Guide to the SunCambridge University Press, 30.3.1995 - 386 sivua The Sun has been an object of scientific interest since the time of the ancient Greeks. The vast amounts of observational data acquired in recent years have led to a greatly improved knowledge of the physics of the Sun. With a minimum of technicalities, this book gives an account of what we now know about the Sun's interior, its surface and atmosphere, its relation to the solar system including the earth, and its relation to other stars. The way that solar power is being converted to useful forms of energy is explained. The book is aimed at anyone with a broad science background interested in learning about the latest developments in solar studies, from those at high-school level to the non-specialist professional. |
Sisältö
II | 1 |
III | 6 |
IV | 14 |
V | 16 |
VI | 20 |
VII | 26 |
VIII | 31 |
IX | 33 |
XXXVIII | 157 |
XXXIX | 160 |
XL | 173 |
XLI | 179 |
XLII | 203 |
XLIII | 207 |
XLIV | 218 |
XLVI | 221 |
X | 34 |
XI | 38 |
XII | 41 |
XIII | 43 |
XIV | 47 |
XV | 53 |
XVI | 58 |
XVII | 67 |
XVIII | 73 |
XIX | 78 |
XX | 79 |
XXI | 81 |
XXII | 87 |
XXIII | 92 |
XXIV | 97 |
XXV | 99 |
XXVI | 103 |
XXVII | 106 |
XXVIII | 109 |
XXIX | 114 |
XXX | 123 |
XXXI | 127 |
XXXIII | 133 |
XXXIV | 137 |
XXXV | 142 |
XXXVI | 149 |
XXXVII | 150 |
XLVII | 227 |
XLVIII | 235 |
XLIX | 243 |
L | 253 |
LI | 257 |
LII | 262 |
LIV | 264 |
LV | 276 |
LVI | 295 |
LVII | 296 |
LVIII | 302 |
LIX | 303 |
LX | 305 |
LXI | 309 |
LXII | 312 |
LXIII | 315 |
LXIV | 325 |
LXV | 334 |
LXVI | 342 |
LXVII | 344 |
LXVIII | 345 |
LXIX | 348 |
LXX | 355 |
LXXI | 360 |
LXXII | 363 |
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absorption active regions altitude amount arc seconds areas astronomical atoms auroral bright centre chromosphere continuum convection core corona coronal holes Courtesy cycle decrease density diameter disc distance Doppler earth earth's atmosphere eclipse electrons emission lines emitted field strength filaments flux footpoints Fraunhofer lines give rise hard X-ray heating helium hydrogen indicated instruments intensity interplanetary ionized ions irradiance K lines km/s latitudes light limb loops magnetic field lines main sequence mass measured metre motion neutrino nucleus Observatory observed occur orbit oscillations ozone particles penumbra period photosphere plane plasma polarity prominence protons radiation radio rotation shows Skylab soft X-ray solar activity solar atmosphere solar energy solar interior Solar Maximum Solar Maximum Mission solar wind spacecraft spectral spectral flux spectrum speed spots stars stellar structure sun's sunspot groups sunspot number surface telescope temperature transition region ultraviolet velocity visible W/m² wavelength waves white-light X-ray