Difference between revisions of "DNA Melting Part 1: Measuring Temperature and Fluorescence"

Contents 1 Overview of the apparatus 1.1 Instrument construction procedure 2 Building the optical system 2.1 Excitation light collimation 2.2 Emitted fluorescent light collection 3 Building the Electrical System 3.1 LED driver 3.2 Heating control 3.3 Temperature detection 3.4 Photodiode signal amplification 3.4.1 The amplification circuit 3.5 Practical matters 4 PC Data Acquisition System 4.1 The DAQ 4.1.1 Summary of DAQ inputs/outputs 4.1.2 Things to watch out for 4.2 PC and Software 4.2.1 LabVIEW VI 5 Debugging the apparatus 6 Experimental procedure 6.1 Make a sample 6.2 Sample disposal 7 Other lab manual sections 8 References 9 Datasheets

DNA Melting Apparatus

Overview of the apparatus

The DNA melting apparatus you will construct consists of five major subsystems:

1. optical excitation,
2. optical emission measurement,
3. heating and cooling,
4. temperature sensing, and
5. data acquisition.

Major components of these subsystems include, respectively, an LED, your DNA sample with SYBR Green I labeling dye, a photodiode and amplifier, a thermoelectric heater/cooler (or TEC, or Peltier heater/cooler because it employs the Peltier effect), a resistive temperature detector (RTD), a data acquisition system (DAQ)], and a PC.

The DNA melting apparatus includes excitation, fluorescence measurement, temperature sensing, and data acquisition functions.

SYBR Green I is a fluorescent dye with peak sensitivity to blue light at 497 nm, and the dye emits green light with an emission peak at 520 nm.^[1] You should familiarize yourself with the spectrum of this dye^[2]. Once you have your sample you will be able to easily observe that a room-temperature sample of dsDNA and SYBR Green I looks yellow from the combination of blue excitation and green fluorescence. At higher temperatures, when there is no dsDNA to which the dye can bind, the sample will appear blue or clear. In order to produce a melting curve, your apparatus will measure the amount of fluorescent emission from the SYBR Green I dye over a range of temperatures.

Fluorescence intensity will be measured by the photodiode (and associated optical system to gather more light and concentrate it on the photodiode). Temperature will be measured by the RTD, which is a kind of resistor that predictably varies in value with temperature. The sample will be heated by the TEC. The DAQ and PC will record the signals from the photodiode and RTD. These signals must then be processed to convert them from raw voltage into temperature and fractional dsDNA concentration, f. The melting temperature, T_m, can be estimated from a plot of f vs. T_m of f vs. dT_m/dt (T_m differentiated with respect to time).

Temperature will be measured by an RTD, which is a kind of resistor that predictably varies in value with temperature. Fluorescence intensity will be measured by a photodiode (and associated optical system). The sample will be heated by a thermoelectric device. A computer data acquisition system will record the signals from the photodiode and RTD. These signals must be processed to convert them from raw quantities to temperature and relative dsDNA concentration. The melting temperature, T_m can be estimated from a graph of this data or its derivative.

As shown in the diagram, an aluminum heating block holds a cuvette containing the sample under test. The sample contains a combination of DNA, SYBR Green I, and a salt (either KCl or NaCl, it doesn't matter which). In addition to being a convenient holder, the block transfers heat to the cuvette and it's sample, while also allowing the block's temperature to be measured without affecting the block temperature. (In your report, tell us about the practical problems with this approach and ways to improve it.)

Light from a blue LED illuminates one side of the cuvette. A 470 nm bandpass optical filter placed between the two will shape the output spectrum of the LED so that only the desired wavelengths of light fall on the sample.

A photodiode placed at 90 degrees to the LED source detects the green light emitted by SYBR Green I bound to the minor groove of dsDNA. The photodiode is placed after a 515 nm long pass optical filter to ensure that only green and longer wavelength light is detected. (In your report, describe how you ensure that only the fluorescent light given off by the sample falls on the photodiode.)

Since photodiodes produce only a very small amount of current, it will be necessary to build a very high gain amplifier to produce a signal that is measurable by the DAQ. Photodiode amplifiers can be challenging because many of the non-ideal characteristics of op amps become apparent at high gain. For this reason it is suggested that you build a two-stage amplifier. And furthermore it is suggested that your first stage be a transimpedence amplifier like the one shown in the figure. (In your report, comment on why a transimpedence amplifier is better for photodiode output amplification.)

An RTD attached to the heating block and wired to a voltage divider provides an indication of temperature. The temperature of the heating block will be a proxy for the sample temperature. It is not a perfect proxy, however, and you will need to determine the transfer function between the temperature you measure on the outside of the block, and the temperature inside the cuvette, say, in the middle of your DNA sample. Refer to your lecture notes and see your Instructors or TA for help with this. Hint: An electrical circuit can be used to describe many types of systems, including thermal systems."

Finally, the DAQ digitizes the amplified photodiode and RTD signals. A LabVIEW virtual instrument (VI) is provided that will control the heating and cooling of your DNA heating block and record the RTD and photodiode signals over time so that data from the DNA melting VI can be saved to a file. The file can be loaded into Matlab for analysis, or if you prefer, Python or equivalent.

Instrument construction procedure

DNA Melting Optical System Diagram

• Build an optical excitation system.
• Build a heating/cooling system that includes an RTD and Controller.
• Build an optical emission measurement system.
• Build an LED driver circuit.
• Build a voltage divider and low pass filter to measure RTD voltage.
• Build a high gain, dual-stage amplifier, with filters of your choice.

Building the optical system

As mentioned above, the optical system consists of an LED, an excitation filter, a sample cuvette, a heating block (because it contains mechanical apertures), an emission filter, optional lenses, a photodiode, and associated mounting hardware. Construct your system on an optical breadboard. The breadboard has a grid of tapped holes for mounting all kinds of optical and mechanical hardware. ThorLabs manufactures most of the hardware stocked in the lab. A few of the components that you will certainly use include: TR2 1/2" diameter posts and PH2 post holders, CP02 cage plates, and SML03 and SML05, 1” diameter lens tubes.

There are a variety of ways to construct the apparatus. A good design will be compact, stable, and simple. For Part 1 of the lab, it is a good idea to shield the optical system from ambient light, so a small footprint could be advantageous.

Excitation light collimation

You will use a high-brightness blue LED manufactured by LedEngin, Inc.^[3] to excite the sample. Light from the LED diverges in a cone with an angle of about 100 degrees. It will be advantageous to include lenses in your system to collimate light from the LED onto the full area of your sample. (Why not focus the light on the sample?)

This LED has a dominant wavelength of 465 nm. A Chroma Technology D470/40 bandpass filter^[4] eliminates unwanted parts of the spectrum that might interfere with detection of the fluorescence signal, such as the very wavelengths you want to measure as fluorescent output. The filters have exposed, delicate coatings and must be handled carefully^[5]. In addition, the filter works better in one direction than the other^[5].

Emitted fluorescent light collection

The Thorlabs SM05PD1A^[6] photodiode is mounted in a short tube with SM05 threads. Use an SM1A6^[7]adapter to mount the photodiode in a CP02 cage plate or lens tube. Mount the photodiode assembly to the breadboard at 90 degrees to the LED. Build a system to hold the Chroma E515LPV2 emission filter^[8] in front of the photodiode. You can use lenses to focus light from the sample onto the detector to improve performance, if you like.

Do not connect the sample block to any other pieces of metal — this will draw off heat and affect your instrument's performance. If you want to link the sample block to the fluorescence detection arm, use hexagonal plastic standoffs to connect two cage rails. This will form much less of a thermal linkage. However you choose to manage this light path, make sure it is mechanically stable during and between your experimental runs.

Building the Electrical System

LED driver

The LED will be powered using 5 V by placing the LED in series with a 25 Ω resistor. Use the fixed 5 V output from your Instek power supply.

Don't forget the resistor. Directly connecting the 5 V will blow out the LED

Heating control

Directly connect a Diablotech power supply to a double TEC stack using the connector provided. It is best to jump the wires using your breadboard, and keep the white/black wire and connector with your setup. Ask a TA or Instructor for assistance if needed.

Temperature detection

Temperature Detection Circuit

The electrical resistance of most materials varies with temperature. An RTD is a special resistor (usually made out of platinum) that exhibits a nearly linear change in its value with temperature. An RTD may be used to accurately measure temperature by including it as an element in a voltage divider. As the resistance of the RTD changes, so will the voltage across it.

A PPG102A1 RTD from US Sensors^[9] has been pre-mounted on the DNA heating block. This RTD has a nominal resistance of 1 kΩ and its value increases with temperature. Note that the maximum current carrying capacity of this device is 1 mA, so if you alter the voltage divider design, be sure that no more than 1 mA flows through the RTD. To test basic functionality of your circuit, you can place your finger over the RTD while your lab partner measures the divider voltage with a digital multimeter.

The diagram to the right shows the suggested temperature detection circuit. The capacitor across the RTD implements a low pass filter whose purpose is to eliminate noise in your temperature reading. Consider the following points when choosing a capacitor value: What is the cutoff frequency above which you want to attenuate noise? Start by thinking about the time constant of the temperature change you wish to observe. What is the time constant of your filter? If it is too large compared to the rate of change of temperature, it could cause a delay in your temperature reading.

Photodiode signal amplification

Excited SYBR Green I molecules emit photons in all directions, some of which pass through the aperture in the heating block then the emission filter and then strike the photodiode. This generates a tiny current in the photodiode, which must be converted to a voltage and amplified to a level that can be conveniently measured. From past experience, the photodiode output current will be on the order of 15 nA but depends on excitation light flux and emission collection optics. (Can you calculate it from first principles?) You may be able to improve upon this with well-designed optics in the emission path.

The amplification circuit

The NI-DAQ interface card used in lab can digitize a voltage between positive and negative 10 Volts. A first approach to providing this voltage swing at the digitizer inputs was demonstrated in the homework: a transimpedance amplifier with a gain of approximately $ 7x10^8 $ V/A would produce this voltage amplitude. (Why not simply use a resistor, and omit the op-amp?) However, implementing the photodiode amplifier in a single stage presents a number of challenges because many of the non-ideal behaviors of op amps become apparent at such high gain values. Because of this it is suggested that you implement a two-stage amplifier as shown in the figure below. Your job as circuit designers will be to fill in the appropriate feedback resistor values in order to achieve the desired gain at the output. If you have another topology in mind, feel free to discuss with your TA and/or Instructors.

Think carefully about how you want to distribute the gain of the system across the stages: how does feedback affect the noise of the amplifier? What are the dominant sources of noise in the DNA melting setup, which ones do you have most control over, and how will you control for them? Applying your knowledge of feedback and transfer functions, you should be able to determine the optimal gain configuration of each stage for lowest output noise.

Multi-stage photodiode amplification circuit

Practical matters

As with most amplifiers, care should be taken with lead dress, component placement and supply decoupling in order to ensure stability.

—LF411 Datasheet

In theory, there is no difference between theory and practice. But, in practice, there is.

—Jan L. A. van de Snepscheut/Yogi Berra/and or Chuck Reid

The universe is rife with electrical noise. Keeping the noise out of sensitive electronic instruments requires a great deal of care. Unfortunately, electronic breadboards are a poor environment in which to construct high gain amplifiers. A few simple tricks can improve things.

• Use power supply bypass capacitors. Connect a large capacitor between all supply voltages and ground. Large, electrolytic capacitors of at least 0.1 μF work well for this purpose. Electrolytic capacitors are polarized. Make sure to put them in the right direction (They may explode, but they will definitely start to smell bad.).
• Use the binding posts on the breadboard to connect your power supplies.
• Power Supplies: Use a seperate power supply for the op-amp circuits, LED driving circuit, and the heating control. Make sure to tie the 5V ground to +15V/-15V ground at the power supply. If you connect the grounds on the breadboard, there will be a potential difference between the grounds. This voltage difference is due to the large current swing of the LED driver flowing through the parasitic resistance of the breadboard.

Even with these optimizations, it will be important to keep your wiring short and neat. The amplifier and wiring will also be susceptible to physical movement, so prevent things from getting bumped during experimental runs. A note about resistors and capacitors: recall that resistors introduce thermal noise, while capacitors do not. Therefore, the optimized system will use as low resistor values as are reasonable in filters and feedback paths.

PC Data Acquisition System

The DAQ

Each lab PC is equipped with a National Instruments USB-6212 or USB-6341 data acquisition (DAQ) card.

The USB-6212^[10] has 16, 16-bit analog input channels which can, in sum total, accomplish 400 thousand samples per second (400kS/s). That is, if there are two channels, each one will be alternately sampled, and EACH sampled at 200kS/s. A multiplexer sequentially selects from among the 16 single-ended and 8 differential input signals. The card also supports two 16 bit analog output channels with an update rate of 250 kS/s and an output range of +/-10 V and up to +/-2 mA.

The USB-6212 also has 32 digital input/output channels and a digital ground. A 50 kΩ pull-down resistor is typically used in series with connections to these channels.

The USB-6341^[11] is s little more powerful. It has 16, 16-bit analog input channels which can, in sum total, accomplish 500 thousand samples per second (500kS/s). Again, a multiplexer sequentially selects from among the 16 single-ended and 8 differential input signals. The card also supports two 16 bit analog output channels but they have an update rate of 900 kS/s and an output range of +/-10 V and up to +/-2 mA.

Finally, the USB-6341 has 24 digital input/output channels and a digital ground, as well as 4, 100 MHz counter/timers.

Summary of DAQ inputs/outputs

Things to watch out for

• The DAQ has only one ADC (analog-to-digital converter), which is multiplexed between all of its analog inputs. The ADC has input limits of +/-10V. If one input is outside this range, it will get confused and give nonsensical values for all inputs. The upshot is, if either your temperature or fluorescence measurement is nonsensical, check to make sure the other one isn't feeding +15V into the DAQ.
• If you short-circuit your DAQ, it will get confused. One symptom of this is the LabView VI refusing to run (for example, wrongly complaining that the limits on the band-pass filter do not satisfy some condition). If this happens, unplug and re-plug the DAQ and use the Measurement and Automation software to check its condition.

PC and Software

LabVIEW VI

The DNA Melting LabVIEW VI is located in the Students/Labs/DNA Melting folder of the course locker. Double click to launch the VI. (The current version is R1.0)

Click the run arrow or select Operate->Run from the menu to start the VI. The top two charts show the digitized voltage at the RTD and diode inputs over time. Use the range settings to get a good view of the signal.

At the end of an experimental run, use the Save Data button to save the most recent result in a tab-delimited file that can be read into Matlab or Excel.

Debugging the apparatus

1. Use freeze spray and the heat gun to make sure the temperature circuit is working properly.
2. Cover and uncover the photodiode to verify operation of the fluorescence measurement system.
3. Use a box and a piece of black cloth to shield your apparatus from ambient light. Can you measure the difference between a cuvette filed with water and one with DNA and SYBR Green?
4. Observe every electrical signal node with the oscilloscope. Are any signals noisy? Is there a way to improve the quality of poor signals?
5. Watch the fluorescence readout over time. Is it stable or does it drift?
6. Is your temperature reading nonsensical? Make sure you are using 15V supply and 15kohm resistor, for your voltage supply. Also make sure that the DAQ input is placed across the RTD not the 15Kohm resistor.
7. Is your LED being driven at the desired carrier frequency? Try turning the carrier frequency down low enough to see it turn on and off (try 5Hz). Try pointing the LED directly at the photodiode. Is the frequency of the photodiode signal what you expect?
8. Is your sampling photobleaching quickly? Turn the amplitude of the LED signal down at the Labview VI. Try an amplitude of 0.25 V and an offset 0.50 V. Turning the amplitude down decreases signal strength, but you can gain signal strength by focusing the green fluorescent light on the photodiode with lenses.

Experimental procedure

Samples are in limited supply, as usual, so to receive your test samples you must first confirm that your apparatus is functioning properly and that your analysis script is functional. Your group can actually get your code running at the same time as your instrument is being created. You may either generate some data from the Simulating DNA melting wiki page, or you may use previous-run data that we provided on Stellar.

To demonstrate a properly running instrument, your TA will provide a sample of 20bp DNA and will evaluate your raw data. As a first step, turn your apparatus on and measure the difference between a cool DNA sample and water. Run the DNA melting LabVIEW VI in the DNAMelting directory of the course locker (First make a copy for yourself in your directory.).

Once your instrument is running to your (and your TA's) satisfaction, you may measure melting curves of each of the test samples. And if you have time, you can run additional experiments. For example, you could gather additional ionic strength data points.

The DNA melting apparatus will generate the best data when both the amplifier circuit and LED have been on for a while and all the components have reached their steady state temperature. Make sure the outputs of the system are stable before you begin taking data.

The steps for each experimental run are:

1. Open the LabView VI
2. Set the carrier frequency, the LED amplitude, the desired temperature, and the filter cutoff frequencies
3. Then prepare a sample and place cuvette in heating block
4. Run the Labview: recording RTD and photodiode output during heating
5. Switch off the heater and record RTD and photodiode output during cooling
6. Make any modifications to the code that will help you

Make a sample

SYBR Green I in DMSO is readily absorbed through skin. Synthetic oligonucleotides may be harmful by inhalation, ingestion, or skin absorption. Wear gloves when handling samples. Wear safety goggles at all times when pipetting the SYBR Green/DNA samples. Do not create aerosols. The health effects of SYBR Green I have not been thoroughly investigated. See the SYBR Green I and synthetic oligonucleotide MSDS in the course locker for more information.

Pipet 500μl of DNA plus dye solution into a glass cuvette. (Ask your TA or an Instructor for one of these reusable, and expensive, cuvettes). Pipet 20μl of mineral oil on top of the sample to help prevent evaporation. Put a disposable top (available in a drawer under the bench) on the cuvette and mark it with a permanent marker. Keep the sample vertical to make sure the oil stays on top. You should be able to use the same sample for several heating/cooling cycles (What makes it go bad? What can you do to limit this effect?). Only discard it if you lose significant volume due to evaporation or your signal gets too low. If you need to leave the sample overnight, store it in the lab refrigerator. If you finish with a sample and it is still in good shape, pass it on to another group.

Sample disposal

Discard pipette tips with DNA sample residue in the Biohazard Sharps container. Do not pour synthetic oligonucleotides or SYBR Green down the drain. Empty the liquid into the waste container provided. Clean your glass cuvettes by flushing with alcohol in the waster container, rinsing with water at the drain, and if you wish by also soaking/rinsing with the Lysol cleaner. You can suck out residual liquid with the vacuum and drawn pipette to the left of the sink.

Other lab manual sections

Top Level: Lab Manual:Measuring DNA Melting Curves

Lab Manual:Processing DNA Melting Data

References

1. ↑ Zipper H, Brunner H, Bernhagen J, Vitzthum F. Investigations on DNA Intercalation and Surface Binding by SYBR Green I, its Structure Determination and Methodological Implications. Nucleic Acids Res. 2004;32:e103–10.
2. ↑ Invitrogen Spectral Viewer
3. ↑ Datasheet for Blue LED from LEDengin
4. ↑ D470/40 Bandpass filter spectrum
5. ↑ ^{5.0 5.1} Handling, orientation, and care of a coated optical filter
6. ↑ Thorlabs SM05PD1A photodiode
7. ↑ Thorlabs SM1A6 adapter
8. ↑ Chroma EV515LPv2 Long pass filter spectrum
9. ↑ Datasheet for PPG102A1 RTD
10. ↑ Datasheet for the USB-6212
11. ↑ Datasheet for the USB-6341

Datasheets

1. National Instruments data acquisition card user manual
2. SYBR Green I datasheet
3. Op-amp datasheet
4. Relay datasheet
5. [http://www.learn-c.com/tip120.pdf Darlington transistor