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E-grāmata: Sunspots and Starspots

(University of Cambridge), (University of Rochester, New York)
  • Formāts: PDF+DRM
  • Sērija : Cambridge Astrophysics
  • Izdošanas datums: 23-Oct-2008
  • Izdevniecība: Cambridge University Press
  • Valoda: eng
  • ISBN-13: 9780511451515
  • Formāts - PDF+DRM
  • Cena: 61,85 €*
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  • Formāts: PDF+DRM
  • Sērija : Cambridge Astrophysics
  • Izdošanas datums: 23-Oct-2008
  • Izdevniecība: Cambridge University Press
  • Valoda: eng
  • ISBN-13: 9780511451515

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The past two decades have seen remarkable advances in observations of sunspots and their magnetic fields, in imaging of spots and fields in distant stars and in associated theoretical models and numerical simulations. This book provides a comprehensive combined account of the properties of sunspots and starspots. It covers both observations and theory, and describes the intricate fine structure of a sunspot's magnetic field and the prevalence of polar spots on stars. The book includes a substantial historical introduction and treats solar and stellar magnetic activity, dynamo models of magnetic cycles, and the influence of solar variability on the Earth's magnetosphere and climate. This volume is a valuable reference for graduate students and specialists in solar and stellar physics, astronomers, geophysicists, space physicists and experts in fluid dynamics and plasma physics.

Recenzijas

Review of the hardback: 'As the 46th title in the Cambridge astrophysics series, this book on sunspots and starspots lives up to the high standards of many of the titles in this series. Both Thomas and Weiss are well-known experts in the field of spots on both the Sun and other stars The authors discuss more recent changes in Earth's temperature and, following a series of well-reasoned arguments, conclude that global warming by anthropogenic greenhouse gases is indeed a serious problem for mankind.' Clare Parnell, Journal of Geophysical and Astrophysical Fluid Dynamics

Papildus informācija

A comprehensive account of sunspots and starspots for graduate students, astronomers, geophysicists, space physicists and experts in solar and stellar physics.
Preface xv
The Sun among the stars
1(14)
Sunspots and solar magnetic activity
1(4)
The Sun as a star
5(5)
Solar structure
5(2)
Properties and classification of stars
7(3)
Starspots and stellar magnetic activity
10(3)
The solar-stellar connection
10(1)
Spots on stars
11(2)
Plan of the book
13(1)
References for background reading
13(2)
Sunspots and starspots: a historical introduction
15(23)
Early observations of sunspots
15(5)
The sunspot cycle
20(3)
The Maunder Minimum
22(1)
Photographic studies of sunspots
22(1)
Fine structure in sunspots
23(3)
Spectroscopy and the sunspot magnetic field
26(2)
Hale's discovery of the sunspot magnetic field
26(1)
The Evershed effect
27(1)
Solar granulation and supergranulation
28(1)
Theoretical advances
29(3)
The development of magnetohydrodynamics
29(1)
Magnetoconvection
30(1)
Dynamo theory
31(1)
The solar wind
31(1)
Recent progress on sunspots
32(1)
Starspots
33(3)
Chronology of key developments (1610-1964)
36(2)
Overall structure of a sunspot
38(30)
Morphology of sunspots
38(3)
Thermal properties of sunspots
41(6)
The cooling of sunspots
41(1)
Brightness of the umbra and penumbra
42(3)
The weak bright ring around a sunspot
45(1)
The Wilson depression
46(1)
Spectroscopy and atmospheric models
47(7)
Spectral analysis of the umbra and penumbra
47(1)
Semi-empirical models of umbral and penumbral atmospheres
48(2)
The chromospheric superpenumbra
50(2)
The transition region and corona above a sunspot
52(2)
Observations of the magnetic field in sunspots
54(6)
The Zeeman effect
54(3)
The magnetic field in a pore
57(1)
Magnetic fields in sunspots
58(2)
Modelling the overall magnetic structure of a sunspot
60(5)
Static axisymmetric models
62(3)
Stability of static models
65(1)
The moat flow
65(3)
Fine structure of the umbra
68(10)
Umbral dots
68(2)
Convection in the umbra
70(5)
Idealized model calculations
71(2)
Realistic simulations
73(1)
Magnetic structure of the umbra
74(1)
Light bridges
75(3)
Fine structure of the penumbra
78(28)
Penumbral filaments
78(5)
Bright grains in penumbral filaments
80(3)
Dark cores within bright filaments
83(1)
The intricate structure of the penumbral magnetic field
83(6)
The interlocking-comb magnetic structure
84(3)
Velocity structure
87(1)
Hyperfine structure and dark cores
88(1)
Convection in the penumbra
89(4)
Travelling patterns in inclined magnetic fields
90(1)
Convection in the inner penumbra
91(1)
Buoyancy braking and the origin of dark cores
92(1)
Dark filaments and convection in the outer penumbra
92(1)
Thin flux tubes in the penumbra
93(1)
The Evershed flow
93(4)
Fine-scale organization of the Evershed flow
94(1)
Theoretical models of the Evershed flow
95(2)
Moving magnetic features in the moat
97(2)
Formation and maintenance of the penumbra
99(7)
Magnetic flux pumping and returning flux tubes
100(3)
Formation of the penumbra
103(3)
Oscillations in sunspots
106(17)
Magneto-atmospheric waves
106(1)
Umbral oscillations
107(10)
Five-minute umbral oscillations
108(2)
Three-minute umbral oscillations and umbral flashes
110(3)
Magnetic field variations
113(1)
Theoretical interpretations of umbral oscillations
114(3)
Penumbral waves
117(1)
Sunspot seismology
118(5)
Absorption of p-modes by a sunspot
118(3)
Time-distance and holographic seismology of sunspots
121(1)
Acoustic halos
122(1)
Sunspots and active regions
123(27)
Description of active regions
123(5)
Pores and their relation to sunspots
123(2)
Faculae and plages
125(3)
Birth and evolution of active regions
128(8)
Magnetic flux emergence in active regions
129(2)
Theoretical models of emerging magnetic flux
131(2)
Intense magnetic elements
133(3)
Formation, growth and decay of sunspots
136(5)
Growth rates of sunspots
136(2)
Lifetimes of sunspots
138(1)
The decay of a sunspot
138(3)
Sunspot groups
141(2)
The magnetic configuration of active regions and sunspot groups
141(1)
Sunspots and solar rotation
142(1)
Dissolution of active regions
143(1)
Flux emergence in the quiet Sun
144(6)
Ephemeral active regions
145(2)
Intergranular magnetic fields and smaller-scale flux emergence
147(3)
Magnetic activity in stars
150(8)
Stellar Ca II emission
150(1)
Variation of activity with rotation rate and age
151(4)
Vigorous activity in late-type stars
155(1)
Other magnetic stars
156(2)
Starspots
158(26)
Observing techniques
158(10)
Photometry
158(2)
Spectroscopy
160(2)
Doppler imaging
162(5)
Zeeman-Doppler imaging
167(1)
Case studies of starspots
168(9)
EK Draconis and other solar analogues
169(2)
RS CVn binaries and FK Com stars
171(1)
BY Draconis
172(1)
AB Doradus
173(3)
T Tauri stars
176(1)
Starspots, differential rotation and dynamo patterns
177(3)
Differential rotation
177(2)
Starspots and surface patterns of activity
179(1)
Starspot cycles from long-term photometry
180(1)
Properties of individual starspots
180(4)
Temperatures and areas
180(1)
Magnetic fields
181(1)
Lifetimes
182(1)
Sunspots as prototypes for starspots?
182(2)
Solar and stellar activity cycles
184(10)
Cyclic activity in the Sun
184(1)
Modulation of cyclic activity and grand minima
185(4)
Differential rotation in the Sun
189(2)
Variable activity in stars
191(3)
Stellar activity cycles
191(2)
Cyclic behaviour in more active stars
193(1)
Solar and stellar dynamos
194(17)
Basic dynamo theory
194(3)
Cowling's theorem
195(1)
Mean-field magnetohydrodynamics and the α-effect
195(2)
Phenomenology of the solar dynamo
197(1)
The solar dynamo
198(7)
Physical mechanisms
199(1)
Location
200(1)
Models of the solar cycle
201(3)
Modulation and grand minima
204(1)
Stellar dynamos
205(4)
Slow rotators
206(1)
Rapid rotators and polar spots
206(1)
Fully convective stars
207(2)
Small-scale dynamo action
209(1)
Numerical simulation of solar and stellar dynamos
210(1)
Solar activity, space weather and climate change
211(18)
The variable solar irradiance
211(5)
Sunspots, faculae and the solar irradiance
213(2)
Spectral variability
215(1)
Interplanetary effects of solar activity
216(5)
Solar flares and coronal mass ejections
216(1)
Space weather
217(3)
Variations in the open solar magnetic flux
220(1)
Solar variability and the Earth's climate
221(6)
Changes in the Earth's orbit
221(1)
Effects of solar variability
222(5)
Global warming
227(2)
The way ahead
229(3)
The structure and dynamics of a sunspot
229(1)
Solar and stellar activity cycles
230(1)
Starspots
230(1)
Prospect for the future
231(1)
Appendix 1 Observing techniques for sunspots 232(6)
Appendix 2 Essentials of magnetohydrodynamic theory 238(8)
References 246(25)
Index 271
John H. Thomas is Professor of Mechanical and Aerospace Sciences, and Astronomy, at the University of Rochester. He has been the Chair of the Solar Physics Division of the American Astronomical Society, and was a Scientific Editor of the Astrophysical Journal for ten years. Nigel O. Weiss is Emeritus Professor of Mathematical Astrophysics at the University of Cambridge. He is a former President of the Royal Astronomical Society, which awarded him a Gold Medal in 2007.