Features of the Gnevyshev-Waldmeier Rule for Various Lifetimes and Areas of Sunspot Groups


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

Based on a sample of 7696 nonrecurrent and 566 recurrent sunspot groups, we have investigated the Gnevyshev–Waldmeier rule using the Catalogue of Solar Activity by R.S. Gnevysheva (1954–1978). The maximum recorded sunspot group lifetime is 160 days. The general Gnevyshev–Waldmeier rule for all lifetimes is Amax = (12.1 ± 0.70)LT (Amax is the maximum sunspot group area during the lifetime and LT is the sunspot group lifetime). However, the general rule has turned out to deviate from the derived linear form for the population of small short-living sunspot groups (SSG): it has a significant nonlinear scaling form Amax = (8.02 ± 0.41)LT(1.105±0.022). For the population of large long-living sunspot groups (LLG) there is a linear form Amax = (12.9 ± 1.1)LT. Allowance only for recurrent sunspot groups with lifetimes more than 40 days gives Amax = (13.93 ± 0.41)LT.

作者简介

Yu. Nagovitsyn

Pulkovo Astronomical Observatory; St. Petersburg State University of Aerospace Instrumentation

编辑信件的主要联系方式.
Email: nag-yury@yandex.ru
俄罗斯联邦, Pulkovskoe sh. 65, St. Petersburg, 196140; Bol’shaya Morskaya ul. 67, St. Petersburg, 190000

V. Ivanov

Pulkovo Astronomical Observatory

Email: nag-yury@yandex.ru
俄罗斯联邦, Pulkovskoe sh. 65, St. Petersburg, 196140

A. Osipova

Pulkovo Astronomical Observatory

Email: nag-yury@yandex.ru
俄罗斯联邦, Pulkovskoe sh. 65, St. Petersburg, 196140

补充文件

附件文件
动作
1. JATS XML

版权所有 © Pleiades Publishing, Inc., 2019