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Solar cells are engines converting energy supplied by the photon flux into work. All known types of macroscopic engines and turbines are also self-oscillating systems which yield a periodic motion at the expense of a usually non-periodic…

统计力学 · 物理学 2015-12-09 Robert Alicki , David Gelbwaser-Klimovsky , Krzysztof Szczygielski

Although 98% of the solar material consists of hydrogen and helium, the remaining chemical elements contribute in a discernible way to the thermodynamic quantities. The contribution of various heavy elements in a set of thermodynamic…

天体物理学 · 物理学 2009-11-07 Zhigang Gong , Werner Dappen , Alan Nayfonov

For most of their existence stars are fueled by the fusion of hydrogen into helium proceeding via two theoretically well understood processes, namely the $pp$ chain and the CNO cycle. Neutrinos emitted along such fusion processes in the…

Nearly all energy generated by fusion in the solar core is ultimately radiated away into space in the solar atmosphere, while the remaining energy is carried away in the form of neutrinos. The exchange of energy between the solar gas and…

太阳与恒星天体物理 · 物理学 2020-04-01 Jorrit Leenaarts

The Sun provides a standard reference against which we compare the chemical abundances found anywhere else in the Universe. Nevertheless, there is not a unique 'solar' composition, since the chemical abundances found in the solar interior,…

太阳与恒星天体物理 · 物理学 2021-06-22 Carlos Allende Prieto

Prompted by high resolution observations, I propose an explanation for the 40+ year old problem of structure and energy balance in the solar transition region. The ingredients are simply cross-field diffusion of neutral atoms from cool…

天体物理学 · 物理学 2009-11-13 Philip G. Judge

The solar atmosphere was traditionally represented with a simple one-dimensional model. Over the past few decades, this paradigm shifted for the chromosphere and corona that constitute the outer atmosphere, which is now considered a dynamic…

Only three processes, operant during the formation of the Solar System, are responsible for the diversity of matter in the Solar System and are directly responsible for planetary internal-structures, including planetocentric nuclear fission…

天体物理学 · 物理学 2007-05-23 J. Marvin Herndon

Cosmic rays reaching the atmosphere of an astrophysical object produce showers of secondary particles that may then escape into space. Here we obtain the flux of gamma rays and neutrinos of energy $E>10$ GeV emitted by the Sun, Jupiter and…

高能天体物理现象 · 物理学 2025-11-19 Pablo de la Torre , Miguel Gutiérrez , Manuel Masip , Alejandro Oliver

Stars of ~8-100 solar masses end their lives as core-collapse supernovae (SNe). In the process they emit a powerful burst of neutrinos, produce a variety of elements, and leave behind either a neutron star or a black hole. The wide mass…

高能天体物理现象 · 物理学 2018-01-30 Yong-Zhong Qian

The solar chemical composition is an important ingredient in our understanding of the formation, structure and evolution of both the Sun and our solar system. Furthermore, it is an essential reference standard against which the elemental…

太阳与恒星天体物理 · 物理学 2014-11-20 Martin Asplund , Nicolas Grevesse , A. Jacques Sauval , Pat Scott

High energy cosmic rays reach the surface of the Sun and start showers with thousands of secondary particles. Most of them will be absorbed by the Sun, but a fraction of the neutral ones will escape and reach the Earth. Here we incorporate…

高能物理 - 唯象学 · 物理学 2020-03-18 Miguel Gutiérrez , Manuel Masip

A quintessential source of heat, the Sun radiates toward the Earth a power ten thousand times greater than humanity's energy needs. Harnessing this energy bounty, however, requires capturing and converting sunlight. Today, this conversion…

科普物理 · 物理学 2026-02-04 Daniel Suchet , Nathan Roubinowitz , Jean-François Guillemoles

The magnetic field of the Sun is the underlying cause of the many diverse phenomena combined under the heading of solar activity. Here we describe the magnetic field as it threads its way from the bottom of the convection zone, where it is…

太阳与恒星天体物理 · 物理学 2010-08-05 Sami K. Solanki , Bernd Inhester , Manfred Schüssler

The Sun is a powerful neutrino source that can be used to study the physical properties of neutrinos and, at the same time, neutrinos are a unique tool to probe the interior of the Sun. For these reasons, solar neutrino physics is both…

太阳与恒星天体物理 · 物理学 2009-10-20 Marco Pallavicini

Efforts to understand unusual weather or abrupt changes in climate have been plagued by deficiencies of the standard solar model (SSM). While it assumes that our primary source of energy began as a homogeneous ball of hydrogen (H) with a…

天体物理学 · 物理学 2007-05-23 O. Manuel , B. W. Ninham , S. E. Friberg

An integrated Magneto-Fluid model, that accords full treatment to the Velocity fields associated with the directed plasma motion, is developed to investigate the dynamics of coronal structures. It is suggested that the interaction of the…

等离子体物理 · 物理学 2009-11-06 Swadesh M. Mahajan , Ryszard Miklaszewski , Kommunela I. Nikol'skaya , Nana L. Shatashvili

The connection between nuclear fusion in the Sun's core and solar irradiance is obscured among other things by uncertainty over the mechanism of coronal heating. Data for solar wind density and velocity, sunspot number, and EUV flux suggest…

太阳与恒星天体物理 · 物理学 2016-09-16 Claudio Vita-Finzi

Much of our understanding of the internal structure of the Sun derives from so-called standard theoretical solar models. Unfortunately, none of those models agrees completely with observation. The discrepancy is commonly associated with…

太阳与恒星天体物理 · 物理学 2019-04-10 Douglas Gough

The article describes new model of the Sun having a hollow core as introduced in [1]. The model helps to explain a number of experimental facts of kinetics, energetics, and Sun spectroscopy based on classic physics. The origin of the Sun's…

天体物理学 · 物理学 2007-05-23 Alexander M. Ilyanok