Binds with target MRNA in mismatch
Translation inhibition
Si RNA
Length 21 nt.
Cis acting
Bind with target Mrna in perfect complementary sequence
Piwi-RNA
Length ; 25 to 36 nt.
Expressed in Germ Cells
Regulates trnasposomes activity
MECHANISM OF RNAI:
First the double-stranded RNA teams up with a protein complex named Dicer, which cuts the long RNA into short pieces.
Then another protein complex called RISC (RNA-induced silencing complex) discards one of the two RNA strands.
The RISC-docked, single-stranded RNA then pairs with the homologous mRNA and destroys it.
THE RISC COMPLEX:
RISC is large(>500kD) RNA multi- protein Binding complex which triggers MRNA degradation in response to MRNA
Unwinding of double stranded Si RNA by ATP independent Helicase
Active component of RISC is Ago proteins( ENDONUCLEASE) which cleave target MRNA.
DICER: endonuclease (RNase Family III)
Argonaute: Central Component of the RNA-Induced Silencing Complex (RISC)
One strand of the dsRNA produced by Dicer is retained in the RISC complex in association with Argonaute
ARGONAUTE PROTEIN :
1.PAZ(PIWI/Argonaute/ Zwille)- Recognition of target MRNA
2.PIWI (p-element induced wimpy Testis)- breaks Phosphodiester bond of mRNA.)RNAse H activity.
MiRNA:
The Double-stranded RNAs are naturally produced in eukaryotic cells during development, and they have a key role in regulating gene expression .
2. Introduction
• First lets consider a double convex lens. Suppose
that several rays of light approach the lens; and
suppose that these rays of light are traveling
parallel to the principal axis. Upon reaching the
front face of the lens, each ray of light will
refract towards the normal to the surface. At
this boundary, the light ray is passing from air
into a more dense medium (usually plastic or
glass). Since the light ray is passing from a
medium in which it travels fast (less optically
dense) into a medium in which it travels
relatively slow (more optically dense), it will
bend towards the normal line. This is the FST
principle of refraction. This is shown for two
incident rays on the diagram below. Once the
light ray refracts across the boundary and enters
the lens, it travels in a straight line until it
reaches the back face of the lens. At this
boundary, each ray of light will refract away
from the normal to the surface. Since the light
ray is passing from a medium in which it travels
slow (more optically dense) to a medium in
which it travels fast (less optically dense), it will
bend away from the normal line; this is the SFA
principle of refraction.
3. Any incident ray traveling parallel to the principal axis
of a converging lens will refract through the lens and
travel through the focal point on the opposite side of
the lens.
Now suppose that the rays of light are traveling
through the focal point on the way to the lens. These
rays of light will refract when they enter the lens and
refract when they leave the lens. As the light rays enter
into the more dense lens material, they refract towards
the normal; and as they exit into the less dense air,
they refract away from the normal. These specific rays
will exit the lens traveling parallel to the principal axis.
4. Refraction Rules for a Converging Lens
• Any incident ray traveling
parallel to the principal
axis of a converging lens
will refract through the
lens and travel through
the focal point on the
opposite side of the lens.
• Any incident ray traveling
through the focal point on
the way to the lens will
refract through the lens
and travel parallel to the
principal axis.
5. These two "rules" will greatly simplify the task
of determining the image location for objects
placed infront of converging lenses. This topic
will be discussed in the next part of Lesson 5.
For now, internalize the meaning of the rules
and be prepared to use them. As the rules are
applied in the construction of ray diagrams,
do not forget the fact that Snells' Law of
refraction of light holds for each of these
rays. It just so happens that geometrically,
when Snell's Law is applied for rays that strike
the lens in the manner described above, they
will refract in close approximation with these
two rules. The tendency of incident light rays
to follow these rules is increased for lenses
that are thin. For such thin lenses, the path
of the light through the lens itself contributes
very little to the overall change in the
direction of the light rays. We will use this so-
called thin-lens approximation in this unit.
Furthermore, to simplify the construction of
ray diagrams, we will avoid refracting each
light ray twice - upon entering and emerging
from the lens. Instead, we will continue the
incident ray to the vertical axis of the lens
and refract the light at that point. For thin
lenses, this simplification will produce the
same result as if we were refracting the light
twice.
The Thin Lens Approximation
6.
7. Refraction Rule for a Diverging Lens
Any incident ray traveling parallel to the principal axis of a diverging
lens will refract through the lens and travel in line with the focal point
(i.e., in a direction such that its extension will pass through the focal
point).
Now suppose that the rays of light are traveling towards the focal
point on the way to the lens. Because of the negative focal length for
double concave lenses, the light rays will head towards the focal point
on the opposite side of the lens. These rays will actually reach the
lens before they reach the focal point. These rays of light will refract
when they enter the lens and refract when they leave the lens. As the
light rays enter into the more dense lens material, they refract
towards the normal; and as they exit into the less dense air, they
refract away from the normal. These specific rays will exit the lens
traveling parallel to the principal axis.
8. Any incident ray traveling parallel
to the principal axis of a diverging
lens will refract through the lens
and travel in line with the focal
point (i.e., in a direction such that
its extension will pass through the
focal point).
Any incident ray traveling towards
the focal point on the way to the
lens will refract through the lens
and travel parallel to the principal
axis.
Refraction Rules for a Diverging Lens
9. The above discussion focuses on the manner
in which converging and diverging lenses
refract incident rays that are traveling parallel
to the principal axis or are traveling through
(or towards) the focal point. But these are not
the only two possible incident rays.There are a
multitude of incident rays that strike the lens
and refract in a variety of ways.Yet, there are
three specific rays that behave in a very
predictable manner.The third ray that we will
investigate is the ray that passes through the
precise center of the lens - through the point
where the principal axis and the vertical axis
intersect.This ray will refract as it enters and
refract as it exits the lens, but the net effect of
this dual refraction is that the path of the light
ray is not changed. For a thin lens, the
refracted ray is traveling in the same direction
as the incident ray and is approximately in line
with it.The behavior of this third incident ray
is depicted in the diagram below..
10. Any incident ray traveling parallel to the
principal axis of a converging lens will refract
through the lens and travel through the focal
point on the opposite side of the lens.
Any incident ray traveling through the focal
point on the way to the lens will refract
through the lens and travel parallel to the
principal axis.
An incident ray that passes through the center
of the lens will in effect continue in the same
direction that it had when it entered the lens.
11. Any incident ray traveling parallel to the
principal axis of a diverging lens will refract
through the lens and travel in line with the focal
point (i.e., in a direction such that its extension
will pass through the focal point).
Any incident ray traveling towards the focal
point on the way to the lens will refract through
the lens and travel parallel to the principal axis.
An incident ray that passes through the center of
the lens will in effect continue in the same
direction that it had when it entered the lens.
12.
13. Here is another creative presentation by your slide maker on
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