Principles & Practice of

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Presentation transcript:

Principles & Practice of Light Microscopy: 2 (Image: T. Wittman, Scripps)

Aperture and Resolution Diffraction spot on image plane = Point Spread Function Intermediate image plane Tube lens Objective Sample Back focal plane aperture

Aperture and Resolution Diffraction spot on image plane = Point Spread Function Intermediate image plane Tube lens Objective Sample Back focal plane aperture

Aperture and Resolution Diffraction spot on image plane = Point Spread Function Intermediate image plane Tube lens Objective Sample Back focal plane aperture

Aperture and Resolution Diffraction spot on image plane = Point Spread Function Intermediate image plane Tube lens Objective  Sample Back focal plane aperture Image resolution improves with Numerical Aperture (NA)  = light gathering angle n = refractive index of sample NA = n sin() where:

Filling the back focal plane In trans-illumination microscopy, to get maximum resolution, the illumination must “fill the back focal plane” Back focal plane For the highest resolution, we need to have condenser  objective NAcondenser  NAobjective with oil immersion objectives, we need an oil immersion condenser! Objective aobjective acondenser Condenser Light source

The Condenser Tasks: Illuminate at all angles < aobjective Concentrate light on the field of view for all objectives to be used Problem: Low mag objectives have large FOV, High mag objectives have large a (With 2X and 100x objectives we need (100/2)2 = 2500 times more light than any objective uses!) Solutions: Compromise Exchangable condensers, swing-out front lenses,… Grade of correction NA

Aperture, Resolution & Contrast Can adjust the condenser NA with the aperture iris Imaging path Intermed. image Tube lens Back aperture Q: Don’t we always want it full open?? A: No Why? Tradeoff: resolution vs. contrast Objective Sample Condenser lens Aperture iris Field lens Illumination path Field iris Collector Light source

Spatial frequencies & the Optical Transfer Function (OTF) (Spatial frequency, periods/meter) k OTF(k) 1 (Image contrast) Resolution limit: kmax = 2 NA / l Observed image Object

Resolution & Contrast vs. Illumination aperture Pupil appearance (“Coherent illumination”) NAcondenser  0 Contrast (= Full aperture, “incoherent illumination”) NAcondenser  NAobj Resolution Resolution limit: kmax = (NAobjective+ NAcondenser)/ l Increasing the illumination aperture increases resolution but decreases contrast

Definitions of Resolution 1 OTF(k) Cutoff frequency kmax = 2 NA / l As the OTF cutoff frequency 1/kmax = 0.5  /NA |k| As the Full Width at Half Max (FWHM) of the PSF FWHM ≈ 0.353  /NA As the diameter of the Airy disk (first dark ring of the PSF) = “Rayleigh criterion” Airy disk diameter ≈ 0.61  /NA

The image of a point object The 3D Point Spread Function (PSF) The image of a point object 2D PSF for different defocus Z=+2µm 3D PSF Calculated Measured z Z=0 Z=-2µm y x x

x - z

Z-resolution, a.k.a. depth of field, for widefield microscopy 2ln / NA2 NA Resolution (nm; X-Y) depth of field (mm) 0.3 1017 11.1 0.75 407 1.77 0.95 321 1.11 1.4 218 0.773

Summary: Numerical Aperture and Resolution Numerical aperture, not magnification, sets the smallest details you can resolve in an image Increasing NA also increases the amount of light collected by the lens, thereby increasing the brightness of the image – this scales as NA2

Specifications for some common objectives Magnification NA Resolution (nm) Depth of Field (nm) Light gathering (arb. units) 10 0.3 1017 16830 0.09 20 0.75 407 2690 0.56 40 0.95 321 1680 0.90 1.3 235 896 1.69 60 1.2 254 926 1.44 1.4 218 773 1.96 100

Aberrations They are the enemy

Aberrations Chromatic aberrations Wavefront aberrations Longitudinal chr. Ab. Lateral chr. Ab. Wavefront aberrations Spherical aberration Astigmatism Coma … Curvature of field Distortion

Geometric Distortion = Radially varying magnification Image Pincushion Object Pincushion distortion Barrel distortion May be introduced by the projection eyepiece

Wavefront Aberrations Aberrated wavefront in the pupil Ideal wavefront in the pupil

Wavefront Aberrations (piston) (tilt) Astigmatism Defocus Coma Trefoil Spherical ab. Secondary coma Secondary spherical ab.

PSF Aberrations (piston) (tilt) Astigmatism Defocus Coma Trefoil Spherical ab. Secondary coma Secondary spherical ab.

Spherical Aberration

Point spread functions Spherical Aberration Point spread functions Ideal 1 wave of spherical ab z x x

Causes of spherical aberration Modern objectives are complicated! The optical design requires specifying the optical path length between the sample and the back focal plane of the lens OPL = l1n1 + l2n2 + … + lnnn

Sources of Spherical Aberration Design compromises Manufacturing tolerances Immersion fluid index error Temperature variation Cover slip thickness (high-NA objectives except oil immersion) Correction collar setting Sample refractive index mismatch

& Spherical Aberration Index Mismatch & Spherical Aberration objective Immersion fluid n1 Spherical aberration unless n2 = n1 Cover glass n2 Sample Focus at cover slip Focus into sample

& Spherical Aberration Index Mismatch & Spherical Aberration z=0 µm n1=1.515 (oil) z=25 µm n2=1.44 (Vectashield) z=50 µm

How to recognize spherical aberration Unaberrated Aberrated 0.5 mm steps 1 mm steps

What can you do about spherical aberration? Use 0.17 mm coverslips (~ #1.5) Work close to the coverslip Match lenses to the refractive index of your samples, and vice versa For aqueous samples, use water immersion / water dipping lenses For fixed samples and oil immersion lenses, mount your sample in a medium with n = 1.515 Adjust objective correction collar when available Use lower NA lenses

Correction collars A correction collar can only eliminate spherical aberration at a single focal plane

Example Aberrated Unaberrated

Index Mismatch & Axial Scaling n1 n2 Optical focus step zo Mechanical step zm If there is index mismatch, your z pixel size is not what you think

Sources of Astigmatism & Coma Off-axis (edges of field of view) All objectives have some Present in the design You get what you pay for On-axis (center of field of view) Should be none, by symmetry. If they are there, they could be from: manufacturing or assembly tolerances dirt or abuse Misalignment (tilt, off-axis shift of something) bad downstream components (mirrors, dichroics, filters…) Air bubble in the immersion fluid or sample Tilted cover slip (dry and water-immersion high-NA lenses)

Spatial frequencies & the Optical Transfer Function (OTF) More about Spatial frequencies & the Optical Transfer Function (OTF)

The response to pure waves is well-defined by the Optical Transfer Function (OTF) Object Observed image (Spatial frequency, periods/meter) k OTF(k) 1 (Image contrast) Resolution limit: kmax = 2 NA / l

Think of Images as Sums of Waves … or “spatial frequency components” one wave another wave (2 waves) + = (25 waves) (10000 waves) + (…) = + (…) =

Frequency Space To describe a wave, Can describe it by we need to specify its: ky kx Distance from origin Direction from origin Magnitude of value Phase of value Can describe it by a value at a point complex k = (kx , ky) Frequency (how many periods/meter?) Direction Amplitude (how strong is it?) Phase (where are the peaks & troughs?) direction period

and the Fourier Transform Frequency Space and the Fourier Transform ky Fourier Transform ky kx kx

Properties of the Fourier Transform Completeness: The Fourier Transform contains all the information of the original image Symmetry: The Fourier Transform of the Fourier Transform is the original image Fourier transform

The OTF and Imaging ?  ? = =  convolution True Observed Object Image PSF ?  ? = Fourier Transform OTF = 

(f  g)(r) = f(a) g(r-a) da Convolutions (f  g)(r) = f(a) g(r-a) da Why do we care? They are everywhere… The convolution theorem: If then A convolution in real space becomes a product in frequency space & vice versa h(r) = (fg)(r), h(k) = f(k) g(k) Symmetry: g  f = f  g So what is a convolution, intuitively? “Blurring” “Drag and stamp” f g fg  = y y y =  x x x

The Transfer Function Lives in Frequency Space Object Observed image |k| OTF(k) ky Observable Region kx

The 2D In-focus Optical Transfer Function (OTF) OTF(k) OTF(k) ky |k| kx (Idealized calculations)

The 3D OTF 2D PSF 2D OTF 2D F.T. 3D PSF 3D OTF 3D F.T. ? ?

Values of the 3D OTF kx kz

= Region where the OTF is non-zero 3D Observable Region = OTF support = Region where the OTF is non-zero ky ky kz kz

So what is the resolution? kx Kxymax = 2 n sin(a) / l = 2 NA / l kz “Missing Cone” of information Kzmax = n (1-cos(a)) / l

So what is the resolution? kx Kxymax = 2 n sin(a) / l = 2 NA / l Lowering the NA Degrades the axial resolution faster than the lateral resolution But low axial resolution = long depth of field This is good, if 2D is enough kz “Missing Cone” of information Kzmax = n (1-cos(a)) / l

So what is the resolution? kx Example: a high-end objective Kxymax = 2 n sin(a) / l = 2 NA / l NA = 1.4 n=1.515 a = 67.5° l = 600 nm Lateral (XY) resolution: 1/ Kxymax = 0.21 µm Axial (Z) resolution: 1/ Kzmax = 0.64 µm kz “Missing Cone” of information Kzmax = n (1-cos(a)) / l

Nomenclature Optical Transfer Function, OTF Complex value with amplitude and phase Contrast Transfer Function, CTF Modulation Transfer Function, MTF Same thing without the phase information

Acknowledgements Resources Slides available at: http://nic.ucsf.edu/edu.html http://www.microscopyu.com http://micro.magnet.fsu.edu Douglas B. Murphy “Fundamentals of Light Microscopy and Electronic Imaging” James Pawley, Ed. “Handbook of Biological Confocal Microscopy, 3rd ed.” Acknowledgements Steve Ross, Mats Gustafsson