How to use CTF in SPARX
In SPARX, the EMAN CTF object are used to store and apply all CTF parameters.
To generate a CTF object, see function generate_ctf(p), here p is a list of parameters [defocus, cs, voltage, apix, bfactor, amp_contrast, astigmatism amplitude, astigmatism anglet]. Their definitions are:
- defocus
defocus in `µ`m. Positive number means underfocus.
- cs
- Spherical aberration constant in mm. (Default 2.0)
- voltage
microscope voltage in `kV`. (Default 300 kV)
- apix
pixel size in `Å`.
- amp_contrast
- Amplitude contrast ratio, unitless, given as percentage of (0,100). (Default 10%)
- bfactor
B-factor defining exponential decay of Fourier amplitudes decay `Å^2`. (Default 0.0, i.e., no decay).
- astigmatism amplitude
- in [nm]. (Default 0.0)
- astigmatism angle
- in [degrees]. (Default 0.0)
Notice: In some other software packages, the defocus value is in Å and amplitude contrast ratio is in the range of (0, 1). This function will automatically determine whether these two CTF parameters are in this convention and convert them into our convention.
To apply CTF object to an image, use filt_ctf(img, ctf), where ctf is a CTF object created using generate_ctf.
- To put a CTF object into the header of an image, it can be done in two ways:
use function set_ctf(img, p), where p is a list of parameters [defocus, cs, voltage, apix, bfactor, ampcont].
if the CTF object already exists, one can use img.set_attr("ctf", ctf) directly.
To recover the numerical values of CTF parameters from CTF object stored in the header of an image, use function p=get_ctf(img).
- To access or set individual parameters in a ctf object, use:
- bfactor = ctf.bfactor
- ctf.bfactor = 200.0
Description
- The Contrast Transfer Function of electron microscope has the following form:
`gamma(K,"defocus")=2pi(-1/2"defocus"*lambda*K^2+1/4*"Cs"*lambda^3*K^4)`
`CTF(K)=(sqrt(1-A^2)*sin(gamma(K,"defocus")) - A*cos(gamma(K,"defocus"))*e^(-"B_factor"/4*K^2)`
where `K=sqrt(K_x^2+K_y^2+K_z^2)` and `A` is amplitude contrast.
Reference
1. J. Frank Optik (1973) 38:519
2. R. Wade & J. Frank Optik (1974) 49:81.
3. Z. Huang, P. R. Baldwin, S.Mullapudi, and P .A. Penczek, Automated determination of parameters describing power spectra of micrograph images in electron microscopy. J. Struct. Biol. 144 (2003), pp. 79-94.