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一种基于调幅的粉红噪声简单模型。

A simple model for pink noise from amplitude modulations.

机构信息

Department of Physics, Ochanomizu University, 2-1-1, Otsuka, Bunkyo, Tokyo, 112-8610, Japan.

General Education, Kyoto-Sangyo University, Motoyama Kamigamo, Kita-ku, Kyoto, 603-8555, Japan.

出版信息

Sci Rep. 2023 May 24;13(1):8364. doi: 10.1038/s41598-023-34816-2.

Abstract

We propose a simple model for the origin of pink noise (or 1/f fluctuation) based on the waves with accumulating frequencies. These waves arise spontaneously in a system with synchronization, resonance, and infrared divergence. Many waves with accumulating frequencies can produce signals of arbitrary small frequencies from a system of small size. This beat mechanism can be understood as amplitude modulation. The pink noise can appear after the demodulation process, which produces a variety of pink noise in many fields. The pink noise thus formed from the beat has nothing to do with dissipation or long-time memory. We also suggest new ways of looking at pink noise in earthquakes, solar flares, and stellar activities.

摘要

我们提出了一个简单的模型,用于解释粉红噪声(或 1/f 波动)的起源,该模型基于累积频率的波动。这些波在具有同步、共振和红外发散的系统中自发产生。许多具有累积频率的波可以从小尺寸系统中产生任意小频率的信号。这种拍频机制可以理解为幅度调制。在解调过程之后,可能会出现粉红噪声,从而在许多领域中产生各种粉红噪声。由此产生的拍频粉红噪声与耗散或长时间记忆无关。我们还建议从新的角度看待地震、太阳耀斑和恒星活动中的粉红噪声。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/81c9/10209100/b7103a53576d/41598_2023_34816_Fig1_HTML.jpg

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