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相关论文: Solar activity around AD 775 from aurorae and radi…

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Only a few red dwarf flaring stars in the solar neighbourhood have undergone exceptional events called superflares. They have been detected with high-energy satellites (i.e. Swift) and have been proven to be powerful events (both in…

We report the latest statistical analyses of superflares on solar-type (G-type main-sequence; effective temperature is 5100 - 6000 K) stars using all of the $Kepler$ primary mission data, and $Gaia$-DR2 (Data Release 2) catalog. We updated…

太阳与恒星天体物理 · 物理学 2021-01-15 Soshi Okamoto , Yuta Notsu , Hiroyuki Maehara , Kosuke Namekata , Satoshi Honda , Kai Ikuta , Daisaku Nogami , Kazunari Shibata

We examine possible sources of a substantial increase in tree ring 14C measurements for the years AD 774-775. Contrary to claims regarding a coronal mass ejection (CME), the required CME energy is not several orders of magnitude greater…

太阳与恒星天体物理 · 物理学 2015-03-26 Brian C. Thomas , Adrian L. Melott , Keith R. Arkenberg , Brock R. Snyder

Using a summary curve of two eigen vectors of solar magnetic field oscillations derived with Principal Components Analysis (PCA) from synoptic maps for solar cycles 21-24 as a proxy of solar activity, we extrapolate this curve backwards…

太阳与恒星天体物理 · 物理学 2021-09-20 V. V. Zharkova , S. J. Shepherd , E. Popova , S. I Zharkov

Solar flares strongly affect the Sun's atmosphere as well as the Earth's environment. Quantifying the maximum possible energy of solar flares of the present-day Sun, if any, is thus a key question in heliophysics. The largest solar flares…

太阳与恒星天体物理 · 物理学 2015-06-12 G. Aulanier , P. Demoulin , C. J. Schrijver , M. Janvier , E. Pariat , B. Schmieder

Single-year spikes in radiocarbon production are caused by intense bursts of radiation from space. Supernovae emit both high-energy particle and electromagnetic radiation, but it is the latter that is most likely to strike the atmosphere…

太阳与恒星天体物理 · 物理学 2016-08-09 Michael Dee , Benjamin Pope , Daniel Miles , Sturt Manning , Fusa Miyake

Short duration flares are well known to occur on cool main-sequence stars as well as on many types of `exotic' stars. Ordinary main-sequence stars are usually pictured as being static on time scales of millions or billions of years. Our sun…

天体物理学 · 物理学 2009-10-31 Bradley E. Schaefer , Jeremy R. King , Constantine P. Deliyannis

Herein we show that the historical records of mid-latitude auroras from 1700 to 1966 present oscillations with periods of about 9, 10-11, 20-21, 30 and 60 years. The same frequencies are found in proxy and instrumental global surface…

地球与行星天体物理 · 物理学 2015-03-20 Nicola Scafetta

Near-Earth Asteroids (NEAs) with small perihelion distances reach sub-solar temperatures of > 1000 K. They are hypothesized to undergo "super-catastrophic" disruption, potentially caused by near-Sun processes such as thermal cracking,…

Excursions in the carbon-14 record measured in tree rings are attributed to various high energy but short-lived cosmic effects. So far, rapid changes at 774-775 CE, 993-994 CE and 660 BCE have been convincingly interpreted as due to rapid…

Context. Solar activity, dominated by the 11-year cyclic evolution, has been observed directly since 1610. Before that, indirect cosmogenic proxy data are used to reconstruct it over millennia. Recently, the precision of radiocarbon…

太阳与恒星天体物理 · 物理学 2026-04-22 Ilya Usoskin , Sami K. Solanki , Natalie A. Krivova , Theodosis Chatzistergos

The Schwabe (~11 yr) value for the annual sunspot number is sometimes uncritically applied to other measures of solar activity, direct and indirect, including the 10.7 cm radio flux, the inflow of galactic cosmic rays, solar flare…

太阳与恒星天体物理 · 物理学 2022-12-08 Claudio Vita-Finzi

In this last Paper III additional evidences that the solar high energetic particles radiation with energies higher as 100 MeV (the solar cosmic rays SCR) is an very important component for the "Sun- climate" relationship are given (see also…

地球与行星天体物理 · 物理学 2010-07-14 Boris Komitov

We present a study of multi-wavelength observations, of a C 2.3 solar flare in Active Region NOAA 12353, observed on 2015 May 23, which reveal new properties of acoustic waves in the flaring region. The space-, and ground-based data…

太阳与恒星天体物理 · 物理学 2022-03-07 A. Wisniewska , E. Chmielewska , K. Radziszewski , M. Roth , J. Staiger

Recent data on superflares on sun-like stars and radiocarbon data on solar activity in the past are both indicative of transient epochs of unusually high magnetic activity. We propose an explanation for the grand activity maxima in the…

太阳与恒星天体物理 · 物理学 2016-05-05 L. L. Kitchatinov , S. V. Olemskoy

Active regions (AR) appearing on the surface of the Sun are classified into $\alpha$, $\beta$, $\gamma$, and $\delta$ by the rules of the Mount Wilson Observatory, California on the basis of their topological complexity. Amongst these, the…

太阳与恒星天体物理 · 物理学 2016-03-09 Piyali Chatterjee , Viggo Hansteen , Mats Carlsson

Recent results of a mixed shell model heated asymmetrically by transient increases in nuclear burning indicate the transient generation of small hot spots inside the Sun somewhere between 0.1 and 0.2 solar radii. These hot bubbles are…

太阳与恒星天体物理 · 物理学 2015-05-18 Attila Grandpierre

The variable Sun is the most likely candidate for natural forcing of past climate change on time scales of 50 to 1000 years. Evidence for this understanding is that the terrestrial climate correlates positively with solar activity. During…

太阳与恒星天体物理 · 物理学 2015-05-27 A. I. Shapiro , W. Schmutz , E. Rozanov , M. Schoell , M. Haberreiter , A. V. Shapiro , S. Nyeki

Solar activity is studied using a cluster analysis of the time-fluctuations of the sunspot number. It is shown that in an Historic period the high activity components of the solar cycles exhibit strong clustering, whereas in a Modern period…

天体物理学 · 物理学 2010-11-02 A. Bershadskii