Homonuclear dipolar recoupling is routinely used for magic-angle spinning NMR-based structure determination. In fully protonated samples, only short proton-proton distances are accessible to broadband recoupling approaches because of high proton density. Selective methods allow detection of longer distances by directing polarization to a subset of spins. Here we introduce the selective pulse sequence MODIST, which recouples spins that have a modest chemical shift offset difference, and demonstrate it to selectively record correlations between amide protons. The sequence was selected for good retention of total signal, leading to up to twice the intensity for proton-proton correlations compared with other selective methods. The sequence is effective across a range of spinning conditions and magnetic fields, here tested at 55.555 and 100 kHz magic-angle spinning and at proton Larmor frequencies from 600 to 1200 MHz. For influenza A M2 in lipid bilayers, cross-peaks characteristic of a helical conformation are observed.
Homonuclear dipolar recoupling is routinely used for magic-angle spinning NMR-based structure determination. In fully protonated samples, only short proton-proton distances are accessible to broadband recoupling approaches because of high proton density. Selective methods allow detection of longer distances by directing polarization to a subset of spins. Here we introduce the selective pulse sequence MODIST, which recouples spins that have a modest chemical shift offset difference, and demonstrate it to selectively record correlations between amide protons. The sequence was selected for good retention of total signal, leading to up to twice the intensity for proton-proton correlations compared with other selective methods. The sequence is effective across a range of spinning conditions and magnetic fields, here tested at 55.555 and 100 kHz magic-angle spinning and at proton Larmor frequencies from 600 to 1200 MHz. For influenza A M2 in lipid bilayers, cross-peaks characteristic of a helical conformation are observed.
Proton-detected magic-angle
spinning (MAS) NMR spectroscopy can be used to determine the structure
and dynamics of proteins with atomic resolution. Proton–proton
correlations obtained by recoupling homonuclear dipolar interactions
are direct indicators of the protein fold.[1−11] One broadly used method for dipolar recoupling is radio-frequency-driven
recoupling (RFDR), first introduced by Gullion and Vega[12] and Bennett et al.[13] for moderate MAS rates and 13C recoupling. It is also
applicable at ultrafast MAS rates of 55–100 kHz and above,
where the effects of finite pulses become important[14] and a heteronuclear version of the sequence becomes possible.[15] Proton–proton RFDR has been widely applied
for protein structure determination,[14,16−23] which, for fully protonated proteins, is done by measuring a dense
network of distances including side-chain protons.A characteristic
of broadband proton–proton recoupling in
fully protonated samples is that only particularly close spins show
correlations, while longer distances are hardly detectable.[24] This is the consequence of high proton density
in fully protonated protein samples and forms the basis for structure
determination involving side-chain protons.[17] Measurement of longer proton distances is challenging in these samples,
even with second-order recoupling schemes[25−30] that have been widely applied at both low and high MAS rates to
correlate carbon and nitrogen spins.Detection of longer distances
is elegantly achieved by selective
spin-labeling of 13C[31−33] or 1H.[34−39] For example, Linser et al.[39] reported
amide proton–proton correlations up to 10 Å for a perdeuterated
microcrystalline sample. Using deuteration and specific methyl proton
labeling, Huber et al.[40] detected 1H–1H correlations for distances up to 6
Å. The former implemented broadband zero-quantum recoupling using
RFDR, while the latter applied a double-quantum sequence, dipolar
recoupling enhanced by amplitude modulation (DREAM).[41] However, selective labeling is not always straightforward,
in particular for membrane proteins, for which amide exchange may
be inhibited.[42]Long-distance proton–proton
correlations can also be measured
by using selective recoupling experiments.[43−50] In band-selective spectral spin diffusion (BASS-SD)[47] selective 1H–1H transfer occurs
during a spin-lock pulse,[51] while in selective
phase-optimized recoupling (SPR)[46] selective 1H–1H transfers occur between spins with
symmetrical frequency offsets[46] (fA = – fB,
where fA and fB are the offsets of protons A and B). Both methods show significant
enhancement of the transferred signals with respect to RFDR. Xiao
et al. recently published theoretical investigations of SPR pulses
at low MAS rates.[52] In particular, they
investigated the behavior of p-SPR5 pulses at different
flip angles, p = π/4, π/2, and 3π/4,
and concluded that small flip angles result in a narrow selective
bandwidth.Here, we present a zero-quantum homonuclear dipolar
recoupling
method, the modest offset difference internuclear selective transfer
(MODIST) pulse sequence, where selective transfer occurs between spins
with small differences in their offsets. We based the MODIST sequence
on the jump-return[53,54] elements of SPR pulses[46] and modified the phase, the flip angles, and
the number of pulses in the block to maximize transfer between amide
spins, minimize transfer between amide and aliphatic spins, and, crucially,
retain maximal total amide signal. MODIST is constructed similarly
to π/4-SPR42, but the modified phase cycling significantly
modifies its transfer characteristics. The MODIST block consists of
16 π/4-pulses with the following phase cycling: yy̅x̅xx̅xy̅yy̅yxx̅xx̅yy̅ (Figure A). The
total length of the sequence corresponds to four rotor periods, such
that each pulse occupies one-quarter of the rotor period, with an
rf-field power of half the MAS rate.
Figure 1
Comparison of RFDR and MODIST transfers
in 2D (H)N(H)H spectra
of microcrystalline SH3. (A) The MODIST pulse sequence −16
π/4 pulses with the phase cycle yy̅x̅xx̅xy̅yy̅yxx̅xx̅yy̅ occupy four rotor periods (TR). (B)
(H)N(H)HMODIST (blue) and (H)N(H)HRFDR (red)
spectra (1.152 ms mixing). (C) Four slices from (H)N(H)HRFDR (red) and (H)N(H)HMODIST (blue) spectra, recorded at
eight different mixing times (in ms): 0.576, 1.152, 1.584, 2.016,
2.592, 3.168, 3.744, and 4.32, as labeled. The chemical shifts of
peaks I–V are (15N in ppm/1H in ppm):
I, (106.8/9.35); II, (113.7/8.74); IV, (128.7/7.8); V, (129.4/7.34).
The (H)NH reference spectrum is shown in gray. The proton carrier
was set to 8.2 ppm for the mixing. Data were recorded from an 800
MHz spectrometer with 55.555 kHz MAS. XY8 phase cycling was used for
RFDR. The full experimental details are given in the Supporting Information.
Comparison of RFDR and MODIST transfers
in 2D (H)N(H)H spectra
of microcrystalline SH3. (A) The MODIST pulse sequence −16
π/4 pulses with the phase cycle yy̅x̅xx̅xy̅yy̅yxx̅xx̅yy̅ occupy four rotor periods (TR). (B)
(H)N(H)HMODIST (blue) and (H)N(H)HRFDR (red)
spectra (1.152 ms mixing). (C) Four slices from (H)N(H)HRFDR (red) and (H)N(H)HMODIST (blue) spectra, recorded at
eight different mixing times (in ms): 0.576, 1.152, 1.584, 2.016,
2.592, 3.168, 3.744, and 4.32, as labeled. The chemical shifts of
peaks I–V are (15N in ppm/1H in ppm):
I, (106.8/9.35); II, (113.7/8.74); IV, (128.7/7.8); V, (129.4/7.34).
The (H)NH reference spectrum is shown in gray. The proton carrier
was set to 8.2 ppm for the mixing. Data were recorded from an 800
MHz spectrometer with 55.555 kHz MAS. XY8 phase cycling was used for
RFDR. The full experimental details are given in the Supporting Information.Numerical simulations of MODIST and comparison with SPR can be
found in Figures S1–S10 of the Supporting Information, where we investigate the efficiency of the method
assuming different values of dipolar coupling constants, offset differences,
flip angles of the selective pulses, carrier frequency settings, phase
cycle schemes, chemical shift anisotropy values, and MAS rates. In
simulations (two amide and two aliphatic proton spins), the ratio
between transferred and untransferred signals is inferior to SPR54, but the total transfer efficiency of MODIST is better overall
due to the high retention of the total amide signals. Although the
transfer efficiency of MODIST pulses is much less dependent on the
position of the proton carrier frequency in comparison to other selective
methods, the position of the carrier has an influence on the width
of the selective transfer, ΔfMODIST. We define ΔfMODIST as the offset
difference with which the transferred signal reaches at least 50%
of the maximal transfer with respect to the signal with zero offset
difference. On the basis of simulations, ΔfMODIST of amide protons is ∼0.64 kHz (Figure S1C), when the position of the carrier
is in the amide region (8.2 ppm). However, it can be increased up
to ∼0.9 kHz by setting the carrier to the aliphatic region
(Figure S6 and Table S1) without loss of efficiency.MODIST selectively transfers
signals at both 55 kHz (Figure ) and 100 kHz MAS (Figure S10). Figure compares MODIST
with an efficient broadband
recoupling method, RFDR, for fully protonated SH3. The MODIST implementation
of the (H)N(H)H experiment, (H)N(H)HMODIST, shows a higher
number of amide–amide correlations than (H)N(H)HRFDR even with a short mixing of 1.152 ms (Figure B). While broadband RFDR recoupling predictably
mixes signal among amide and aliphatic protons, MODIST results in
minimal signal in the aliphatic region between 0 and 6 ppm. The buildup
of selected peaks as a function of mixing time is shown in Figure C. Figures S11 and S12 compare XY414 and
XY8 phase cycles for RFDR pulses as a function of mixing time.[55]Table summarizes the assignments of isolated peaks (indexed as
I, II, IV, and V), the corresponding distances, and the 1H–1H offset differences.
Table 1
Assignments,
Distances (Proton–Proton),
and 1H–1H Offset Differences of Selected
Peaks from Figure a
H–H
distance (Å)
1H–1H offset diff
(ppm)
G51 HN–V44
HN
I
2.81
0.82
N35 HN–L34 HN
II
2.07
1.41
W41 HNε1–W41 Hδ1
III
2.60
2.8
A55 HN–A56 HN
IV
2.8
0.51
W42 HNε1–W42 Hδ1
V
2.56
1.87
Distances were taken from the
crystal structure of the SH3 domain (PDB: 2NUZ).
Distances were taken from the
crystal structure of the SH3 domain (PDB: 2NUZ).While peaks I, II, and IV cannot be distinguished from the noise
when using RFDR, they are above noise in the MODIST spectrum. However,
for peak V, RFDR results in twice the transfer efficiency, and peak
III (Figure B) is
lower than the noise level for MODIST. Peaks III and V are intra-side-chain
correlations between protons of W41 and W42 indole, respectively.
The low MODIST signal for these peaks is explained by the comparably
large offset difference between aromatic HNε1 and
Hδ1 proton spins, which is 1.87 and 2.8 ppm (or 1.5
and 2.24 kHz at an 800 MHz spectrometer) for W42 (peak V) and W41
(peak III), respectively. The intensity of peaks I–III is retained
at relatively long MODIST mixing time (Figure C), which again emphasizes that MODIST retains
total signal during mixing.To resolve long-distance correlations
and to test the method at
higher magnetic field where the amide frequency range is increased,
we recorded a 3D (H)N(H)(H)NHMODIST spectrum with 6.48
ms mixing at a 1200 MHz spectrometer. The proton carrier frequency
was set to 3 ppm. Figure shows the 15N–15N projection
with the assignment of selected peaks based on the chemical shifts.[34,56,57] With 6.48 ms mixing, we detect
seven peaks correlated to G51, with the longest distance at 6.8 Å
(G51-K43). The longest assigned distance is 7.3 Å, between D14
and M25. Peaks corresponding to these long distances likely arise
due to significant contribution of relayed transfer rather than direct
transfer alone. From the SH3 structure, it is evident that direct
transfer is detected for distances of at least 4.5 Å (Figure ). We also recorded
a 3D (H)N(H)(H)NHMODIST spectrum with 2.016 ms mixing using
an 800 MHz spectrometer. Although numerous correlations were observed
in the spectrum, most belong to nuclei within 4.5 Å due to a
short mixing of 2.016 ms. This spectrum is displayed in Figure S13A. Additional assignments of Figure are displayed in Figure S13B.
Figure 2
15N–15N projection
of the 3D (H)N(H)(H)NHMODIST spectrum (6.48 ms mixing)
recorded at 1200 MHz with
55.555 kHz MAS. Two strips, extracted from the 3D at the proton frequencies
of V9 and W42 ε1, are shown at the right, together with assignments
for the observed correlations, internuclear distances, and isotropic
chemical shift differences (Δδ). Distances were taken
from the crystal structure of SH3 (PDB code 2NUZ). The proton carrier
frequency was set to 3 ppm for the duration of mixing (further experimental
details are given in the Supporting Information).
15N–15N projection
of the 3D (H)N(H)(H)NHMODIST spectrum (6.48 ms mixing)
recorded at 1200 MHz with
55.555 kHz MAS. Two strips, extracted from the 3D at the proton frequencies
of V9 and W42 ε1, are shown at the right, together with assignments
for the observed correlations, internuclear distances, and isotropic
chemical shift differences (Δδ). Distances were taken
from the crystal structure of SH3 (PDB code 2NUZ). The proton carrier
frequency was set to 3 ppm for the duration of mixing (further experimental
details are given in the Supporting Information).Because MODIST has minimal dependence
on the carrier frequency
position, the approach is expected to be suitable for simultaneous
Hα–Hα and Hmethyl–Hmethyl mixing within (H)C(H)(H)CH spectra, where the carrier frequency
position is set to −1 ppm. Figure S14 shows the 13C–13C projection of such
a spectrum, recorded on SH3 using a 600 MHz spectrometer. As expected,
the peak intensity is reduced far from the diagonal (proton and carbon
frequencies of aliphatic moieties are correlated), and Hα–Hα
correlations can be observed. Because of the relatively small frequency
separation in the aliphatic spectrum, some mixing also occurs between
the alpha and methyl regions.Figure S15 compares MODIST and RFDR
for deuterated SH3 using an 850 MHz spectrometer. The frequency selectivity
of the method is evident in the suppression of cross-peaks to protons
near the extreme edge of the amide region, around 7 ppm. With 30.48
ms MODIST mixing, an additional peak, G51 to L33 (9.63 Å), is
detected. This correlation likely arises due to relayed transfer.We also evaluated MODIST spectra of the uniform 13C,15N-labeled influenza A M2 membrane protein (Figures and 4). The M2 protein assembles as a dimer of dimers,[58] such that each residue gives rise to two peaks, here indexed
as A and B in Figure . Upon comparison of 2D (H)N(H)HRFDR and (H)N(H)HMODIST spectra (Figures S16 and S17), MODIST again shows excellent retention of amide signal, while
RFDR efficiently mixes signal into the side-chain.
Figure 3
1D (H)N(H)H spectra of
the membrane protein influenza A M2 with
SPR42 (A), BASS-SD (B), or MODIST (C) mixing. The carrier
was set to either 13.7 ppm (green), 8.4 ppm (blue), or 3.7 ppm (red).
Descriptions of BASS-SD and SPR pulses are in Figure S21. The artifact peak from water at 4.7 ppm was removed
digitally. Data were recorded from a 600 MHz spectrometer with 55.555
kHz MAS.
Figure 4
15N–15N projections
of 3D (H)N(H)(H)NH
spectra of influenza A M2 comparing MODIST (blue, 2.736 ms mixing,
8.4 ppm carrier frequency) (A) with SPR42 (green, 2.736
ms mixing, 13.7 ppm carrier frequency) and (B) with BASS-SD (green,
4.608 ms mixing, 8.4 ppm carrier frequency). (C) Four slices from
the MODIST (blue), SPR42 (green), and BASS-SD (red) spectra,
marked with dashed lines in panel A. ∗ indicates artifacts.
Data were recorded from a 600 MHz spectrometer with 55.555 kHz MAS.
Further experimental details are provided in the Supporting Information.
1D (H)N(H)H spectra of
the membrane protein influenza A M2 with
SPR42 (A), BASS-SD (B), or MODIST (C) mixing. The carrier
was set to either 13.7 ppm (green), 8.4 ppm (blue), or 3.7 ppm (red).
Descriptions of BASS-SD and SPR pulses are in Figure S21. The artifact peak from water at 4.7 ppm was removed
digitally. Data were recorded from a 600 MHz spectrometer with 55.555
kHz MAS.15N–15N projections
of 3D (H)N(H)(H)NH
spectra of influenza A M2 comparing MODIST (blue, 2.736 ms mixing,
8.4 ppm carrier frequency) (A) with SPR42 (green, 2.736
ms mixing, 13.7 ppm carrier frequency) and (B) with BASS-SD (green,
4.608 ms mixing, 8.4 ppm carrier frequency). (C) Four slices from
the MODIST (blue), SPR42 (green), and BASS-SD (red) spectra,
marked with dashed lines in panel A. ∗ indicates artifacts.
Data were recorded from a 600 MHz spectrometer with 55.555 kHz MAS.
Further experimental details are provided in the Supporting Information.For M2 at 55.555 kHz, MODIST compares favorably with two selective
methods shown at 100 kHz MAS to improve amide–amide transfer
with respect to RFDR: BASS-SD[47] and SPR.[46]Figure compares 1D (H)N(H)H spectra obtained by using BASS-SD, π/4-SPR42, or MODIST, with the proton carrier frequency set to three
different values (13.5 ppm, green; 8.4 ppm, blue; 3.7 ppm, red). Of
the three, MODIST shows the highest retention of the total amide signal
as well as less dependence on the position of the carrier frequency. Table summarizes the normalized
intensities of amide signals for all three methods at 4.609 ms mixing.
For the three carrier frequencies, the aliphatic region is similar
for MODIST, while for BASS-SD and π/4-SPR42 strong
aliphatic transfer occurs for certain conditions. Figures S18–S20 show additional 2D (H)N(H)H spectra
comparing MODIST, SPR54, and π/4-SPR42. For SH3 at 100 kHz, similar peak intensities were observed for
both MODIST and BASS-SD.
Table 2
Maximal Intensity
(%) of π/4-SPR42, BASS-SD, and MODIST Signals at
4.608 ms Mixing for Three
Different Positions of the Carrier Frequency (Intensities Taken from Figure )
method
13.7 ppm
8.4 ppm
3.7 ppm
π/4-SPR42
19
0
8
BASS-SD
34
27
11
MODIST
33
40
46
Comparisons of transferred signals are shown in 15N–15N projections of 3D (H)N(H)(H)NH spectra with MODIST, BASS-SD,
or SPR42 mixing (Figure ). We chose 2.736 ms mixing for comparison of MODIST
and SPR42. Typical BASS-SD mixing is longer, and we therefore
compare a BASS-SD spectrum at 4.6 ms (a MODIST spectrum at 4.6 ms
is shown in Figure S21). Correlations in
the (H)N(H)(H)NHMODIST spectrum (blue) have ∼2 times
higher intensities than when employing SPR42 (green) and
BASS-SD (red), and at least five correlations could only be observed
when using MODIST. Cross-peak intensities can be compared in the slices
of the 15N–15N projection shown in Figure C. Three additional
correlations are observed in the 3D (H)N(H)(H)NHMODIST spectrum
with 4.608 ms mixing, two of which were assigned to correlations separated
by three residues, which confirms the known helical secondary structure
(Figure S21). At 4.6–5 Å, these
contacts correspond to relatively long distances. Figure S22 shows the 15N–15N
projection of the corresponding 3D spectrum using SPR54 (1.296 ms mixing), a double quantum mixing sequence.In summary,
we described MODIST, a selective dipolar recoupling
sequence, and demonstrated its performance for amide protons in fully
protonated samples. MODIST achieves efficient selective transfers
for a broad range of carrier frequency values. We presented MODIST
spectra of two fully protonated proteins, microcrystalline SH3 and
the membrane protein M2, and compared them with the broadband mixing
sequence RFDR and two selective methods, BASS-SD and SPR (π/4-SPR42 and SPR54). The advantageous features of MODIST
allowed the detection of 1HN–1HN correlations with up to 2-fold improvement in intensity
as compared with other state-of-the-art selective dipolar recoupling
sequences. The bandwidth of MODIST approximately covers the amide
region even at a magnetic field of 28.18 T (a 1200 MHz spectrometer),
which is the highest magnetic field currently available for high-resolution
NMR.
Authors: Mukul G Jain; Daniela Lalli; Jan Stanek; Chandrakala Gowda; Satya Prakash; Tom S Schwarzer; Tobias Schubeis; Kathrin Castiglione; Loren B Andreas; P K Madhu; Guido Pintacuda; Vipin Agarwal Journal: J Phys Chem Lett Date: 2017-05-15 Impact factor: 6.475