wave-theory-3-wave-statistics
Sub-skill of wave-theory: 3. Wave Statistics.
Best use case
wave-theory-3-wave-statistics is best used when you need a repeatable AI agent workflow instead of a one-off prompt.
Sub-skill of wave-theory: 3. Wave Statistics.
Teams using wave-theory-3-wave-statistics should expect a more consistent output, faster repeated execution, less prompt rewriting.
When to use this skill
- You want a reusable workflow that can be run more than once with consistent structure.
When not to use this skill
- You only need a quick one-off answer and do not need a reusable workflow.
- You cannot install or maintain the underlying files, dependencies, or repository context.
Installation
Claude Code / Cursor / Codex
Manual Installation
- Download SKILL.md from GitHub
- Place it in
.claude/skills/3-wave-statistics/SKILL.mdinside your project - Restart your AI agent — it will auto-discover the skill
How wave-theory-3-wave-statistics Compares
| Feature / Agent | wave-theory-3-wave-statistics | Standard Approach |
|---|---|---|
| Platform Support | Not specified | Limited / Varies |
| Context Awareness | High | Baseline |
| Installation Complexity | Unknown | N/A |
Frequently Asked Questions
What does this skill do?
Sub-skill of wave-theory: 3. Wave Statistics.
Where can I find the source code?
You can find the source code on GitHub using the link provided at the top of the page.
SKILL.md Source
# 3. Wave Statistics
## 3. Wave Statistics
**Spectral Parameters:**
```python
def calculate_spectral_parameters(
S: np.ndarray,
frequencies: np.ndarray
) -> dict:
"""
Calculate spectral wave parameters.
Args:
S: Wave spectrum (m²/Hz)
frequencies: Frequency array (Hz)
Returns:
Spectral parameters
"""
# Spectral moments
m0 = np.trapz(S, frequencies)
m1 = np.trapz(S * frequencies, frequencies)
m2 = np.trapz(S * frequencies**2, frequencies)
m4 = np.trapz(S * frequencies**4, frequencies)
# Significant wave height
Hs = 4 * np.sqrt(m0)
# Mean period
Tm01 = m0 / m1
# Zero-crossing period
Tz = np.sqrt(m0 / m2)
# Peak period (from spectrum maximum)
peak_idx = np.argmax(S)
Tp = 1 / frequencies[peak_idx]
# Spectral width
epsilon = np.sqrt(1 - m2**2 / (m0 * m4))
# Wave steepness
k_mean = 2 * np.pi / (9.81 * Tz**2 / (2*np.pi)) # Deep water approx
steepness = k_mean * Hs / 2
return {
'm0': m0,
'm1': m1,
'm2': m2,
'm4': m4,
'Hs': Hs,
'Tp': Tp,
'Tz': Tz,
'Tm01': Tm01,
'spectral_width': epsilon,
'steepness': steepness
}
# Example
params = calculate_spectral_parameters(S, freq)
print(f"Spectral Parameters:")
print(f" Hs: {params['Hs']:.2f} m")
print(f" Tp: {params['Tp']:.2f} s")
print(f" Tz: {params['Tz']:.2f} s")
print(f" Spectral width: {params['spectral_width']:.3f}")
```
**Wave Height Distribution:**
```python
def rayleigh_distribution(
H: np.ndarray,
Hs: float
) -> np.ndarray:
"""
Rayleigh distribution for wave heights in irregular seas.
P(H) = probability that wave height exceeds H
Args:
H: Wave height array (m)
Hs: Significant wave height (m)
Returns:
Exceedance probability
"""
# Rayleigh parameter
H_rms = Hs / np.sqrt(2)
# Exceedance probability
P = np.exp(-(H / H_rms)**2)
return P
def significant_wave_statistics(Hs: float) -> dict:
"""
Calculate wave statistics from Hs using Rayleigh distribution.
Args:
Hs: Significant wave height (m)
Returns:
Wave statistics
"""
H_rms = Hs / np.sqrt(2)
# Various statistical wave heights
H_mean = H_rms * np.sqrt(np.pi / 2)
H_1_10 = H_rms * np.sqrt(2 * np.log(10)) # Average of highest 1/10
H_1_100 = H_rms * np.sqrt(2 * np.log(100)) # Average of highest 1/100
H_max_1000 = H_rms * np.sqrt(2 * np.log(1000)) # Most probable max in 1000 waves
return {
'Hs': Hs,
'H_mean': H_mean,
'H_rms': H_rms,
'H_1_10': H_1_10,
'H_1_100': H_1_100,
'H_max_1000': H_max_1000
}
# Example
stats = significant_wave_statistics(Hs=8.5)
print(f"Wave Statistics (Hs = {stats['Hs']} m):")
print(f" Mean height: {stats['H_mean']:.2f} m")
print(f" H_1/10: {stats['H_1_10']:.2f} m")
print(f" H_1/100: {stats['H_1_100']:.2f} m")
print(f" H_max (in 1000 waves): {stats['H_max_1000']:.2f} m")
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