Source: Mahamdeh, M., et al. Implementation of Interference Reflection Microscopy for Label-free, High-speed Imaging of Microtubules. J. Vis. Exp. (2019).
In this video, we describe the interference reflection microscopy (IRM) technique to visualize microtubules growing on a coverslip surface in the presence of a suitable buffer. Upon illumination with incident light, the coverslip-buffer interface and buffer-microtubule interface reflect light, which combines to create an interference pattern, enabling the visualization of microtubules as high-contrast images against a bright background.
1. Microscope modification and objective lens
2. Chamber preparation to adhere microtubules to the surface
3. Microscope alignment
4. Imaging stabilized microtubules or 40 nm gold particle
NOTE: Stabilized microtubules and gold nanoparticles serve as good control samples. It is recommended to image surface-attached microtubules or gold nanoparticles as a first step to assess IRM performance and help in setting the optimal aperture diaphragm opening (section 7).
5. Imaging microtubule dynamics
6. Image processing and analysis
NOTE: For analysis, this protocol uses Fiji, but the reader is free to use any software she/he finds suitable.
7. Aperture diaphragm size
NOTE: An important factor for acquiring high-contrast images of microtubules using IRM is setting the illumination numerical aperture (INA) correctly. The INA can be changed by changing the size of the incoming illumination beam at the objective's exit pupil which is controlled by the size of the AD (the AD is located at a conjugate plane with the exit pupil (back focal plane) of the objective, Figure 1):
where DAD is the diameter of the aperture diaphragm, fobjective is the focal length of the objective and Dep is the objective's exit pupil diameter. Typically, the AD is left fully open for fluorescence imaging, so the INA equals the objective's NA. In a fluorescence microscope, the AD scale does not indicate its diameter, thus the INA can't be calculated. It's possible to calibrate the AD size with the help of an objective. Yet, it's not necessary since the AD size would be fixed to the size that produces the highest contrast.
Figure 1. Schematic representation of IRM. (A) Epi-illumination from the light source passes through the aperture diaphragm before reaching the 50/50 mirror. The aperture diaphragm sets the beam width thus the illumination NA. The 50/50 mirror partially reflects the light up to the objective to illuminate the sample. Light reflected from the sample is collected and then projected onto the camera chip (by the tube lens) where it interferes to generate the image. Image contrast is the result of the interference between the light reflected from the glass/water interface (I1) and the light reflected from the water/microtubule interface (I2). Depending on the microtubule/surface distance (h), the optical path difference between I1 and I2 will result in a constructive (bright signal) or destructive (dark signal), or anything in between. For example, if light with a wavelength of 600 nm is used for imaging, the contrast will switch between dark and bright when the microtubule height changes by about 100 nm. The asterisk indicates conjugate planes. (B) Example of the 50/50 mirror installation. A suitable filter cube was opened, and the mirror was inserted where a dichroic mirror usually sits. The mirror was oriented as per manufacturer’s instructions. Then the cube was inserted in the filter wheel which was inserted back to the microscope (not shown). During the installation, gloves were used, and the mirror was only held by the edges.
Figure 2. Optimal Aperture diaphragm setting. (A) Same field of view was imaged at different aperture diaphragm openings without background subtraction. Visually, the contrast increased as the size of the aperture diaphragm increased till it reached a plateau and started to degrade afterward. This was confirmed by (B) SBR measurements of background-subtracted images. Error bars are standard deviations. Scale bars are 500 μm (AD) and 3 μm (microtubules).
Figure 3. Measuring signal-to-background noise ratio. Microtubules were isolated in regions of interest. Each region of interest was thresholded to separate the microtubule from the background. The average microtubule signal was obtained from a line scan across the microtubule. The scan line width was set to equal the microtubule length. This way, every point on the scan is an average of the signals of all pixels along the microtubule axis that are parallel to that point. The background noise is the standard deviation of all the pixels below the threshold cut-off.
The authors have nothing to disclose.
Microscope | Nikon | Ti-Eclipse | An inverted microscope used for perfoming the expriments |
50/50 beam splitter | Chroma | 21000 | When buying make sure to choose the splitter dimensions that fit the cube used in the microscope |
NIKON PLAN FLUOR 100X/0.5-1.3 Iris objective | Nikon | MRH02902 | Imaging objective. This objective has a NA adjusting iris that was opened to NA 1.3 |
Mucasol universal detergent | Sigma-Aldrich | Z637181-2L | Used for cleaning coverslips and slides |
Plastic paraffin film (commerical name Parafilm M) | Sigma-Aldrich | P7793 | Used for constructing flow channels |
Anti-TAMRA antibody | Invitrogen | A-6397 | Used to bind TAMRA-labeled molecules (e.g. microtubules) to the sample surface. RRID (AB_2536196) |
Poloxamer 407 (commercial name Pluronic F-127) | Sigma-Aldrich | Used for blocking the channel surface to prevent nonspecific binding | |
40 nm gold nanoparticles | Sigma-Aldrich | 753637 | Used as a control sample |
20 nm gold nanoparticles | Sigma-Aldrich | 753610 | Used as a control sample |
Zyla 4.2 Camera | Andor | Zyla 4.2 | 2048×2048 pixles (6.5µm pixel size) with quantum efficiency of 72% and 16bit dynamic range |
Feista tracking software | https://www.bcube-dresden.de/ fiesta/wiki/FIESTA | ||
Stabilized microtubules | Prepared in house (see references in text) |