Normal-inverse Gaussian distribution¶
A four-parameter probability law formed by mixing a normal mean and variance with an inverse Gaussian variable.
Core Idea¶
A normal-inverse Gaussian (NIG) distribution is a probability law formed by mixing a conditional normal distribution with a positive inverse Gaussian variable. Given \(V\), the outcome \(X\) is normal with mean \(\mu+\beta V\) and variance \(V\); averaging over \(V\) gives the marginal law. The mathematical mixer is not automatically a measured physical cause.[1][2]
The four parameters describe tail shape \(\alpha\), asymmetry \(\beta\), scale \(\delta\) and location \(\mu\), with \(\alpha>|\beta|\) and \(\delta>0\) in the stated parameterization. Setting \(\beta=0\) gives a symmetric member.[3][2]
How would you explain it like I'm…
Blended Bell Curves
Normal Mixed by Inverse Gaussian
Structural Signature¶
- Outcome: a real-valued random variable with an NIG marginal law.
- Conditional kernel: a normal distribution conditional on a positive variable \(V\).
- Mixing law: \(V\) has an inverse Gaussian distribution.
- Coupling: \(V\) controls conditional variance and shifts the mean through \(\beta V\).
- Marginal: integrating over \(V\) yields a four-parameter law; a fitted parameter vector is one member of the family.[1][2][3]
What It Is Not¶
A generic heavy-tailed distribution or a normal mixture with another mixer is not automatically NIG. An inverse Gaussian variable alone is the mixer, not the resulting marginal. A time-indexed NIG process adds joint behavior; a fit to one marginal does not establish independent increments or a literal physical mixing mechanism.[1][4]
Scope of Application¶
The law can be specified mathematically without data, then fitted to real-valued observations. Its use in financial returns or solar-wind increments does not imply that either system contains an observed inverse Gaussian clock.[5][3]
Clarity¶
Distinguish the family, a member with fixed parameters, a fit to data and a process over time. A symmetric member remains NIG; skewness is possible, not mandatory.[2][3]
Examples¶
Symmetric member. Choose \(\beta=0\), \(\alpha>0\), \(\delta>0\) and any real \(\mu\). The conditional normal and inverse Gaussian mixture still define an NIG law, now symmetric about its location.[2][3]
Two fitted settings. One study compared NIG with other generalized-hyperbolic subclasses for high-frequency IBEX35 returns. Another fitted NIG densities to solar-wind Elsasser increments at multiple scales. These are case-specific marginal fits, not proof of a common physical mixer or a complete temporal model.[5][3]
Reasoning and Boundary¶
Check the admissible density or equivalent conditional-normal/inverse-Gaussian representation before calling a law NIG. Then distinguish an estimated marginal from a time-indexed process. A common family across scales does not require one fixed parameter vector.[2][3][4]
Neighborhood in Abstraction Space¶
Normal-inverse Gaussian distribution sits in a sparse region of the domain-specific corpus (94th percentile for distinctiveness): few abstractions share its structure, so a faithful description tends to retrieve it precisely.
Family — Unclustered & Miscellaneous (2835 abstractions)
Nearest neighbors
- Q-function — 0.80
- Gamma Distribution — 0.80
- Mixture Distribution — 0.78
- Tail dependence — 0.77
- Modified half-normal distribution — 0.77
Computed from structural-signature embeddings · 2026-10-31
References¶
[1] Ole E. Barndorff-Nielsen, “Normal Inverse Gaussian Distributions and Stochastic Volatility Modelling”, Scandinavian Journal of Statistics 24 (1997), 1–13. Publisher abstract and metadata inspected; the full original article was not available in this pass. The publisher lists a 2007 online date for the 1997 volume. registry ↩a ↩b ↩c
[2] SciPy, scipy.stats.norminvgauss documentation, v1.11.3, Notes. Official implementation documentation used as an independent check of the conditional representation and standardized/four-parameter conventions, not as the original discovery source. registry ↩a ↩b ↩c ↩d ↩e ↩f
[3] Juan C. Palacios, Jean C. Perez, and Sofiane Bourouaine, “Parametric description of intermittent probability distribution functions in solar wind and magnetohydrodynamic turbulence”, Monthly Notices of the Royal Astronomical Society 531 (2024), 24–34. Publisher full text §§3–5, especially §4.2 equations (26)–(29), inspected. The source uses Λ where this entry uses δ for scale. registry ↩a ↩b ↩c ↩d ↩e ↩f ↩g
[4] Ole E. Barndorff-Nielsen, “Processes of normal inverse Gaussian type”, Finance and Stochastics 2 (1997), 41–68. Publisher abstract and metadata inspected; it discusses multiple NIG-marginal process types with different dependence structures, not a particular empirical financial fit. registry ↩a ↩b
[5] Pablo Suárez-García and David Gómez-Ullate, “Scaling, stability and distribution of the high-frequency returns of the IBEX35 index”, author manuscript, published in Physica A 392 (2013), 1409–1417. Abstract, §2.2, and §3 inspected (one-based PDF pp. 1, 3–6); the comparative conclusion is limited to their data and tested families. registry ↩a ↩b