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RbNO3, 87Rb (I=3/2) STMASΒΆ
87Rb (I=3/2) staellite-transition off magic-angle spinning simulation.
The following is an example of the STMAS simulation of \(\text{RbNO}_3\). The \(^{87}\text{Rb}\) tensor parameters were obtained from Massiot et. al. 1.
import matplotlib as mpl
import matplotlib.pyplot as plt
import mrsimulator.signal_processing as sp
import mrsimulator.signal_processing.apodization as apo
from mrsimulator import Simulator, SpinSystem, Site
from mrsimulator.methods import ST1_VAS
# global plot configuration
font = {"size": 9}
mpl.rc("font", **font)
mpl.rcParams["figure.figsize"] = [4.25, 3.0]
Generate the site and spin system objects.
Rb87_1 = Site(
isotope="87Rb",
isotropic_chemical_shift=-27.4, # in ppm
quadrupolar={"Cq": 1.68e6, "eta": 0.2}, # Cq is in Hz
)
Rb87_2 = Site(
isotope="87Rb",
isotropic_chemical_shift=-28.5, # in ppm
quadrupolar={"Cq": 1.94e6, "eta": 1.0}, # Cq is in Hz
)
Rb87_3 = Site(
isotope="87Rb",
isotropic_chemical_shift=-31.3, # in ppm
quadrupolar={"Cq": 1.72e6, "eta": 0.5}, # Cq is in Hz
)
sites = [Rb87_1, Rb87_2, Rb87_3] # all sites
spin_systems = [SpinSystem(sites=[s]) for s in sites]
Step 2: Select a satellite-transition variable-angle spinning method. The following ST1_VAS method correlates the frequencies from the two inner-satellite transitions to the central transition. Note, STMAS measurements are highly suspectable to rotor angle mismatch. In the following, we show two methods, first set to magic-angle and the second deliberately miss-sets by approximately 0.0059 degrees.
angles = [54.7359, 54.73]
method = []
for angle in angles:
method.append(
ST1_VAS(
channels=["87Rb"],
magnetic_flux_density=7, # in T
rotor_angle=angle * 3.14159 / 180, # in rad (magic angle)
spectral_dimensions=[
{
"count": 256,
"spectral_width": 3e3, # in Hz
"reference_offset": -2.4e3, # in Hz
"label": "Isotropic dimension",
},
{
"count": 512,
"spectral_width": 5e3, # in Hz
"reference_offset": -4e3, # in Hz
"label": "MAS dimension",
},
],
)
)
Create the Simulator object, add the method and spin system objects, and run the simulation.
The plot of the simulation.
data = [sim.methods[0].simulation, sim.methods[1].simulation]
fig, ax = plt.subplots(1, 2, figsize=(8.5, 3), subplot_kw={"projection": "csdm"})
titles = ["STVAS @ magic-angle", "STVAS @ 0.0059 deg off magic-angle"]
for i, item in enumerate(data):
cb1 = ax[i].imshow(item / item.max(), aspect="auto", cmap="gist_ncar_r")
ax[i].set_title(titles[i])
plt.colorbar(cb1, ax=ax[i])
ax[i].invert_xaxis()
ax[i].invert_yaxis()
plt.tight_layout()
plt.show()
Add post-simulation signal processing.
processor = sp.SignalProcessor(
operations=[
# Gaussian convolution along both dimensions.
sp.IFFT(dim_index=(0, 1)),
apo.Gaussian(FWHM="50 Hz", dim_index=0),
apo.Gaussian(FWHM="50 Hz", dim_index=1),
sp.FFT(dim_index=(0, 1)),
]
)
processed_data = []
for item in data:
processed_data.append(processor.apply_operations(data=item))
processed_data[-1] /= processed_data[-1].max()
The plot of the simulation after signal processing.
ax = plt.subplot(projection="csdm")
cb = ax.imshow(processed_data[1].real, cmap="gist_ncar_r", aspect="auto")
plt.colorbar(cb)
ax.invert_xaxis()
ax.invert_yaxis()
plt.tight_layout()
plt.show()
- 1
Massiot, D., Touzoa, B., Trumeaua, D., Coutures, J.P., Virlet, J., Florian, P., Grandinetti, P.J. Two-dimensional magic-angle spinning isotropic reconstruction sequences for quadrupolar nuclei, ssnmr, (1996), 6, 1, 73-83. DOI: 10.1016/0926-2040(95)01210-9
Total running time of the script: ( 0 minutes 0.913 seconds)