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fit-hidden-markov-model

pjt222
업데이트됨 2 days ago
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이 스킬은 시장 상황 구분이나 생물학적 서열 분석처럼 관찰할 수 없는 잠재 상태를 가진 시나리오에 대해, 바움-웰치 알고리즘을 사용하여 시계열 데이터에 은닉 마르코프 모델(HMM)을 적합시킵니다. 가장 가능성 높은 상태 경로를 위한 비터비 디코딩, 순방향-역방향 확률, 그리고 다양한 은닉 상태 수를 비교하기 위한 모델 선택 등 핵심 기능을 제공합니다. 관찰된 데이터로부터 잠재 구조를 추론하거나, 시퀀스 확률을 계산하거나, 은닉 상태 시퀀스를 디코딩해야 할 때 사용하세요.

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Claude Code

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기본
npx skills add pjt222/agent-almanac -a claude-code
플러그인 명령대체
/plugin add https://github.com/pjt222/agent-almanac
Git 클론대체
git clone https://github.com/pjt222/agent-almanac.git ~/.claude/skills/fit-hidden-markov-model

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문서

Fit Hidden Markov Model

Fit hidden Markov model (HMM) to sequential watch data using Baum-Welch expectation-maximization algorithm, decode most likely hidden state sequence via Viterbi, and pick right number of hidden states through info criteria.

When Use

  • You see sequence of emissions but the under generative states not directly visible
  • You suspect your data is made by system that switches between finite number of regimes
  • You need to slice time series into latent phases (e.g., market regimes, speech phonemes, biological sequence annotation)
  • You want to compute probability of observed sequence under generative model
  • You need most likely sequence of hidden states given observations (decoding)
  • You compare models with different counts of hidden states for best complex-fit trade-off

Inputs

Required

InputTypeDescription
observationssequence/matrixObserved data sequence (univariate or multivariate)
n_hidden_statesintegerNumber of hidden states to fit (or a range for model selection)
emission_typestringDistribution family for emissions: "gaussian", "discrete", "poisson", "multinomial"

Optional

InputTypeDefaultDescription
initial_paramsdictrandom/heuristicInitial transition matrix, emission parameters, and start probabilities
n_restartsinteger10Number of random restarts to mitigate local optima
max_iterationsinteger500Maximum EM iterations per restart
convergence_tolfloat1e-6Log-likelihood convergence threshold for EM
state_rangelist of ints[n_hidden_states]Range of state counts for model selection
covariance_typestring"full"For Gaussian emissions: "full", "diagonal", "spherical"
regularizationfloat1e-6Small constant added to diagonal of covariance matrices to prevent singularity

Steps

Step 1: Define Hidden States and Observation Model

1.1. Set count of hidden states K (or candidate range for model pick in Step 5).

1.2. Pick emission distribution family by data type:

  • Continuous data: Gaussian (univariate or multivariate)
  • Count data: Poisson or negative binomial
  • Categorical data: discrete/multinomial

1.3. Set model bits:

  • Transition matrix A of size K x K: A[i,j] = P(z_t = j | z_{t-1} = i)
  • Emission params theta_k for each state k: distribution-specific (e.g., mean and covariance for Gaussian)
  • Initial state distribution pi: pi[k] = P(z_1 = k)

1.4. Check watch data is formatted right: no missing values in sequence, consistent dim, and enough length vs count of params.

Got: Clearly set HMM shape with K states, picked emission family, and clean watch data of length T >> K^2.

If fail: Data has missing values? Fill in or remove affected segments. T too small vs K? Drop K or get more data.

Step 2: Initialize Parameters

2.1. Make initial params for each of n_restarts restarts:

  • Transition matrix: Random stochastic matrix (each row from Dirichlet distribution) or slightly perturbed uniform matrix.
  • Emission params: Use K-means clustering on observations to init means; compute cluster variances for Gaussian emissions.
  • Initial distribution: Uniform or proportional to cluster sizes from K-means.

2.2. For first restart, use K-means-informed init (usually strongest start). For later restarts, use random perturbations.

2.3. Check all initial params are valid:

  • Transition matrix rows sum to 1 with all entries positive.
  • Emission params in valid domain (e.g., covariance matrices are positive definite).
  • Initial distribution sums to 1.

Got: n_restarts sets of valid initial params, with at least one data-driven init.

If fail: K-means fails to converge? Use pure random init with more restarts. Covariance matrices singular? Add regularization constant to diagonal.

Step 3: Run Baum-Welch EM for Parameter Estimation

3.1. E-step (Forward-Backward algorithm):

  • Compute forward probs alpha[t,k] = P(o_1,...,o_t, z_t=k | model) using recursion:
    • alpha[1,k] = pi[k] * b_k(o_1)
    • alpha[t,k] = sum_j(alpha[t-1,j] * A[j,k]) * b_k(o_t)
  • Compute backward probs beta[t,k] = P(o_{t+1},...,o_T | z_t=k, model):
    • beta[T,k] = 1
    • beta[t,k] = sum_j(A[k,j] * b_j(o_{t+1}) * beta[t+1,j])
  • Compute state posterior gamma[t,k] = P(z_t=k | O, model):
    • gamma[t,k] = alpha[t,k] * beta[t,k] / P(O | model)
  • Compute transition posterior xi[t,i,j] = P(z_t=i, z_{t+1}=j | O, model).

3.2. M-step (Param re-estimation):

  • Update transition matrix: A[i,j] = sum_t(xi[t,i,j]) / sum_t(gamma[t,i])
  • Update emission params using weighted sufficient stats:
    • Gaussian mean: mu_k = sum_t(gamma[t,k] * o_t) / sum_t(gamma[t,k])
    • Gaussian covariance: weighted scatter matrix plus regularization
    • Discrete: b_k(v) = sum_t(gamma[t,k] * I(o_t=v)) / sum_t(gamma[t,k])
  • Update initial distribution: pi[k] = gamma[1,k]

3.3. Compute log-likelihood: log P(O | model) = log sum_k(alpha[T,k]). Use log-sum-exp trick to block underflow.

3.4. Scaling: Use scaled forward-backward vars to block numerical underflow for long sequences. Normalize alpha at each time step and accumulate log scaling factors.

3.5. Repeat E-step and M-step until log-likelihood change is below convergence_tol or max_iterations hit.

3.6. Across all restarts, keep param set with highest final log-likelihood.

Got: Monotonically non-decreasing log-likelihood across iterations, converging within max_iterations. Final params are valid (stochastic matrices, positive-definite covariances).

If fail: Log-likelihood drops? There is bug in E-step or M-step -- check formulas. Convergence very slow? Try better init or bump max_iterations. Covariance becomes singular? Increase regularization.

Step 4: Apply Viterbi Decoding for Most Likely State Sequence

4.1. Init Viterbi vars:

  • delta[1,k] = log(pi[k]) + log(b_k(o_1))
  • psi[1,k] = 0 (no predecessor)

4.2. Recurse forward for t = 2,...,T:

  • delta[t,k] = max_j(delta[t-1,j] + log(A[j,k])) + log(b_k(o_t))
  • psi[t,k] = argmax_j(delta[t-1,j] + log(A[j,k]))

4.3. End:

  • z*_T = argmax_k(delta[T,k])
  • Best path log-prob: max_k(delta[T,k])

4.4. Backtrace for t = T-1,...,1:

  • z*_t = psi[t+1, z*_{t+1}]

4.5. Output decoded state sequence z* = (z*_1, ..., z*_T) and its log-prob.

4.6. Compare Viterbi path prob to total sequence prob from forward algorithm to check how dominant the best path is.

Got: Single most-likely state sequence of length T with each entry in {1,...,K}. Viterbi log-prob should be less than or equal to total log-likelihood.

If fail: Viterbi path has log-prob of negative infinity? Some transition or emission prob is zero where it should not be. Add floor values to block log(0).

Step 5: Perform Model Selection (BIC/AIC Across Model Orders)

5.1. For each candidate count of hidden states K in state_range, fit full HMM (Steps 2-4).

5.2. Compute count of free params p:

  • Transition matrix: K * (K - 1) (each row is simplex)
  • Emission params: depends on family (e.g., Gaussian with full covariance in d dimensions: K * (d + d*(d+1)/2))
  • Initial distribution: K - 1

5.3. Compute info criteria:

  • BIC = -2 * log_likelihood + p * log(T)
  • AIC = -2 * log_likelihood + 2 * p
  • AICc = AIC + 2*p*(p+1) / (T - p - 1) (small-sample correction)

5.4. Pick model with lowest BIC (preferred for consistency) or AIC (preferred for prediction). Report both.

5.5. Tabulate results: for each K, show log-likelihood, count of params, BIC, AIC, convergence status.

5.6. If best K is at edge of state_range, extend range and re-fit.

Got: Clear min in BIC/AIC spotting best count of hidden states. Picked model should have converged and have interpretable state meanings.

If fail: No clear min exists (monotonically decreasing BIC)? Model may be misspec -- think different emission family. All models have poor log-likelihood? Data may not follow HMM structure.

Step 6: Validate with Held-Out Data and Posterior Decoding

6.1. Split data into training and check sets (e.g., 80/20 or use many sequences if open).

6.2. Fit model on training data. Compute log-likelihood on held-out data using forward algorithm (do not re-fit params).

6.3. Posterior decoding (swap for Viterbi):

  • For each time step, give state with highest posterior prob: z^_t = argmax_k(gamma[t,k])
  • This maxes expected count of rightly decoded states (vs Viterbi which maxes joint path prob).

6.4. Compare Viterbi and posterior decoding:

  • Compute agree rate between the two decoded sequences.
  • Regions of disagreement show ambiguous state assignments.

6.5. Check state interpretability:

  • Check emission params for each state (means, variances, discrete distributions).
  • Confirm states match meaningful regimes in domain context.
  • Check state dwell times (implied by diagonal of A) are reasonable.

6.6. Compute held-out log-likelihood per observation and compare across model orders to confirm training-set model pick.

Got: Held-out log-likelihood is reasonably close to training log-likelihood (no big overfit). Viterbi and posterior decoding agree on 90%+ of time steps. States have distinct, interpretable emission distributions.

If fail: Held-out likelihood much worse than training? Model is overfit -- drop K or bump regularization. States not interpretable? Try different inits or different emission family.

Validation

  • Log-likelihood is monotonically non-decreasing across Baum-Welch iterations for each restart
  • Transition matrix is row-stochastic (rows sum to 1, all entries non-negative)
  • Emission params in valid domain (positive-definite covariances, valid probability distributions)
  • Viterbi path log-prob does not exceed total sequence log-prob
  • BIC/AIC curves show clear min at picked model order
  • Held-out log-likelihood confirms model works beyond training set
  • Forward and backward prob computations agree: P(O) = sum_k(alpha[T,k]) = sum_k(pi[k] * b_k(o_1) * beta[1,k])

Pitfalls

  • Local optima in EM: Baum-Welch algorithm converges to local max, not always global. Always use many random restarts and pick best.
  • Numerical underflow: Forward-backward probs shrink exponentially with sequence length. Use log-space compute or scaled vars to block underflow to zero.
  • Overfit with too many states: Each extra hidden state adds O(K + d^2) params. Use BIC (not just likelihood) for model pick and check on held-out data.
  • Label switching: Hidden states identifiable only up to swap. When compare models across restarts, match states by emission params, not by index.
  • Degenerate states: State may collapse to explain single observation (Gaussian with near-zero variance). Regularization on covariance matrices blocks this.
  • Mix Viterbi and posterior decoding: Viterbi gives single best joint path; posterior decoding gives best marginal state at each time step. They answer different questions and can clash big.
  • Ignore state dwell times: Geometric dwell-time distribution built into standard HMMs may be poor fit for data with long regime durations. Think hidden semi-Markov models if dwell times are non-geometric.

See Also

  • Model Markov Chain -- pre-req for grasping transition structure that under hidden layer
  • Simulate Stochastic Process -- can be used to make synthetic HMM data for testing and to simulate from fitted model for posterior predictive checks

GitHub 저장소

pjt222/agent-almanac
경로: i18n/caveman/skills/fit-hidden-markov-model
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agentsagentskillsai-assisted-developmentclaude-codeskillsteams

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