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NMR Training for Advanced Users . Huaping Aug 18, 2008. Two Insider Scoops. Receiving efficiency conceptually, it is similar to extinction coefficient in UV spectrospcopy; it characterizes how efficient a unit magnetization can produce a signal by a given NMR receiver

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two insider scoops
Two Insider Scoops
  • Receiving efficiency
    • conceptually, it is similar to extinction coefficient in UV spectrospcopy; it characterizes how efficient a unit magnetization can produce a signal by a given NMR receiver
    • NMR signal size is proportional to receiving efficiency
    • Receiving efficiency can be pre-calibrated as a function of 90° degree pulse length
    • receiving efficiency is the same for all nuclei of the same type (indifferent to chemical shifts) in the same sample
  • Solvent signal offers a universal and robust concentration internal standard
    • Normalized NMR signal size is strictly proportional to concentration for a given sample, regardless how concentrated or dilute the sample is
    • Unit magnetization generates the same amount of total NMR response, which is indifferent to chemical shift or line-shape
outlines
Outlines
  • Basic preparations for NMR: safety, sample, lock, shim and tune
  • Understanding NMR: excitation and observation
  • RF pulse calibration
  • NMR observables:
    • Chemical shift, scalar couplings, NOE and relaxations
  • Introduction to basic 2D's
  • Simulations for spin systems, pulses and sequences
safety
Safety
  • Personal safety
    • Cryogens: do not lean on or push magnets
    • Cryoprobes: avoid contact with transfer line
    • Magnetic and RF hazards
  • Instrument safety
    • Know the limits of instruments
    • Probe limits: avoid excessive long decoupling and long hard pulses or their equivalents
    • Be conservative
    • Double check pulse program and parameters for any non-standard new experiment
  • Data Safety
    • Back up data promptly and regularly
    • Data processing or manipulation has no impact on the raw (FID) data
    • Do not change parameters after data are acquired
sample
Sample
  • Rule #1: for Bruker NMR spectrometers, the NMR tube insert cannot exceed max depth (19mm or 20mm) from the center of the RF coil
    • Longer insert than recommended may present problems for the probe, as well as cause frictions during spinning
    • Varian is more flexible in allowing longer insert
  • Rule #2: center of NMR sample should be as close as possible to the center of RF coil.
    • Normal sample needs to about 500 ul or slight more
    • Too much solvent is a waste!
    • Too little solvent may make shim difficult, but it does work!
  • 10% deuterated solvent is sufficient for locking

RF coil

18mm

Coil Center

 20mm

samples of smaller volumes
Samples of smaller volumes
  • Follow rule # 1 and then rule #2
  • Shimming might be challenging due to air/glass and air/solution interfaces
  • Consider Shigemi tubes
  • Be careful with spinning
    • Non-spinning is recommended for volume ~ 300 ul or less

300ul

400ul

500ul

sensitivity for smaller volumes
Sensitivity for smaller volumes
  • Volume less than 300 ul may not offer additionally sensitivity improvement over that achieved by 300 ul, if the total amount of analyte is constant
tune and match the probe
Tune and match the probe
  • Only higher fields (500, 600 and 800 HMz) in our facility need tuning
  • Most of the time only proton channel requires tuning
  • Drx500-2 with BBO needs special attention
    • Proton always needs tuning
    • BB (used for 13C or 31P etc) channel needs tuning, by first dialing the numbers to the pre-set values

Carrier frequency

RF reflection

tune

match

Frequency

significance of tuning matching
Significance of tuning/matching
  • Shorter 90 degree pulse
    • More efficient use of RF power
      • Protects transmitter
    • More uniform excitation in high power
  • Better sensitivity
    • Reciprocity: if excitation is inefficient, then detection is equally inefficient
  • Potentially quantitative:
    • The product of NMR signal size is inversely proportional to the 90 degree pulse length
recognizing bruker probe types
Recognizing Bruker probe types

side view

side view

magnet

1H tuning/matching rods are labeled as yellow

bottom view

Do not touch those!

Dials for broadband (BB) tuning/matching

Tabulated values for BB tuning/matching

BB Dialing stick

BBO probe on drx500-2

TXI probe

slide11
Lock
  • Lock depends on shim: bad shim makes bad lock
    • Initialize shim by reading a set of good shims (i.e. rsh shims.txi)
    • Inheriting a shim set from previous users may present difficulties
    • Unusual samples (esp. small volumes) may need significant z1/z2 adjustments
  • Use “lock_solvent” or “lock” command
    • The default (bruker) chemical shift may appear as dramatically changed if the spectrometer assumes another solvent
  • Avoid excessive lock power
    • Lock signal may go up and down if lock power is too high due to saturation of deuterium signal
    • Apply sufficient lock power and gain so that lock does not drift to another resonance (this may happen by autolock if multiple deuterium signals exist)
slide12
Shim
  • The goal of shim is to make the total magnetic field within the active volume homogeneous (preferably <1Hz).

Total magnetic field =

static field (superconductor) + cryoshim (factory set) + RT shim (user adjust)

  • Shim can be done either manually or by gradient, which can be very efficient and consistent if done properly
  • Sample spinning may improve shim
    • However, spinning-side band appear
  • Recommendation:
    • Start from a known good shim set (by rsh on bruker or rts on varian).
    • Do not inherit shims from other users unless you know they’re good
    • Non-spinning and higher order (spinning) shims should not change dramatically from sample to sample for most applications
lock lock gain
Lock: lock gain

recommended

not recommended

higher lock gain

Lower lock level

due to lower lock gain

may easily lose lock;

change in lock level (during shimming) is less visible

lock avoid high lock power
Lock: avoid high lock power

Bad lock

Good lock

Lock power okay

Lock power too high

unstable lock and lower level

evaluate shims
Evaluate shims
  • Look for a sharp peak
    • No clear distortion
    • Full width at half height should be about 1 Hz or less for small molecules
    • Small (1% or smaller) or free of spinning side-bands
  • Check if peak distortions are individual or universal
  • Make sure that phasing is not causing peak distortions
  • Maximize the lock level
    • Higher lock level => better shim
  • Lock level does not drop significantly when spinning is turned off
shim by line shape
Shim by line-shape

Plot made by G. Pearson, U. Iowa, 1991

make z4 smaller first

z4 too small

z4 too big

understanding nmr
Understanding NMR
  • Modern NMR spectrum is an emission spectrum
  • Equilibrium state
    • Magnetization is along +z axis
    • It is desired to have the largest +z magnetization prior to excitation
  • Excitation by a RF pulse
    • A projection of magnetization is made on xy plane
    • It is desired to have the largest xy plane project for observation
  • Observation
    • Precession of the projected xy- plane magnetization
rf pulses
in

out

coarse attenuator

fine attenuator

RF pulses
  • RF pulse manipulates spins
    • Important in excitation and decoupling
    • Defined by length, power and shape
  • RF power is expressed in decibels
    • Bruker
      • Power range: typically 0db (high power) to 120db (low power)
    • Varian:
      • Coarse power: typically 60db (high) to 0db (low); 1 db increment; absolute
      • Fine power: 4095 (high) to 0 (low); default is 4095; relative
        • e.g. 54.5db can be roughly achieved through setting coarse power to 55 and fine power to 3854
rf pulse calibration
RF pulse calibration
  • Hard pulse (high power pulse) can be calibrated directly or indirectly
  • For best calibrations, pulses need to be on resonance (know the chemical shift or resonance frequency!)
  • Soft or shaped pulsed can be first calculated and then fine-tuned to optimum
    • Shapetool (by Bruker) or Pbox (by Varian) can be used for calculation and simulation
    • Be aware of possible minute phase shift (several degrees for soft pulses), which can be critical in water flip back or watergate
proton pulse calibration
Proton pulse calibration
  • Most hard (highest power) 90° pulses are typically from 5 us to 20 us.
  • Direct observation for high power proton pulse calibration (or even for heteronuclei if sensitivity is sufficient)
    • 360° method (not quite sensitive to radiation damping or relaxation)
    • 180° method

90º

First pulse with 2 us; 2 us increment

90º

180º

360º

450º

270º

180º

360º

270º

nmr observables
NMR observables
  • Chemical shifts
    • expressed in ppm
  • Scalar couplings
    • expressed in Hz
    • 2D or nD bond correlations
  • NOEs / relaxation / line-shapes
  • Peak size
    • Potentially useful in quantitative analysis
chemical shifts
Chemical shifts
  • Reflects chemical environment:
    • Ring current effect
      • Outside of ring: high ppm
      • Inside: low ppm
    • Effect of electron withdrawing groups
      • Donating: low ppm
      • Withdrawing: high ppm
example aliasing
Example: aliasing

okay

sw=16ppm

aliased

(from arx300) aliased from 0 ppm with phase distortion,

because the peak is out of the “detection window”

  • Oversampled proton spectrum on higher fields (500 – 800 MHz) does not have the aliasing issue: peaks outside of sw will disappear
spectral aliasing cont d
Spectral aliasing (cont’d)
  • In direct observe dimension, spectral aliasing is generally avoided by either increasing spectral width (sw) or moving center frequency (sfo1)
  • Sometimes the indirect detection dimension (in nD spectrum) may intentionally adopt aliasing to improve resolution in that dimension
scalar coupling
1

JAB

JAB

AB system

“roofing”

1:1

dA

dB

1:2:1

1:3:3:1

Scalar coupling
scalar coupling simulation helps
a

b

Scalar coupling: simulation helps!

pro-chiral!

8Hz

12Hz

8Hz

These are not impurities!

Ha and Hb are not exactly equivalent, with

chemical shift difference of 0.025ppm

Observed (300 MHz)

simulated

example satellites and spinning side bands
Example:satellites and spinning side-bands

6.6 Hz; 29Si satellites; 2.3% each

spinning sideband; 20 Hz from center

120 Hz; 13C satellites; 0.55% each

TMS

dipolar coupling noe
Dipolar coupling: NOE
  • NOE depends on correlation time (molecule size) and resonance frequency
  • NOE does not always enhance the observed signal

13C

31P

1H

15N

Molecule size

Temperature

noe implication in quantification
NOE implication in Quantification
  • The observed nucleus should be free of interference from other nuclei
  • Pre-saturation in aqueous samples may not be appropriate for accurate quantification
    • Small molecules tend to gain signal size due to positive NOE from saturated water
    • Large molecules tend to lose signal size due to spin diffusion
relaxation
Relaxation
  • T1 relaxation allows magnetization to recover back to +z axis
    • Nuclei with larger gyromagnetic ratios (resonance frequencies) tend to relax faster
      • 1H: 0.1 – 10 s (proteins have short T1’s)
      • 13C, 15N, 31P: much longer than 1H
    • Nuclei in a proton rich environment tend to relax faster
  • T2 relaxation contributes to the observed resonance line-shape
    • T2~T1 for small molecules
    • Line-shape offers an estimate of T2
line shape
Line-shape
  • Full Width at Half Maximum is 1/(pT2*) Hz, with T2* as apparent spin lattice relaxation time
  • Magnetic inhomogeneity (shim) can increase FWHM (2l) or distort the line-shape (reduce T2*)
  • T1 > T2 > T2*
  • Small molecules
    • 1H: T1 ~ T2 in the order of seconds
    • 13C: seconds to tens of seconds; even longer if no proton attached (CO and quaternary)
  • Large molecules
    • 1H: T1 ~ T2 hundreds of mini-seconds or shorter
    • 13C: seconds or sub-seconds

FWHM (2)

Lorentzian: A(w)=  / (2 + (-0)2)

2=1/(pT2*)

multiple chemical environments chemical or conformational exchange
multiple chemical environments:chemical or conformational exchange
  • Fundamentally, chemical shift reflects chemical environment surrounding a nucleus’
  • Multiple chemical environments may alter chemical shift or even cause significant peak broadening

Fast exchange

slow exchange

Jin, Phy. Chem. Chem. Phys. (1999)

n h line shape influence of relaxation and scalar coupling
(N)H line-shape: influence of relaxation and scalar coupling

In addition to chemical exchange, (N)H proton line-shape is also influenced by the coupled nucleus 14N

JNH ~65 Hz

Slow 14N relaxation (compared to JNH)

medium14N relxation

Fast relaxation

this might be the very reason why CHCl3 proton appears as a singlet though JH-35Cl and JH-37Cl exist

improving sensitivity
Improving Sensitivity
  • More scans in a given amount of time
  • Use Ernst angle a for excitation:

cos a = exp(-Tc/T1)

  • Increase concentration with less solvent / salt

Tc/T1

sensitivity

Pulse angle (degrees)

improving sensitivity1
Improving sensitivity
  • Receiver gain needs to be maximized which requires good water suppression
  • Avoiding excessive large receiver gain (for signal clipping)
  • Excessive acquisition time end up with spending time collecting noise and down-grade signal to noise ratio
missing a carbonyl carbon presumably due to insufficient relaxation
Missing a carbonyl carbonpresumably due to insufficient relaxation

About 5 mg in CD3OD. 2800 scans (~4 hrs)

?

Missing a carbonyl

solution use h 2 o
Solution: Use H2O
  • Why it works:
  • Carbonyl 13C is reduced due to presence of a proton rich environment in H2O.
  • Potential intra-molecular hydrogen bond is weakened or broken, and decoupled from ring movement

In H2O:D2O (1:1). 1400 scans (~2 hrs).

direct observe 31 p 13 c or 15 n
Direct observe: 31P, 13C or 15N
  • 19F, 31P and 13C can be observed directly on all PINMRF 300 and 400 MHz instruments (please follow local PINMRF instructions)
  • 13C can be observed on higher fields (500 MHz and above), without any cable change
  • Drx500-2 with BBO probe offers higher sensitivity for 31P, 13C, 15N and most other heteronuclei (19F excluded)
    • Observed nucleus needs to be cabled to x-broadband pre-amplifier
    • BBO tuning is needed for both proton and observed nucleus
    • Double check filters if re-cabled
direct observe 31 p 13 c or 15 n1
Direct observe: 31P, 13C or 15N
  • Satellite peaks can frequently be indirectly observed in proton spectrum (so that we know the less sensitive heteronuclei are there to be observed directly!)
  • Decoupling of proton may improve signal by
    • Sharper peaks
    • NOE
    • Proton channel has to be tuned!
1d acquisition for very long hours
1D acquisition for very long hours
  • helpful
    • Split long experiments into smaller blocks and save data regularly (multiple data can always be summed if needed)
    • Dissolve the compound in water (H2O) might be helpful (shorter relaxation time)
    • Lower sample temperature may help
  • Not helpful
    • Save several days’ data into one single FID
    • Use 300 ul or less volatile solvent
from 1d to 2d
From 1D to 2D

FT

1D

t2

w1

time domain

frequency domain

FT(t2)

FT(t1)

2D

w1

t1

t1

t2

w2

w2

frequency domains

time domains

2d nmr
2D NMR
  • Correlate resonances through bond or space
    • COSY: coupling
      • Magnitude mode recommended.
      • 1 mg or less will do
      • Minutes to a couple of hours
    • TOCSY: coupling network
      • ~ 70 ms mixing time
      • 1 mg or less will do
      • An hour or longer
    • NOESY / ROESY: distance / NOE
      • Mixing time ranging from less than 100 ms (proteins) to 500 ms (small molecules)
      • 1 mg or more
      • Hours or longer
    • HSQC/HMQC: proton correlation to X, typically through one-bond scalar couplings (two or three bond correlation possible)
      • 1mg or less will do
      • An hour or longer
    • HMBC: proton correlation to X, through multiple bond scalar couplings
      • 1 mg or more
      • Hours or longer
2d nmr1
2D NMR
  • Resolve overlapping peaks
    • Resolution is provided largely through the indirect dimension
    • No need to have highest resolution in the direct detected dimension
      • Limit direct acquisition time to 100ms or less if heteronuclear decoupling is turned on
      • Lower decoupling power if longer acquisition time is needed
    • Change in experimental conditions may help
2d nmr essentials acquisition
2D NMR essentials: acquisition
  • Proton tuning and matching
  • Calibration of proton (90 degree) pulse length
    • Standard pulse lengths can be used if the solution is not highly ionic (< 50 mM NaCl equivalent)
    • All proton pulses are likely getting longer if the solution is ionic and/or the probe is not tuned
  • Modest receiver gain
    • rg about half of what rga gives or less
  • Carrier frequency (center of spectrum in Hz) and SW (sweep width) in both dimensions (avoid aliasing unless intended to)
  • Number of scans (NS)
    • The pulse program recommends NS (a integer times 1, 2, 4, 8 or 16)
    • Needs some dummy scans, especially with decoupling / tocsy
  • Number of increments in the indirect dimension (td1)
    • Larger td1 improves resolution in the indirect dimension
    • Rarely exceeds 512 (except occasionally in COSY
  • Detection method in the indirect dimension
    • Determined by the pulse program
    • Typically is either states (and/or TPPI) or echo-antiecho
  • Acquisition time (aq) less than 100 ms with decoupling
  • Modest gradients (cannot be more than the full power of 100% and typically less than 2 ms in duration)
  • Go through the pulse program if you really care
2d processing
2D processing
  • Window functions
    • Allow FID approach zero at the end of the acquisition time
    • Sine bell functions with some shifts are recommended most of the time
  • Zero filling
    • Typically double data points in each dimension
  • Phasing
    • Indirect dimension zeroth and 1st order corrections are recommended in the pulprogram. If not, use 0 for both
    • Direct dimension first order phase is rarely more than 50 degrees. Zeroth order can be anywhere from 0 to 360 degrees
    • Phase in the 2D mode to best appearance
  • Referencing
    • Can be done by picking a known resonance in the spectrum
    • Or referenced by (external) protons
hsqc a block diagram
Magnetization transfer pathway:

F1(H) -> F2(X) -> F2(X,t1) -> F1(H) -> F1(H,t2)

INEPT

HSQC: a Block Diagram

90

180

1/4J

1/4J

1/4J

H

1/4J

acq

90

180

t1/2

t1/2

X

dec

States: =x and =y are acquired for same t1 and treated as a complex pair in Fourier transform. No need to change receiver phase

TPPI: =x, y, -x and –y are acquired sequentially in t1, and receiver phase is incremented too. Real Fourier transform.

hmqc or hsqc
HMQC or HSQC

codeine

Magnitude HMQC (9 mins)

Easy set up and slightly higher sensitivity

Phase sensitive HSQC (18 mins)

Better resolution

adapted from acornnmr.com

hmqc and hsqc comparison
HMQC

Fewer pulses

More tolerant to pulse mis-calibrations

Allows homonuclear (proton) coupling in the indirect dimension

HSQC

More pulses

Less tolerant to pulse mis-calibrations

No homonuclear (proton) coupling in the indirect dimension

HMQC and HSQC comparison
data presentation
Data Presentation
  • Processed data can be readily viewed, manipulated and printed by xwinplot (wysiwyg)
  • Xwinplot can readily output .png, .jpg or .pdf files for publications or presentations
  • Files can be transferred through secure ftp
pulse sequence the heart and soul of nmr
Pulse sequence:the heart and soul of NMR

;zggpwg

;this is a bruker sequence

prosol relations=

#include

#include

"d12=20u"

1 ze

2 30m

d1

10u pl1:f1

p1 ph1

50u UNBLKGRAD

p16:gp1

d16 pl0:f1

(p11:sp1 ph2:r):f1

4u

d12 pl1:f1

(p2 ph3)

4u

d12 pl0:f1

(p11:sp1 ph2:r):f1

46u

p16:gp1

d16

4u BLKGRAD

go=2 ph31

30m mc #0 to 2 F0(zd)

exit

ph1=0 2

ph2=0 0 1 1 2 2 3 3

ph3=2 2 3 3 0 0 1 1

ph31=0 2 2 0

;comments for parameters…

Delay only; be very careful with critical command in a labeled line

90x

180x

label

1H

90-x

90-x

Delay

define f1 power level

G

90° pulse on f1

Gradient pulse

On-res: dephased by two gradients

Off-res: refocused by two gradients

Shaped 90° pulse

Acq. and go to label 2

Write to disc. And go to label 2

Phases

where things are bruker file structure
Where Things are: Bruker File Structure
  • User NMR data /u/data/username/nmr
  • Pulse programs /u/exp/stan/nmr/lists/pp
  • Gradient programs /u/exp/stan/nmr/lists/gp
  • Shaped pulses /u/exp/stan/nmr/lists/wave
  • decoupling /u/exp/stan/nmr/lists/cpd
  • Frequency(f1) lists /u/exp/stan/nmr/lists/f1
  • Parameter sets /u/exp/stan/nmr/par
  • Shim sets /u/exp/stan/nmr/lists/bsms
  • Macros /u/exp/stan/nmr/mac
gradients
Gradients
  • Homospoil gradients
    • Size of duration may not matter much
    • Stronger ones tend to clean up unwanted magnetization better
  • Gradient echoes:
    • Exact ratios between multiple gradients must follow
    • Diffusion loss must be considered for small molecules, especially during long echoes
      • Log of signal size is proportional to -g2g2d2D
simulations
Simulations
  • Can be easily performed for pulses, spin-systems or pulse sequences
  • Save experimental time
  • Enhance our understanding of NMR
  • Most frequently used for shaped pulses
shaped pulse what and why
Shaped Pulse: What and Why
  • What
    • Narrow sense: amplitude modulation only, while phase is constant
    • Broad sense: amplitude and phase modulation
  • Why
    • To achieve perturbation over a certain frequency range (uniform and selective)
      • Narrow bandwidth: shaped pulse. e.g. Gaussian
      • Wide bandwidth: adiabatic pulse
how is shaped pulse different
How is Shaped Pulse Different
  • Composite pulse is typically a block of square pulses with constant phases
    • Pulse integration does not correlate with pulse angle
    • Pulse calibration come from individual component
  • Adiabatic pulse sweeps frequency (phase has strong time dependence)
    • Pulse integration does not correlate with pulse angle
    • Pulse calibration depends on sweep range, and somewhat on adiabaticity too
  • Simple shaped pulse can be calibrated by integration
    • Caveat: a 180° pulse is not necessarily twice of a 90° pulse
    • Some shaped pulses are good for 180° inversions (z -> -z) while others are good for 90° excitations (z -> x/y)
shaped pulse examples
Shaped Pulse Examples
  • Square pulse: simplest shaped pulse; good for simple hard excitation
  • Gaussian and Sinc: good selectivity; for proton
  • Gaussian cascade: G4, G3, Q5 and Q3; for carbon
    • G4 for excitation
    • G3 for inversion
    • Q5 for 90°
    • Q3 for 180°

Gauss

Sinc1

G4

G4: four Gaussian lobes

choosing shaped pulses
Choosing Shaped Pulses
  • Define the goal
    • excitation, inversion or refocusing
    • length or power level
      • Rule of thumb: bandwidth is ~ 1/P360 or RF strength (for square pulses)
    • shape
  • Power requirement
    • peak power may not exceed certain level
  • Length requirement
    • Be aware of probe limit on length in case of high power
    • While longer pulses tend to have better selectivity, relaxation / scalar coupling may limit pulse length
  • Run pulse simulation and calculation
    • Bandwidth needs to be first satisfied
    • Simulated frequency profile is to have top-hat behavior
    • Phase needs to be linear in the region of interest
shaped pulse calculation
Shaped Pulse Calculation
  • Rule of thumb:
    • 6db change in power results two fold change in pulse length

DdB = 20 log (P90/P90ref)

    • e.g. 10us @0db => 20us @6db for the sample pulse angle
  • For a shaped pulse with a imperfect linear amplifier,

DdB = 20 log (P90*shape_integ/P90hard*comp_ratio)

Modern spectrometers have comp_ratio close to 1

  • Adiabatic pulses require different treatments
example setting up a sinc pulse
1 means one sinc lobeExample: Setting up a Sinc Pulse
  • Within xwinnmr, launch shape tool by typing “stdisp” or from menu
  • Within shape tool, choose shapes -> sinc. Change lobe number to 1 and click “OK”
  • On the left is the amplitude profile (sinc shape) and (constant) phase is shown on the right
example a sinc pulse cont d
Example: a Sinc Pulse (cont’d)
  • Within shape tool, choose analyze -> integrate pulse. Make necessary updates. In this particular case, we assume the reference is 9.5 us @1.5db and you wish to calculate for 1000us 90 degree pulse. Then click OK
  • The power level is calculated as 35.8db compared with the reference. Click “seen”
  • If satisfied, you can save this shaped pulse under /u/exp/nmr/stan/lists/wave/.
  • Go back to xwinnmr->ased, and update the sinc1 shaped pulse as pulse length of 1ms, and power level to be 35.8 + 1.5 (since reference 9.5us is @ 1.5db) = 37.3db
  • If needed, the shaped pulse power can be fine tuned by gs, or a careful calibration
pulse simulation
Pulse Simulation
  • Within shape tool, choose analyze -> simulate. Update the length as 1000us and rotation angle as 90 (for sinc1 we just set up). Click “OK”.
  • A new Bloch module will show default (x,y) profile for excitation. Click on z to view z profile.

z

pulse simulation cont d
Pulse Simulation (cont’d)
  • If you decide that the starting magnetization is x, you can click (in Bloch module) “calculate”->”excitation profile”. Change initial Mx to 1 and Mz to 0. Click “OK” and then the excitation profile will be updated.
  • If you wish to examine trajectory (how a magnetization at a given frequency responds to the sinc1 pulse), you can click “time evolution”, and update initial values etc (may not allow too many steps). Click “OK”.
advanced nmr training

Advanced NMR Training

10-12 noon, 8/18 (Monday)

BROWN 3106

Contact Huaping Mo for details

slide65
Demo
  • Sample preparation; Shigemi tube
  • Lock and shim
  • Tune and match
  • Calibration of 90 degree pulse
  • Calculation / simulation of pulses
  • Set up 2D: COSY and HSQC
  • Processing and present data (xwinplot)
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