Total water level (relative to MSL) is the superposition of offshore ocean water level and the wave effects,
$$ {\rm TWL} = \eta_{A} + \eta_{\rm NTR} + R_{2} , $$
(1)
where \(\eta_{A}\) is the astronomical tide, \(\eta_{\rm NTR}\) is the non-tidal residual (associated primarily with atmospheric forcing), and \(R_{2}\) is the 2% exceedance vertical level of wave runup. The ocean water level, the sum of \(\eta_{A}\) and \(\eta_{\rm NTR}\), is the TWL component unrelated to nearshore waves.
Ocean water level
Water levels measured with the IB pier radar and the La Jolla tide gauge are very similar (correlation = 0.998, root mean square error (RMSE) = 0.03 m) with no discernible time difference. Although the San Diego Bay tide gauge is closer to IB than to La Jolla, tides measured in San Diego Bay differ noticeably in amplitude and phase from the open coast IB and La Jolla.
The NOAA tidal prediction at La Jolla is \(\eta_{A}\) and \(\eta_{\rm NTR}\) is the difference between measured hourly-averaged water level at La Jolla (referenced to MSL) and \(\eta_{A}\). The tide dominates ocean water level fluctuations at IB, with the standard deviations of \(\eta_{A}\) and \(\eta_{\rm NTR}\) from the pier radar equal to 0.49 m and 0.03 m, respectively. The \(\eta_{\rm NTR} \) at the time of the forecast is assumed to persist for the full 6-day forecast period. The RMSE of ocean water level predicted at IB using the La Jolla tide gauge introduces normally distributed errors ranging from 0.03 m for nowcasts to 0.08 m at 6-days lead time (Fig. 5).
Runup model
The wave runup contribution to TWL, \(R_{2}\), is defined as the elevation exceeded by 2% of uprushing waves. Assuming Gaussian runup statistics, the 2% exceedance level is given by
$$ R_{2} = \overline{\eta } + \frac{S}{2}\,\,{\rm where}\,\,S = \left( {S_{SS}^{2} + S_{IG}^{2} } \right)^{\frac{1}{2}} $$
(2)
where \(\overline{\eta }\) is the super-elevation of water level due to wave breaking (wave setup), and \({S_{ss}} \) and \(S_{IG}\) are significant sea-swell (4–20 s) and infragravity band (20–250 s) swash heights. Many empirical runup parameterizations have been developed to estimate \(R_{2}\) (see review by Gomes da Silva et al. 2020). The most widely applied is Stockdon et al. (2006), where empirical fits define setup and runup components in terms of the incident wave height (\(H_{o} ), \) the deep-water wavelength (\(L_{o} )\), and the foreshore beach slope (\(\beta_{f} )\)
$$ R_{2} = 1.1\left( {0.35\beta_{f} \left( {H_{o} L_{o} } \right)^{\frac{1}{2}} + \frac{{\left[ {H_{o} L_{o} \left( {0.563\beta_{f}^{2} + 0.004} \right)} \right]^{\frac{1}{2}} }}{2}} \right). $$
(3)
The \(H_{0} L_{0}\) parameterizations follow from Hunt (1959), who proposed that the ratio of sea-swell runup to incident wave height scales with the Iribarren number (Battjes 1974), a dimensionless measure of dynamic beach steepness. Values of free parameters in (3) were fit to measurements from six beaches with varying morphology under a range of wave conditions. Other studies have used surfzone parameters to define runup (e.g. Stockdon et al 2006; Cohn and Ruggiero 2016), and the average period or frequency, rather than the peak (Atkinson et al. 2017, O’Grady et al. 2019; Dodet et al. 2019; Gomes da Silva et al. 2020, and references therein). These formulae usually approximate the beach profile with \(\beta_{f}\) and characterize the incident wave spectrum with \(H_{o}\) and \(L_{o}\).
With shoreward propagating waves specified at an offshore boundary, and with a fixed depth profile, runup in narrow laboratory wave channels can be accurately simulated with numerical models based on the Navier–Stokes equations (Lara et al. 2011; Torres-Freyermouth et al. 2019). However, the computation times are long and may be needlessly complex. Phase-resolving Boussinesq (Lynett et al. 2002) and non-hydrostatic models (Zijlema et al. 2011; Tonelli and Petti 2012; Tissier et al. 2012; Roeber and Cheung 2012; Smit et al. 2014) are a viable compromise between computational effort and accuracy. Bouss1D, BOSZ, and COULWAVE are nonlinear Boussinesq-type models that have been used to investigate wave and runup processes on beaches and coral reefs (Lynett et al. 2002; Yao et al. 2020; Roeber et al. 2010, 2012; Pinault et al. 2020 and many others). The SWASH (Simulating WAves till SHore, Zijlema et al. 2011) model has accurately simulated nonlinear surfzone wave evolution (Smit et al. 2014, Rijnsdorp et al. 2015), wave runup (Ruju et al. 2019) and wave overtopping (Suzuki et al. 2017) in the laboratory. Verification with field observations of runup for this class of models is more limited, but promising. Given the depth profile and in situ observations of shoreward propagating waves at the offshore boundary, the surfzone wave transformation and the resulting runup are well simulated by the 1D SWASH model (Fiedler et al. 2018).
Fiedler et al. (2020) (hereafter F20) showed the utility of runup formulae optimized for a given location based on SWASH runup simulations using typical storm waves and beach bathymetry with variable foreshore slopes. Simulations are used to calibrate a relatively simple, empirical parameterization. A notable difference from the \(H_{o} L_{o}\) dependence of S06 is the use of frequency-weighted integrals of sea-swell wave frequency spectra, \(E\left( f \right),\) which accounts for broad-banded and multi-peaked wave fields. The F20 approach, called the IPA (Integrated Power law Approximation), uses SWASH to simulate extreme storm wave events on a representative eroded beach profile determined from historical surveys. SWASH simulations are computed for many storm wave conditions identified in the regional Monitoring and Prediction (MOP) system (O’Reilly et al. 2016) wave hindcasts (Sect. 3.3). A general empirical power law form for the energy of the wave-driven components of TWL at the shoreline is
$$ \left[ {E_{IG,SS,\eta } } \right]_{\rm shoreline} = \left[ {\alpha \beta_{f}^{l} \mathop \int \limits_{SS}^{{}} E\left( f \right)^{m} f^{n} {\rm d}f} \right]_{\rm deep} $$
(4)
where \(\alpha\) is dimensional, \(E\left( f \right)\) is the incident wave spectrum at frequency \(f\), and (l,m,n) are powers determined for each wave-driven component. F20 used the MOP \(E\left( f \right)\) and SWASH runup to parameterize the components of \(R_{2}\), and found IB conditions at Cortez Ave, yield best-fits of
$$ \overline{\eta } = 0.21\mathop \int \limits_{SS}^{{}} E\left( f \right)^{0.45} f^{ - 1} {\rm d}f $$
(5)
$$ S_{ss}^{2} = 16*0.99\beta_{f}^{2} \mathop \int \limits_{SS}^{{}} E\left( f \right)^{0.45} f^{ - 1.85} {\rm d}f $$
(6)
$$ S_{IG}^{2} = 16*0.15\mathop \int \limits_{SS}^{{}} E\left( f \right)^{0.9} f^{ - 0.65} {\rm d}f $$
(7)
where integrals are evaluated over the incident sea-swell frequency band. Equations 5–7 are a model of the SWASH model on a typical winter profile with variable foreshore slopes. The left-hand side units are \(m^{2}\) in Eq. 5 and 6, and \(m\) in Eq. 4. The units are the same for the right-hand side, where f is in Hz and \(E\left( f \right)\) is \(m^{2} Hz^{ - 1}\). S06 include a \(\beta_{f}\) dependence for \(\overline{\eta }\) as well as \(S_{SS}\), whereas for the IB conditions, only the IPA \(S_{SS}\) depends on beach slope. The classic Hunt (1959) parametrization uses \(H_{o} L_{o}\), which scales as \(E^{1/2} f^{ - 2}\), most similar to \(S_{SS}\) (Eq. 5). The scaling consistency of IPA with Hunt (1959) is affirming, as Hunt (1959) examined runup on steep slopes where sea-swell may have dominated runup. The negative frequency exponents in \(\overline{\eta }\) and \(S_{IG}\) are smaller than the − 1.85 of \(S_{SS}\), indicating a weaker inverse dependence on wave frequency. (When the exponent is 0, there is no frequency dependence.)
Using SWASH model simulations on historical beach profiles, F20 show that IPA yields a more accurate runup hindcast than S06, even if S06 is tuned to the SWASH database. Note that IPA Eq. 6 is derived with a known foreshore \(\beta_{f}\). Scatter between SWASH and IPA arises from uncertainty in (submerged and subaerial) \(h\left( x \right)\), and in the offshore IG boundary condition for a given sea-swell spectrum. For later uncertainty assessments, note that the IPA-SWASH \(R_{2} \) emulation of F20 for a known beach slope has RMSD scatter ~ 9% of \(R_{2}\). We have increased this to 20% to account for h(x) uncertainty accompanying a larger training dataset (Fig. 6), as errors would be larger if the beach bathymetry were much different than observed in the F20 historical profiles.
Incident waves
The CDIP MOP system provides the incident wave spectrum \(E\left( f \right) \) in 10-m depth at locations spaced 100-m longshore. MOP hindcasts of \(E\left( f \right)\) are based on observations from a network of wave buoys. MOP forecasts up to 6 days in advance are specified using the NOAA WaveWatch III model forecasts at the buoy locations (O’Reilly et al. (2016)). The relatively strong dependence on wave frequency in \(\overline{\eta }\) and \(S_{IG}\) (Eqs. 5, 7) increases the importance of swell to \(R_{2}\) relative to high frequency seas. The warning system benefits from the relative predictability (a few days in advance) of the swell that drives extreme wave runup. Errors for individual wave events can be substantial. Overall, the buoy-driven MOP model hindcasts have relatively low bias and therefore are better suited for quantifying mean (e.g., monthly or annual) nearshore wave climate conditions rather than extreme or individual wave events. Nevertheless, despite these limitations, the MOP model proved useful for flood warnings at IB.
Errors in runup components caused by errors in MOP incident wave spectrum are evaluated as the difference in \(\overline{\eta },\) \(S_{SS}\), and \(S_{IG}\) (Eqs. 4–6) estimated using the observed buoy and MOP \(E\left( f \right)\). Typical time series of each are depicted (Fig. 7, a–c). Errors are approximated as normal and increase with amplitude (Fig. 7d–f), with normalized RSMEs of 0.16, 0.12, and 0.17, for \(\overline{\eta },\) \(S_{SS}\), and \(S_{IG} ,\) respectively.
Foreshore beach slope
IPA sea-swell swash energy depends on foreshore beach slope (Eq. 5). Beach slope variability is examined using Cortez Ave elevation profiles above MLLW during Dec-Mar of 2018/19 and 2019/20, when nourishment influences were reduced (Fig. 4c, d). The foreshore profile varies considerably, as expected for an equilibrium-like beach response to energetic winter swell (Yates et al. 2009; Ludka et al. 2015). The time-averaged subaerial beach slope (\(\beta ) \) over these 14 winter surveys increases approximately linearly with elevation z above MSL
$$ \beta \left( z \right) = 0.029z + 0.042 $$
(8)
with RMS slope difference of the 14 profiles compared to the mean profile = 0.03 (Fig. 8). For IPA estimates (Eq. 6), we compute the spatially-averaged foreshore beach slope \(\beta_{f}\) following S06 using Eq. 8, and assume the RMSE for \( \beta_{f} = 0.03\). The increase in slope with elevation (i.e., concave foreshore beach) causes \(\beta_{f}\), and hence \(S_{SS}\), to increase with tidal height for approximately steady wave conditions. The effect of the 0.03 RMSE \( \beta_{f} \) uncertainty on \(S_{ss}^{2}\) (Eq. 5) is substantial, but \(S_{IG}^{2}\) and \(\overline{\eta }\) are unaffected. Extension of IPA to other seasons would require an evaluation of the IPA parameters (Eqs. 5–7) for non-winter wave and beach conditions, and specification of seasonal changes to \( \beta_{f}\).