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Epi-illumination is form of Kohler Illumination:

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Presentation on theme: "Epi-illumination is form of Kohler Illumination:"— Presentation transcript:

1 Epi-illumination is form of Kohler Illumination:
Objective is also condenser White light (regular Kohler) Brightfield, phase, etc Light is focused At back aperture Of the objective, Conjugate to condenser aperture Different illumination And image paths Lamp or laser lens detector Detect at 90 degrees Split with dichroic mirror Greatly increases S/N

2 dichroic mirror objective lens specimen Epi-illumination separates
light source, Fluorescence signal Second barrier filter Selects signal From background First barrier filter Selects excitation Arc lamp dichroic mirror objective lens specimen

3 Excitation filter typically interference bandpass
Dichroic is longwave pass For one dye-maybe no emission filter

4 Dielectric layers or Metallic layers used as filter coating
Reflect, transmit colors of choice by using multilayers

5 Coatings work by interference
Reflectance depends on Wavelength, film thickness material (index*length), incident angle. Fabry-Pérot interferometer

6 Use of bandpass interference filters in wavelength selection
Block 3-6 OD outside of band Transmit 10-50% (worse for UV)

7 Dichroic Mirrors: separate colors by using coatings
Beam separator: Separate different colors (fluorescence) At right angles: used in microscopes Beam combiner: Multiple lasers Transition should be sharp

8 How CCD Camera Works Serial readout limit speed. A partial solution is using Frame-Transfer.

9 Comparison: Detector Quantum Yield

10 Efficiency & Signal/Noise?
Collection efficiency of microscopy: ~25% Detector quantum yield: ~70-90% Thermal noise Shot noise (quantum noise): Read noise (A/D conversion) V^2 = 4kTR

11 CCD Dark counts Cooling methods: Liquid Nitrogen Thermal Electric
in ultrahigh vacuum

12 EM-CCD Largely eliminate read noise Introduces amplification noise
Net effect is S/N improvement for extremely low light level situation

13

14 Detecting A Single Fluorescent Molecule?
Size: ~ 1nm Absorption Cross-section: ~ cm2 Quantum Yield: ~1 Absorbance of 1 molecule = ? How many fluorescence photons per excitation photons?

15 Single Molecule “Blinks”

16 How to Analyze Single Molecule Measurements (I) -- Histograms
Most Probable Value vs Average value

17 Single molecule fluorescence: experimental considerations
• Emission – Wavelength dependence of detectors – Spectral separation from excitation – Efficient detection optics – Autofluorescence and contaminant fluorescence – Photobleaching and ISC – Scatter: • elastic (Rayleigh) • inelastic (Raman) • Excitation – High NA objective lens – “Bright” fluorophores • High extinction coefficient • High quantum yield – Exclude quenchers • particularly molecular oxygen! • O2 scavengers include β-mercaptoethanol (BME), catalase

18 Back to Single Protein Detection
Myosin V has two heavy chains like myosin II, but myosin V has a longer neck region, and a shorter coiled coil region is followed by a  globular domain at the end of each heavy chain tail. Light chains that associate with each heavy chain in the neck region are calmodulin or calmodulin-like proteins. Light chains may provide stiffening in neck domains and in some cases have a regulatory role. For example, each myosin II monomer binds two distinct light chains, designated essential and regulatory. The neck domain of each myosin V monomer has 6 binding sites for calmodulin, which serves as light chains. (To review the structure and role of calmodulin, see notes on calcium signals.) Myosin V -- a motor protein.

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20 De-convolution Microscopy
Thompson, RE; Larson, DR; Webb, WW, Biophys. J. 2002,

21 Paul Selvin

22 Photodiode PMT: photomultiplier CCD APD: Avalanche Photodiode

23 PMT APD Both can work under Single-photon Counting mode
Both can work under Single-photon Counting mode

24 Typical Dark Counts CCD APD Temperature -70 C -20 C Sensitive Area
0.001 e/sec/pixel e/sec/pixel

25 Total Internal Reflection Fluorescence Microscopy
TIRFM Total internal reflection: the reflection that occurs when light, in a higher refractive-index medium, strikes an interface with a medium that has a lower refractive index, at an angle of incidence (α1) greater than the critical angle.

26 Snell’s law

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28 Minimal depth is about 1/7 of wavelength

29 Application Example 1 – Cytoskeleton
TIRF Epi

30 Setting up the TIRF microscope
Prism-TIRF Objective-TIRF

31 A little History: EVDLS

32 1980s: start to apply TIR principle
to fluorescence and bio-imaging. Daniel Axelrod

33 Prism Based TIRF Setup 1 Add the webpage demostration

34 Spherical Aberration from Aqueous Sample
Sample near glass coverslip Sample in the bulk water

35 Water Immersion Objective
Fully water immersion Water immersion with coverslip

36 Prism-TIRF Objective-TIRF

37 Key Points: NA requirement Oil immersion Size of the beam 柳田敏雄
Toshio Yanagida

38 Through Objective TIR Design 1: direct coupling

39 Through Objective TIR Design 2: Fiber Optics
Optical fiber based light delivery Easy conversion from non-TIR to TIR Compatible with Arc lamp

40

41 Other Practical Concerns:
Upright or inverted microscope? Light sources? Polarization?

42 Arc Lamp TIRF

43 Fresnel equations

44 Polarization Control


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