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Hace 7 horas · A specific set of spherical harmonics, denoted (,) or (), are known as Laplace's spherical harmonics, as they were first introduced by Pierre Simon de Laplace in 1782. These functions form an orthogonal system, and are thus basic to the expansion of a general function on the sphere as alluded to above.
Hace 1 día · Bayesian decision theory is a mathematical model of reasoning and decision-making under uncertain conditions. Proponents of Bayesian decision theory are usually called Bayesians. Their viewpoint is usually called Bayesianism. The Bayesian framework hinges upon two core concepts: subjective probability (a numerical measure of the degree to which ...
Hace 3 días · 1 Laboratoire de Météorologie Dynamique/Institut Pierre-Simon Laplace (LMD/IPSL), Sorbonne Université, Centre National de la Recherche Scientifique (CNRS), École Polytechnique, École Normale Supérieure (ENS), Paris, France 2 Institut Universitaire de France (IUF Paris, France), Paris, France
Hace 1 día · Pierre-Simon Laplace was a French mathematician and astronomer who made significant contributions to the fields of statistics, mathematical physics, and celestial mechanics. He is best known for his work on the Laplace transform, as well as the development of the Laplace equation and the theory of probability.
Hace 3 días · Laplace's equation is a second-order partial differential equation named after Pierre-Simon Laplace who, beginning in 1782, studied its properties while investigating the gravitational attraction of arbitrary bodies in space.
Hace 2 días · The Southern Ocean (south of 35°S) is a primary region for anthropogenic carbon dioxide (CO 2) uptake, accounting for ~40% of the total ocean CO 2 sink ( 1, 2 ). Yet, it remains the most uncertain region with regard to CO 2 flux estimates ( 3 – 5 ). This is essentially due to the sparsity of shipboard surface ocean CO 2 fugacity ( f CO 2w ...
Hace 4 días · Sus orígenes se remontan a los esfuerzos de matemáticos del siglo XVIII, como Pierre-Simon Laplace, por identificar los errores de observación en la astronomía. En cualquier conjunto de datos científicos, lo más probable es que los errores sean muy pequeños, y solo es probable que unos pocos sean grandes.
