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Option C: Imaging (Core topics)
Description
Overview of essential ideas for this option
C.1: The progress of a wave can be modelled via the ray or the wavefront. The change in wave speed when moving between media changes the shape of the wave.
C.2: Optical microscopes and telescopes utilize similar physical properties of lenses and mirrors. Analysis of the universe is performed both optically and by using radio telescopes to investigate different regions of the electromagnetic spectrum.
C.3: Total internal reflection allows light or infrared radiation to travel along a transparent fibre. However, the performance of a fibre can be degraded by dispersion and attenuation effects.
Directly related questions
- 20N.3.SL.TZ0.12b: Sketch a ray diagram to find the position of the images for both lenses in the compound...
- 20N.3.SL.TZ0.12b: Sketch a ray diagram to find the position of the images for both lenses in the compound...
- 20N.3.SL.TZ0.b: Sketch a ray diagram to find the position of the images for both lenses in the compound...
- 20N.3.SL.TZ0.13: A single pulse of light enters an optic fibre which contains small impurities that scatter the...
- 20N.3.SL.TZ0.13: A single pulse of light enters an optic fibre which contains small impurities that scatter the...
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17N.3.HL.TZ0.15a:
Calculate the maximum angle β for light to travel through the fibre.
Refractive index of core = 1.50
Refractive index of cladding = 1.48 -
17N.3.HL.TZ0.15a:
Calculate the maximum angle β for light to travel through the fibre.
Refractive index of core = 1.50
Refractive index of cladding = 1.48 -
17N.3.HL.TZ0.a:
Calculate the maximum angle β for light to travel through the fibre.
Refractive index of core = 1.50
Refractive index of cladding = 1.48 - 17N.3.HL.TZ0.15b: Outline how the combination of core and cladding reduces the overall dispersion in the optic fibres.
- 17N.3.HL.TZ0.15b: Outline how the combination of core and cladding reduces the overall dispersion in the optic fibres.
- 17N.3.HL.TZ0.b: Outline how the combination of core and cladding reduces the overall dispersion in the optic fibres.
- 17N.3.SL.TZ0.9c.iv: The screen is now correctly positioned to form a focused image of point R. However, the top of...
- 17N.3.SL.TZ0.9c.iv: The screen is now correctly positioned to form a focused image of point R. However, the top of...
- 17N.3.SL.TZ0.c.iv: The screen is now correctly positioned to form a focused image of point R. However, the top of...
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17N.3.SL.TZ0.9b.i:
Determine the position of the image.
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17N.3.SL.TZ0.9b.i:
Determine the position of the image.
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17N.3.SL.TZ0.b.i:
Determine the position of the image.
- 17N.3.SL.TZ0.9c.i: On the diagram, draw two rays to locate the point Q′ on the image that corresponds to point Q on...
- 17N.3.SL.TZ0.9c.i: On the diagram, draw two rays to locate the point Q′ on the image that corresponds to point Q on...
- 17N.3.SL.TZ0.c.i: On the diagram, draw two rays to locate the point Q′ on the image that corresponds to point Q on...
- 17N.3.SL.TZ0.9a.ii: State the maximum possible distance from an object to the lens in order for the lens to produce...
- 17N.3.SL.TZ0.9a.ii: State the maximum possible distance from an object to the lens in order for the lens to produce...
- 17N.3.SL.TZ0.a.ii: State the maximum possible distance from an object to the lens in order for the lens to produce...
- 17N.3.SL.TZ0.9a.i: Sketch a ray diagram to show how the magnifying glass produces an upright image.
- 17N.3.SL.TZ0.9a.i: Sketch a ray diagram to show how the magnifying glass produces an upright image.
- 17N.3.SL.TZ0.a.i: Sketch a ray diagram to show how the magnifying glass produces an upright image.
- 17N.3.SL.TZ0.9b.ii: State three characteristics of the image.
- 17N.3.SL.TZ0.9b.ii: State three characteristics of the image.
- 17N.3.SL.TZ0.b.ii: State three characteristics of the image.
- 17N.3.SL.TZ0.9c.ii: Calculate the vertical distance of point Q′ from the principal axis.
- 17N.3.SL.TZ0.9c.ii: Calculate the vertical distance of point Q′ from the principal axis.
- 17N.3.SL.TZ0.c.ii: Calculate the vertical distance of point Q′ from the principal axis.
- 17N.3.SL.TZ0.9c.iii: A screen is positioned to form a focused image of point Q. State the direction, relative to Q, in...
- 17N.3.SL.TZ0.9c.iii: A screen is positioned to form a focused image of point Q. State the direction, relative to Q, in...
- 17N.3.SL.TZ0.c.iii: A screen is positioned to form a focused image of point Q. State the direction, relative to Q, in...
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18M.3.SL.TZ2.10b.i:
Calculate the maximum attenuation allowed for the signal.
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18M.3.SL.TZ2.10b.i:
Calculate the maximum attenuation allowed for the signal.
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18M.3.SL.TZ2.b.i:
Calculate the maximum attenuation allowed for the signal.
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18M.3.HL.TZ2.13c:
It is proposed to build an array of radio telescopes such that the maximum distance between them is 3800 km. The array will operate at a wavelength of 2.1 cm.
Comment on whether it is possible to build an optical telescope operating at 580 nm that is to have the same resolution as the array.
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18M.3.HL.TZ2.13c:
It is proposed to build an array of radio telescopes such that the maximum distance between them is 3800 km. The array will operate at a wavelength of 2.1 cm.
Comment on whether it is possible to build an optical telescope operating at 580 nm that is to have the same resolution as the array.
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18M.3.HL.TZ2.c:
It is proposed to build an array of radio telescopes such that the maximum distance between them is 3800 km. The array will operate at a wavelength of 2.1 cm.
Comment on whether it is possible to build an optical telescope operating at 580 nm that is to have the same resolution as the array.
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18M.3.SL.TZ2.8b:
The diagram shows an incomplete ray diagram which consists of a red ray of light and a blue ray of light which are incident on a converging glass lens. In this glass lens the refractive index for blue light is greater than the refractive index for red light.
Using the diagram, outline the phenomenon of chromatic aberration.
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18M.3.SL.TZ2.8b:
The diagram shows an incomplete ray diagram which consists of a red ray of light and a blue ray of light which are incident on a converging glass lens. In this glass lens the refractive index for blue light is greater than the refractive index for red light.
Using the diagram, outline the phenomenon of chromatic aberration.
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18M.3.SL.TZ2.b:
The diagram shows an incomplete ray diagram which consists of a red ray of light and a blue ray of light which are incident on a converging glass lens. In this glass lens the refractive index for blue light is greater than the refractive index for red light.
Using the diagram, outline the phenomenon of chromatic aberration.
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18M.3.SL.TZ2.9a:
Identify, with the letter X, the position of the focus of the primary mirror.
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18M.3.SL.TZ2.9a:
Identify, with the letter X, the position of the focus of the primary mirror.
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18M.3.SL.TZ2.a:
Identify, with the letter X, the position of the focus of the primary mirror.
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18M.3.SL.TZ2.10a:
An optic fibre of refractive index 1.4475 is surrounded by air. The critical angle for the core – air boundary interface is 44°. Suggest, with a calculation, why the use of cladding with refractive index 1.4444 improves the performance of the optic fibre.
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18M.3.SL.TZ2.10a:
An optic fibre of refractive index 1.4475 is surrounded by air. The critical angle for the core – air boundary interface is 44°. Suggest, with a calculation, why the use of cladding with refractive index 1.4444 improves the performance of the optic fibre.
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18M.3.SL.TZ2.a:
An optic fibre of refractive index 1.4475 is surrounded by air. The critical angle for the core – air boundary interface is 44°. Suggest, with a calculation, why the use of cladding with refractive index 1.4444 improves the performance of the optic fibre.
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18M.3.SL.TZ2.10b.ii:
An amplifier can increase the power of the signal by 12 dB. Determine the minimum number of amplifiers required.
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18M.3.SL.TZ2.10b.ii:
An amplifier can increase the power of the signal by 12 dB. Determine the minimum number of amplifiers required.
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18M.3.SL.TZ2.b.ii:
An amplifier can increase the power of the signal by 12 dB. Determine the minimum number of amplifiers required.
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18M.3.SL.TZ2.10b.iii:
The graph shows the variation with wavelength of the refractive index of the glass from which the optic fibre is made.
Two light rays enter the fibre at the same instant along the axes. Ray A has a wavelength of λA and ray B has a wavelength of λB. Discuss the effect that the difference in wavelength has on the rays as they pass along the fibre.
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18M.3.SL.TZ2.10b.iii:
The graph shows the variation with wavelength of the refractive index of the glass from which the optic fibre is made.
Two light rays enter the fibre at the same instant along the axes. Ray A has a wavelength of λA and ray B has a wavelength of λB. Discuss the effect that the difference in wavelength has on the rays as they pass along the fibre.
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18M.3.SL.TZ2.b.iii:
The graph shows the variation with wavelength of the refractive index of the glass from which the optic fibre is made.
Two light rays enter the fibre at the same instant along the axes. Ray A has a wavelength of λA and ray B has a wavelength of λB. Discuss the effect that the difference in wavelength has on the rays as they pass along the fibre.
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18M.3.SL.TZ2.10c:
In many places clad optic fibres are replacing copper cables. State one example of how fibre optic technology has impacted society.
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18M.3.SL.TZ2.10c:
In many places clad optic fibres are replacing copper cables. State one example of how fibre optic technology has impacted society.
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18M.3.SL.TZ2.c:
In many places clad optic fibres are replacing copper cables. State one example of how fibre optic technology has impacted society.
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18M.3.SL.TZ2.8a.ii:
calculate the linear magnification.
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18M.3.SL.TZ2.8a.ii:
calculate the linear magnification.
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18M.3.SL.TZ2.a.ii:
calculate the linear magnification.
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18M.3.SL.TZ2.9b:
This arrangement using the secondary mirror is said to increase the focal length of the primary mirror. State why this is an advantage.
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18M.3.SL.TZ2.9b:
This arrangement using the secondary mirror is said to increase the focal length of the primary mirror. State why this is an advantage.
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18M.3.SL.TZ2.b:
This arrangement using the secondary mirror is said to increase the focal length of the primary mirror. State why this is an advantage.
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18M.3.SL.TZ2.9c:
Distinguish between this mounting and the Newtonian mounting.
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18M.3.SL.TZ2.9c:
Distinguish between this mounting and the Newtonian mounting.
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18M.3.SL.TZ2.c:
Distinguish between this mounting and the Newtonian mounting.
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18M.3.SL.TZ1.8a.i:
Identify whether the image is real or virtual.
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18M.3.SL.TZ1.8a.i:
Identify whether the image is real or virtual.
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18M.3.SL.TZ1.a.i:
Identify whether the image is real or virtual.
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18M.3.SL.TZ1.8a.ii:
The lens is 18 cm from the screen and the image is 0.40 times smaller than the object. Calculate the power of the lens, in cm–1.
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18M.3.SL.TZ1.8a.ii:
The lens is 18 cm from the screen and the image is 0.40 times smaller than the object. Calculate the power of the lens, in cm–1.
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18M.3.SL.TZ1.a.ii:
The lens is 18 cm from the screen and the image is 0.40 times smaller than the object. Calculate the power of the lens, in cm–1.
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18M.3.SL.TZ1.8a.iii:
Light passing through this lens is subject to chromatic aberration. Discuss the effect that chromatic aberration has on the image formed on the screen.
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18M.3.SL.TZ1.8a.iii:
Light passing through this lens is subject to chromatic aberration. Discuss the effect that chromatic aberration has on the image formed on the screen.
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18M.3.SL.TZ1.a.iii:
Light passing through this lens is subject to chromatic aberration. Discuss the effect that chromatic aberration has on the image formed on the screen.
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18M.3.SL.TZ1.8b:
A system consisting of a converging lens of focal length F1 (lens 1) and a diverging lens (lens 2) are used to obtain the image of an object as shown on the scaled diagram. The focal length of lens 1 (F1) is 30 cm.
Determine, using the ray diagram, the focal length of the diverging lens.
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18M.3.SL.TZ1.8b:
A system consisting of a converging lens of focal length F1 (lens 1) and a diverging lens (lens 2) are used to obtain the image of an object as shown on the scaled diagram. The focal length of lens 1 (F1) is 30 cm.
Determine, using the ray diagram, the focal length of the diverging lens.
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18M.3.SL.TZ1.b:
A system consisting of a converging lens of focal length F1 (lens 1) and a diverging lens (lens 2) are used to obtain the image of an object as shown on the scaled diagram. The focal length of lens 1 (F1) is 30 cm.
Determine, using the ray diagram, the focal length of the diverging lens.
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18M.3.SL.TZ1.9a:
Calculate the critical angle at the core−cladding boundary.
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18M.3.SL.TZ1.9a:
Calculate the critical angle at the core−cladding boundary.
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18M.3.SL.TZ1.a:
Calculate the critical angle at the core−cladding boundary.
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18M.3.SL.TZ1.9b:
The use of optical fibres has led to a revolution in communications across the globe. Outline two advantages of optical fibres over electrical conductors for the purpose of data transfer.
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18M.3.SL.TZ1.9b:
The use of optical fibres has led to a revolution in communications across the globe. Outline two advantages of optical fibres over electrical conductors for the purpose of data transfer.
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18M.3.SL.TZ1.b:
The use of optical fibres has led to a revolution in communications across the globe. Outline two advantages of optical fibres over electrical conductors for the purpose of data transfer.
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18M.3.SL.TZ1.9c.i:
Draw on the axes an output signal to illustrate the effect of waveguide dispersion.
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18M.3.SL.TZ1.9c.i:
Draw on the axes an output signal to illustrate the effect of waveguide dispersion.
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18M.3.SL.TZ1.c.i:
Draw on the axes an output signal to illustrate the effect of waveguide dispersion.
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18M.3.SL.TZ1.9c.ii:
Calculate the power of the output signal after the signal has travelled a distance of 3.40 km in the fibre.
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18M.3.SL.TZ1.9c.ii:
Calculate the power of the output signal after the signal has travelled a distance of 3.40 km in the fibre.
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18M.3.SL.TZ1.c.ii:
Calculate the power of the output signal after the signal has travelled a distance of 3.40 km in the fibre.
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18M.3.SL.TZ1.9c.iii:
Explain how the use of a graded-index fibre will improve the performance of this fibre optic system.
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18M.3.SL.TZ1.9c.iii:
Explain how the use of a graded-index fibre will improve the performance of this fibre optic system.
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18M.3.SL.TZ1.c.iii:
Explain how the use of a graded-index fibre will improve the performance of this fibre optic system.
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18N.3.SL.TZ0.8b.ii:
Hence state how the defect of the converging lens in (a) may be corrected.
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18N.3.SL.TZ0.8b.ii:
Hence state how the defect of the converging lens in (a) may be corrected.
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18N.3.SL.TZ0.b.ii:
Hence state how the defect of the converging lens in (a) may be corrected.
- 18N.3.SL.TZ0.8a: On the diagram, draw lines to show the rays after they have refracted through the lens. Label the...
- 18N.3.SL.TZ0.8a: On the diagram, draw lines to show the rays after they have refracted through the lens. Label the...
- 18N.3.SL.TZ0.a: On the diagram, draw lines to show the rays after they have refracted through the lens. Label the...
- 18N.3.SL.TZ0.10b.iii: Suggest whether this fibre could be used to transmit information at a frequency of 100 MHz.
- 18N.3.SL.TZ0.10b.iii: Suggest whether this fibre could be used to transmit information at a frequency of 100 MHz.
- 18N.3.SL.TZ0.b.iii: Suggest whether this fibre could be used to transmit information at a frequency of 100 MHz.
- 18N.3.SL.TZ0.10a.ii: The refractive indices of the glass and cladding are only slightly different. Suggest why this is...
- 18N.3.SL.TZ0.10a.ii: The refractive indices of the glass and cladding are only slightly different. Suggest why this is...
- 18N.3.SL.TZ0.a.ii: The refractive indices of the glass and cladding are only slightly different. Suggest why this is...
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18N.3.SL.TZ0.10b.i:
Show that the longest path is 66 m longer than the shortest path.
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18N.3.SL.TZ0.10b.i:
Show that the longest path is 66 m longer than the shortest path.
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18N.3.SL.TZ0.b.i:
Show that the longest path is 66 m longer than the shortest path.
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18N.3.SL.TZ0.8b.i:
Suggest how the refracted rays in (a) are modified when the converging lens is replaced by a diverging lens.
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18N.3.SL.TZ0.8b.i:
Suggest how the refracted rays in (a) are modified when the converging lens is replaced by a diverging lens.
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18N.3.SL.TZ0.b.i:
Suggest how the refracted rays in (a) are modified when the converging lens is replaced by a diverging lens.
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18N.3.SL.TZ0.10a.i:
Calculate n.
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18N.3.SL.TZ0.10a.i:
Calculate n.
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18N.3.SL.TZ0.a.i:
Calculate n.
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18N.3.SL.TZ0.9b.i:
Calculate the distance between the lenses.
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18N.3.SL.TZ0.9b.i:
Calculate the distance between the lenses.
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18N.3.SL.TZ0.b.i:
Calculate the distance between the lenses.
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18N.3.SL.TZ0.10b.ii:
Determine the time delay between the arrival of signals created by the extra distance in (b)(i).
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18N.3.SL.TZ0.10b.ii:
Determine the time delay between the arrival of signals created by the extra distance in (b)(i).
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18N.3.SL.TZ0.b.ii:
Determine the time delay between the arrival of signals created by the extra distance in (b)(i).
- 18N.3.SL.TZ0.9a: Draw rays on the diagram to show the formation of the final image.
- 18N.3.SL.TZ0.9a: Draw rays on the diagram to show the formation of the final image.
- 18N.3.SL.TZ0.a: Draw rays on the diagram to show the formation of the final image.
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18N.3.SL.TZ0.9b.ii:
Determine the magnification of the microscope.
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18N.3.SL.TZ0.9b.ii:
Determine the magnification of the microscope.
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18N.3.SL.TZ0.b.ii:
Determine the magnification of the microscope.
- 19M.3.SL.TZ2.11ai: Construct rays, on the diagram, to locate the image of this object formed by the lens. Label this...
- 19M.3.SL.TZ2.11ai: Construct rays, on the diagram, to locate the image of this object formed by the lens. Label this...
- 19M.3.SL.TZ2.ai: Construct rays, on the diagram, to locate the image of this object formed by the lens. Label this...
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19M.3.SL.TZ2.11bii:
The image at I is the object for a second converging lens. This second lens forms a final image at infinity with an overall angular magnification for the two lens arrangement of 5. Calculate the distance between the two converging lenses.
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19M.3.SL.TZ2.11bii:
The image at I is the object for a second converging lens. This second lens forms a final image at infinity with an overall angular magnification for the two lens arrangement of 5. Calculate the distance between the two converging lenses.
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19M.3.SL.TZ2.bii:
The image at I is the object for a second converging lens. This second lens forms a final image at infinity with an overall angular magnification for the two lens arrangement of 5. Calculate the distance between the two converging lenses.
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19M.3.SL.TZ2.11biii:
A new object is placed a few meters to the left of the original lens. The student adjusts spacing of the lenses to form a virtual image at infinity of the new object. Outline, without calculation, the required change to the lens separation.
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19M.3.SL.TZ2.11biii:
A new object is placed a few meters to the left of the original lens. The student adjusts spacing of the lenses to form a virtual image at infinity of the new object. Outline, without calculation, the required change to the lens separation.
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19M.3.SL.TZ2.biii:
A new object is placed a few meters to the left of the original lens. The student adjusts spacing of the lenses to form a virtual image at infinity of the new object. Outline, without calculation, the required change to the lens separation.
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19M.3.SL.TZ2.11aii:
Determine, by calculation, the linear magnification produced in the above diagram.
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19M.3.SL.TZ2.11aii:
Determine, by calculation, the linear magnification produced in the above diagram.
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19M.3.SL.TZ2.aii:
Determine, by calculation, the linear magnification produced in the above diagram.
- 19M.3.SL.TZ2.12biv: A signal consists of a series of pulses. Outline how the length of the fibre optic cable limits...
- 19M.3.SL.TZ2.12biv: A signal consists of a series of pulses. Outline how the length of the fibre optic cable limits...
- 19M.3.SL.TZ2.biv: A signal consists of a series of pulses. Outline how the length of the fibre optic cable limits...
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19M.3.SL.TZ2.12biii:
Explain the shape of the signal you sketched in (b)(ii).
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19M.3.SL.TZ2.12biii:
Explain the shape of the signal you sketched in (b)(ii).
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19M.3.SL.TZ2.biii:
Explain the shape of the signal you sketched in (b)(ii).
- 19M.3.SL.TZ2.11aiii: Suggest an application for the lens used in this way.
- 19M.3.SL.TZ2.11aiii: Suggest an application for the lens used in this way.
- 19M.3.SL.TZ2.aiii: Suggest an application for the lens used in this way.
- 19M.3.SL.TZ2.11bi: Identify, with a vertical line, the position of the focussed image. Label the position I.
- 19M.3.SL.TZ2.11bi: Identify, with a vertical line, the position of the focussed image. Label the position I.
- 19M.3.SL.TZ2.bi: Identify, with a vertical line, the position of the focussed image. Label the position I.
- 19M.3.SL.TZ2.12bii: An input signal to the fibre consists of wavelengths that range from 1299 nm to 1301 nm. The...
- 19M.3.SL.TZ2.12bii: An input signal to the fibre consists of wavelengths that range from 1299 nm to 1301 nm. The...
- 19M.3.SL.TZ2.bii: An input signal to the fibre consists of wavelengths that range from 1299 nm to 1301 nm. The...
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19N.3.SL.TZ0.8c:
Determine, in cm, the focal length of the objective lens.
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19N.3.SL.TZ0.8c:
Determine, in cm, the focal length of the objective lens.
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19N.3.SL.TZ0.c:
Determine, in cm, the focal length of the objective lens.
- 19N.3.SL.TZ0.7a(iii): Describe two features of the image.
- 19N.3.SL.TZ0.7a(iii): Describe two features of the image.
- 19N.3.SL.TZ0.a(iii): Describe two features of the image.
- 19N.3.SL.TZ0.8a: State what is meant by normal adjustment when applied to a compound microscope.
- 19N.3.SL.TZ0.8a: State what is meant by normal adjustment when applied to a compound microscope.
- 19N.3.SL.TZ0.a: State what is meant by normal adjustment when applied to a compound microscope.
- 19N.3.SL.TZ0.7b(i): Sketch, on the diagram, the wavefront of red light passing through point P. Label this wavefront R.
- 19N.3.SL.TZ0.7b(i): Sketch, on the diagram, the wavefront of red light passing through point P. Label this wavefront R.
- 19N.3.SL.TZ0.b(i): Sketch, on the diagram, the wavefront of red light passing through point P. Label this wavefront R.
- 19N.3.SL.TZ0.9a: Describe why a higher data transfer rate is possible in optic fibres than in twisted pair cables.
- 19N.3.SL.TZ0.9a: Describe why a higher data transfer rate is possible in optic fibres than in twisted pair cables.
- 19N.3.SL.TZ0.a: Describe why a higher data transfer rate is possible in optic fibres than in twisted pair cables.
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19N.3.SL.TZ0.9b(ii):
Determine the distance at which the signal must be amplified.
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19N.3.SL.TZ0.9b(ii):
Determine the distance at which the signal must be amplified.
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19N.3.SL.TZ0.b(ii):
Determine the distance at which the signal must be amplified.
- 19N.3.SL.TZ0.9b(i): State one cause of attenuation in the optic fibre.
- 19N.3.SL.TZ0.9b(i): State one cause of attenuation in the optic fibre.
- 19N.3.SL.TZ0.b(i): State one cause of attenuation in the optic fibre.
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19N.3.SL.TZ0.7a(ii):
Estimate the linear magnification of the image.
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19N.3.SL.TZ0.7a(ii):
Estimate the linear magnification of the image.
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19N.3.SL.TZ0.a(ii):
Estimate the linear magnification of the image.
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19N.3.SL.TZ0.7b(ii):
Explain chromatic aberration, with reference to your diagram in (b)(i).
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19N.3.SL.TZ0.7b(ii):
Explain chromatic aberration, with reference to your diagram in (b)(i).
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19N.3.SL.TZ0.b(ii):
Explain chromatic aberration, with reference to your diagram in (b)(i).
- 19N.3.SL.TZ0.7b(iii): An achromatic doublet reduces the effect of chromatic aberration. Describe an achromatic doublet.
- 19N.3.SL.TZ0.7b(iii): An achromatic doublet reduces the effect of chromatic aberration. Describe an achromatic doublet.
- 19N.3.SL.TZ0.b(iii): An achromatic doublet reduces the effect of chromatic aberration. Describe an achromatic doublet.
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19N.3.SL.TZ0.7a(i):
Construct a ray diagram in order to locate the position of the image formed by the mirror. Label the image .
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19N.3.SL.TZ0.7a(i):
Construct a ray diagram in order to locate the position of the image formed by the mirror. Label the image .
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19N.3.SL.TZ0.a(i):
Construct a ray diagram in order to locate the position of the image formed by the mirror. Label the image .
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19N.3.SL.TZ0.8b:
Calculate, in cm, the distance between the eyepiece and the image formed by the objective lens.
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19N.3.SL.TZ0.8b:
Calculate, in cm, the distance between the eyepiece and the image formed by the objective lens.
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19N.3.SL.TZ0.b:
Calculate, in cm, the distance between the eyepiece and the image formed by the objective lens.
- 17N.3.SL.TZ0.10a: Complete the diagram, with a Newtonian mounting, continuing the two rays to show how they pass...
- 17N.3.SL.TZ0.10a: Complete the diagram, with a Newtonian mounting, continuing the two rays to show how they pass...
- 17N.3.SL.TZ0.a: Complete the diagram, with a Newtonian mounting, continuing the two rays to show how they pass...
-
17N.3.SL.TZ0.10b:
When the Earth-Moon distance is 363 300 km, the Moon is observed using the telescope. The mean radius of the Moon is 1737 km. Determine the focal length of the mirror used in this telescope when the diameter of the Moon’s image formed by the main mirror is 1.20 cm.
-
17N.3.SL.TZ0.10b:
When the Earth-Moon distance is 363 300 km, the Moon is observed using the telescope. The mean radius of the Moon is 1737 km. Determine the focal length of the mirror used in this telescope when the diameter of the Moon’s image formed by the main mirror is 1.20 cm.
-
17N.3.SL.TZ0.b:
When the Earth-Moon distance is 363 300 km, the Moon is observed using the telescope. The mean radius of the Moon is 1737 km. Determine the focal length of the mirror used in this telescope when the diameter of the Moon’s image formed by the main mirror is 1.20 cm.
- 17N.3.SL.TZ0.10d: The Hubble Space reflecting telescope has a Cassegrain mounting. Outline the main optical...
- 17N.3.SL.TZ0.10d: The Hubble Space reflecting telescope has a Cassegrain mounting. Outline the main optical...
- 17N.3.SL.TZ0.d: The Hubble Space reflecting telescope has a Cassegrain mounting. Outline the main optical...
-
18M.3.SL.TZ2.8a.i:
determine the focal length of the lens.
-
18M.3.SL.TZ2.8a.i:
determine the focal length of the lens.
-
18M.3.SL.TZ2.a.i:
determine the focal length of the lens.
- 19M.3.SL.TZ2.12a: Outline the differences between step-index and graded-index optic fibres.
- 19M.3.SL.TZ2.12a: Outline the differences between step-index and graded-index optic fibres.
- 19M.3.SL.TZ2.a: Outline the differences between step-index and graded-index optic fibres.
- 20N.3.SL.TZ0.10a: Construct a single ray showing one path of light between the eye, the mirror and the object, to...
- 20N.3.SL.TZ0.10a: Construct a single ray showing one path of light between the eye, the mirror and the object, to...
- 20N.3.SL.TZ0.a: Construct a single ray showing one path of light between the eye, the mirror and the object, to...
- 20N.3.SL.TZ0.10b: The image observed is virtual. Outline the meaning of virtual image.
- 20N.3.SL.TZ0.10b: The image observed is virtual. Outline the meaning of virtual image.
- 20N.3.SL.TZ0.b: The image observed is virtual. Outline the meaning of virtual image.
-
20N.3.SL.TZ0.11a:
Draw on the diagram the three wavefronts after they have passed through the lens.
-
20N.3.SL.TZ0.11a:
Draw on the diagram the three wavefronts after they have passed through the lens.
-
20N.3.SL.TZ0.a:
Draw on the diagram the three wavefronts after they have passed through the lens.
-
20N.3.SL.TZ0.11b:
Lens A has a focal length of . An object is placed to the left of A. Show by calculation that a screen should be placed about from A to display a focused image.
-
20N.3.SL.TZ0.11b:
Lens A has a focal length of . An object is placed to the left of A. Show by calculation that a screen should be placed about from A to display a focused image.
-
20N.3.SL.TZ0.b:
Lens A has a focal length of . An object is placed to the left of A. Show by calculation that a screen should be placed about from A to display a focused image.
-
20N.3.SL.TZ0.11c:
The screen is removed and the image is used as the object for a second diverging lens B, to form a final image. Lens B has a focal length of and the final real image is from the lens. Calculate the distance between lens A and lens B.
-
20N.3.SL.TZ0.11c:
The screen is removed and the image is used as the object for a second diverging lens B, to form a final image. Lens B has a focal length of and the final real image is from the lens. Calculate the distance between lens A and lens B.
-
20N.3.SL.TZ0.c:
The screen is removed and the image is used as the object for a second diverging lens B, to form a final image. Lens B has a focal length of and the final real image is from the lens. Calculate the distance between lens A and lens B.
-
20N.3.SL.TZ0.11d:
Calculate the total magnification of the object by the lens combination.
-
20N.3.SL.TZ0.11d:
Calculate the total magnification of the object by the lens combination.
-
20N.3.SL.TZ0.d:
Calculate the total magnification of the object by the lens combination.
-
20N.3.SL.TZ0.12a:
Outline the meaning of normal adjustment for a compound microscope.
-
20N.3.SL.TZ0.12a:
Outline the meaning of normal adjustment for a compound microscope.
-
20N.3.SL.TZ0.a:
Outline the meaning of normal adjustment for a compound microscope.
Sub sections and their related questions
C.1 – Introduction to imaging
- 17N.3.SL.TZ0.9a.i: Sketch a ray diagram to show how the magnifying glass produces an upright image.
- 17N.3.SL.TZ0.9a.ii: State the maximum possible distance from an object to the lens in order for the lens to produce...
-
17N.3.SL.TZ0.9b.i:
Determine the position of the image.
- 17N.3.SL.TZ0.9b.ii: State three characteristics of the image.
- 17N.3.SL.TZ0.9c.i: On the diagram, draw two rays to locate the point Q′ on the image that corresponds to point Q on...
- 17N.3.SL.TZ0.9c.ii: Calculate the vertical distance of point Q′ from the principal axis.
- 17N.3.SL.TZ0.9c.iii: A screen is positioned to form a focused image of point Q. State the direction, relative to Q, in...
- 17N.3.SL.TZ0.9c.iv: The screen is now correctly positioned to form a focused image of point R. However, the top of...
-
18M.3.SL.TZ1.8a.i:
Identify whether the image is real or virtual.
-
18M.3.SL.TZ1.8a.ii:
The lens is 18 cm from the screen and the image is 0.40 times smaller than the object. Calculate the power of the lens, in cm–1.
-
18M.3.SL.TZ1.8a.iii:
Light passing through this lens is subject to chromatic aberration. Discuss the effect that chromatic aberration has on the image formed on the screen.
-
18M.3.SL.TZ1.8b:
A system consisting of a converging lens of focal length F1 (lens 1) and a diverging lens (lens 2) are used to obtain the image of an object as shown on the scaled diagram. The focal length of lens 1 (F1) is 30 cm.
Determine, using the ray diagram, the focal length of the diverging lens.
-
18M.3.SL.TZ2.8a.i:
determine the focal length of the lens.
-
18M.3.SL.TZ2.8a.ii:
calculate the linear magnification.
-
18M.3.SL.TZ2.8b:
The diagram shows an incomplete ray diagram which consists of a red ray of light and a blue ray of light which are incident on a converging glass lens. In this glass lens the refractive index for blue light is greater than the refractive index for red light.
Using the diagram, outline the phenomenon of chromatic aberration.
-
18M.3.SL.TZ2.9a:
Identify, with the letter X, the position of the focus of the primary mirror.
- 18N.3.SL.TZ0.8a: On the diagram, draw lines to show the rays after they have refracted through the lens. Label the...
-
18N.3.SL.TZ0.8b.i:
Suggest how the refracted rays in (a) are modified when the converging lens is replaced by a diverging lens.
-
18N.3.SL.TZ0.8b.ii:
Hence state how the defect of the converging lens in (a) may be corrected.
-
18N.3.SL.TZ0.9b.i:
Calculate the distance between the lenses.
- 19M.3.SL.TZ2.11ai: Construct rays, on the diagram, to locate the image of this object formed by the lens. Label this...
-
19M.3.SL.TZ2.11aii:
Determine, by calculation, the linear magnification produced in the above diagram.
- 19M.3.SL.TZ2.11aiii: Suggest an application for the lens used in this way.
- 19M.3.SL.TZ2.11bi: Identify, with a vertical line, the position of the focussed image. Label the position I.
-
19N.3.SL.TZ0.7a(i):
Construct a ray diagram in order to locate the position of the image formed by the mirror. Label the image .
-
19N.3.SL.TZ0.7a(ii):
Estimate the linear magnification of the image.
- 19N.3.SL.TZ0.7a(iii): Describe two features of the image.
- 19N.3.SL.TZ0.7b(i): Sketch, on the diagram, the wavefront of red light passing through point P. Label this wavefront R.
-
19N.3.SL.TZ0.7b(ii):
Explain chromatic aberration, with reference to your diagram in (b)(i).
- 19N.3.SL.TZ0.7b(iii): An achromatic doublet reduces the effect of chromatic aberration. Describe an achromatic doublet.
- 19N.3.SL.TZ0.8a: State what is meant by normal adjustment when applied to a compound microscope.
-
19N.3.SL.TZ0.8b:
Calculate, in cm, the distance between the eyepiece and the image formed by the objective lens.
- 20N.3.SL.TZ0.10a: Construct a single ray showing one path of light between the eye, the mirror and the object, to...
- 20N.3.SL.TZ0.10b: The image observed is virtual. Outline the meaning of virtual image.
-
20N.3.SL.TZ0.11a:
Draw on the diagram the three wavefronts after they have passed through the lens.
-
20N.3.SL.TZ0.11b:
Lens A has a focal length of . An object is placed to the left of A. Show by calculation that a screen should be placed about from A to display a focused image.
-
20N.3.SL.TZ0.11c:
The screen is removed and the image is used as the object for a second diverging lens B, to form a final image. Lens B has a focal length of and the final real image is from the lens. Calculate the distance between lens A and lens B.
-
20N.3.SL.TZ0.11d:
Calculate the total magnification of the object by the lens combination.
- 19M.3.SL.TZ2.11ai: Construct rays, on the diagram, to locate the image of this object formed by the lens. Label this...
-
19M.3.SL.TZ2.11aii:
Determine, by calculation, the linear magnification produced in the above diagram.
- 19M.3.SL.TZ2.11aiii: Suggest an application for the lens used in this way.
- 19M.3.SL.TZ2.11bi: Identify, with a vertical line, the position of the focussed image. Label the position I.
- 19M.3.SL.TZ2.ai: Construct rays, on the diagram, to locate the image of this object formed by the lens. Label this...
-
19M.3.SL.TZ2.aii:
Determine, by calculation, the linear magnification produced in the above diagram.
- 19M.3.SL.TZ2.aiii: Suggest an application for the lens used in this way.
- 19M.3.SL.TZ2.bi: Identify, with a vertical line, the position of the focussed image. Label the position I.
-
19N.3.SL.TZ0.7a(i):
Construct a ray diagram in order to locate the position of the image formed by the mirror. Label the image .
-
19N.3.SL.TZ0.7a(ii):
Estimate the linear magnification of the image.
- 19N.3.SL.TZ0.7a(iii): Describe two features of the image.
- 19N.3.SL.TZ0.7b(i): Sketch, on the diagram, the wavefront of red light passing through point P. Label this wavefront R.
-
19N.3.SL.TZ0.7b(ii):
Explain chromatic aberration, with reference to your diagram in (b)(i).
- 19N.3.SL.TZ0.7b(iii): An achromatic doublet reduces the effect of chromatic aberration. Describe an achromatic doublet.
-
19N.3.SL.TZ0.a(i):
Construct a ray diagram in order to locate the position of the image formed by the mirror. Label the image .
-
19N.3.SL.TZ0.a(ii):
Estimate the linear magnification of the image.
- 19N.3.SL.TZ0.a(iii): Describe two features of the image.
- 19N.3.SL.TZ0.b(i): Sketch, on the diagram, the wavefront of red light passing through point P. Label this wavefront R.
-
19N.3.SL.TZ0.b(ii):
Explain chromatic aberration, with reference to your diagram in (b)(i).
- 19N.3.SL.TZ0.b(iii): An achromatic doublet reduces the effect of chromatic aberration. Describe an achromatic doublet.
- 19N.3.SL.TZ0.8a: State what is meant by normal adjustment when applied to a compound microscope.
-
19N.3.SL.TZ0.8b:
Calculate, in cm, the distance between the eyepiece and the image formed by the objective lens.
- 19N.3.SL.TZ0.a: State what is meant by normal adjustment when applied to a compound microscope.
-
19N.3.SL.TZ0.b:
Calculate, in cm, the distance between the eyepiece and the image formed by the objective lens.
- 20N.3.SL.TZ0.10a: Construct a single ray showing one path of light between the eye, the mirror and the object, to...
- 20N.3.SL.TZ0.10b: The image observed is virtual. Outline the meaning of virtual image.
- 20N.3.SL.TZ0.a: Construct a single ray showing one path of light between the eye, the mirror and the object, to...
- 20N.3.SL.TZ0.b: The image observed is virtual. Outline the meaning of virtual image.
-
20N.3.SL.TZ0.11a:
Draw on the diagram the three wavefronts after they have passed through the lens.
-
20N.3.SL.TZ0.11b:
Lens A has a focal length of . An object is placed to the left of A. Show by calculation that a screen should be placed about from A to display a focused image.
-
20N.3.SL.TZ0.11c:
The screen is removed and the image is used as the object for a second diverging lens B, to form a final image. Lens B has a focal length of and the final real image is from the lens. Calculate the distance between lens A and lens B.
-
20N.3.SL.TZ0.11d:
Calculate the total magnification of the object by the lens combination.
-
20N.3.SL.TZ0.a:
Draw on the diagram the three wavefronts after they have passed through the lens.
-
20N.3.SL.TZ0.b:
Lens A has a focal length of . An object is placed to the left of A. Show by calculation that a screen should be placed about from A to display a focused image.
-
20N.3.SL.TZ0.c:
The screen is removed and the image is used as the object for a second diverging lens B, to form a final image. Lens B has a focal length of and the final real image is from the lens. Calculate the distance between lens A and lens B.
-
20N.3.SL.TZ0.d:
Calculate the total magnification of the object by the lens combination.
- 17N.3.SL.TZ0.9a.i: Sketch a ray diagram to show how the magnifying glass produces an upright image.
- 17N.3.SL.TZ0.9a.ii: State the maximum possible distance from an object to the lens in order for the lens to produce...
-
17N.3.SL.TZ0.9b.i:
Determine the position of the image.
- 17N.3.SL.TZ0.9b.ii: State three characteristics of the image.
- 17N.3.SL.TZ0.9c.i: On the diagram, draw two rays to locate the point Q′ on the image that corresponds to point Q on...
- 17N.3.SL.TZ0.9c.ii: Calculate the vertical distance of point Q′ from the principal axis.
- 17N.3.SL.TZ0.9c.iii: A screen is positioned to form a focused image of point Q. State the direction, relative to Q, in...
- 17N.3.SL.TZ0.9c.iv: The screen is now correctly positioned to form a focused image of point R. However, the top of...
- 17N.3.SL.TZ0.a.i: Sketch a ray diagram to show how the magnifying glass produces an upright image.
- 17N.3.SL.TZ0.a.ii: State the maximum possible distance from an object to the lens in order for the lens to produce...
-
17N.3.SL.TZ0.b.i:
Determine the position of the image.
- 17N.3.SL.TZ0.b.ii: State three characteristics of the image.
- 17N.3.SL.TZ0.c.i: On the diagram, draw two rays to locate the point Q′ on the image that corresponds to point Q on...
- 17N.3.SL.TZ0.c.ii: Calculate the vertical distance of point Q′ from the principal axis.
- 17N.3.SL.TZ0.c.iii: A screen is positioned to form a focused image of point Q. State the direction, relative to Q, in...
- 17N.3.SL.TZ0.c.iv: The screen is now correctly positioned to form a focused image of point R. However, the top of...
-
18M.3.SL.TZ1.8a.i:
Identify whether the image is real or virtual.
-
18M.3.SL.TZ1.8a.ii:
The lens is 18 cm from the screen and the image is 0.40 times smaller than the object. Calculate the power of the lens, in cm–1.
-
18M.3.SL.TZ1.8a.iii:
Light passing through this lens is subject to chromatic aberration. Discuss the effect that chromatic aberration has on the image formed on the screen.
-
18M.3.SL.TZ1.8b:
A system consisting of a converging lens of focal length F1 (lens 1) and a diverging lens (lens 2) are used to obtain the image of an object as shown on the scaled diagram. The focal length of lens 1 (F1) is 30 cm.
Determine, using the ray diagram, the focal length of the diverging lens.
-
18M.3.SL.TZ1.a.i:
Identify whether the image is real or virtual.
-
18M.3.SL.TZ1.a.ii:
The lens is 18 cm from the screen and the image is 0.40 times smaller than the object. Calculate the power of the lens, in cm–1.
-
18M.3.SL.TZ1.a.iii:
Light passing through this lens is subject to chromatic aberration. Discuss the effect that chromatic aberration has on the image formed on the screen.
-
18M.3.SL.TZ1.b:
A system consisting of a converging lens of focal length F1 (lens 1) and a diverging lens (lens 2) are used to obtain the image of an object as shown on the scaled diagram. The focal length of lens 1 (F1) is 30 cm.
Determine, using the ray diagram, the focal length of the diverging lens.
-
18M.3.SL.TZ2.8a.i:
determine the focal length of the lens.
-
18M.3.SL.TZ2.8a.ii:
calculate the linear magnification.
-
18M.3.SL.TZ2.8b:
The diagram shows an incomplete ray diagram which consists of a red ray of light and a blue ray of light which are incident on a converging glass lens. In this glass lens the refractive index for blue light is greater than the refractive index for red light.
Using the diagram, outline the phenomenon of chromatic aberration.
-
18M.3.SL.TZ2.a.i:
determine the focal length of the lens.
-
18M.3.SL.TZ2.a.ii:
calculate the linear magnification.
-
18M.3.SL.TZ2.b:
The diagram shows an incomplete ray diagram which consists of a red ray of light and a blue ray of light which are incident on a converging glass lens. In this glass lens the refractive index for blue light is greater than the refractive index for red light.
Using the diagram, outline the phenomenon of chromatic aberration.
-
18M.3.SL.TZ2.9a:
Identify, with the letter X, the position of the focus of the primary mirror.
-
18M.3.SL.TZ2.a:
Identify, with the letter X, the position of the focus of the primary mirror.
- 18N.3.SL.TZ0.8a: On the diagram, draw lines to show the rays after they have refracted through the lens. Label the...
-
18N.3.SL.TZ0.8b.i:
Suggest how the refracted rays in (a) are modified when the converging lens is replaced by a diverging lens.
-
18N.3.SL.TZ0.8b.ii:
Hence state how the defect of the converging lens in (a) may be corrected.
- 18N.3.SL.TZ0.a: On the diagram, draw lines to show the rays after they have refracted through the lens. Label the...
-
18N.3.SL.TZ0.b.i:
Suggest how the refracted rays in (a) are modified when the converging lens is replaced by a diverging lens.
-
18N.3.SL.TZ0.b.ii:
Hence state how the defect of the converging lens in (a) may be corrected.
-
18N.3.SL.TZ0.9b.i:
Calculate the distance between the lenses.
-
18N.3.SL.TZ0.b.i:
Calculate the distance between the lenses.
C.2 – Imaging instrumentation
- 17N.3.SL.TZ0.10a: Complete the diagram, with a Newtonian mounting, continuing the two rays to show how they pass...
-
17N.3.SL.TZ0.10b:
When the Earth-Moon distance is 363 300 km, the Moon is observed using the telescope. The mean radius of the Moon is 1737 km. Determine the focal length of the mirror used in this telescope when the diameter of the Moon’s image formed by the main mirror is 1.20 cm.
- 17N.3.SL.TZ0.10d: The Hubble Space reflecting telescope has a Cassegrain mounting. Outline the main optical...
-
18M.3.SL.TZ2.9b:
This arrangement using the secondary mirror is said to increase the focal length of the primary mirror. State why this is an advantage.
-
18M.3.SL.TZ2.9c:
Distinguish between this mounting and the Newtonian mounting.
-
18M.3.HL.TZ2.13c:
It is proposed to build an array of radio telescopes such that the maximum distance between them is 3800 km. The array will operate at a wavelength of 2.1 cm.
Comment on whether it is possible to build an optical telescope operating at 580 nm that is to have the same resolution as the array.
- 18N.3.SL.TZ0.9a: Draw rays on the diagram to show the formation of the final image.
-
18N.3.SL.TZ0.9b.ii:
Determine the magnification of the microscope.
-
19M.3.SL.TZ2.11bii:
The image at I is the object for a second converging lens. This second lens forms a final image at infinity with an overall angular magnification for the two lens arrangement of 5. Calculate the distance between the two converging lenses.
-
19M.3.SL.TZ2.11biii:
A new object is placed a few meters to the left of the original lens. The student adjusts spacing of the lenses to form a virtual image at infinity of the new object. Outline, without calculation, the required change to the lens separation.
-
19N.3.SL.TZ0.8b:
Calculate, in cm, the distance between the eyepiece and the image formed by the objective lens.
-
19N.3.SL.TZ0.8c:
Determine, in cm, the focal length of the objective lens.
-
20N.3.SL.TZ0.12a:
Outline the meaning of normal adjustment for a compound microscope.
- 20N.3.SL.TZ0.12b: Sketch a ray diagram to find the position of the images for both lenses in the compound...
-
19M.3.SL.TZ2.11bii:
The image at I is the object for a second converging lens. This second lens forms a final image at infinity with an overall angular magnification for the two lens arrangement of 5. Calculate the distance between the two converging lenses.
-
19M.3.SL.TZ2.11biii:
A new object is placed a few meters to the left of the original lens. The student adjusts spacing of the lenses to form a virtual image at infinity of the new object. Outline, without calculation, the required change to the lens separation.
-
19M.3.SL.TZ2.bii:
The image at I is the object for a second converging lens. This second lens forms a final image at infinity with an overall angular magnification for the two lens arrangement of 5. Calculate the distance between the two converging lenses.
-
19M.3.SL.TZ2.biii:
A new object is placed a few meters to the left of the original lens. The student adjusts spacing of the lenses to form a virtual image at infinity of the new object. Outline, without calculation, the required change to the lens separation.
-
19N.3.SL.TZ0.8b:
Calculate, in cm, the distance between the eyepiece and the image formed by the objective lens.
-
19N.3.SL.TZ0.8c:
Determine, in cm, the focal length of the objective lens.
-
19N.3.SL.TZ0.b:
Calculate, in cm, the distance between the eyepiece and the image formed by the objective lens.
-
19N.3.SL.TZ0.c:
Determine, in cm, the focal length of the objective lens.
-
20N.3.SL.TZ0.12a:
Outline the meaning of normal adjustment for a compound microscope.
- 20N.3.SL.TZ0.12b: Sketch a ray diagram to find the position of the images for both lenses in the compound...
-
20N.3.SL.TZ0.a:
Outline the meaning of normal adjustment for a compound microscope.
- 20N.3.SL.TZ0.b: Sketch a ray diagram to find the position of the images for both lenses in the compound...
- 17N.3.SL.TZ0.10a: Complete the diagram, with a Newtonian mounting, continuing the two rays to show how they pass...
-
17N.3.SL.TZ0.10b:
When the Earth-Moon distance is 363 300 km, the Moon is observed using the telescope. The mean radius of the Moon is 1737 km. Determine the focal length of the mirror used in this telescope when the diameter of the Moon’s image formed by the main mirror is 1.20 cm.
- 17N.3.SL.TZ0.10d: The Hubble Space reflecting telescope has a Cassegrain mounting. Outline the main optical...
- 17N.3.SL.TZ0.a: Complete the diagram, with a Newtonian mounting, continuing the two rays to show how they pass...
-
17N.3.SL.TZ0.b:
When the Earth-Moon distance is 363 300 km, the Moon is observed using the telescope. The mean radius of the Moon is 1737 km. Determine the focal length of the mirror used in this telescope when the diameter of the Moon’s image formed by the main mirror is 1.20 cm.
- 17N.3.SL.TZ0.d: The Hubble Space reflecting telescope has a Cassegrain mounting. Outline the main optical...
-
18M.3.SL.TZ2.9b:
This arrangement using the secondary mirror is said to increase the focal length of the primary mirror. State why this is an advantage.
-
18M.3.SL.TZ2.9c:
Distinguish between this mounting and the Newtonian mounting.
-
18M.3.SL.TZ2.b:
This arrangement using the secondary mirror is said to increase the focal length of the primary mirror. State why this is an advantage.
-
18M.3.SL.TZ2.c:
Distinguish between this mounting and the Newtonian mounting.
-
18M.3.HL.TZ2.13c:
It is proposed to build an array of radio telescopes such that the maximum distance between them is 3800 km. The array will operate at a wavelength of 2.1 cm.
Comment on whether it is possible to build an optical telescope operating at 580 nm that is to have the same resolution as the array.
-
18M.3.HL.TZ2.c:
It is proposed to build an array of radio telescopes such that the maximum distance between them is 3800 km. The array will operate at a wavelength of 2.1 cm.
Comment on whether it is possible to build an optical telescope operating at 580 nm that is to have the same resolution as the array.
- 18N.3.SL.TZ0.9a: Draw rays on the diagram to show the formation of the final image.
-
18N.3.SL.TZ0.9b.ii:
Determine the magnification of the microscope.
- 18N.3.SL.TZ0.a: Draw rays on the diagram to show the formation of the final image.
-
18N.3.SL.TZ0.b.ii:
Determine the magnification of the microscope.
C.3 – Fibre optics
-
17N.3.HL.TZ0.15a:
Calculate the maximum angle β for light to travel through the fibre.
Refractive index of core = 1.50
Refractive index of cladding = 1.48 - 17N.3.HL.TZ0.15b: Outline how the combination of core and cladding reduces the overall dispersion in the optic fibres.
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18M.3.SL.TZ1.9a:
Calculate the critical angle at the core−cladding boundary.
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18M.3.SL.TZ1.9b:
The use of optical fibres has led to a revolution in communications across the globe. Outline two advantages of optical fibres over electrical conductors for the purpose of data transfer.
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18M.3.SL.TZ1.9c.i:
Draw on the axes an output signal to illustrate the effect of waveguide dispersion.
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18M.3.SL.TZ1.9c.ii:
Calculate the power of the output signal after the signal has travelled a distance of 3.40 km in the fibre.
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18M.3.SL.TZ1.9c.iii:
Explain how the use of a graded-index fibre will improve the performance of this fibre optic system.
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18M.3.SL.TZ2.10a:
An optic fibre of refractive index 1.4475 is surrounded by air. The critical angle for the core – air boundary interface is 44°. Suggest, with a calculation, why the use of cladding with refractive index 1.4444 improves the performance of the optic fibre.
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18M.3.SL.TZ2.10b.i:
Calculate the maximum attenuation allowed for the signal.
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18M.3.SL.TZ2.10b.ii:
An amplifier can increase the power of the signal by 12 dB. Determine the minimum number of amplifiers required.
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18M.3.SL.TZ2.10b.iii:
The graph shows the variation with wavelength of the refractive index of the glass from which the optic fibre is made.
Two light rays enter the fibre at the same instant along the axes. Ray A has a wavelength of λA and ray B has a wavelength of λB. Discuss the effect that the difference in wavelength has on the rays as they pass along the fibre.
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18M.3.SL.TZ2.10c:
In many places clad optic fibres are replacing copper cables. State one example of how fibre optic technology has impacted society.
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18N.3.SL.TZ0.10a.i:
Calculate n.
- 18N.3.SL.TZ0.10a.ii: The refractive indices of the glass and cladding are only slightly different. Suggest why this is...
-
18N.3.SL.TZ0.10b.i:
Show that the longest path is 66 m longer than the shortest path.
-
18N.3.SL.TZ0.10b.ii:
Determine the time delay between the arrival of signals created by the extra distance in (b)(i).
- 18N.3.SL.TZ0.10b.iii: Suggest whether this fibre could be used to transmit information at a frequency of 100 MHz.
- 19M.3.SL.TZ2.12a: Outline the differences between step-index and graded-index optic fibres.
- 19M.3.SL.TZ2.12bii: An input signal to the fibre consists of wavelengths that range from 1299 nm to 1301 nm. The...
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19M.3.SL.TZ2.12biii:
Explain the shape of the signal you sketched in (b)(ii).
- 19M.3.SL.TZ2.12biv: A signal consists of a series of pulses. Outline how the length of the fibre optic cable limits...
- 19N.3.SL.TZ0.9a: Describe why a higher data transfer rate is possible in optic fibres than in twisted pair cables.
- 19N.3.SL.TZ0.9b(i): State one cause of attenuation in the optic fibre.
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19N.3.SL.TZ0.9b(ii):
Determine the distance at which the signal must be amplified.
- 20N.3.SL.TZ0.13: A single pulse of light enters an optic fibre which contains small impurities that scatter the...
- 19M.3.SL.TZ2.12a: Outline the differences between step-index and graded-index optic fibres.
- 19M.3.SL.TZ2.12bii: An input signal to the fibre consists of wavelengths that range from 1299 nm to 1301 nm. The...
-
19M.3.SL.TZ2.12biii:
Explain the shape of the signal you sketched in (b)(ii).
- 19M.3.SL.TZ2.12biv: A signal consists of a series of pulses. Outline how the length of the fibre optic cable limits...
- 19M.3.SL.TZ2.a: Outline the differences between step-index and graded-index optic fibres.
- 19M.3.SL.TZ2.bii: An input signal to the fibre consists of wavelengths that range from 1299 nm to 1301 nm. The...
-
19M.3.SL.TZ2.biii:
Explain the shape of the signal you sketched in (b)(ii).
- 19M.3.SL.TZ2.biv: A signal consists of a series of pulses. Outline how the length of the fibre optic cable limits...
- 19N.3.SL.TZ0.9a: Describe why a higher data transfer rate is possible in optic fibres than in twisted pair cables.
- 19N.3.SL.TZ0.9b(i): State one cause of attenuation in the optic fibre.
-
19N.3.SL.TZ0.9b(ii):
Determine the distance at which the signal must be amplified.
- 19N.3.SL.TZ0.a: Describe why a higher data transfer rate is possible in optic fibres than in twisted pair cables.
- 19N.3.SL.TZ0.b(i): State one cause of attenuation in the optic fibre.
-
19N.3.SL.TZ0.b(ii):
Determine the distance at which the signal must be amplified.
- 20N.3.SL.TZ0.13: A single pulse of light enters an optic fibre which contains small impurities that scatter the...
-
17N.3.HL.TZ0.15a:
Calculate the maximum angle β for light to travel through the fibre.
Refractive index of core = 1.50
Refractive index of cladding = 1.48 - 17N.3.HL.TZ0.15b: Outline how the combination of core and cladding reduces the overall dispersion in the optic fibres.
-
17N.3.HL.TZ0.a:
Calculate the maximum angle β for light to travel through the fibre.
Refractive index of core = 1.50
Refractive index of cladding = 1.48 - 17N.3.HL.TZ0.b: Outline how the combination of core and cladding reduces the overall dispersion in the optic fibres.
-
18M.3.SL.TZ1.9a:
Calculate the critical angle at the core−cladding boundary.
-
18M.3.SL.TZ1.9b:
The use of optical fibres has led to a revolution in communications across the globe. Outline two advantages of optical fibres over electrical conductors for the purpose of data transfer.
-
18M.3.SL.TZ1.9c.i:
Draw on the axes an output signal to illustrate the effect of waveguide dispersion.
-
18M.3.SL.TZ1.9c.ii:
Calculate the power of the output signal after the signal has travelled a distance of 3.40 km in the fibre.
-
18M.3.SL.TZ1.9c.iii:
Explain how the use of a graded-index fibre will improve the performance of this fibre optic system.
-
18M.3.SL.TZ1.a:
Calculate the critical angle at the core−cladding boundary.
-
18M.3.SL.TZ1.b:
The use of optical fibres has led to a revolution in communications across the globe. Outline two advantages of optical fibres over electrical conductors for the purpose of data transfer.
-
18M.3.SL.TZ1.c.i:
Draw on the axes an output signal to illustrate the effect of waveguide dispersion.
-
18M.3.SL.TZ1.c.ii:
Calculate the power of the output signal after the signal has travelled a distance of 3.40 km in the fibre.
-
18M.3.SL.TZ1.c.iii:
Explain how the use of a graded-index fibre will improve the performance of this fibre optic system.
-
18M.3.SL.TZ2.10a:
An optic fibre of refractive index 1.4475 is surrounded by air. The critical angle for the core – air boundary interface is 44°. Suggest, with a calculation, why the use of cladding with refractive index 1.4444 improves the performance of the optic fibre.
-
18M.3.SL.TZ2.10b.i:
Calculate the maximum attenuation allowed for the signal.
-
18M.3.SL.TZ2.10b.ii:
An amplifier can increase the power of the signal by 12 dB. Determine the minimum number of amplifiers required.
-
18M.3.SL.TZ2.10b.iii:
The graph shows the variation with wavelength of the refractive index of the glass from which the optic fibre is made.
Two light rays enter the fibre at the same instant along the axes. Ray A has a wavelength of λA and ray B has a wavelength of λB. Discuss the effect that the difference in wavelength has on the rays as they pass along the fibre.
-
18M.3.SL.TZ2.10c:
In many places clad optic fibres are replacing copper cables. State one example of how fibre optic technology has impacted society.
-
18M.3.SL.TZ2.a:
An optic fibre of refractive index 1.4475 is surrounded by air. The critical angle for the core – air boundary interface is 44°. Suggest, with a calculation, why the use of cladding with refractive index 1.4444 improves the performance of the optic fibre.
-
18M.3.SL.TZ2.b.i:
Calculate the maximum attenuation allowed for the signal.
-
18M.3.SL.TZ2.b.ii:
An amplifier can increase the power of the signal by 12 dB. Determine the minimum number of amplifiers required.
-
18M.3.SL.TZ2.b.iii:
The graph shows the variation with wavelength of the refractive index of the glass from which the optic fibre is made.
Two light rays enter the fibre at the same instant along the axes. Ray A has a wavelength of λA and ray B has a wavelength of λB. Discuss the effect that the difference in wavelength has on the rays as they pass along the fibre.
-
18M.3.SL.TZ2.c:
In many places clad optic fibres are replacing copper cables. State one example of how fibre optic technology has impacted society.
-
18N.3.SL.TZ0.10a.i:
Calculate n.
- 18N.3.SL.TZ0.10a.ii: The refractive indices of the glass and cladding are only slightly different. Suggest why this is...
-
18N.3.SL.TZ0.10b.i:
Show that the longest path is 66 m longer than the shortest path.
-
18N.3.SL.TZ0.10b.ii:
Determine the time delay between the arrival of signals created by the extra distance in (b)(i).
- 18N.3.SL.TZ0.10b.iii: Suggest whether this fibre could be used to transmit information at a frequency of 100 MHz.
-
18N.3.SL.TZ0.a.i:
Calculate n.
- 18N.3.SL.TZ0.a.ii: The refractive indices of the glass and cladding are only slightly different. Suggest why this is...
-
18N.3.SL.TZ0.b.i:
Show that the longest path is 66 m longer than the shortest path.
-
18N.3.SL.TZ0.b.ii:
Determine the time delay between the arrival of signals created by the extra distance in (b)(i).
- 18N.3.SL.TZ0.b.iii: Suggest whether this fibre could be used to transmit information at a frequency of 100 MHz.