蛍光顕微鏡の紹介

Fluorescence occurs when a fluorophore absorbs light at a specific wavelength, exciting an electron to a higher energy state. As the electron relaxes back to its ground state, it emits a photon of light at a longer wavelength and lower energy than the absorbed light. This emission enables visualization of fluorescently labeled structures in microscopy applications.

Fluorescence microscopy combines magnification with fluorescence detection, requiring specialized components beyond traditional light microscopy. Key differences include a powerful xenon or mercury arc lamp that is 10-100 times brighter than incandescent sources, specialized exciter and barrier filters, and a dichroic mirror to separate excitation and emission wavelengths. These additions enable detection of fluorescently labeled molecules within cells and tissues.

Stokes Shift is the difference between the peak absorption wavelength and the peak emission wavelength of a fluorophore. A larger Stokes Shift makes it easier to separate excitation and emission wavelengths using filters, reducing background noise and improving image quality. This separation is critical for obtaining clear fluorescent images without contaminating light from the microscope components.

Photobleaching occurs when prolonged excitation weakens or eliminates a fluorophore's ability to fluoresce. To reduce photobleaching, add anti-fade mounting medium to slides and seal edges with nail polish. Additionally, keep slides in the dark when not being imaged to minimize unnecessary light exposure and preserve fluorescence intensity for accurate imaging.

The exciter filter selects the excitation wavelength, the dichroic mirror reflects excitation light toward the sample while allowing emission light to pass through, and the barrier filter selects emission wavelength while blocking contaminating light. These three components can be assembled into a filter cube, which can be changed during imaging to accommodate different fluorophores and their specific wavelength requirements.

Allow the xenon or mercury light source to warm up for 15 minutes to reach constant illumination. Place the sample on the stage and focus using the lowest objective. Turn off room lights to reduce background, select the appropriate filter cube for your fluorophore, and open the shutter to illuminate the sample. Adjust exposure time as needed, keeping it constant when comparing samples with the same dye.

Common labeling methods include conjugating fluorescent compounds to antibodies that target specific proteins, integrating fluorescent protein genes like GFP into organism DNA for expression in specific cell types, and labeling macromolecular assemblies such as the F-actin cytoskeletal network. Each method enables visualization of different cellular structures and molecular components for research and diagnostic applications.