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This review provides an introduction to the generation and evolution of the Sun's magnetic field, summarising both observational evidence and theoretical models. The eleven year solar cycle, which is well known from a variety of observed…

Solar and Stellar Astrophysics · Physics 2011-10-17 Alan W. Hood , David W. Hughes

Beautiful dune patterns can be found in deserts and along coasts due to the instability of a plain sheet of sand under the action of the wind. Barchan dunes are highly mobile aeolian dunes found in areas of low sand availability and…

Other Condensed Matter · Physics 2009-11-10 O. Duran , V. Schwaemmle , H. Herrmann

There are at least four unexplained anomalies connected with astrometric data. Perhaps the most disturbing is the fact that when a spacecraft on a flyby trajectory approaches the Earth within 2000 km or less, it often experiences a change…

General Relativity and Quantum Cosmology · Physics 2009-08-07 John D. Anderson , Michael Martin Nieto

Clouds seem like an every-day experience. But -- do we know how clouds form on brown dwarfs and extra-solar planets? How do they look like? Can we see them? What are they composed of? Cloud formation is an old-fashioned but still…

Astrophysics · Physics 2014-11-17 Christiane Helling

Popular scientific summary -- The atmosphere of the Sun is envisioned as composed of inherently complex, non-homogeneous, and dynamic layers. A detailed understanding of the physical processes involved in these layers is still lacking. For…

Solar and Stellar Astrophysics · Physics 2021-10-22 Souvik Bose

A theory is described based on resonant thermal diffusion waves in the sun that appears to explain many details of the paleotemperature record for the last 5.3 million years. These include the observed periodicities, the relative strengths…

Astrophysics · Physics 2010-05-19 Robert Ehrlich

Arcades of flare loops form as a consequence of magnetic reconnection powering solar flares and eruptions. We analyse the morphology and evolution of flare arcades that formed during five well-known eruptive flares. We show that the arcades…

Solar and Stellar Astrophysics · Physics 2021-03-24 Juraj Lörinčík , Jaroslav Dudík , Guillaume Aulanier

Optical activity is ubiquitous across natural and artificial media and is conventionally understood in terms of scattering from electric and magnetic moments. Here we demonstrate experimentally and confirm numerically a type of optical…

The Sun likely formed as part of a group of stars. A close stellar flyby by one of the solar siblings is probably responsible for the sharp outer edge in the solar system`s mass distribution. The frequency of such close flybys can be used…

Earth and Planetary Astrophysics · Physics 2020-07-15 Susanne Pfalzner , Kirsten Vincke

Based on the spatial distribution of objects in the solar neighbourhood with a radius of 20 parsecs, and after correcting for the incompleteness of observational data, an expression was obtained for estimating the probability of finding an…

Solar and Stellar Astrophysics · Physics 2026-01-01 Diana Bakirova , Oleg Malkov

We have made high resolution observations of the Sun in which we identify individual sunquakes and see power from these seismic events being pumped into the resonant modes of vibration of the Sun. A typical event lasts about five minutes.…

Astrophysics · Physics 2009-10-30 P. L. Goode , L. H. Strous , T. R. Rimmele , R. T. Stebbins

Evidence for fine-tuning of physical parameters suitable for life can perhaps be explained by almost any combination of providence, coincidence or multiverse. A multiverse usually includes parts unobservable to us, but if the theory for it…

High Energy Physics - Theory · Physics 2007-05-23 Don N. Page

Catalogues and other records of aurora-borealis events were used to study the long-term spatial and temporal variation of these phenomena in the period from 1700 to 1905 in the Northern Hemisphere. For this purpose, geographic and…

Solar and Stellar Astrophysics · Physics 2015-06-17 M. Vázquez , J. M. Vaquero , M. C. Gallego

The annual temperature cycle of the earth closely follows the annual cycle of solar flux. At temperate latitudes, both driving and response cycles are well described by a strong annual sinusoidal component and a non-vanishing semiannual…

Atmospheric and Oceanic Physics · Physics 2020-11-13 Yunxiang Song , Kyle B. Lawlor , Thomas A. Witten

The improvements of the observations of the solar system allowed by the use of probes and big instruments let appear several problems: The frequencies of the radio signals received from the probes sent over 5 UA from the Sun are too high;…

General Physics · Physics 2007-05-23 Jacques Moret-Bailly

We analyze complex zebra patterns and fiber bursts during type-IV solar radio bursts on August 1, 2010. It was shown that all of the main details of sporadic zebra patterns can be explained within the model of zebra patterns and fiber…

Solar and Stellar Astrophysics · Physics 2018-12-12 G. P. Chernov , V. V. Fomichev , R. A. Sych

The importance of the investigation of magnetic superstorms is not limited to academic interest, because these superstorms can cause catastrophic impact on the modern civilisation due to our increasing dependency on technological…

Solar and Stellar Astrophysics · Physics 2020-09-01 Hisashi Hayakawa , José R. Ribeiro , Yusuke Ebihara , Ana P. Correia , Mitsuru Sôma

It has been argued that the solar magnetic cycle consists of two main periodic components: a low-frequency component (Hale's 22-year cycle) and a high-frequency component (quasi-biennial cycle). The existence of the double magnetic cycle on…

Astrophysics · Physics 2009-10-31 E. E. Benevolenskaya

The transition between the L dwarf and T dwarf spectral classes is one of the most remarkable along the stellar/brown dwarf Main Sequence, separating sources with photospheres containing mineral condensate clouds from those containing…

Solar and Stellar Astrophysics · Physics 2015-06-12 Adam J. Burgasser

In the Sun, the two forbidden [OI] lines at 630 and 636 nm were previously found to provide discrepant oxygen abundances. aims: We investigate whether this discrepancy is peculiar to the Sun or whether it is also observed in other stars.…

Solar and Stellar Astrophysics · Physics 2015-06-15 Elisabetta Caffau , Hans-G. Ludwig , Jean-M. Malherbe , Piercarlo Bonifacio , Matthias Steffen , Lorenzo Monaco
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