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Review
. 2019 Jun-Aug:112-113:55-102.
doi: 10.1016/j.pnmrs.2019.05.002. Epub 2019 May 11.

Characterizing micro-to-millisecond chemical exchange in nucleic acids using off-resonance R relaxation dispersion

Affiliations
Review

Characterizing micro-to-millisecond chemical exchange in nucleic acids using off-resonance R relaxation dispersion

Atul Rangadurai et al. Prog Nucl Magn Reson Spectrosc. 2019 Jun-Aug.

Abstract

This review describes off-resonance R relaxation dispersion NMR methods for characterizing microsecond-to-millisecond chemical exchange in uniformly 13C/15N labeled nucleic acids in solution. The review opens with a historical account of key developments that formed the basis for modern R techniques used to study chemical exchange in biomolecules. A vector model is then used to describe the R relaxation dispersion experiment, and how the exchange contribution to relaxation varies with the amplitude and frequency offset of an applied spin-locking field, as well as the population, exchange rate, and differences in chemical shifts of two exchanging species. Mathematical treatment of chemical exchange based on the Bloch-McConnell equations is then presented and used to examine relaxation dispersion profiles for more complex exchange scenarios including three-state exchange. Pulse sequences that employ selective Hartmann-Hahn cross-polarization transfers to excite individual 13C or 15N spins are then described for measuring off-resonance R(13C) and R(15N) in uniformly 13C/15N labeled DNA and RNA samples prepared using commercially available 13C/15N labeled nucleotide triphosphates. Approaches for analyzing R data measured at a single static magnetic field to extract a full set of exchange parameters are then presented that rely on numerical integration of the Bloch-McConnell equations or the use of algebraic expressions. Methods for determining structures of nucleic acid excited states are then reviewed that rely on mutations and chemical modifications to bias conformational equilibria, as well as structure-based approaches to calculate chemical shifts. Applications of the methodology to the study of DNA and RNA conformational dynamics are reviewed and the biological significance of the exchange processes is briefly discussed.

Keywords: Chemical exchange; Hoogsteen; Nucleic acid dynamics; R(1ρ) relaxation dispersion; Tautomers.

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Conflict of interest statement

Declaration of Interests

Hashim M. Al-Hashimi (H.M.A.) is an advisor to and holds an ownership interest in Nymirum Inc., which is an RNA-based drug discovery company. The research reported in this article was performed by Duke University faculty and students and was funded by NIH and NIGMS contracts to H.M.A.

Figures

Figure 1.
Figure 1.
Time diagram showing key developments in RD NMR techniques for characterizing chemical exchange in biomolecules with emphasis placed on R studies and their application to nucleic acids.
Figure 2.
Figure 2.
Historical progression of the development of R RD techniques for applications to nucleic acids. A) The on-resonance R(1H) RD profile measured for formamide by Solomon et al.[55] was the first reported measurement of R in liquids. Reproduced with permission from Bibliotheque nationale de France (BNF).B) The chair-chair inter-conversion in cyclohexane was one of the earliest conformational transitions characterized by RD methods[62, 63].C) R(19F)measurements on N-trifluoroacetyl phenylalanine in exchange between free and enzyme-bound states by Sykes et al.[73] constituted the first application of R RD in the context of biological macromolecules. D) Some of the earliest applications of R in studies of conformational exchange in biomolecules targeted 1H nuclei (red circles) in nucleic acid duplexes in the early 1990s[–111]. E) On-resonance R(15N) RD profile for backbone amide 15N of C38 in bovine pancreatic trypsin inhibitor was one of the first reported characterizations of conformational exchange in isotopically labeled proteins using R[122]. Reprinted by permission from [122]. F) Secondary structure transition in U6RNA involving flipping out of a bulge nucleotide; this was one of the first validated models for ESs in nucleic acids[135]. G) First structure of an ES by Kay et al.[153] for a folding intermediate of the G48V mutant of the Fyn SH3 domain obtained using chemical shifts measured using CPMG RD and structurebased chemical shift calculations. Reprinted by permission from [153]. H) Expressions for R outside the fast exchange limit by Palmer et al.[23] allowed extensions of the R method by demonstrating the feasibility of extracting all exchange parameters at a single magnetic field. RD profiles were shown to be centered at the ES chemical shift. Simulated off-resonance profiles (for pES = 0.048, kex = 1500 s−1, Δω = 2400 rad s−1, R1,GS = R1,ES = 1.5 s−1, R2,GS = R2,ES = 11 s−1 and ω1/2π = 1000 Hz) are shown using the asymmetric population expression in Palmer et al.[23] (dotted line) and fast exchange expression (dashed line). The exact numerical solution is shown as a solid black line. Reproduced with permission from [23]. I) Off-resonance R(15N) RD profile for the amide 15N of Q11 in a G48M mutant of the Fyn-SH3 domain; this was the first experimental measurement of off-resonance R using low spin-lock amplitudes and selective excitation experiments[163]. This study also represented the first instance wherein a complete set of exchange parameters was extracted using R measurements. Reprinted with permission from [163]. J) Excited state Hoogsteen BPs in duplex DNA were the first ESs to be structurally characterized in nucleic acids using R RD.Rates and populations were obtained using off-resonance R experiments as described by Al-Hashimi et al.[115].
Figure 3.
Figure 3.
Thermodynamic and kinetic characteristics of a system undergoing two-state chemical exchange. A) Free energy diagram for two-state exchange. B) Time evolution of a molecule exchanging between a dominant GS and sparsely populated and short-lived ES. C) Distribution of τGS and τES, the dwell times for the GS and ES.
Figure 4.
Figure 4.
Chemical exchange under free precession. A) NMR spectra for a system undergoing two-state GS-ES chemical exchange simulated using the B-M equations. Columns correspond to different values of pGS while rows correspond to different values of kex. Simulations were performed assuming Δω¯ (13C)=3 ppm, γ(1H)B0/2π = 700 MHz and R2,GS = R2,ES = 10 s−1. B) Magnetization of GS (blue) and ES (red) spins in the rotating frame of the GS at the slow exchange limit. Black arrows represent the passage of time while colored arrows represent exchange events. Dots surrounded by circles denote vectors perpendicular to the plane of the figure. C) GS-ES chemical exchange leads to dephasing with time of the bulk magnetization corresponding to the GS (black arrow). The black dot near the x-axis corresponds to the receiver phase. D) Exponential decay due to chemical exchange of the bulk GS magnetization along the x axis (MGSx) as a function of time. E) The magnetization of the GS (blue) and ES (red) spins in the rotating frame of the population-weighted average (AVG) resonance in the fast exchange limit.
Figure 5.
Figure 5.
The mono-exponential decay of magnetization due to chemical exchange under free precession conditions is a consequence of the exponential dwell time distributions of the GS and ES. (A and B) Normalized bulk x-magnetization MGSx (black dots) of the GS as a function of time for a system undergoing GS-ES exchange, simulated using the vector model. An exponential fit to the magnetization is shown in red. Panel A is simulated assuming exponential probability distributions for the GS and ES dwell times (< τGS > = 0.33 s and < τES > = 0.14 s), while panel B is simulated assuming that the ES and GS dwell times follow a standard normal distribution. Expressions for the probability distributions of τGS and τES are given in the inset. Simulations assumed the following exchange parameters: Δω¯ (13C)=3 ppm, γ(1H)B0/2π = 700 MHz, and R1,GS= R1,ES = R2,GS = R2,ES = 0 s−1 for panels A and B.
Figure 6.
Figure 6.
Line-width at half maximum (LW1/2, units Hz) for the dominant GS resonance as a function of Δω¯ for a system undergoing GS-ES exchange under free precession, simulated using the B-M equations (kex = 1500 in red and kex = 2750 in black). Simulations assumed the following exchange parameters: pES = 0.05, γ(1H)B0/2π = 700 MHz, R1,GS= R1,ES = R2,GS = R2,ES = 0.0 s−1, while Δω¯ (13C) was varied linearly between 0.1 and 40 ppm in 100 equally spaced increments. Solid lines denote (R2+pESkex)/π while dotted lines denote a Δω value where (kex/Δω) ~ 0.2.
Figure 7.
Figure 7.
Influence of the spin-locking field during an R experiment in the absence of chemical exchange. A) In the lab frame (left), the spin-locking field B1 (black arrow) can be decomposed into two fields B1+ and B1 rotating in opposite directions (green and cyan arrows). The short black arrow represents the passage of time. A black dot surrounded by a circle represents a vector perpendicular to the plane of the figure. Black dots near the x-axes correspond to the receiver phase. ωrf is the angular frequency of the spin-lock. Variation of the spin-locking field amplitude as a function of time is shown on the right. B) Evolution of B1+ and B1 in the rotating frame of B1+. The static magnetic field is reduced to ΔB. C) Effective fields under on- and off-resonance conditions in the rotating frame of the spin-lock.
Figure 8.
Figure 8.
Modulation of the effective field by variation of the spin-lock amplitude (ω1) and offset frequency (Ω) in an R experiment in the absence of chemical exchange. Influence of changing ω1 (A) and Ω (B) on the effective field ωeff in the rotating frame.
Figure 9.
Figure 9.
Schematic representation of the R experiment in the absence of chemical exchange. The equilibrium magnetization tilted along z′, the direction of ωeff,OBS, is immediately spin-locked by the application of an RF field (green arrow), after which it decays exponentially due to relaxation with a rate constant R. A cross within a circle denotes a vector perpendicular to the plane of the figure. All vector diagrams are in the rotating frame where the spin-locking field appears stationary.
Figure 10.
Figure 10.
Time course of the evolution of normalized magnetization during an R experiment in the absence of chemical exchange, as a function of the spin-lock amplitude ω1, the offset Ω and the relaxation rates, simulated using the B-M equations. A) R1 = 2.5 s−1 and R2 = 22.5 s−1; B) R1 = 25 s−1 and R2 = 225 s−1. The time course for the position of the tip of the net magnetization vector M (with its base at the origin) is denoted as a solid black line, with green and red dots denoting the positions of the vector tip at the start and end (Tmax = 0.015s) of the relaxation period, respectively. The effective field direction is denoted using a dashed red line.
Figure 11.
Figure 11.
R in the presence of chemical exchange. A) ωeff,GS (blue) and ωeff,ES (red) in the rotating frame where the spin-locking field ω1 appears stationary, for two-state and n-state exchange. B) Alignment of the net magnetization at the start of an R experiment for a system undergoing GS-ES exchange under fast and slow exchange regimes. C) Rotation of the magnetization of GS/ES spins around their respective effective fields leads to dephasing of the bulk magnetization along ωeff,OBS during the R experiment. Shown is a representative example under conditions of fast exchange.
Figure 12.
Figure 12.
Comparison of off-resonance R RD profiles as obtained from B-M simulations and the vector model, in the absence of relaxation, for a wide variety of exchange parameters. Rows correspond to variations in kex while columns correspond to variations in pES. Spin-lock amplitudes are color coded while solid vertical green lines correspond to an offset Ω = –Δω; Δω¯(13C)=3 ppm, γ(1H)B0/2π = 700 MHz. 10,000 spins were used for the vector model simulations. The initial alignment of the magnetization for the B-M and vector simulations was performed as described in Section 6.1. In the vector model simulations, the magnetization of the GS and ES spins initially aligned along ωeff,OBS was allowed to precess about ωeff,GS and ωeff,ES with angular velocities ωeff,GS and ωeff,ES, respectively. The dwell times of the spins in the GS and ES were sampled from exponential probability distributions as described in Section 3.1, following which they were allowed to exchange with each other, while retaining the same orientation of the magnetization in 3D space prior to exchange. The sum of the magnetization of all the spins is projected along ωeff,OBS as a function of time to obtain R, which is used to obtain Rex, as described in Section 3.2 – 3.4.
Figure 13.
Figure 13.
Time course of the evolution of the normalized GS, ES and net magnetization during an off-resonance R experiment, simulated using the B-M equations. Time course for the positions of the tips of the GS, ES and net magnetization vectors (each with their base at the origin), denoted as solid blue, red and black lines respectively, with green dots in each case denoting the positions of the vector tips at the start of the relaxation period, and violet dots denoting their positions at the end of the relaxation period, respectively. Directions for the GS,ES and AVG effective fields are denoted using blue, red and green dashed lines, respectively. Also shown as insets are the variations of the normalized projections of the net magnetization along ωeff,OBS (M) as a function of time (black dots), along an exponential fit of the same (red line). Simulations were performed using kex = 20000 s−1 for panel A, kex = 20 s−1 for panels B and C. The other parameters used for all simulations were pES = 0.1, Δω¯(13C)=3 ppm, γ(1H)B0/2π = 700 MHz, R1,GS = R1,ES = 2.5 s−1, R2,GS = R2,ES = 22.5 s−1 and Tmax = 0.25 s. The initial alignment of the magnetization for the B-M and vector simulations was achieved as described in Section 6.1.
Figure 14.
Figure 14.
Dependence of on-resonance R on exchange and spin-lock parameters.A) Δω and ω1 modulate Rex via changes in φ, the angle between ωeff,GS and ωeff,ES. Also shown are positions of the magnetization vectors corresponding to GS (blue circles) and ES (red circles) obtained using vector model simulations in the form of Sanson-Flamsteed projections[192]. ωeff,GS and ωeff,ES are indicated by black and red stars respectively. Simulations were performed with the following parameters - pES = 0.01, kex = 20,000 s−1, Δω¯(13C)=3 ppm, γ(1H)B0/2π = 700 MHz, ω1/2π = 1000 Hz when on-resonance with the AVG state. Positions of the spins for a larger Δω¯(13C)=10 ppm (right) and ω1/2π = 3000 Hz (left) are also shown. Simulations employed 10,000 spins with a relaxation delay of 0.012s.B) Variation of R2 + Rex with ω1 under on-resonance conditions as a function of exchange parameters, as obtained using B-M simulations. Rows and columns correspond to the indicated values of kex and pES, respectively. Dashed line denotes the value of R2. The other exchange parameters used were Δω¯(13C)=3 ppm, γ(1H)B0/2π = 700 MHz, R1,GS= R1,ES = 2.5 s−1 and R2,GS = R2,ES = 22.5 s−1. The initial alignment of the magnetization during the B-M simulations was performed as described in Section 6.1.
Figure 15.
Figure 15.
Vector model simulations to illustrate the dependence of Rex on φ, ωeff,GS and ωeff,ES during an on-resonance R experiment for a system undergoing two-state GS-ES exchange. A) Variation of Rex with φ for a fixed ωeff,GS and ωeff,ES, under fast and slow exchange conditions. Simulations were performed using ωeff,GS = 1000*2π rad s−1 and ωeff,ES = 1131*2π rad s−1 when on-resonance with the GS under slow exchange conditions. ωeff,GS = 1000*2π rad s−1 and ωeff,ES = 1128*2π rad s−1 under fast exchange conditions while maintaining the AVG state onresonance by suitably adjusting the offset of the GS and ES. Similar trends are observed for alternative values of the precession frequencies (data not shown). B) Heat maps of Rex as a function of ωeff,GS and ωeff,ES for a fixed φ under fast and slow exchange conditions. Horizontal dotted lines (blue) correspond to the condition ωeff,ES = kex. Orientations of the effective fields were kept fixed at those corresponding to application of ω1/2π = 1000 Hz on resonance. Similar trends are also observed for R, and for both Rex and R under off-resonance conditions, as long as the magnetization decay is mono-exponential (data not shown). For panels A and B, simulations were performed using 10,000 spins with pES = 0.01, Δω¯(13C)=3 ppm, γ(1H)B0/2π = 700 MHz, R1,GS= R1,ES = 0.0 s−1, R2,GS = R2,ES = 0.0 s−1. The relaxation delays used were 3 s and 0.6 s for kex = 200 and 20000 s−1, respectively. For both panels, the initial alignment of magnetization and its projection to calculate Rex, was performed as described in Section 6.1.
Figure 16.
Figure 16.
Variation of R2 + Rex as a function of ω1 under on-resonance conditions as a function of exchange parameters, obtained using B-M simulations. Rows and columns correspond to the indicated values of kex and pES respectively. Panels with dotted lines correspond to exchange scenarios where the decay of the magnetization is not mono-exponential. Other parameters were: Δω¯(13C)=3 ppm, γ(1H)B0/2π = 700 MHz, R1,GS = R1,ES = 2.5 s −1 and R2,GS = R2,ES = 22.5 s−1. The initial alignment of the magnetization was performed as described in Section 6.1.
Figure 17.
Figure 17.
Variation of R, φ and Rex with ΩGS during an off-resonance R experiment under slow-exchange conditions with ωeff,ES < kex. Representative diagrams showing ωeff,GS (blue vector) and ωeff,ES (red vector) at selected offsets are also shown. The exchange parameters used were: pES = 0.01, kex = 200 s−1, Δω¯(13C)=3 ppm, γ(1H)B0/2π = 700 MHz, R1,GS= R1,ES = 0.0 s−1, R2,GS = R2,ES = 0.0 s−1, ω1/2π = 600 Hz along with a relaxation delay of 3.0 s. The initial alignment of the magnetization during the B-M simulation was performed as described in Section 6.1.
Figure 18.
Figure 18.
Changes in R2 + Rex as a function of kex and pES for two-state exchange during an off-resonance R experiment, simulated using the B-M equations. Horizontal comparisons show changes in kex while vertical comparisons show changes in pES. Spin-lock amplitudes are denoted using different colors. Solid gray vertical lines correspond to an offset of –Δω, while the yellow star denotes exchange parameters typical of Watson-Crick to Hoogsteen exchange in B-DNA[115]. Other exchange parameters used are: Δω¯(13C)=3 ppm, γ(1H)B0/2π = 700 MHz, R1,GS = R1,ES = 2.5 s −1 and R2,GS = R2,ES =22.5 s−1. The initial alignment of the magnetization was performed as described in Section 6.1.
Figure 19.
Figure 19.
Variation of R2 + Rex with kex during an R experiment when on-resonance with the ES (pES = 0.01, Δω¯(13C)=3 ppm, γ(1H)B0/2π = 700 MHz, R1,GS = R1,ES = 2.5 s −1 and R2,GS = R2,ES =22.5 s−1). Spin-lock amplitudes are color-coded. Vertical lines denote the indicated values of kex. The initial alignment of the magnetization during the B-M simulations was performed as described in Section 6.1.
Figure 20.
Figure 20.
Representative experimental off-resonance R RD profiles for two-state exchange under fast and intermediate exchange. The profiles were measured for U31-C1′ and C24-C1′ in HIV-1 TAR at 25 °C and 35 °C, respectively[166]. Spin-lock amplitudes are color-coded. Error bars represent experimental uncertainties determined by a Monte-Carlo scheme (Section 6.3). Solid lines denote global fits to the RD data using the B-M equations[166]. The initial alignment of the magnetization during the B-M fitting was performed as described in Section 6.1. Gray vertical lines correspond to the offset value when on resonance with the ES. Reproduced with permission from [166].
Figure 21.
Figure 21.
Variation of R2 + Rex during off-resonance R experiments, for a wide range of kex and pES values for two-state exchange, simulated using the B-M equations. Horizontal comparisons show changes in kex while vertical comparisons show changes in pES. Different spin-lock amplitudes are denoted by colors. Dotted lines correspond to cases where the decay of the magnetization is not mono-exponential. Solid gray vertical lines correspond to an offset of –Δω, while the yellow star denotes a typical Watson-Crick to Hoogsteen exchange scenario in DNA[115]. Simulations assumed the following parameters: Δω¯(13C)=3 ppm, γ(1H)B0/2π = 700 MHz, R1,GS = R1,ES = 2.5 s −1 and R2,GS = R2,ES = = 22.5 s−1. The initial alignment of the magnetization was performed as described in Section 6.1.
Figure 22.
Figure 22.
Exploring the limits of the sensitivity for off-resonance R experiments using B-M simulations for R(15N)(left) and R(13C) (right), at γ(1H)B0/2π = 700 MHz. For each Δω¯ value, detectability of R was assessed for 10,000 (pES, kex) combinations. 100 pES values ranging between 0.005 % to 20 % were chosen such that they were equally spaced on a logarithmic scale. For each of these pES values, 100 kex values ranging from 1 to 400000 s−1 were chosen such that they were equally spaced on a logarithmic scale. For each (pES, kex) combination, offresonance R RD Profiles were simulated using the B-M equations, assuming spin-locking amplitudes ω1/2π = 100, 250, 500, 1000 and 2000 Hz, each with 24 offset points Ω evenly spaced such that −3.5*ω1 < Ω < +3.5*ω1, without experimental error. A rate Rex of at least 5 Hz above the baseline R2 was assumed to be the threshold of detectability. The above curves were obtained by drawing a line through the lowest detectable pES for every kex value; thus all combinations of kex and pES to the right of the curves are detectable. Similar limits are observed when profiles are simulated with 5% error and re-fit to the Bloch-McConnell equations, and considered to be detectable when the fitted exchange parameters deviate from the simulated exchange parameters by less than 2-fold. For each panel, the Δω¯ values are color-coded. For all simulations, R1,GS = R1,ES = 2.5 s−1 and R2,GS = R2,ES = 22.5 s−1. The initial alignment of the magnetization during the B-M simulations was performed as described in Section 6.1.
Figure 23.
Figure 23.
Off-resonance R RD profiles for three-state exchange simulated using B-M equations. A) Off-resonance R RD profiles for three-state exchange in a star-like topology with pES1 = 1 %, pES2 = 2 %, kex,1 = 2,000 s−1, Δω¯1(13C) = 5 ppm 13C, Δω¯2(13C) = −7 ppm, γ(1H)B0/2π = 700 MHz, R1,GS = R1,ES = 2.5 s-1 and R2,GS = R2,ES = 22.5 s-1, with kex,2 = 1,000 s-1 (left) and kex,2 = 10,000 s−1 (right). Dotted lines correspond to RD profiles for individual GS-ES1 and GS-ES2 exchange, while the solid lines correspond to the RD profiles for the three-state exchange process. Solid blue and green lines correspond to offsets of -Δω1 and -Δω2 respectively. B) ESs exchanging in a three-state star-like topology with similar chemical shifts (Δω¯1(13C) = Δω¯2(13C)= 3 ppm, γ(1H)B0/2π = 700 MHz) but different exchange rates and populations (pES1 = 3 %, pES2 = 5 %, kex,1 = 15000 s-1, kex,2 = 1000 s-1, R1,GS = R1,ES = 2.5 s-1 and R2,GS = R2,ES = 22.5 s-1) can be resolved using off-resonance R RD (fitted parameters: pES1 = 2.5 ± 0.4 %, pES2 = 5.0 ± 0.7 %, kex,1= 14092 ± 1605 s−1, kex,2= 926 ± 220 s−1, Δω¯1(13C)=3.2±0.3 ppm and Δω¯2(13C)=3.1±0.7 ppm. The B-M profiles were corrupted by noise with 5 % errors in R prior to fitting. A vertical green line denotes an offset of -Δω1. In both panels, spin-lock amplitudes are color coded. The direction of the initial alignment of the magnetization during B-M simulations was determined as described in Section 6.1, while taking into consideration the ES with the highest population.
Figure 24.
Figure 24.
Representative experimental off-resonance R RD profiles for a system with threestate exchange in a star-like topology. Measurements were performed on C15-C3′ in A6-DNA at pH 6.8, 25 °C, as described by Al-Hashimi et al.[117]. Spin-lock amplitudes are color-coded. Error bars represent experimental uncertainties determined by a Monte-Carlo scheme (Section 6.3). Solid lines denote a global fit to the RD data[117]. The initial alignment of the magnetization during the B-M fitting was performed as described in Section 6.1, while taking into consideration the ES with the highest population. Vertical black lines correspond to offsets of -Δω1 and -Δω2. Reprinted by permission from [117].
Figure 25.
Figure 25.
Off-resonance R RD profiles for three-state exchange in the presence of direct “minor” exchange between the ES1 and ES2, simulated using B-M equations. Variation of offresonance R RD profiles for three-state exchange with triangular and linear exchange topologies as a function of kex,minor and kex,1. Vertical blue and green lines correspond to offsets Δω1 and -Δω2, respectively. The RD profile in gray corresponds to three-state exchange in a star-like topology (pES1 = 1 %, pES2 = 2 %, kex,1= 2000 s−1, kex,2 = 1000 s−1, Δω¯1(13C)=5 ppm,Δω¯2(13C)=7 ppm, γ(1H)B0/2π = 700 MHz, R1,GS = R1,ES = 2.5 s−1 and R2,GS = R2,ES = 22.5 s−1). Exchange parameters (other than kex values) for the linear exchange topologies were the same as for the star-like topology. Different spin-lock amplitudes are indicated by colors. The direction of initial alignment of the magnetization during B-M simulations was determined as described in Section 6.1, while taking into consideration the ES with the highest population.
Figure 26.
Figure 26.
Representative experimental off-resonance R RD profiles showing three-state exchange with “minor” exchange i.e., direct exchange between the two excited states[195]. Shown in solid lines are three-state fits to the experimental off-resonance R RD profiles (hpGT-GGC, pH 8.0, 10 °C) with and without direct “minor” exchange between the two excited states[195], with the inclusion of “minor” exchange fitting the data better. Spin-lock amplitudes are color-coded. Error bars represent experimental uncertainty determined based on a Monte-Carlo error propagation scheme (Section 6.3). The direction of initial alignment of the magnetization during B-M fitting was determined as described in Section 6.1, while taking into consideration the ES with the highest population. Reprinted by permission from [195].
Figure 27.
Figure 27.
Impact of unequal R2,GS and R2,ES on off-resonance R RD profiles for two-state exchange simulated using B-M equations. Variation of off-resonance R RD profiles with ΔR2 as function of kex for A) Δω¯(13C)=15 ppm, B) Δω¯(13C)=3 ppm and C) Δω¯(13C)=0 ppm. Different ΔR2 values are color coded. Exchange parameters are specified in inset. For all simulations γ(1H)B0/2π = 700 MHz and R1,GS = R1,ES = 2.5 s−1. Direction of initial alignment of the magnetization during B-M simulations was determined as described in Section 6.1. While fitting the mono-exponential decay, the magnetization for the first 0.05 s was not considered, in order to exclude the fast initial decay, as proposed by Kay et al.[187].
Figure 28.
Figure 28.
A) Pulse sequences for measuring off-resonance R(13C) and R(15N) in nucleic acids with selective excitation and low spin-lock amplitudes. Hard90° pulses are denoted using filled narrow rectangles, while open narrow rectangles (excluding the purge elements in the 13C sequence) denote hard pulses with flip angles φ. The flip angle φ of the hard pulses φ3 and φ4 is equal to arctan(ω1/Ω), where ω1 and Ω are the spin-locking amplitude and offset for 13C or 15N. The flip angle of the hard pulse on the proton channel in the 15N R sequence is equal to tan−11HH) where ω1H is the amplitude of the proton spin-locking field and ΩH is the frequency offset of the signal of interest from water. Wide open rectangles denote periods of continuous RF irradiation. Reprinted with permission from [9].(B) The different spins that can be targeted for R RD measurements in uniformly 13C/15N enriched nucleic acids using the pulse sequences in part (A) are highlighted by red circles. The 1H spins that can be targeted using the 1D R pulse sequence developed by Petzold et al.[222] are also shown using red circles. Spectral crowding in RNA between the C3′ and C2′ sugar carbons prevents measurement of R(C3′ and C2′) in RNA[166] unless one uses selectively labeled samples, while relaxation contributions from germinal protons complicates R(C5′) measurements in both DNA and RNA[166] and R(C2′) measurements in DNA unless selective deuteration is used[131].
Figure 29.
Figure 29.
Flowchart describing the various steps for measuring and analyzing R RD data using the pulse sequences shown in Fig. 28A.
Figure 30.
Figure 30.
Calibration of the spin-lock amplitude in R experiments. A) Nutation curve showing variation of signal intensity (black dots) as a function of time during an R calibration experiment. The red line is a fit of the intensity to the equation in the inset. B) Variation of the actual spin-lock frequency ω1,real, with the power P of the spin-lock field, obtained by fitting nutation curves in part (A) (black dots). The red line denotes a fit to the equation in the inset.
Figure 31.
Figure 31.
Asymmetries near 0 offset observed in off-resonance R RD profiles due to improper alignment of the initial magnetization under intermediate exchange conditions for two-state exchange, obtained using B-M simulations. A) Line shape (LS) simulation using the B-M equations in free precession conditions in the absence of a spin-locking field, for a system in intermediate exchange (pES = 10 %, kex = 3000 s−1, Δω¯(13C)=5 ppm, γ(1H)B0/2π = 700 MHz,R1,GS = R1,ES = 0 s−1, R2,GS = R2,ES = 16 s−1). B) Directions of the effective fields (ωeff,GS: blue, ωeff,ES: red, ωeff,AVG: green, ωeff,OBS: black dotted lines) and initial alignment of the bulk magnetization (GS: blue, ES: red arrows) at the start of the R experiment (ω1/2π = 100 Hz, Ω = −300 Hz) for the system in (A) where the magnetization is initially aligned along the effective field of the ground state (GS Align, left), population weighted average (AVG Align, middle) and the observed (OBS) resonance obtained from a lineshape simulation (LS Align, right) . (C) Offresonance R RD profiles for the system in (A) with R1,GS = R1,ES = 2.5 s−1, when the magnetization is initially aligned along ωeff,GS (GS Align, left), ωeff,AVG (AVG align, middle) and ωeff,OBS (LS Align, right). Note that in all cases, the magnetization at the end of the relaxation delay (0.05 s) is projected parallel to the initial alignment direction to calculate R. The different spin-lock amplitudes are color coded. Also shown in insets are representative decays of the normalized magnetization (black dots) along the initial alignment direction during the relaxation decay, along with exponential fits (red line).
Figure 32.
Figure 32.
Deducing the number of ESs sensed by R RD measurements. A plot of pES vs. kex as obtained from R measurements on individual spins in a given molecule displays clusters corresponding to kinetic and/or thermodynamically distinct ESs. Shown is a representative pES vs. kex plot obtained from 13C R RD (C6/C8/C4′/C1′ spins) measurements on HIV-1 TAR (secondary structure shown on the left) at pH 6.4, 25 °C[166], indicating the presence of two distinct ESs (ES1 and ES2). The zoomed in view of the ES2 region is provided in the inset. Errors were estimated using a Monte-Carlo approach while fitting the individual RD profiles, as explained in Section 6.3.
Figure 33.
Figure 33.
Thermodynamics and kinetics of GS-ES exchange characterized using temperature dependent R RD measurements. Free energy diagram (1 kcal/mol = 4.184 kJ/mol) for the Watson-Crick to Hoogsteen transition (κ = 1, left and κ = 3.3 * 10−6, right) for A16-T9 in A6-DNA at pH 5.4, 25 °C obtained using off-resonance R RD, as reported by Al-Hashimi et al.[17]. The secondary structure of A6-DNA is shown in inset.
Figure 34.
Figure 34.
Chemical shift/structure relationships in nucleic acids can aid structural elucidation of ESs. A) Scatter plot of 13C chemical shifts obtained from the BMRB for different secondary structure contexts in RNA (Watson-Crick BPs in A-form helices: black; nucleotides in bulges, internal or apical loops: gold; syn bases: blue). B) Distribution of 1H and 15N chemical shifts for U-N3 and G-N1 as a function of the BP type (G-C Watson-Crick BPs: red; U-A Watson-Crick BPs: blue; G-U wobbles: purple; U-G and U-U wobbles: green; sheared G-A mispairs: orange, with the base whose shifts are shown being colored), as obtained from the BMRB. C) Correlation between the C1′ and C4′ chemical shifts in RNA as obtained from a survey of the BMRB for nucleotides in different structural contexts (helical: blue; non-helical: orange; flanking,i.e., helical BP neighboring loops or bulges: green). Black lines correspond to the upper boundaries for C3′-endo sugar chemical shifts as obtained based on the average and standard deviation of the chemical shifts for helical nucleotides.(A) and (B) were reprinted with permission from [9] while (C) was reproduced with permission from [166].
Figure 35.
Figure 35.
Probing base pairing in nucleic acid ESs using mutations or chemical modifications designed to stabilize the ES relative to the GS. A) Secondary structure of HIV-1 TAR RNA with the Δω¯ values obtained from off-resonance R RD experiments[16, 166, 264], color-coded for ES1 and ES2. White circles correspond to sites where no RD was observed. B) Kinetic network of chemical exchange for HIV-1 TAR with ES1 and ES2[16, 264]. Regions undergoing structural changes when transforming into the ES are indicated in red. The exchange rates and populations shown were obtained using NMR RD measurements[16, 264]. Mutations used for stabilizing the ESs are indicated in green. C) Secondary structure of the G28U mutant of HIV-1 TAR in the GS and ES2 conformations. The mutation site is highlighted in red. D)Correlation between Δω¯mutant, the chemical shift difference between the indicated mutant and unmodified HIV-1 TAR and Δω¯RD, the change in chemical shift obtained using RD measurements on unmodified HIV-1 TAR, monitoring the GS to ES2 exchange[16, 264]. Vertical line of points at Δω¯RD=0 correspond to resonances where RD was flat and Δω¯RD was assumed to be equal to zero. E) m1A and m1G disrupt Watson-Crick base pairing and create an energetic bias towards the formation of Hoogsteen BPs in DNA. In panels (B) and (C) Watson-Crick BPs and G-U mismatches are indicated using thick lines while thin lines correspond to all other mismatches.
Figure 36.
Figure 36.
Probing the structure of nucleic acid ESs using mutations or chemical modifications designed to stabilize the GS relative to the ES. A) Replacement of the HIV-1 TAR apical loop with a UUCG tetraloop destabilizes ES2[264]. B) N6,6-dimethyl adenine (m6,6A) disrupts base pairing of adenine via the Watson-Crick face in RNA, thereby shifting the GS-ES1 equilibrium in HIV-1 TAR towards the GS[16], in which A35 is unpaired. C) N7-deaza guanine and adenine disrupt Hoogsteen hydrogen bonding and bias A-T and G-C BPs towards the native Watson-Crick conformation[112]. D) Inosine disrupts hydrogen bonding involving the Guanine amino group thereby destabilizing Watson-Crick-like mismatched BPs[165]. In all cases, modifications are highlighted in red. In panels (A) and (B) Watson-Crick BPs and G-U mismatches in the secondary structures are indicated using thick lines while thin lines correspond to all other mismatches.
Figure 37.
Figure 37.
High-resolution structural characterization of ES Hoogsteen BPs in B-DNA.A) Validation of the ES mutant (m1A) using an extensive set of chemical shifts. Shown is a representative example of A6-DNA (secondary structure on the left), with the site of m1A16 modification to trap Hoogsteen BPs indicated in red. Correlation between Δω¯m1AA (the chemical shift difference between the Hoogsteen-stabilizing A6-DNAm1A16 and unmodified A6-DNA duplex), and Δω¯RD values obtained from R RD measurements on unmodified A6-DNA, monitoring the Watson-Crick to Hoogsteen exchange at A16. B) Correlation between Δω¯Ens, the calculated chemical shift difference between the ensembles of the A6-DNAm1A16 and A6-DNA duplexes, and Δω¯RD (C) Dynamic ensembles for A6-DNA (green, left) and A6-DNAm1A16 (red, right) obtained as described by Al-Hashimi et al.[116]. The average inter-helical kink angle β, obtained from an Euler angle analysis[296, 297] is also indicated. In panels A and B, two RMSD and R values are shown. The first value is calculated with the inclusion of all the resonances for which RD was measured, while the second value is calculated excluding data with flat RD where Δω¯RD was assumed to be zero. Reprinted by permission from [117].
Figure 38.
Figure 38.
Watson-Crick-like G-T mismatches and their roles in generating spontaneous mutations during DNA replication. A) Kinetic topology for transforming between G-T/U wobble mismatches and their Watson-Crick-like counterparts formed via tautomerization or ionization. The exchange rates shown were obtained using NMR RD measurements[195, 197]. B) Minimal kinetic model for Watson-Crick BP incorporation by DNA polymerases. The incorporation of a G-T mismatch requires in addition, as shown in the lower pathway, a tautomerization or ionization step allowing for the formation of a Watson-Crick-like species.(Bottom left) Histograms showing Fpol, the fidelity of dTTP/5BrdUTP mis-incorporation errors catalyzed by Alfalfa Mosaic Virus Reverse Transcriptase (AMV RT) as computed using kinetic simulations allowing incorporation of tautomeric (blue, MES1), ionic (green, MES2) or both (orange, MES1 + MES2) Watson-Crick-like excited states, and experimentally measured values (gray).(Bottom right) Measured and simulated rates (kobs) of mis-incorporation for dTTP/5BrdUTP catalyzed by human DNA polymerase β. Reprinted by permission from [195].
Figure 39.
Figure 39.
RNA ESs feature localized changes in secondary structure. Shown are the secondary structures of ES determined for A) bacterial A-site, B) p5abc and C) HIV-SL1 using selective 1D R RD measurements. The part of the ES undergoing structural changes on transforming from the GS is indicated in red. Thick lines correspond to Watson-Crick BPs and G-U mismatches, whereas thin lines denote other non-canonical mispairing. The populations of the states and the rate constants for GS-ES exchange, as obtained using R RD measurements[9, 16] are also shown.

References

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