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NMR Spectroscopy
A short introduction
How it all began....
How it all began....
Bloch, Felix, (1905–83), Swiss-American physicist and Nobel laureate, born in Zürich, Switzerland, and educated at the Federal Institute of Technology there and in Germany at the University of Leipzig. He left Germany in 1933 and a year later he joined the faculty of Stanford University in California, where he taught until his retirement in 1971. Bloch’s doctoral dissertation (1928) is recognized as the basis of the modern theory of solids. He also made significant contributions to theoretical physics, particularly to the fields of superconductivity and magnetism. During World War II he worked on the Manhattan Project (the first atomic bomb) and on war-related counter-radar research. In 1946, Bloch became known for his method of determining the magnetic moment (a measure of magnetic strength) of the neutron and the development of the technique called nuclear magnetic resonance. He shared the 1952 Nobel Prize in physics with the American physicist Edward M. Purcell, who had independently discovered, in a different way, nuclear magnetic resonance at about the same time.
..and we need a magnetic field
400MHz = 9.395 T (tesla)
= 9.395*104 G (gauss)
..and we need a magnetic field
Basics of NMR Spectroscopy
Quantum spin number 0 nucleus is magnetically active
e.g. 1H, 13C, 15N, 19F, 31P (I = 1/2)
They will be observed at different (well separated ) frequencies.
We normally just detect one nucleus at a time!
15N 13C 31P 19F 1H
Nuclear Spins
The nucleus has a spin (rotation)
The angular momentum pp is a vector parallel to the axis of rotation
The magnitude of the angular momentum is given by the spin quantum number II::
p = h/2 * I(I+1)
pp
Nuclear Spins
A circulating current creates a ring current
The ring current creates a dipolar magnetic moment:
= p
: gyromagnetic ratio
The gyromagnetic ratio is a constant for each nucleus, describing its magnetic properties
pp
Nuclear Spins
The magnetic moment is a vector parallel to the angular momentum ppp
Nuclear Spins
Outside a magnetic field the nuclear spins have no orientation
N
S
NN
SS
NN
SS
NNSS
NN
SS
Nuclear Spins
Inside a magnetic field the nuclear spins will be aligned along the magnetic field axis
The picture shown here is not really correct: quantum mechanics allows only discrete orientations
The number of possible orientations is given by the spin quantum number I
N
S
NN
SS
NN
SS
NN
SS
NN
SS
NN
SS
Bo
Nuclear Spins
Not all nuclei align parallel
The number of nuclei with parallel and anti-parallel orientation is described by Boltzmann‘s law:
Nm = No
m
N
S
NN
SS
NN
SS
NN
SS
NN
SS
NN
SS
Bo
SS
NN
SS
NN
SS
NN
e-Em / kT
e-Em / kT
Nuclear Spins
Nm : number of spins in state m
No : total number of spins
Em : energy of state m
k : Boltzmann constant
T : temperature
Nm = No
m
N
S
NN
SS
NN
SS
NN
SS
NN
SS
NN
SS
Bo
SS
NN
SS
NN
SS
NN
e-Em / kT
e-Em / kT
Nuclear Spins
How many spins have parallel and anti-parallel orientation?
N+ - N- = No E /2kT
Assuming: Bo = 1 Tesla (43MHz)
No = 2‘000‘000
N+ = 1‘000‘001
N- = 999‘999
N
S
NN
SS
NN
SS
NN
SS
NN
SS
NN
SS
Bo
SS
NN
SS
NN
SS
NN
Nuclear Spins
N
S
NN
SS
NN
SS
NN
SS
NN
SS
NN
SS
Bo
SS
NN
SS
NN
SS
NN
Bo E
E = h Bo
m=-1/2
m=1/2
The energy levels are called Zeeman levels
What do we Observe ? (1)
In a magnetic field, the Zeeman levels are splitted according to:
type of the nucleus strength of the magnetic field
1H has a higher frequency than 13C at the same field strength
1H is more sensitive than 13C at the same field strength
E
field
13C splitting
1H splitting
What do we Observe ? (2)
Levels with different energies have different populations p:
Equilibrium population
We use rf pulses (MHz) in order to perturb the system :
Perturbed population
We observe populations going back to equilibrium: B A
E
p 0
E
p 0
A
B
Nuclear Spins: macroscopic magnetisation
E
m=-1/2
m=+1/2
From Microscopic to Macroscopic
M = magnetisation vectorB0 = static magnetic field
B 0
y
z
x
M
rf pulse 90° flip angle
y
z
xM
Macroscopic Signal
Magnetisation precesses at a frequency given by :
the type of nucleus the electronic environment in the molecule
Magnetisation relaxes towards equilibrium
The detected signal, the FID ("Free Induction Decay") shows :
frequency of precession damping due to relaxation
y
z
x M
time
T =1/
y
z
x M
Macroscopic Signal
Resonance Condition of NMR Spectroscopy:
I = I Bo
I : Larmor frequency
I : gyromagnetic ratio
Bo: magnetic field
y
z
x M
z
I
Signal Processing
To understand the signal, we go from the time domain signal, the FID, to the frequency domain signal, the spectrum
via the Fourier Transform
FT
time Frequency orchemical shift
Summary
• Nuclei have a spin which creates a magnetic moment.• Due to the magnetic moment the nuclei will orientate in the
magnetic field and thus create a net-magnetisation, called ‚macroscopic‘ magnetisation.
• The orientation of the macroscopic magnetisation will be disturbed by a RF pulse, thus creating a magnetisation vector in the x,y frame.
• The magnetisation rotates in the x,y, frame and induces a voltage in a receiver coil.
• The induced signal is processed by Fourier transformation
Laboratory and Rotating Frame
y’
z
x’
M
o
z
y
x
M
o
Laboratory Frame:•The x,y, frame is fix with respect to an
external observer.•The magnitization is seen rotating with the
Larmor frequency o
Rotating Frame:•The x,y, frame is rotating with the Larmor
frequency o
•The magnetisation is seen at a fix position
The RF pulse
z
y
x
B1
1. A coil is installed with its long axis oriented along the x axis.
2. This ‚transmitter coil‘ is feeded with an alternating current
3. A magnetic field oscillating linearly along the x axis
Laboratory FrameLaboratory Frame
The RF pulse
1. The oscillating B1 field can be considered as being composed of two opposite rotating components.
2. These two components are located in the x,y frame
B1
time
The RF pulse
1. The oscillation frequency of B1c and B1ac is: = 2
2. The oscillating frequency will be set equal to the frequency of the rotating frame:
= o3. One component, B1c or B1ac
then will be static with respect to the rotating frame
z
y
x B1
B1ac
B1c
B1ac: B1 component, rotates anti clockwise
B1c: B1 component, rotates clockwise
Laboratory FrameLaboratory Frame
The RF pulse
1. The macroscopic magnetization Mz will rotate along the static component of the B1 field.
2. Any macroscopic magnetization aligned exactly with the static component of the B1 field will not move.
z
y
xB1c static
Rotating FrameRotating Frame
Mz
The RF pulse
1. The rotation angle depends on how long the field B1 is applied
2. Definitions:
pulse or flip angle
tp: time of B1 switched on
tp(90) time required for a 90o rotation
90o pulse: RF flips a macroscopic magnetization by 90o
Rotating FrameRotating Framez
y
xB1c static
Mz
time
tp
RF
The RF pulse
1. The excitation bandwidth is defined by the length of the 90o pulse
2. The excitation profile is described by a SINC-function
2. A short duration for the 90o pulse is required for a uniform excitation over the entire spectral range
time
tp
RF
-40-20160 140 120 100 80 60 40 20 0 ppm
frequency
+1/tp -1/tp
Excitation profile = sinc(0.5(Excitation profile = sinc(0.5(--)t)tpp))
The RF pulse
1. The intensity and phase of the NMR signal is given by the size and phase of the Mx,y magnetization
2. The magnetization vector can be described by the two projections to the z- and the x-/y-axis
3. The magnetization Mz does not create a NMR signal
z
y
x
M
My
Mz
The NMR experiment: what do we need?
1. The magnet2. The probe head3. Generation of RF pulses for excitation4. Preamplification of received signals5. Digital processing of analog NMR signal
The NMR experiment: what do we need?
1. The magnet:1. The magnet:
Requires control of field homogeneity SHIMRequires stabilisation of main field LOCKSHIM:SHIM:
additional coils with special field distribution,e.g. Z, Z2, Z3, X, Y, X3....We have cryo shims and room temperature shims
LOCKLOCK1.contineously determines frequency of 2H signal of the solvent (deuterated solvents)2. add a small extra field to the main field of the magnet to keep the overall field constant3. 2H signal also used for shimming
Basics of shims
Shims are used to compensate the magnetic field inhomogeneity in the sample area
Compensation is done by creating a magnetic field profile which has:– opposite sign compared to the inhomogeneity– same absolute intensity as inhomogeneity
Compensation requires a shim system to create the compensation field
Basics of shims
Shim field functional forms of some on-axis shims
Z
Z Z
Z Z
Z1 Z2 Z3
Z4 Z5
The Z axis is the axisof the magnet and the NMR sample tube
Basics of shims
Example: an inhomogeneity which would require the shim functions Z1 and Z2 to be adjusted
Z
Bo
Z
BShim
Z
B0
Z2
Z Z
Z1
The magnet‘s field before correction
correction field of the shim coil
superposition of magnet‘s field andthe correction field
1. The magnet:1. The magnet:
Requires control of field homogeneity SHIMRequires stabilisation of main field LOCKSHIM:SHIM:
additional coils with special field distribution,e.g. Z, Z2, Z3, X, Y, X3....We have cryo shims and room temperature shims
LOCKLOCK1.contineously determines frequency of 2H signal of the solvent (deuterated solvents)2. add a small extra field to the main field of the magnet to keep the overall field constant3. 2H signal also used for shimming
The NMR experiment: what do we need?
The lock: details
The lock channel can be understood as a ‚completely indepenant spectrometer within the spectrometer‘:
Transmitter 2H ProbeProbe Receiver 2H
Regulator
Shim systemShim system
amplitude,frequency
Ho
The resonance condition of NMR:
= Bo but: Bo is not stable
= (Bo+Ho) (Bo+Ho) = const.
The lock: lock phase
The lock receiver has two quadrature channels:
signal
=0o absorption:
=90o dispersion:
The lock: field homogenisation
The absorption signal is used for field homogenisation
The signal intensity is a measure for the field homogeneity:
sharp signal, high lock level
broad signal, low lock level
Intensity
The lock: field stabilisation
The dispersion signal is used for field stabilisation
The position of the zero-crossing of the signal is permanently checked
Determination of the zero-crossing frequency is more sensitive than determination of the frequency at maximum peak position
The lock: field stabilisation
(2H) (2H)
The lock: lock phase
If the lock phase is not adjusted correctly, absorption and dispersion signals will be mixed
Non-pure phases will result in:
– imperfect field homogenisation (shimming)– imperfect field homogenisation– field shifts during experiment using pulsed field
gradients
8.18.28.38.48.58.68.78.88.9 ppm
WATERGATE experiment:top: correct lock phasebottom: lock phase wrong by 30o
The lock: lock phase and GRASP
The lock: regulation parameters
Regulation parameters:Loop Gain: how strong to react on field disturbance
Loop Time: how fast to react „ „ „
Loop Filter: smoothing the lock signal to remove noise,
low pass filter
Wrong settings will result in:– instable signal position: suppression artifacts (NOE-
difference,...)
– noise around the signal
Use xau loopadj for adjusting the loop parameters
The lock: further parameters
Lock power:– 2H transmitter output power
– Due to different relaxation behavior of 2H for individual solvents, the lock power has to be adjusted for each solvent
– Too high lock power will result in an unstable lock signal
Lock gain:– receiver gain of the lock channel
– Gain too low: field homogenisation not optimum
– Gain too high:receiver is not linear, field homogenisation not optimum, spikes around NMR signals
The NMR experiment: what do we need?
2. The probe head:
Mainly is an antennatypically 3 RF channels:
2H: for the LOCK and shimming1H: for 1H-NMR and 1H-decouplingX: e.g. 13C, for 13C-NMR and 13C decoupling
The susceptibility of the coil material is crucial forbest line shape of the NMR signal
Helmholtz coils are mainly used for high resolution applications.
Example of a Helmholtz coil design
The NMR experiment: the probe
Sample location in the probehead
The NMR experiment: what do we need?
The probe
Pulse power:– Do not apply pulses at a power higher than specified for
the probe
– During endtest of the spectrometer the shortest possible pulses are calibrated. For pulse sequences those power levels might be too high, e.g. for 1H trim pulses in HSQC
– Carefully check the tuning and matching of the transmitter and decoupler channel
The probe
Additional notes:– Solvent volume: has to be adapted to the active length of
the coil used for observation
– Observe and decoupler coil: The decoupler coil is longer than the observe coil. Measuring a spectrum via the decoupler coil requires more solvent volumn:
• observe coil: >450l
• decoupler coil: >600l
The DEPT experiment
WALTZ16
90o 180o
90o 180o
1H
13C
1H channel:1H channel:different pulsespulse phases2 power levels
13C channel:13C channel:different pulsespulse phasesreceive signal
We have to create:We have to create:different frequencies with different phasesfast change of power levels for pulsesamplification of weak syntheziser outputexact timing of each actionswitch to the receiving modedigital preprocessing of the received data (FID)
The spectrometer
We have to create:We have to create:
•DPX,DRX,DMX:different frequencies with different phases FCU, syntheziserFCU, syntheziserfast change of power levels for pulses ASUASUamplification of weak syntheziser output BLAH, BLAXBLAH, BLAXexact timing of each action TCUTCUreceive signal HPPR, RX22 (SE451)HPPR, RX22 (SE451)digital preprocessing of the received data (FID) RCURCU
•Avance:different frequencies with different phases FCU, SGUFCU, SGUfast change of power levels for pulses SGUSGUamplification of weak syntheziser output BLAH, BLAXBLAH, BLAXexact timing of each action TCUTCUreceive signal HPPR, RX22HPPR, RX22digital preprocessing of the received data (FID) RCURCU
The Spectrometer: components
RF transmit path in the DRX console:RF transmit path in the DRX console:
FCU1
FCU2
Amplifier 1H
Syntheziser LOT ASU ROUTER
Amplifier X
Preamp 1H
Preamp X
BSMS 2H transmitter Preamp 2H
ProbeProbe
The Spectrometer: components
RF receive path in the DRX console:RF receive path in the DRX console:
Preamp 1H
Preamp X
Preamp 2H
FCU1
FCU2
Amplifier 1H
Syntheziser LOT ASU ROUTER
Amplifier X
BSMS 2H transmitter
ProbeProbe
BSMS 2HReceiver
RX22
The Spectrometer: components
RF receive path in the DRX console:RF receive path in the DRX console:
Preamp 1H
Preamp X
Preamp 2H
FCU1
FCU2
Amplifier 1H
Syntheziser LOT ASU ROUTER
Amplifier X
BSMS 2H transmitter
ProbeProbe
BSMS 2HReceiver
RX22
1. digitizing analog signal2. digital signal processing3. transfer to work station
1. digitizes analog signal2. analysis for field correction3. display signal
The receiver channel
Overview
ProbeProbeADC
Receiver Analog Digital Filters Antialiasing Filters
LO1 LO2
CH B
CH ARCU
The receiver channel
ProbeProbeADC
Receiver Analog Digital Filters Antialiasing Filters
LO1 LO2
CH B
CH ARCU
-40-20160 140 120 100 80 60 40 20 0 ppm
FID low frequency digitized FID digital filteringFID data reduction
The receiver: parameters for individual components
receiver gain of RX22 or SE451 rg, rga– RG chosen too low: bad dynamic, signals of low intensity
have bad sensitivity
– RG chosen too high: baseline distortion, phase cycles do not work,....
Analog antialiasing filters fw– automatically set by the software for RX22
– for SE451: fw=1.5*swh
Analog digital converter ADC– no parameters to set
The receiver: parameters for individual components
Digital filters on the RCU
User defined parameters:– DIGMOD: analog, digital or homodecoupling-digital
defines sampling rate of the ADC
– DSPFIRM: sharp, smooth or medium
defines number of coefficients for
the digital filter, depends on sweep width
– AQ_mod: qsim or DQD
DQD for perfect suppression of quadrature
images and O1-spikes
Some notes on digital filters
Digital filters and oversampling belong together
What is oversampling? – the FID is sampled faster than what is required for a
given spectral width
Dwell time DW
Some notes on digital filters
Sampling rate and spectral width SWH:
SWH = 1/2DW
-40-20160 140 120 100 80 60 40 20 0 ppm
DW[sec] SWH [Hz]
FT
Some notes on digital filters
Sampling rate and spectral width SWH:
SWHoversampling = 1/2DWoversampling
-40-20160 140 120 100 80 60 40 20 0 ppm
DW[sec] SWH [Hz]
FTDWoversampling
SWHoversampling [Hz]
Some notes on digital filters
The digital filter is a bandpass filter
The region of interest is extracted mathematically
-40-20160 140 120 100 80 60 40 20 0 ppm
SWH [Hz]
SWHoversampling [Hz]
A short demo of a digital filter
Demo using an audio WAV file:– selecting a frequency with a lowpass / highpass filter
– parameters for digital filter and filter quality
A short demo of a digital filter
Excitation parameters
Excitation frequency: O1, O1P
Spectral window: SW
Time domain data points: TD
Excitation sequence / pulse program: PULPROG
Excitation power e.g. for hard pulse: PL1
Length of 90o pulse: P1
Excitation parameters
Dwell time DW
TD
Time domain data points TD and acquisition time AQ:
AQ = TD * DW= TD/2SWH– The value for TD should result in an AQ which is long
enough to allow complete decay of the FID
Excitation parameters
O1 / O1P define the center of the spectral window:
-40-20160 140 120 100 80 60 40 20 0 ppm
SW/2 SW/2
O1 / O1P
Summary: essential acquisition parameters
Excitation:– excitation sequence: pulprog
– power level and 90o pulse: pl1, p1
– excitation center: o1p or o1
Acquisition:– attenuation of incoming RF: rg
– spectral window: sw
– # of sampled points: td
– mode for digital filters: digmod
– dummy scans ds
– coadded scans ns
Summary: essential processing parameters
General:– data points: si = 0.5* TD
– time domain baseline correction: bcmod
Window functions:– parameter for exponential window: lb
– parameter for gaussian window: lb, gb
– parameter for sin, sin2 window: ssb
End of document