The OLIS Polarization Toolbox is the sample compartment used on the
DSM 172, DSM 245, CPL Solo, and NIR CPL Solo
This sample compartment is unique in providing user selected positioning of the polarization hardware. This hardware – one or two polarizers and a modulator – can be positioned before or after the sample. In this way, one can configure a single sample compartment for circular dichroism and circularly polarized luminescence¹.
In both acquisition modes, a ‘direct subtractive method’ of data acquisition and processing is used. This DSM software allows use of a single detector and a polarizer fixed in position, obviating the need for G-factor correction for emission measurements. (It also obviating the need for electronic calibration in CD, but this is addressed in detail elsewhere.)
Rapid switching (50 kHz) between polarization states also supports kinetic studies such as stopped flow spectroscopy.
The light source is external to the Polarization Toolbox. The light source is a host spectrophotometer (i.e., lamp and scanning monochromator) or an LED.
For the DSM 172and 245, which support CD and CPL, the host spectrophotometer is a xenon arc lamp and a double monochromator.
For the CPL Solo, a wavelength specific LED is used. A well-chosen LED will have higher intensity and greater stability than the light from a xenon arc lamp through a double monochromator.
Polarizer Location One: At the entrance of the Polarization Toolbox, there is a shelf for a polarizer immediately after the entrance of the incoming light.
Circular dichroism is a measure using circularly polarized light, so the incoming light is polarized with this first polarizer. That is, with a polarizer here, the measurement light is polarized.
Circularly polarized luminescence is a measure of circularly polarized emitted light, so polarizing this exciting light is desirable only when polarized excitation is intentionally to be examined. Polarized excitation is not always the preference, because the polarizer does absorb some of the exciting light, ultimately reducing sensitivity, and because your sample’s emission might not be changed by polarization of the light. That is, the exciting light is non-polarized or polarized, as the user prefers for a given experiment.
Modulator: The means by which polarization is modulated left/ right or parallel/perpendicular
Circular dichroism employs a 50 kHz photoelastic modulator to produce the left circularly polarized and right circularly polarized light as the measurement beam. CD is equal to the difference in the absorbance by the sample of these two polarization states of the light, i.e., CD = abs(L) – abs(R). This switching of polarization states happens 50,000 times per second. The modulator is before the sample.
Circularly polarized luminescence employs the same photoelastic modulator. However, now the PEM is located after the sample to analyze the emitted light. The emission by the (chiral) sample is modulated to be linearly polarized. The modular is after the sample.
Polarizer Location Two: At the exit of the Polarization Toolbox, there is a shelf for a polarizer immediately before the exit port to the emission detection hardware.
Circular dichroism does not employ a polarizer after the sample. The light travels at 180 degrees from the sample directly into the (absorbance) detector. No polarizer is used in this position.
Circularly polarized luminescence employs the linear polarizer after the sample to analyze the polarization from the sample. CPL = emission(L) - emission(R). “CPL provides the differential emission intensity of right and left circularly polarized light, thereby providing information on the excited state properties of the chiral molecular systems.”² A polarizer is always in this position.
The detection hardware is external to the Polarization Toolbox.
Circular dichroism employs a high speed, high sensitivity photomultiplier tube, which sends its raw abs(L) and abs(R) tagged photons to our 16 bit A/D converter card and OLIS software.
Circularly polarized luminescence employs a high throughout single monochromator and an exquisitely sensitive gated photon counting detector for capturing and sorting the flu() and flu(R) signals, ultimately processed by the OLIS software. Because the polarization state of detected light is always horizontal, there is no effect of polarization (including Wood’s anomalies in the monochromator) on the intensity. Thus, no G-factor correction is required.
There are no moving parts in this module because neither polarizer has to be rotated during the experiment.
¹ CPL is a technique used to characterize transition metal ligand complexes (a signal is seen only when coordinated to a chiral ligand), trivalent lanthanide complexes, and chiral lactones. In addition, bio-macromolecular molecules have been probed by using Tb3+[ref], dansyl, acridine, and intrinsic tryptophan. These probes, particularly tryptophan, are sensitive to tertiary structure. Unfolded proteins exhibit zero CPL signal.
Further Reading:
DEVICE FOR ENABLING SLOW AND DIRECT MEASUREMENT OF FLUORESCENCE POLARIZATION
US Patent 6,970.241 B1, assigned to Richard J. De Sa
Recording Anisotropy Spectrometer -- A Unique Application of Piezoelectric Birefringence Modulation
John E. Wampler and Richard J. De Sa, Analytical Chemistry, 46,563 (1974)
How does OLIS achieve a single spectrophotometer which optimizes for CD, CPL, and anisotropy?
We call the answer our “Polarization Toolbox.”
The Polarization Toolbox is a sample compartment developed to allow immediate and fail-safe positioning of polarizer(s) and a modulator before or after the sample. Let’s call this positionable polarization hardware a “Polarization Modulator Assembly” or PMA.
If the PMA is before the sample, incoming light is switched between L&R. The Toolbox is measuring CD. If the PMA is after the sample, the polarized emission light is being analyzed for CPL and anisotropy.
This document focuses on the emission measurements.
With a vertically polarized excitation and where I‖ and I are the intensities of the vertically & horizontally polarized emission.
Fluorescence anisotropy (r) : r = (I‖ – I )/ (I‖ +2I )
Polarization of fluorescence (P): P = (I‖ – I )/ (I‖ +I )
The method for emission data collection is described in the 1974 Analytical Chemistry paper, “Recording polarization of fluorescence spectrometer: Unique application of piezoelectric birefringence modulation,” https://pubs.acs.org/doi/ abs/10.1021/ac60340a004
DeSa realized that the use of “piezoelectric birefringence modulation” would eliminate the need for two detectors, rotation of polarizers at each moncohromator, and the associated four G-factor corrections. His colleague and co-author, 1 Wampler, wrote the math for this novel advance in polarization measurements. With their ‘74 method, a single detector is used, no movement of the polarizer is needed, and no G-factor correction is required for anisotropy or CPL measurements.
The ‘74 Method simplifies the hardware and collects the desired data directly and thus perfectly.
Richard DeSa’s motto: Why do manually what can be done electronically? Electronically is failsafe, easy, perfect.
Very commonly, the modulator is a photoelastic modulator (PEM), as is used for circular dichroism. This 50 kHz modulation rate switches the polarization 50,000 time per second. A PEM is always used for CD mode and anisotropy stopped-flow.
The same PMA can be moved to a 90-degree position and used for CPL. For CPL, we commonly choose a quarter waveplate instead of the PEM, because this frees data collection from the 50 kHz modulation rate. The freedom to collect Lum(L) and Lum(R) at slow speed has considerable advantages.
The following figures show PMA positioning for the measurements. The software does the rest:
1 A G-factor is the correction to the effect of the inherent bias of monochromators to the 1 orientation of a polarizer. Every monochromator has some polarization bias. This bias causes changes in the transmitted intensities between the two orientations of the polarizer. When a measurement requires a change in the orientation of the polarizer, a correction factor must be applied to cancel this effect, i.e., the G-factor correction.
For Anisotropy, the excitation light (“measurement beam”) passes through a vertically oriented linear polarizer before striking the sample.
The light emitted by the sample is captured at 90-degrees after it passes through a fixed polarizer and either a filter (shown) or scanning monochromator, and then to the detector.
Unlike L-format polarization systems which other manufacturers are limited to -- in which the polarizer must be physically rotated between the vertical and horizontal positions – the DeSa-Wampler method is more direct, simple, and perfect.
DeSa’s utilization of a modulator – a 50 kHz photoelastic modular (PEM), liquid crystal variable retarder (LCVR), or waveplate -- rotates the plane of polarization of the emitted light rather than moving the polarizers.
One of the beneficial consequences is that no G-factor correction is needed to correct for the different intensity responses of the monochromators to the two states of polarization.
The OLIS method has the sample between fixed and stationary polarizers. In the case of the LCVR and waveplate, switching between L and R (or parallel and perpendicular) can be made at an arbitrary speed, liberating data collection from the 50 kHz rate of the PEM.
So, if the emission polarizer has been fixed in the horizontal position, and the modulator is off so that no alteration of the emission light is occurring, IH can be measured. When the modulator is turn on (to a level that the polarization of the emission light is rotated 90 degrees) the detector will measure Iv.
That is, the polarization of the left and right will have some Horizontal character since the modulator rotated 90 degrees. Vertical has become horizontal and passes through the fixed horizonal polarizer.
Detection is handled by the exquisitely sensitive gated photon counting PMT for maximum sensitivity.
By synchronizing the detection with the modulator, the appropriate Ivv and Ivh values can be obtained and used to calculate anisotropy or CPL.
Because the polarization state of detected light is always horizontal, there is no effect of polarization (including Wood’s anomalies in the monochromator) on the intensity. There are no moving parts; neither polarizer is rotated.
The following figure shows an example of a dilute fluorescein solution in glycerol. The temperature was increased from 20°C to 80ºC as measured in a Peltier temperature-controlled cell. The recorded polarization decreases as a function of temperature, reflecting the increased motion of the fluorescein molecule.
The choice of the modulator -- PEM, LCVR, or waveplate -- should be based on two aspects of the measurement. The first is the switching rate required. Applications such as stopped flow and CD, which require rapid switching, require the PEM. Slower anisotropy and all CPL measurements can be done with the PEM, LCVR, or waveplate.
In addition to speed of modulation, one must also consider the wavelength range required. The respective spectral ranges are 170 nm – 1400 nm for the PEM, 340 nm -2000 nm for the LCVR, and 270-2700 nm for the waveplate.
Circularly polarized luminescence (CPL) is the differential emission of left and right circularly polarized light from a chiral fluorophore. CPL is extremely sensitive to the environment of the excited state. CPL has been used to characterize transition metal ligand complexes (a signal is seen only when coordinated to a chiral ligand), trivalent lanthanide complexes, and chiral lactones. In addition, bio macromolecular molecules have been probed by using Tb3+[ref], dansyl, acridine, and intrinsic tryptophan. These probes, particularly tryptophan, are sensitive to tertiary structure.
The units for CPL are G(LUM2 ), where
G(LUM) = 2 [(IL-IR)/IL+IR)]
Interesting fact: Unfolded proteins, exhibit zero CPL signal.
A CPL spectrum of Europium(III) tris[3-(trifluoromethylhydroxymethylene)-dcamphorate in DMSO.
X-axis = 570-720 nm; Y-axis = -0.9 - 0.1 G(LUM)
The Polarization Toolbox is a self-contained sample compartment which we offer on three OLIS instruments:
1. The CPL Solo is the Polarization Toolbox, emission monochromator and emission detector, and one or more LEDs.
2. The OLIS DSM 172 is the Polarization Toolbox, double prism-grating monochromator, emission monochromator, 150-watt xenon arc lamp, and detectors for both CD (PMT) and CPL (photon counting PMT). This model has both UV/Vis and NIR: CD is 185-1700 nm and CPL is 230-850 nm.
3. The OLIS DSM 245 is the Polarization Toolbox, double grating monochromator, emission monochromator, 150-watt xenon arc lamp, and detectors for both CD (PMT) and CPL (photon counting PMT). This model supports 170-700 nm for CD and 230-850 nm for CPL.
An On-Line Spectrofluorimeter System for Rapid Collection of Absolute Luminescence Spectra.
Wampler and De Sa, Applied Spectroscopy, 25, No. 6, 623-627 (1971).
Today, we strongly recommend the I and IV, as the limited detection performance of low cost commercial NIR detectors is useful only with large CPL signals and lengthy acquisition times.
Models I, II, IV & VI are for strong and weak emission samples. They have the best detectors for their given ranges.
Models III & V are low-cost alternatives to IV and VI. They have the penultimate detector. The sensitivity difference is 100-1000 fold less than the more expensive IV and VI.
Models III and V are successful with strongly emissive samples; models IV and VI are for a wider range of signal strengths.
OLIS CPL Solo I 350-800 nm
OLIS CPL Solo II 400-1100 nm
OLIS CPL Solo III 800-1700 nm
OLIS CPL Solo IV 800-1700 nm
OLIS CPL Solo V 1100-2700 nm
OLIS CPL Solo VI 1100-2700 nm