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The Sun Recorded Through History

ISBN-13: 9781441928290 / Angielski / Miękka / 2010 / 382 str.

J. M. Vaquero; M. Vazquez
The Sun Recorded Through History J. M. Vaquero M. Vazquez 9781441928290 Springer - książkaWidoczna okładka, to zdjęcie poglądowe, a rzeczywista szata graficzna może różnić się od prezentowanej.

The Sun Recorded Through History

ISBN-13: 9781441928290 / Angielski / Miękka / 2010 / 382 str.

J. M. Vaquero; M. Vazquez
cena 603,81
(netto: 575,06 VAT:  5%)

Najniższa cena z 30 dni: 578,30
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The Sun is nowadays observed using di?erent techniques that provide an almost instantaneous 3-D map of its structure. Of particular interest is the studyofthevariabilityinthesolaroutputproducedbythedissipationofm- netic energy on di?erent spatial and temporal scales the so-called magnetic activity. The 11-year cycle is the main feature describing this phenomenon. Apart from its intrinsic scienti?c interest, this topic is worth studying because of the interaction of such processes with the terrestrial environment. A ?eet of space and ground-based observatories are currently monitoring the behaviour of our star on a daily basis. However, solar activity varies not only on this decadal time-scale, as has been attested mainly through two methods: (a) records of the number of sunspots observed on the solar surface from 1610, and (b) the records of 14 10 cosmogenic isotopes, such as Cand Be, measured in tree-rings and i- cores, respectively. The study of the long-term behaviour of solar activity may be comp- mented by the study of historical accounts describing phenomena directly or indirectly related to solar activity. Numerous scienti?c and non-scienti?c d- uments have reported these events and we can make use of them as a proxy of solar activity in past times."

Kategorie:
Nauka, Fizyka
Kategorie BISAC:
Science > Astrofizyka
Science > Earth Sciences - Meteorology & Climatology
Science > Astronomia, przestrzeń i czas
Wydawca:
Springer
Język:
Angielski
ISBN-13:
9781441928290
Rok wydania:
2010
Numer serii:
000036061
Ilość stron:
382
Waga:
0.55 kg
Wymiary:
15.6 x 23.39 x 2.08
Oprawa:
Miękka
Wolumenów:
01

From the reviews: "Packed with many hundreds of references to both past and contemporary astronomical and historical literature, the book is a must for historians of science and professional astronomers and solar physicists interested in the historical reconstructions of solar activity. ... interested readers should find their money's worth. ... In The Sun Recorded Through History, long-gone solar astronomers tell us what they saw." (Paul Charbonneau, Physics Today, December, 2009) "This monograph is primarily a historical survey of solar activity from the dawn of historic observations ... to the invention of photography in 1840. ... highlight is a detailed discussion of observed sunspot minima and maxima over the past 2,000 years, and the possible contributing role of sociological factors in these observations. The illustrations are well chosen and often fascinating ... . The work will be of interest primarily to historians of astronomy and solar astronomers ... . Summing Up: Recommended. Researchers, faculty, and professionals." (R. L. Mutel, Choice, Vol. 47 (4), December, 2009)

Preface.- The Sun.- The Solar Structure.- The Photosphere.- Observing the Solar Surface.- The Chromosphere.- The Corona.- The Solar Wind.- 3-D Topology of the Magnetic Field.- Observing the Outer Layers.- Time Scales of Solar Variability.- Solar Terrestrial Relations.- Naked-eye Sunspots.- The Human Eye as a Detector of Light.- Visibility Criteria.- Naked-eye Sunspot Observations.- Naked-eye Sunspots and Temporal Evolution of Solar Activity.- Solar Drawings.- Pretelescopic Instruments.- The Invention of the Telescope.- First Telescopic Observations of Sunspots.- The Maunder Minimum.- The Rise of Solar Activity and the Dalton Minimum: 18th and 19th Centuries.- Sunspots Drawings in the Photography Era.- The First Granulation Drawings.- Sunspot Fine Structures.- Faculae.- White-light Flares.- The Outer Layers of the Sun.- The Influence of the Eye in Solar Drawings.- Physics from Drawings.- Modern Solar Drawings.- Solar Eclipses.- The Basics of Solar Eclipses.- Historical Solar Eclipse Observations.- Science Using Early Reports of Solar Eclipses.- The Solar Diameter and the Astronomical Unit.- The Earth’s Orbit.- Measuring the Known World.- Observing Methods of Solar Diameter.- Theoretical Background.- Long-term Variations.- Planetary Transits.- Terrestrial Aurorae and Solar-Terrestrial Relations.- Auroral Physics in Brief.- Folklore, Omen and Myths.- Reports During the Last Two Millennia.- The Search for the Cause.- Catalogues of Aurorae Observations.- Aurorae and Secular Solar Activity.- Aurora and Great Space Weather Events.- Reconstruction of Solar Activity During the Telescopic Era.- Wolf’s Reconstruction.- The Reconstruction by Hoyt and Schatten.- Improving and Finding Lost Observations.- Final Comments.- Index.

M. Vázquez is a senior solar astronomer and author of "Ultraviolet Radiation in the Solar System", already published by Springer in 2005

J.M.Vaquero has written approximately thirty papers about the use of historical observations and measurements in modern astronomical and geophysical studies

The Sun Recorded Through History is a text that reconstructs past solar activity based on information from historical documents, complementing studies using other techniques. Historical accounts describing phenomena related to solar activity, such as aurorae, sunspots, and corona observed during solar eclipses can be used as a proxy of solar activity in the past. These descriptions are reviewed, on the one hand providing primary material for the history of astronomy and, on the other, verifying or refuting current ideas concerning the time variability of the Sun on the scale of centuries.

Documents predating the discovery of photography (around 1840) that contain information on these topics are highlighted, but modern drawings are also included. The lower temporal limit of study is set by the archaeoastronomy of prehistoric sources. In addition, the necessary background on the Sun is provided, with special emphasis on observing techniques and the influences of telescopes and the Earth's atmosphere on the data obtained from solar observations.

This book contains over two hundred figures, many of which are reproductions of historical documents and hand drawings. It is an essential resource on the evolution of solar observations and will be of interest to students and researchers in solar physics, as well as astronomers and historians of science.



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