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INFORMATION/FAQs (Frequently Asked Questions)

The following page is dedicated to information provided to users to better help them understand and operate their instruments.

There are four sections below - Please click on the one you want

Microscopes

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Choosing a Microscope
Microscope FAQs
Cleaning a Microscope
Lubrication
Slipping stage
Setting Koehler Illumination

The Basics of Light Microscopy
Objective Lenses
Transmitted Light Microscopy
Phase Microscopy
More on Koehler Illumination
Terminology/Definitions


Choosing A Microscope

Your application is the most important factor in choosing a microscope. What you need to see and what you want to do with that image will determine what kind of microscope you need.

The most common is the compound microscope. It is the one most people visualize when they think about microscopes. It comes with one eyepiece called a monocular; two eyepieces called a binocular or it might have an additional camera tube and is called a trinocular. It has a number of objectives (the lens closest to the object being viewed) of varying magnification mounted in a rotatable nosepiece. It uses a light source beneath the stage to illuminate slides. These microscopes are generally used to view very small objects such as cells or bacterium. Magnification of these scopes range from 40X up to 1000X. Actual magnification can be figured by multiplying the power of the eyepiece by the power of the objective lens.

The other type of microscope is called a stereo or dissecting microscope. It uses two eyepieces and two paired objectives. There are models that have full zooming capability and models that just have only two magnification settings. It is particularly useful for biologists performing dissections, technicians building or repairing circuit boards, paleontologists cleaning and examining fossils or any one who needs to work with their hands on small objects. It may use a built in light source from above, below, or none at all. Magnification is usually much less than that of a compound microscope, but is figured in the same way.


Microscope FAQ's 

These FAQ's are here for your use. If you would like to contribute microscope information please contact us. Check back often, we will be adding more information as time goes on.

1. Question: What can I use to clean the lens on my microscope?
Answer: Lens cleaning fluids are the best. Use lens paper if available. The type for reading glasses works well. I suggest not using kleenex-type tissue as it is very "dusty" and will leave a lot of lint on the lens. Make sure the first tissue is wet with lens cleaner in case there are bits of glass from the slides on the lens that scratch it.

2. Question: What do I use to clean the body of the microscope?
Answer: I have tried many products over the years but have found that 409 cleaner seems to do the best job and does not damage the finish. Try not to get it into the bearings on the stage or focus assembly as it will dilute the lubrication.

3. Question: Lint seems to be a real problem on the eyepieces. How do I remove it without always having to use lens cleaner and papers?
Answer: Get some canned air from a computer or office supply store. Spray the compressed air at the eyepieces and that should remove most of the dust. Do not shake the can as you spray because you will cause the propellant in the can to come out of the nozzle and coat the lens. Then you will have to use the lens cleaner to remove this coating. Just hold the can still and spray. Remember that a lot of the particles you see on the eyepieces are from your eyes. They are flakes of dead skin that drop off your eyelids every time you blink.

4. Question: It is hard to see through the 40X or the 100X objectives. What could be the problem?
Answer: On most microscopes the 40X and 100X objective's front lens is slightly concave in design. This causes problems when users go to clean the objective. If you only use lens paper and cleaner you will not get to the contamination that has built up in the concave portion of the objective. My recommendation is to use a soft cotton swab (Q-tip). First, wet it with the lens cleaner and use a soft drilling type motion right into the concave portion of the front lens. Next, use a dry swab and use the same type motion to dry the lens. You may have to perform several repetitions of this procedure to truly clean the lens. If this does not help then you may have oil inside of the objective itself. If this happens you might have to replace the objective with a new one. The reason the oil penetrates the objective is due to either not cleaning off the oil after usage or leaving the objective in oil on the slide after reading it. Always clean the oil off the objective after use.

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5. Question: What product should I use to lubricate the bearings on the stage of the microscope?
Answer: Each manufacture has it's own line of lubrications they recommend. If you bought everyone for each product it would be extremely expensive. We use a product called Super Lube made by Permatex. It should be available from many stores in your area. We use this product on all brands

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6. Question: My stage seems to slip down out of focus for no reason. What can I do to prevent this?
Answer: There are two main reasons for this problem. Either the tension control is too loose, or the main bearing system in the stage mechanics needs some adjustments. We will just review the first problem dealing with the tension control. The second problem should be dealt with by a qualified microscope repair technician.

Many microscopes have focus tension controls attached next to the coarse focus control. This control may be the simple type that you can adjust by just using your hand, or it may take a special tool. On the Olympus or Nikon scopes the adjustment is usually on the right side of the scope as the stage faces the user. It is a thin control knob or disc that is placed between the microscope stand and the coarse focus control. All you have to do is turn this device one way or the other and it will increase or decrease the tension on the coarse focus control knob. This in turn will keep the stage from slipping down. Make sure you are not turning the stage lock control, which is normally on the opposite side of the tension controller. If your scope takes a special tool to adjust the tension and you have lost this tool you will have to contact the scope manufacture or the company you purchased your scope from and request a tool.

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One confusing point when shopping for a microscope is the reference to the word Stereo. This does not refer to having two eyepieces. That is called binocular. Monocular means one eyepiece. Trinocular means that you have two standard eyepieces and one extra port or access for viewing your material. This extra port is generally used to mount some type of camera device such as a 35mm, polaroid-type or video camera.

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7. Question: I have heard of the term Koehler illumination. What is it and what does it do for the microscope?
Answer: Koehler Illumination is a process which provides optimum contrast and resolution by focusing and centering the light path and spreading the light evenly over the field of view. All microscopes do not have the ability to be setup for Koehler. They must have a field diaphram and controls to adjust the substage condenser to complete the alignment. Using the following setup, Koehler Illumination can greatly compliment the operation of your microscope by improving the specimen contrast.

a. Rotate to the 10X objective.
b. Close the condenser aperture diaphram by turning the control to the right.
c. Raise the condenser with the condenser focus knob.
d. Close the field diaphram to it's smallest opening with the field diaphram control.
e. Focus the field diaphram image with the condenser focus knob until the edges on the octagonal images are sharp.
f. Center the diaphram image with the condenser centering screws. This centers the light path onto the specimen plane.
g. Switch to desired objective.
h. Enlarge the field diaphram image toward edge of the field of view with the field diaphram control.
i. Recenter the field diaphram image.
j. Further enlarge the field diaphram image until it is just outside the field of view. This provides enough light to fully and evenly cover the observation area.
k. Remove the right eyepiece and look down the eyepiece tube. The circular beam of light is the image of the condenser.
l. Adjust the condenser diaphram with the condenser diaphram control until the beam fills 3/4 of the tube (1/4 of the area will be dark and 3/4 will be light).
m. Replace the eyepiece.
n. Adjust the light intensity with the brightness control.

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We want to thank the UCLA BRAIN RESEARCH INSTITUTE MICROSCOPY CORE FACILITIES for permission to reprint the following information.

The Basics of Light Microscopy

• The Basics
Modern biologists work with fairly small components of living organisms, tissues, cells and biomolecules. To actually see them, one needs optical instruments which can magnify (or more properly, make magnified images) of these components. The compound microscope is the instrument designed for this task.
The Compound Microscope
To magnify an image, one needs a magnifier or a lens, a piece of glass which makes everything appear larger. But there is a limit to how far a simple magnifier can make things bigger; that is about 8-10-fold. Lenses must be added, one behind another, (compounded) to increase this magnification. Then one can magnify the image up to 2000 times life size. The classic compound microscope magnifies in two steps: first with an objective lens which produces an enlarged image of the object in an "intermediate" image plane. This intermediate image is then magnified by the ocular lens or eyepiece.
In the modern research microscopes made in the past ten years, another improvement has been made in the lens system of the compound microscope. In these microscopes, the objective lens is made to project its image at an infinite distance, hence the name infinity-corrected optics (infinity color-corrected system, ICS). In these microscopes, a tube lens is added to support the objective; it forms the intermediate image for ocular magnification. This means that after the objective lens, the light rays are all parallel until they reach the tube lens. This allows one to place other optical components (fluorescence filters, dichroic mirrors, polarizers) without disturbing the light path. That means that there is no need to add even more optics to correct for aberrations in light path that such components could introduce.


• OBJECTIVE LENSES

How does one go about properly selecting an objective for a microscopic task at hand? The first consideration is the type and size of the specimen. What microscopic technique is to be employed and how large do you wish to magnify the specimen? Magnification is fairly simple and straightforward. We all know that 10X means that the objective lens has an effective magnification of ten times life size and when combined in the compound with a 10X ocular lens will give a final magnification of 100X (10 X 10). But what are all the other markings on the lens and how can they help us in selecting the objective lens suited to our needs?

This section covers this subject because knowledge of the markings on an objective will give you the information concerning its proper use and whether it is suitable for the microscopic task you have in mind.

Lens Type. The first thing that most lenses have is some lettering such as Plan-Neofluar, Plan Fluotar, Planapochromat, Plan or Achroplan. These are all different types of objective which have many glass, fluorite, or quartz elements for light path corrections. The types of lenses listed here are based on the Zeiss objectives as the Facility microscope is a Zeiss LSM 310. However, the names listed here should allow you to determine the type of objective from any manufacturer. If not, you will have to contact the manufacturer to explain the name and markings.


1. The term Plan stands for flat field. Lenses which are uncorrected for flatness of field will have the center of the field in focus and the outer edges out of focus (or vice versa depending on how you focus the lens). So Plan means the lens is corrected to allow the whole field to be in focus. Achroplans are best for transmitted light while Epiplans are designed for reflected light use. Some microscope manufacturers will list their flat field achromatic lenses as simply "Plan".


2. Achromat lenses have good color correction for two wavelenths of light. They are budget priced lenses. Planachromats are achromats with correction for flatness of field as well as the aforementioned color correction.


3. Plan-Neofluar or Plan-Fluotar lenses are semiapochromatic lenses. They have good color correction for at least three wavelengths and also have the all around flatness of field. They are excellent for polarization microscopic techniques such as differential interference. As they also transmit UV very well, they are excellent lenses for all types of fluorescence microscopy. Any lens with the term fluar in it has fluorite elements in it and all of these are very good for fluorescence work.


4. Zeiss recently introduced a new line of semiapochromatic lenses named Fluar lenses. These are objectives without a flat field made especially to increase the brightness of fluorescence. The image from a fluar lens is approximately 10% brighter than the equivalent Plan-Neofluar. In the UV range, the light transmission increases by 25-50%. This line of objective lenses was introduced about two years ago.


5. Apochromatic lenses (Planapochromat)are the most highly color corrected objectives: they are corrected for four wavelengths and are top of the line in objective lenses. These most often have the highest numerical apertures (see below). Be careful in using these lenses for fluorescence, however. They do not transmit UV light. They work very well for visible light excitation in the blue and green ranges.

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Immersion. Lenses will be marked for the immersion medium in which they are designed to be used:


1. (Oel) or (Oil) for oil.
2. (W) for water immersion.
3. (Imm) Multi-immersion, for oil, water, and glycerin.


Phase marking. If the lens has a phase ring and can be used for darkphase illumination, the lens will be marked above the lens type with a "Ph" followed by a number corresponding to the manufacturer's phase ring number system for matching to a ring in the condenser. Phase lenses are generally not as good for fluorescence applications as the light transmission is reduced by the presence phase ring inside the lens.
Magnification. As stated before, this is obvious and self-explanatory.
Numerical Aperture. After the imprint of the magnification on any quality objective lens, there is usually a slash followed by a number which may be anything from 0.035 to 1.4. This number is the numerical aperture (N.A.) of the lens. This number is directly related to the resolution and second, for those of you doing fluorescence microscopy, it is related to the amount of brightness of the specimen brought into the lens (obviously very important for fluorescence microscopy!) The higher the N.A. of a lens the better its resolving power and the brighter the image it can produce. Resolution is defined as the ability of a lens to distinguish between small objects. Obviously, this differs greatly from magnification which is just the ability of the lens to enlarge the image of an object. It does not mean that you will necessarily be able to resolve details in the object.

Tube Length and Coverslip Thickness. The marks on the line below the the magnification and the numerical aperture are the tube length/coverslip thickness. The mechanical tube length (between the objective flange and the eyepiece seating face) is normally 160 (in mm) for older objective lenses or ( infinity for infinity-corrected objectives). The number after the slash is the thickness in millimeters of the cover glass for which the objective was designed and corrected. For most objectives for close working distance, this number is 0.17. This designation means that you should use No. coverglasses which range between 0.16 and 0.19 mm in thickness. No. 0, 1, and 2 coverglasses are not recommended. Some lenses will have a - sign. This means that the objective is meant to be used with no coverglass. LD (long working distance) objectives may go up to 1.5 mm so that one may look through slides or tissue culture flasks or dishes.
Some lenses will also have a rotatable ring which allows one to correct for a coverslip thickness. They are sometimes labeled with "Korr."

• Transmitted Light Microscopy


Transmitted light microscopy is the general term used for any type of microscopy where the light is transmitted from a source on the opposite side of the specimen from the objective. Usually the light is passed through a condenser to focus it on the specimen to get very high illumination. After the light passes through the specimen, the image of the specimen goes through the objective lens and to the oculars where the enlarged image is viewed.

Transmitted light microscopic techniques were the first ones developed as the microscope was being developed.

The microscopic techniques requiring a transmitted light path include brightfield, darkfield, Zernicke phase (or just phase) and differential interference contrast (or Nomarski) optics. Other not as commonly used transmitted light techniques include Hoffman modulation, Varel optics, and polarization optics.

In order to get a usable image in the microscope, the specimen must be properly illuminated. The light path of the microscope must be properly set up for each optical method and the components used for image generation. The condenser was invented to concentrate the light on the specimen in order to obtain a bright enough image to be useful. Different ways of setting up the light path were worked out. But the best setup for proper specimen illumination and image generation is known as Köhler illumination after the man who invented it. It is used for most of the optical setups listed above.

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• HOW TO SET UP A MICROSCOPE PROPERLY FOR TRANSMITTED LIGHT ILLUMINATION:
KÖHLER ILLUMINATION


In order to get the best image possible from brightfield, phase contrast, differential interference contrast, or polarization optical setups with the light microscope, it is crucial that the light path be set up properly.

The method for doing this is called Köhler illumination after August Köhler, the man who invented it. It is also know as double diaphragm illumination because it employs both a field and an aperture iris diaphragm to set up the illumination. If the light path is set up properly, you will have the advantages of an evenly illuminated field, a bright image without glare and minimum heating of the specimen.

The following instructions apply to any microscope, upright or inverted which is equipped for transmitted light bright field illumination. Focussing of the field diaphragm as discussed here should be done for phase and differential interference optics as well.

• To set up Köhler illumination:
1. Switch on the light source and make sure that light is coming through the field diaphragm at the base (upright microscope) or the top (inverted microscope) of the microscope stand. It may help to place a piece of paper over the field stop to see the light.
Place your specimen on the stage and turn the nosepiece (which holds the objective lenses) to the 10X or 20X lens. Open the field diaphragm as far as it will go.


2. Notice whether or not your specimen is illuminated. It will help to place a piece of paper over the top of the specimen to see if light is getting through to it. If you are using the brightfield condenser stop, open the iris diaphragm (or aperture diaphragm) on the condenser turret (which contains the stops for brightfield and phase, etc) wide open to give the maximum illumination. If there is a swing-in front lens for the condenser (directly above (inverted) or below (upright) the specimen), you may need to swing it into the light path.
The front lens should be about 1-3 mm above or below the specimen. There are condenser focussing knobs to do this.


3. Now bring your specimen into focus with the coarse and fine focussing knobs. The best way to do this is to rack the lens as close possible to the specimen watching the objective lens all the time(and NOT looking into the oculars) to make sure that the lens does not run into the slide. Then rack the lens away from the stage (or vice versa) while looking through the oculars to bring the specimen into focus (details are as sharp as they can be). If the light is too bright, reduce it with the rheostat on the light source.


4. When the specimen is in focus, start to close the field diaphragm and also begin to carefully move the condenser up and down with the condenser focussing knobs. Look for a sharp image of the edge of the field diaphragm. This may be a little with a long working distance condenser. Also, if the iris diaphragm in the condenser turret is open wide, the glare may obscure the edge of the field diaphragm silhouette somewhat. Furthermore, you may find that this edge is not centered.


5. When the edge of the field diaphragm silhouette is sharply defined, center it with the two knobs (usually knurled knobs) coming out diagonally from the condenser. Close down the field diaphragm most or all the way to get it centered properly. When it is centered, open the field diaphragm until its edge is outside the field. If you are doing brightfield or differential interference microscopy, do not yet open the field diaphragm.


6. As stated before, you may notice some glare around the edge of the field diaphragm, that the edge area outside the edge is not completely dark like the outer part of the whole field as you should see it now. This glare comes from light bouncing around in the light path and going in and illuminating the specimen in such a way as to obscure detail in the specimen. To reduce this glare, close down the iris aperture in the condenser turret until all of the dark area outside of the field stop silhouette is evenly dark. Now open up the field diaphragm until the edge of the diaphragm silhouette is outside the field of view. You should also now be able to turn up the light at the power source.


7. Your specimen should be properly illuminated and should give you a great image. If it does not, check to make sure your lenses and other optical components are clean. Then recheck to see that you have followed each step properly.

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• Phase Microscopy


Phase or dark phase or Zernicke phase microscopy is a microscopic method which allows the viewing of unstained specimens by using the light phase amplitude differences within microscopic objects. When an unstained biological specimen is observed in the normal brightfield microscope, it is quite difficult to see because most biological material is uncolored and transparent. To overcome this problem without staining or otherwise treating the specimen, microscopists have used a trick to change the amplitude or brightness of the light passing through the specimen. The amplitude of a light wave was discussed earlier . Amplitude can be changed in two ways. First, it can be reduced by placing a neutral density filter in the light path. This is not very useful because all the light, that passing through the object as well as the background light, is reduced the same amount. If one looks at an unstained specimen, it is difficult to see without altering the amplitude of the light passing through it making darker or lighter relative to the background. However, the second way that the amplitude can be altered adoes allow to create differences in brightness between the object and the background. This is by making use of phase differences of the light. When a light wave passes through an object, it is deviated, that is, it becomes phase retarded or phase shifted.

 




Refractometers

Refraction

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How Does It Work

Principals of Refractometers
Transparent Systems

Reflection Systems

About the Brix Scale



How does it work

Water is placed in a reservoir. When a pencil is dipped into the water, the tip appears bent. Now put concentrated sugar water into a cup and try the same thing. The tip of the pencil should appear even more bent. This is the phenomenon of light refraction. Refractometers are measuring instruments in which this phenomenon of light refraction is put to practical use. They are based on the principal that as the density of a substance (e.g. when sugar is dissolved in water), it's refractive index rises proportionately.

Water Concentrated
Sugar Water

Principals of Refractometers


When a straw is placed into a glass of water, the straw appears bent. Now if a straw is placed in a glass with water containing dissolved sugar, the straw should appear even more bent (see illustrations). This phenomenon is known as the principle of light refraction. Refractometers are measuring instruments which put this phenomenon of light refraction to practical use. They are based on the principle that as the density of a substance increases (e.g. when sugar is dissolved in water), its refractive index (how much the straw appears bent) rises proportionately. Refractometers were devised by Dr. Ernst Abbe, a German/Austrian scientist in the early 20th century.

The prism in a refractometer has a greater refractive index than the sample solution. Measurements are read at the point where the prism and solution meet. With a low concentration solution, the refractive index of the prism is much greater than that of the sample, causing a large refraction angle and a low reading. The reverse (lower refraction angle and higher reading) would happen with a highly concentrated solution.

There are two detection systems for refractive index: transparent systems and reflection systems. Hand-held refractometers and Abbe refractometers use transparent systems, while digital refractometers use reflection systems.

There are two detection systems for refractive index: transparent systems and reflection systems. Hand-held refractometers and Abbe refractometers use transparent systems, while digital refractometers use reflection systems.

Transparent Systems
The detection system for hand-held refractometers (transparent system) is summarized below.

1. In the figure below the detection is done by utilizing the refractive phenomenon produced on the boundary of the prism and sample. The refractive index of the prism is much larger than that of the sample
2. If the sample is thin, the angle of refraction is large (see "a") because of the large difference in refractive index between the prism and the sample.
3. If the sample is thick, the angle of refraction is small (see "b") because of the small difference in refractive index between the prism and the sample.

 

Reflection Systems

In the figure below, Light A, being incident from the lower left of the prism, is not reflected back by the boundary, but exits through the sample. Light B is reflected by the boundary face to the right, directly along the prism boundary. Light C, having an incident angle too large to be let through to the sample side, is totally reflected toward the lower right of the prism.

As a result, a boundary line is produced dividing light and dark fields on either side of the dotted line "B' " in the figure. Since the angle of reflection of this boundary line is proportional to refractive index, the position of the boundary line between light and dark fields is caught by a sensor and converted into refractive index.

About the Brix ( % ) Scale
The Brix (%) shows the concentration percentage of the soluble solids content in a sample (water solution). The soluble solids content is the total of all the solids dissolved in the water, including sugar, salts, protein, acids, etc., and the measurement reading is the sum total of these. Basically, Brix (%) is calibrated to the number of grams of cane sugar contained in 100g of cane sugar solution. So, when measuring a sugar solution, Brix (%) should perfectly match the actual concentration. With solutions containing other components, especially when one wants to know the exact concentration, a conversion chart is necessary.

 

 




POLARIMETERS
How Polarimeters Work


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The Simple Explanation
Imagine tying a piece of thick rope to a hook in a wall, and then shaking the rope vigorously. The rope will be vibrating in all possible directions - up-and-down, side-to-side, and all the directions in-between - giving it a really complex overall motion.

Now, suppose you passed the rope through a vertical rectangular hole, like this: []. The rope has a really thight fit in the hole. The only vibrations still happening at the other side of the hole will be vertical ones. All the others will have been prevented by the hole.

What emerges from the hole could be described as "plane polarised rope", because the vibrations are only in a single (vertical) plane.
Now look at the possibility of putting a second hole on the rope. If it is aligned the same way as the first one, the vibrations will still get through.

But if the second hole is at 90° to the first one (so horizontally), the rope will stop vibrating entirely to the right of the second hole. The second hole will only let through horizontal vibrations - and there aren't any.

Light is also made up of vibrations - this time, electromagnetic ones. Some materials have the ability to screen out all the vibrations apart from those in one plane and so produce plane polarised light.
The most familiar example of this is the material that Polaroid sunglasses are made of. If you wear one pair of Polaroid sunglasses and hold another pair up in front of them so that the glasses are held vertically rather than horizontally, you'll find that no light gets through - you will just see darkness. This is equivalent to the two holes at right angles in the rope analogy. The polaroids are described as being "crossed".
(This not exactly the way Polaroid glasses work, but it gives a good idea).

A polarimeter works the same way: You have two polaroid glasses, like the two holes with the rope, one glass is the polariser, the other glass is the analyser. The polariser ensures that only a beam of polarised monochromatic light (light of only a single frequency - in other words a single colour) is passed through the solution behind the polariser. After the tube with the solution is the analyser.
The polarimeter is originally set up with water in the tube. Water isn't optically active - it has no effect on the plane of polarisation. The analyser is rotated until you can't see any light coming through the instrument. The polaroids are then "crossed".

An optically active substance is a substance which can rotate the plane of polarisation of plane polarised light. If you shine the polarised monochromatic light through a solution with an optically active substance, then light emerges: its plane of polarisation is found to have rotated. The substance rotates the plane of polarisation of the light, and so the analyser won't be at right-angles to it any longer and some light will get through. You would have to rotate the analyser in order to cut the light off again.
The rotation may be either clockwise or anti-clockwise. Assuming the original plane of polarisation was vertical, you can easily tell whether the plane of polarisation has been rotated clockwise or anti-clockwise, and by how much.

 

More detailed explanation

Light waves as it travels. As shown in Figure 1, light may seem to travel unidirectionally. In actuality light travels in all directions as shown in Figure 2.


When light, which waves in all directions, goes through a grating placed in its course of travel, only the light wave that oscillates in the direction parallel to the bars of the grating passes through, Light waves that oscillate in other directions get blocked by the bars of the grating. ( Figure 3 ) Such light, which waves in one particular direction, is called polarized light, and the grating is called a polarizing plate.


When polarized light travels through an observation tube filled with a sample solution that does not make light rotate ( water, for example ) , the light continues to wave in the same direction even after passing through the solution. ( Figure 4 )

In contrast, when it travels through an observation tube filled with a sample solution that makes light rotate ( sucrose solution, for example ) , the light wave begins to rotate as it passes through the solution. ( Figure 5 ) This is called optical rotation.

Those samples that make light rotate have a molecular formula that contains asymmetric carbon ( indicated by "C" ) . Sugar is the most common. The explanation of the asymmetric carbon can be highly technical.Discussion on asymmetric carbon will be discussed in a later section.

Imagine making a light path by placing a polarizing plate, an observation tube, another polarizing plate, and a sensor one after another. ( Figure 6 and 7 )
The path in Figure 6 has an observation tube filled with water, in Figure 7 a sample solution, such as sucrose solution, that makes light rotate.


In Figure 6 a certain amount of light reaches the sensor.

In Figure 7 the light does not reach the sensor. ( Technically speaking, in terms of a vector an imperceptible amount of light does reach the sensor, but let's assume that the light does not reach the sensor here. )

When the second polarizing plate is rotated as shown in Figure 8, the same amount of light as in Figure 6 now reaches the sensor.


Conducting Zero-Setting on a Polarimeter
Conduct zero-setting in the step shown in Figure 6. In the actual adjustment procedure, the observation tube filled with water is not necessary and zero-setting is conducted by letting light travel through the air. Next, place an observation tube filled with a sample solution that makes light rotate as shown in Figure 8. Rotate the second polarizing plate so that the equal amount of light reaches the sensor as it did when zero-setting was conducted. The measured angle of the rotated polarizing plate is the angle of rotation of the sample solution.


 

 

 

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