Calculation of pulse EPR spectra.
saffron(Sys,Exp) saffron(Sys,Exp,Opt) y = saffron(...) [x,y] = saffron(...) [x,y,p] = saffron(...) [x1,x2,y,p] = saffron(...)See also the examples on how to use
saffron.
This function calculates pulse EPR (ESEEM and ENDOR) spectra of powder and single crystals.
The output contain the abscissa data in x (time in microseconds or frequency in MHz) and the simulated
data in y (time domain trace or ENDOR spectrum). For 2D experiments such as HYSCORE, the two axes are
returned in x1 and x2. For ESEEM simulations, p
contains the frequency abscissa (in MHz) in p.f and the spectrum obtained by Fourier transform
from the time domain data in p.fd.
If you don't request any output, saffron plots the simulated data.
The three input arguments to the function are
Sys: spin system (paramagnetic molecule)Exp: experimental parametersOpt: simulation options
Sys is a spin system structure.
Fields available in Sys include all needed for the construction of the spin Hamiltonian.
Line broadening parameters used by other simulation functions (lw, lwpp,
gStrain, etc.) are not recognized, except HStrain. HStrain is used in
excitation window computations (see Exp.ExciteWidth) when orientation selection is wanted.
saffron supports any spin system with one electron spin (arbitrary S) and any number of nuclei.
If no orientation selection is required, then even the g tensor (and the microwave frequency) can be omitted. Only the nuclear parameters (and the field) need to be given:
Sys.Nucs = '14N'; Sys.A_ = [0.2 0.3]; Sys.Q = [-1 -1 2]*0.1;
Exp contains the experimental parameters, most importantly the magnetic field
and the pulse sequence.
Field | Magnetic field (in mT) at which the experiment is performed. |
Sequence |
Specifies the pulse sequence, '2pESEEM', '3pESEEM', 'HYSCORE',
or 'MimsENDOR'.
|
nPoints |
Number of points in the ESEEM time trace or in the ENDOR spectrum. If only one number is given and
a two-dimensional experiment is simulated, the number is used in both dimensions. If you give two
numbers, each refers to one dimension. E.g. [31 256] indicates 31 points in the first
dimension and 256 points in the second dimension. The defaults for nPoints are 512
for 1D and 256 for 2D experiments.
|
dt |
For ESEEM, time increment (dwell time), in microseconds. For 1D experiments, this should be
a single number. For 2D sequences, dt applies to both dimensions if it's only one
number, alternatively one number for each dimension can be given, e.g. dt = [0.024 0.008].
|
tau | For three-pulse ESEEM, HYSCORE and Mims ENDOR, this gives the value of τ, in microseconds. For two-pulse ESEEM, it is the starting τ value. |
T | For three-pulse ESEEM, this gives the starting T value, in microseconds. For the other sequences, this value has no effect. |
t1,t2 | For HYSCORE, these give the starting values of t1 and t2, in microseconds. |
T1T2 |
An array [T1 T2] with two numbers, the longitudinal relaxation time constant T1 and the transverse relaxation
time constant T2.
|
Range | Contains lower and upper limit of the frequency range for ENDOR. Values should be in MHz, e.g. Exp.Range=[0 30]. |
For orientation selection, the following additional parameters are needed.
mwFreq | EPR spectrometer frequency in GHz. Needs only to be given if orientation selection is wanted. |
ExciteWidth |
The excitation width of the microwave in MHz (responsible
for orientation selection). The excitation profile is assumed to be
Gaussian, and ExciteWidth is its FWHM. The default is infinity.
To obtain the full excitation with for a given orientation, ExciteWidth
is combined with HStrain from the spin system structure.
|
For user-defined pulse experiments, the following fields are
Flip |
List of pulse flip angles in multiples of 90°, e.g. [1 1 2 1] for HYSCORE.
|
Inc |
Incrementation information for every inter-pulse delay. 0 indicates no incrementation,
1 increment along first dimension, 2 increment along second dimensions.
Example: [0 1 2 0] for HYSCORE and [1 1] for two-pulse ESEEM. Currently, not
all incrementation schemes are supported.
|
t | List of initial delays, in microseconds. |
tp |
List of pulse lengths, in microseconds. If not given, all pulses are assumed to be infinitely short (ideal).
If given, saffron integrates the signal over a small offset distribution. See Opt.nOffsets
and Opt.lwOffset. Some of the values in tp can be zero, in which case ideal pulses are used.
E.g. [0.200 0 0] is a three-pulse sequence with one selective pulse followed by two ideal hard pulses.
|
Filter |
Coherence filter, one character for each inter-pulse delay. '+' stands for electron coherence
order +1, '-' for -1, 'a' for 0 (alpha), 'b' for 0 (beta), '0'
for 0 (alpha or beta), 1 for +1 or -1, and '.' for anything. Examples: '.ab.'
selects the coherence transfer pathways in HYSCORE that leads to alpha/beta cross peaks.
|
To simulate single crystals, use
Orientations |
3xN array of real Specifies single-crystal orientations for which the ENDOR spectrum should be computed. Each column of Orientation
contains the three Euler rotation angles [phi;theta;chi] of the
magnetic field in a molecule fixed frame. If Orientation is empty
or not specified, the full powder spectrum is computed.
Exp.Orientations = [0;0;0]; % crystal with z axis aligned with B0 Exp.Orientations = [0;pi/2;0]; % crystal with z axis perpendicular to B0 Exp.Orientations = [0 0 0;0 pi/2 0].'; % two orientations Exp.Orientations = []; % powder |
CrystalSymmetry |
Specifies the symmetry of the crystal, if single-crystal spectra to be simulated
(that is, if |
The fields in the structure Opt specify parameters for the simulation algorithm
nKnots |
A number giving the number of orientations (knots) for which spectra
are explicitly calculated. nKnots gives the number of
orientations on
quarter of a meridian, i.e. between θ = 0 and θ = 90°.
The default value is 31, corresponding to a 3° spacing between orientations.
For highly anisotropic spectra, esp. for HYSCORE, the value often has to
be increased to 181 (0.5° spacing) or beyond.
|
Expand | Expansion factor used in the simulation, should be between 0, 1, 2, 3 or 4. The higher, the more accurate is a simulation, but the slower it becomes, especially for 2D simulations. Default values are 4 for 1D and 2 for 2D. |
ProductRule | Determines whether product rule is used or not (1 or 0). By default, it is not used, but simulations with spin systems with more than two nuclei it might run faster with the product rule. The spectral result is independent of this choice. |
nOffsets | Number of points for the offset integration in the case of finite-length pulses. Typical values are between 10 and 100, but should be determined for each case individually. |
lwOffset | FWHM (in MHz) of the Gaussian distribution of offset frequencies use in the offset integration in the case of finite-length pulses. Typically, this is about the inverse of the length of the first pulse in a pulse sequence, e.g. 100 MHz for a 10ns pulse. |
logplot |
A 1 indicates that the HYSCORE spectrum should be plotted with a logarithmic intensity scale.
If 0 (the default), a linear scale is used.
|
Window | Apodization window used before FFT. See apowin for details. |
ZeroFillFactor |
The factor by which the time domain signal array should be padded with zeros before FFT. E.g. with
ZeroFillFactor=4, a 256-point array is padded to 1024 points.
|
For both ESEEM and ENDOR, saffron uses matrix-based methods similar to those employed by Mims (1972) to compute
frequencies and amplitudes of all peaks. With these peaks, a spectrum histogram is constructed, from which
the time-domain signal is obtained by inverse Fourier transform.
For the pre-defined sequences, saffron assumes ideal pulses with standard flip angles (two-pulse ESEEM: 90°-180°, three-pulse ESEEM
90°-90°-90°, HYSCORE 90°-90°-180°-90°).
For systems with several nuclei, saffron by default simulates without using product rules,
but can employ them if wanted (see Options).
For high-electron spin systems, all terms in the zero-field splitting, even the nonsecular ones, are taken into account.
To generate the spectrum from the time-domain signal, saffron performs (1) baseline correction,
(2) apodization with a Hamming window, (3) zero-filling, and (4) FFT.
All the theory is described in