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INTRODUCTION TO FLUORESCENCE
MICROSCOPY
Fluorescence microscopy offers a unique approach to
the study of living and fixed cells because of its sensitivity,
specificity and versatility. Fluorescence emitted from
the biological sample can be simultaneously detected
as both an image and as photometric data using the microscope,
and has great potential for qualitative and quantitative
studies on the function and structure of cells.
Stokes identified the phenomenon of fluorescence in
the mid 19th century, and the first fluorescence microscopes
were developed at the beginning of the 20th Century.
These were used to study autofluorescence in organic
and inorganic compounds. Imaging of secondary fluorescence
(whereby specific tissues and bacteria which did not
autofluoresce were labeled with a fluorescent marker
and subsequently imaged) was developed in the 1930’s
by Haitigen, and by the 1950’s, Koons and Caplan
were using fluorescence microscopy to observe the location
of antigens labeled with a fluorophore-tagged antibody
(Wang and Lansing Taylor, 1989).
More recently, increasingly elaborate techniques including
fluorescence recovery after photobleaching (FRAP), fluorescence
lifetime imaging microscopy (FLIM), and fluorescence
resonance energy transfer (FRET) have been developed
that enable the visualization and analysis of ever more
complex events in cells, organelles and sub-organelle
components within the biological specimen. Our experience
in this central facility, however, is that these techniques
are often shrouded in jargon and can baffle the inexperienced
microscopist to such an extent that they would rather
try and avoid doing it altogether. This short article
therefore attempts to dispel some of the mysticism surrounding
FLIM, FRET and FRAP by describing the basic principles
of these techniques, how they are performed on a variety
of fluorescence microscopes, and what practical benefit
they might be to the cell biologist.
Before we consider the technicalities and practicalities
of FRAP, FLIM and FRET, it is worth reminding ourselves
of the principles of fluorescence and fluorescence microscopy.
Each of these techniques in some way takes advantage
of a particular aspect of the processes by which fluorophores
are excited and damaged during excitation, or undergo
non-radiative decay prior to photon emission, and a
given system will necessarily have to employ different
hardware to achieve this.
Fluorescence is a type of luminescence where light is
emitted from molecules for only a short period of time
following the absorption of light. When the delay between
absorption and emission is in the order of nanoseconds
or less, the emitted light is called fluorescence. When
this delay is in the order of microseconds, it is called
delayed fluorescence, and a delay greater than this
is called phosphorescence.
In fluorescence microscopy, naturally occurring autofluorescent
molecules and introduced fluorophores targeted to cellular
structures of interest are irradiated with high intensity
light. When these molecules absorb a quantum of light,
a valence electron is boosted up into a higher energy
orbit, creating an excited state. When this electron
returns to its original, lower energy orbit, termed
the ground state, a quantum of light may be emitted
(see Fig 1).
Absorption occurs only at wavelengths of light whose
quantum energy is equivalent to the difference in energy
between the ground electronic state and the excited
state. Consequently, a given fluorescent molecule will
have a discrete wavelength at which it will become excited;
this is know as its excitation spectrum (lakowicz, 1999).
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Basic model of fluorescence
excitation. When a fluorophore is excited, it can relax
back to the ground state by releasing energy in the
form of light. Other relaxation events, such as vibrational
relaxation, also occur. This means that light emitted
by the fluorophore has less energy than the light used
to excite it. |
| Because fluorescence offers a pathway for
a molecule to relax from an excited state back down to
a non-excited state, it is known as a relaxation process.
However, fluorescence is only one of a number of possible
‘de-excitation pathways’ available to molecules.
One of the most fundamentally important of these is vibrational
relaxation. The loss of some energy through vibrational
relaxation means that less energy is available for emission
as fluorescence. Because wavelength varies inversely to
radiative energy, fluorescence emission is at a longer
(i.e. lower energy) wavelength than the light used to
excite it. This is known as Stokes Law, and the difference
in emission wavelength relative to excitation wavelength
is called Stokes shift (see Fig 2). Stokes shift varies
among different fluorophores, so not only do fluorophores
have characteristic excitation spectra, they have characteristic
emission spectra as well (see Wang and Lansing Taylor,
1989 and Lakowicz et al., 1992). |
Fluorophores have discrete excitation
and emission spectra. In this simplified example,
a fluorophore excited with blue light emits fluorescent
light in the green spectrum. Light is emitted at a
longer wavelength than the light used to excite the
fluorophore because it has less energy due to vibrational
relaxation. The difference between excitation and
emission wavelength is called Stokes shift.
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Fluorescence microscopy - what it means
in practice
The optical paths for image formation of the specimen
are similar in fluorescence microscopy to those of a
standard bright field microscope. The fundamental differences
between bright field and fluorescence microscopy lie
in the requirements of the fluorescence microscope to
maximize the collection of emitted fluorescent light,
while minimizing the collection of the incident excitation
light. One of the key benefits of fluorescence microscopy,
after all, is the increase in resolution through contrast
made available by the selectivity of fluorophores to
specific regions of the sample. Image contrast is critically
dependent on the ability of the microscope to pass fluorescent
light to the detector (typically a CCD camera or photomultiplier
tube) while substantially blocking the excitation light.
Any light microscope relies on 3 components: an illumination
source, a magnifying lens, and an image acquisition
device. In the simplest light microscope this might
consist of a candle, a convex lens, and the human eye.
In a widefield microscope, the entire sample is illuminated
simultaneously, and the image can be viewed directly
either by eye or a camera. For a widefield fluorescence
microscope, the candle is replaced by a high power lamp
(typically a mercury or xenon source), which causes
the fluorescently labeled sample to emit light, and
images are typically acquired using a CCD camera. As
we have seen already, fluorophores have characteristic
excitation spectra, so an excitation filter (usually
a band pass filter) is placed between the lamp and the
sample to narrow the bandwidth of light reaching the
sample. We have also seen that emitted light will be
at a longer wavelength than the excitation light, and
therefore an emission filter (either a long pass or
band pass filter) is placed between the sample and the
camera to block the excitation light from the image.
Successful fluorescence excitation relies on an intense
source of light. In the past 20 years or so, lasers
have provided an alternative excitation source to mercury
and xenon lamps, and are commonly utilised in confocal
and mulitphoton laser scanning microscopy to illuminate
the sample. Lasers generally produce high intensity,
monochromatic light. Because the light source is monochromatic,
no excitation filter is required. An emission filter
is still necessary to stop the laser reaching the acquisition
device. Laser scanning microscopes operate by scanning
the laser over the sample and building up an image,
pixel by pixel, throughout the duration of the scan
by collecting emitted light with a photomultiplier tube.
In the case of confocal laser scanning microscopy, the
mercury lamp is replaced by the laser, the excitation
filter is removed, and the camera is replaced by a photomultiplier
tube. The respective merits and application requirements
that have led to the development of widefield fluorescence,
fluorescence deconvolution, confocal laser scanning,
and multiphoton microscopes are beyond the scope of
this article (see reviews in Pawley, 1995 for further
information).
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Last updated October 27, 2004 |
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