|
|
 |
Technical
Information:
Introduction To Fluorescence Filters |
How
are fluorescence filters used?
| |
 |
Optical
fluorescence occurs when a molecule known as a fluorophore (usually
a fluorescent dye) absorbs light with wavelengths within its absorption
band, and then nearly instantaneously emits light at longer wavelengths
within its emission band. Fluorophores are specifically attached
to biological molecules, to cell regions, and to other targets
of interest to enable quantification, identification, and even
real-time tracking of activity on a microscopic scale. Fluorescence
is widely used in biotechnology and analytical applications due
to its extraordinary sensitivity, high specificity, simplicity,
and low cost compared to other analytical techniques.
Most fluorescence
instruments, including fluorescence microscopes, use optical filters
to control the spectra of the excitation light and emission light.
Filters make it possible for the sample to "see" only
light within the absorption band, and the detector to "see"
only light within the emission band. Without filters, the detector
would not be able to distinguish the desired fluorescence from
scattered excitation light (especially within the emission band)
and autofluorescence from the sample, substrate, and other optics
in the system. |
| |
 |
| |
A
system with a broadband light source, such as a fluorescence microscope,
has three basic filters: an excitation filter, a dichroic beamsplitter,
and an emission filter. The exciter is typically a bandpass filter
that passes only the wavelengths absorbed by the fluorophore, thus
minimizing excitation of other sources of fluorescence and blocking
light in the fluorescence emission band. The dichroic is an edge
filter used at an oblique angle of incidence to efficiently reflect
light in the excitation band and to transmit light in the emission
band. The emitter is also typically a bandpass filter that passes
only the wavelengths emitted by the fluorophore and blocks all undesired
light outside this band – especially the excitation light.
Systems with laser illumination might or might not use an exciter
or a dichroic, but most include some variation of these filters.
The fluorescence filters function as a set to provide the optimum
signal with minimal noise.
In most fluorescence instruments, the best performance is obtained
with thin-film filters, as opposed to other types of fixed or tunable
filters, such as those based on diffraction gratings. Thin-film
filters comprise multiple thin layers of transparent materials with
high and low indexes of refraction on a glass substrate. The complex
layer structure determines the spectrum of light transmission by
a filter – the more layers and the more precisely they are
deposited, the more complex and accurately reproduced a desired
spectrum can be made. Thin-film filters are simpler, are less expensive,
and provide excellent optical performance: high transmission over
an arbitrarily determined bandwidth, steep edges, and high blocking
of undesired light over the widest possible wavelength range. Recent
advances in thin-film filter technology permit even higher performance
while resolving the longevity and handling issues that can affect
filters made with older technology. |
What
should I look for when selecting fluorescence filters?
Better optical filters
can increase the signal, or brightness, attained by a microscope or other
instrument. Better optical filters can reduce the background that comes
from sample and instrument autofluorescence outside the emission band.
And better optical filters can reduce excitation light noise, or stray
and scattered light from the excitation source. In summary, by choosing
the right filters one can achieve the best possible signal and signal-to-noise
ratio. For more details on how filters impact signal and signal-to-noise
ratio, see Optical
Filters Impact Fluorescence Fidelity (PDF).
In an ideal set of filters the spectra of the exciter and emitter filters
would exhibit perfectly rectangular passband profiles with 100% transmission
in each passband and complete blocking outside the passbands (including
within the passband of the companion filter).
The spectrum of the dichroic beamsplitter would have 100% reflection in
the exciter passband, 100% transmission in the emitter passband, and a
perfectly vertical transition between the two bands. To prevent excitation
light noise between the passbands, the
exciter and emitter filters must not overlap.
Although real filters do not possess these ideal properties, manufacturers
must try to come as close as possible. Key specifications that distinguish
filters are the average passband transmission, bandwidth, edge steepness,
and edge wavelength accuracy. The last of these
is not apparent from looking at a single plot of the filter spectra, but
rather is based on a statistical sample of a large number of filters.
It is crucial for guaranteeing consistency in high-volume instrumentation
applications as well as in end-user systems such as microscopes. Another
critical feature of fluorescence filters is blocking – the filters
must provide sufficient blocking over the most critical wavelength ranges.
In some cases, the blocking must be much higher than is possible to measure
directly with standard test and measurement instrumentation, making it
difficult for one to determine how well the filters will function without
trying them in the actual instrument.
Why
are BrightLine® filters better than other fluorescence filters?
The patented* BrightLine
filter technology has set a new standard for fluorescence filters. Semrock's
superior coating technology – combined with its expertise in designing
optical filters specifically for fluorescence systems – has resulted
in the simplest, most durable, and highest-performance fluorescence filters
available anywhere. With
BrightLine filters, you'll find:
Maximum Brightness
| |
BrightLine
filters offer the highest throughput for blazing measurement speed! |
|
|
| |
The
high transmission of BrightLine® filters results from a simple
filter structure with thin-film coatings on the outer surfaces
of a single piece of glass. These exceptionally durable coatings
are as hard as the underlying glass, allowing them to be easily
handled and cleaned. |
|
| |
-
fewer
interfaces means lower reflection and scattering losses
-
no
adhesive means the clearest possible optical path with no
autofluorescence
-
no
uncoated surfaces means there's no need for additional anti-reflection
(AR) coatings
|
|
|
| |
|
|
| |
 |
Just
one look at the transmission spectra of BrightLine filters and you’ll
see the difference. The spectra demonstrate the high average passband
transmission, precise bandwidths, steep spectral features and exceptional
wavelength accuracy that is characteristic of all Semrock filters.
But if filter spectra alone aren’t convincing, then take a look
at some fluorescence images to see
what you've been missing! |
|
| |
| Typical
spectra of BrightLine filters for the popular fluorophore
FITC |
Unrivaled Filter Life
All Semrock filters
are made exclusively with hard coatings for unrivaled
reliability and longevity. These
extremely durable coatings are deposited onto the outer surfaces of a
single piece of glass, with no adhesive to leak or degrade. The conventional
approach to making high-performance fluorescence filters makes use soft
coatings that are easily damaged and absorb water vapor, causing significant
spectral shifts and ultimately permanent degradation. To protect the soft
coatings as much as possible, multiple glass substrates are laminated
together with adhesives, resulting in compromised filter performance.
| |
The
Semrock Standard |
|
Conventional
Approach |
|
| |
 |
Exciter
or
Emitter |
 |
|
| |
 |
Dichroic
Beamsplitter |
 |
|
The hard coatings used
on BrightLine® filters are as durable as the glass substrate itself.
Therefore, handling of these filters is greatly simplified, and a dirty
filter can simply be cleaned with alcohol or even acetone. With this improvement
fluorescence microscope users
can even populate their own filter cubes!
Zero Pixel Shift Imaging Performance
Semrock has uniquely solved the problem of poor image registration.
Poor
image registration, or "pixel shift," results when a filter
in an imaging path (for example, the emitter or dichroic beamsplitter
in a fluorescence microscope) with a non-zero wedge angle deviates
the light rays so as to cause a shift of the image detected on a
high resolution CCD camera. When two or more images of the same
object acquired using different filter sets are overlaid (in order
to simultaneously view fluorescence from multiple fluorophores),
a non-zero filter wedge angle means that the images will not be
registered to identical pixels on the CCD camera. Hence, images
produced by different fluorophores cannot be accurately correlated
or combined. |
| |
| This
schematic of a typical epi-fluorescence geometry (as in a standard
microscope) shows how filter wedge causes pixel shift. |
|
Composite
images produced from conventional filter sets (left), typically
having much greater than 1 pixel shift, are distorted, whereas –ZERO™
pixel shift filter sets (right) yield precise multi-color images.
(Simulation) |
 |
|
 |
How does Semrock
eliminate the problem of pixel shift?
| BrightLine®
filter patented* technology is based on a single glass substrate
coated by durable, hard coatings. BrightLine
ZERO filter substrates are manufactured to a very high
tolerance. |
 |
| The
conventional approach to high-performance fluorescence filters requires
multiple substrates, typically bonded together with adhesive, resulting
in significant wedge angle and therefore pixel shift. |
 |
Now end users and OEMs alike who need zero-pixel-shift performance can
have it just by choosing BrightLine ZERO
filters.
* U.S.
Patent No. 6,809,859 and pending.
|