Fast Tocsy On AM-400/500

                                           February 15, 1992  R. Nunlist

The TOCSY (TOtal Correlation SpectroscopY) experiment is ordinarily used to map spins belonging to a common system. This is accomplished by the application of a spin lock pulse with a suitable mixing time to let magnetization propagate through the mutual spin-spin couplings. If the mixing time is short, the total correlation fails: All we get is a regular COSY - like spectrum. By itself, this is nothing extraordinary; why not use the regular COSY experiment? The answer is found in a paper by Marion (J. Magn Reson 85, 393, 1989). The TOCSY experiment uses a 'trim' pulse which leads to rapid de-phasing of the magnetization. This eliminates the need for phase cycling. By using the trim pulse, we can therefore work with one scan per increment and reduce the recycle delay to about T1!
By comparison, the COSY type experiments require a minimum phase cycle of four steps, often more steps are used to further reduce artifacts. In addition, if the recycle delay is shorter than 3 x T1, further problems can arise.
Using the TOCSY experiment with a short mixing time (10 to 12 ms), it is possible to acquire a COSY equivalent at least four times faster. Of course, it is assumed that the S/N is not the limiting factor. With most samples, this is not a problem.

Below is an example of our old favorite, rotenone. About 5 mg of sample, using the QNP probe, yielded this in about 6 minutes!

A mixing time of about 12 ms, L6 = 6 was used. With no dummy scans, and NS = 1, 77 increments were acquired before I ran out of time. Most time was spent writing to disk - acquisition plus disk write averaged about 6 seconds on the AM-400.
The VBAMX should produce the same result in less than 2 minutes - the disk write takes only 30 ms!

A quick and dirty way to get it done:

1) Flip REVERSE/NORMAL switch to REVERSE.
2) RJ COSYDQQ.400=D1, PJ COSYDQQ.400=D1, RJ2D COSYDQQ.400=D1.
Set SI=SI2=1k. Set SI1=512W, TD1=512W. Set WDW=WDW1=SINE.
Set SSB2=SSB1=2.

Assuming the system is shimmed and locked, determine O1 for regular proton nmr (default or use SO). Then, set O2 to that value.
Set PR = H 1 (this MUST be done).

Use AS INVH1.AU to set up the proton parameters.

Set NS = 1, P1 = 37, S1 = 6. AU to set the receiver gain.
Set P1 around 75, determine the 180 deg pulse (not very critical).

Now we are ready:

AS MLEV17PH.AU.
Set P1 to 1/2 of what you found the 180 deg pulse to be.  S1 should already be
set.
Set P2 to 180 deg.
Set P4 to 2000 (the 2 ms trim pulse).
Set D1 to about T1.
L6 should be set such that (L6 x 66 x P1) is about 10 to 12 ms.
Set NE to 256.

After the acquisition has finished, use NET (BRUKNET) from the second terminal
to send the .SER file to the X32 workstation. 


Parameter Examples for AM-500/400:

Size:		1k x 256w, zero filled to 512w x 512w final matrix
Acquisition:	5 to 30 minutes,  depending on NS, D1 and NE
Processing:	About 10 minutes on the X32
Plotting:	5 minutes

Set-up

The experimental set up is similar to COSYPHDQ.AU and the phase sensitive version of COSY (COSYPH.AU).

Set-up using Job Files (the long way)

First, obtain a 1D spectrum using the normal mode. Set observe window to the actually needed region with OW or, in EP, CTRL/O. Re-run spectrum to be sure that possible foldover does not obscure any region of interest. FW may need to be reduced. Process and check reference peak assignment. For later plotting, in EP, set for full expansion by 'CTRL/R, U'. Note F1 and F2 limits for input in OW below. Select DU=D4 (or D2)! Set MAXY=CY=5. Use 'TI' if title is desired. Store the spectrum on disk, e.g. MYTOCSY1D.001.

1) Use: RJ COSYDQB.500( or COSYDQQ.400)=D1 followed by PJ <cr><cr>, RJ2D COSYDQB.500. This sets default values for size, window functions etc. The width is set for 8 ppm to 0.25 ppm. (TMS will fold at 0.5 ppm!). For solvents other then CDCl3, use 'SO' to determine new O1, then set O2 to that value. If the window needs changing, use 'OW' to select new window. Note that after SO, SR1 and SR2 need to be changed to the same value as SR. If OW was used, 'ST2D' is needed again; now set I2D back to 1. Be sure that O2 and DW have been typed!

Set NS =1, DS=0.

If the 90 deg decoupler pulse is not known, determine it as follows:

- Set PR = H 1 (this MUST be done).
- Use AS  INVH1.AU to set up the proton parameters.
- Set  NS = 1, P1 = 37, S1 = 6.  AU to set the receiver gain.
- Set P1 around 75, determine the 180  pulse by varying P1 (not very
  critical).
- Set P1 to half the value of the 180  pulse.

Now proceed:
	Set NE.
	'WJ2D MYTOCSY.001'  For later parameter print-out.
	Set MAXY=CY=5. 'TI' if title is desired. Store spectrum on disk.

2)Be sure all parameters are set as follows:

          F2           F1
TD=       1k           256w
SI=       1k           1k
SF=      (SF of 1D)    (SF of 1D)
SW=      (SW of 1D)    (will be SW/2)
HZ/PT=	» 2 to 10
WDW=	  S             S
LB=       i.            i.
GB=       i.            i.
SSB=      2             2
HZ/PT2/HZ/PT1= 1

SIZE.SER IN K=256k   REDF= N
SIZE.SMX IN K        REV=  Y
MC2= W       MAXM= >500
NE= 256      ND0=  2
set I2D = 1. (this resets SI1, Set SI1=1k again)

The SI, TD and NE values may need to be adjusted to obtain digital resolution of 2 to 6 Hz, depending on sweep width SW! This is best done by setting:

New SI, TD. Enter new NE (= SI/4 for square matrix). Type ST2D to update the relevant 2D parameters. Store the new parameters with 'WJ2D MYTOCSY.001'.


Explanation of the Parameters and Settings

	F2		F1
	TD 1k       TD1 256w    Number of points to acquire
	SI 1k       SI1 1k      Number of points to transform
	SSB1=       SSB2=2      90 ([[pi]] /2) shifted sine-bell
	WDW1=       WDW2=S      window for both dimensions

MC2  = W	for phase sensitive calculation
REV  = Y	to reverse diagonal
REDF = N
ND0  = 2	Two D0's in pulse sequence. Set SI1 again to 1k
I2   = 1	sets SW1 = SW/2 for square matrix
NE  = 256	number of increments (serial files)

3) Without exiting the parameter display, type 'AS MLEV17PH.AU' to set up the pulse program parameters.

	PW = RD =0 
	P1 = 90  deg       37.5 usec @S1 = 6 (on AM-400)
	P2 = 180 deg
	P4 = 2000          (2 ms trim pulse)
	P6 = 180 deg       75 usec @S1 = 6 (on AM-400)
	D0 = 3E-6           (3 usec)
	L6 = 5             (12 ms mix)
	D1 = about T1.     This depends on your sample!
	NS = 1..
	DS =0
	IN =set by SW1 

4)	EXPT estimate time required.  (Note: EXPT sums all delays 
         whether they are used or not.  It may give an unreasonable
         estimate if unused delays  are not set to zero.)

5)	AU 	File name will be asked for. MUST HAVE .SER extension, e.g.
        MYTOCSY.SER.
While the 2D spectrum is acquired, the 1D FID can be sent to the X32 and processed for use as projections. use NET (BRUKNET) from the second terminal to send the FID, e.g. MYTOCSY.001=D3.

6) After the end of acquisition:

Send the MYTOCSY.SER to the X32 for processing. If you insist to process on the instrument:

	RJ COSYDQQ.400=D1, PJ <cr><cr>.
	ST2D MYTOCSY.SER=D2 (or D4).
	RJ2D MYTOCSY.001 (or COSYDQQ.400) to get parameters back.
	XFB [MYTOCSY.SER] to transform in both dimensions and generate MYTOCSY.SMX
Before processing, the phase parameters need to be set. The 1D phases should be used. If not noted above, switch jobs, PJ MYTOCSY1D.001. Type TY to read phase values. In 2D job, set PC0 = PHZ0-90deg. , PC1 = PHZ1. Execute phase correction with 'PZ'. These values will be used for phase correction after first FT.

Type ST2D [MYTOCSY.SER]. SET SI1 =SI2. Set, if needed: SR1 = SR2(1D), ND0=2, WDW1 = WDW2 = S, SSB1 = SSB2, = 2 ([[paragraph]] /2).

XFB [MYTOCSY.SER] to transform in both dimensions and generate MYTOCSY.SMX
View positive ('+') and negative levels ('-'). AP2D, etc. as in COSY. To plot, use CPLB or CPPB. See Bruker manual for details.

Note:
Additional phase correction in the second dimension can be performed with the 'XF1P' command. The phase parameters can be established by reading a column (RSC) and subsequent phase correction in EP. XF1P will then use those values.

7) The following plot parameters have been set by reading COSYDQB.500:
CX =CY =18; MAXY =24; DPO for X, Y-axis, offset=0.


Processing in Uxnmr:

Uxnmr does not know that the spectra were acquired in reverse mode.
  • Uxnmr on X32:
    To fix this, type '2s bf1', enter 500.13, type '2s o1', enter 8000. (400.13 and 6300 an AM-400) or whatever values you used. The macro "aminv" prompts for these parameters. Type (xmac) 'aminv'. to run the macro.


  • Other Applications

    The same approach can probably be used for many other purposes. For instance, nuclei with a wide shift range (19F) require a long experimental time. Using the TOCSY approach should make it more feasible to run a homonuclear 2D correlation.

    Adding trim pulses at the end of an acquisistion might possibly be useful with other experiments as well.


    Measurements

           AM-500:		          7/25/91
    
      Inverse probe
    
      90deg.  Reverse Mode Decoupler pulse	@ 0H =   8.2 usec.
    					@ 1H =  17 usec.
    
     5 mm Broad Band Probe:
      90deg.  Decoupler pulse		@ 0H =     usec
      90deg.  Decoupler pulse		@ 0H =     usec (reverse mode)
    					@ 1H =     usec
    					@ 2H =     usec
    ________________________________________
    
         AM-400:
    
         QNP Probe:                   (2/14/92)
    
    90deg.  Reverse  mode Decoupler pulse 	@ 0H = 10.3
    					@ 1H =      usec
    					@ 2H =      usec
    					@ 6H = 37.5 usec
    
      Inverse Broad Band Probe:
    
    For the BB probe the 
    90deg.  decoupler pulse 	        @ 1H = is about 9 usec.
    

    Wiring Changes

    No wiring changes are needed BUT: For REVERSE MODE (Proton pulses from Decoupler):

    On the Console: Flip the NORMAL/REVERSE switch to REVERSE (up) .position


    Checklist

  • Before the experiment:
  • Is the REVERSE-NORMAL Switch set?
  • Is O2 set for O1 etc?
  • Is PR = H 1 ?
  • After the experiment:
  • Is the REVERSE-NORMAL Switch back to the NORMAL Position?
  • Fill out the Log book, please! If something was omitted, the next user might have a chance to figure out what to do!


    Questions, comments to: Rudi Nunlist rnunlist@bloch.cchem.berkeley.edu

    Last Update: 12/23/94.