Solar and Stellar Magnetic Activity
C.J. Schrijver & Cornelis Zwaan
Book 1 of Sun
Language: English
37.15.00=Geomagnetism and high atmospheric layers 41.21.00=Sun 41.23.00=Stars 41.51.00=Observatories. Instruments active active main-sequence active region activity adv angular momentum angular-momentum loss area astron astron astrophys astrophys atmosphere atmospheric heating binary bright broadband photometry caillault case cen change chemically homogeneous chromosphere chromospheric collier cameron completely convective component concentration conf constructive interference content convection convective convective collapse convective envelope convective motion convective zone cool core corona coronal coronal condensation cycle cyr data day density developed devices and methods of astronomical observations diagram discussed disk disperses distribution dor dynamo electromotive force emergence emission energy envelope evolution factor feature force acting fully convective function giant grain gravitational collapse greenwich photoheliographic heating height high highly intermittent increase intergranular lane intersupergranular lane lac landi deglinnocenti late lateral inux latitude loop lorentz force loss lower-limit magnetic magnetic brake magnetic braking magnetic grain magnetic monopoles magnetic pressure magnetic tension magnetostatic equilibrium main mass model momentum deposition nearest neighbor network nuclear reaction number numerical experiment observed ohmic diffusion opposite-polarity outer outer atmosphere parameter pattern period photosphere photospheric phys plage plasma point polarity pressure property publ pyx radiative random environments random walk random walks range rapid rotators rate red-giant branch region relationship result rev rigid rotation roche lobe rosa rotation san francisco sanchez almeida scale schrijver sequence ser sharply bounded soc soft x-rays sol sol phys solar spectral spectrum spot star stellar stellar analog strength strong structure study sun sunspot surface taylor theorem temperature term thermal equilibrium tidal bulge time time scale tube turbulent diffusivity type ursae majoris van ballegooijen van driel-gesztelyi van rijsbergen velocity vice versa von kluber von steiger wave weighted preferentially wilson wind zone zwaan
Description:
"SOLAR AND STELLAR MAGNETIC ACTIVITY C.J. SCHRIVER C.ZWAAN CAMBRIDGE UNIVERSITY PRESS This timely volume provides the first comprehensive review and synthesis of the current understanding of the origin, evolution, and effects of magnetic fields in the Sun and other cool stars. Magnetic activity results in a wealth of phenomena—including starspots, nonradiatively heated outer atmospheres, activity cycles, deceleration of rotation rates, and even, in close binaries, stellar cannibalism—all of which are covered clearly and authoritatively. This book brings together for the first time recent results in solar studies, with their wealth of observational detail, and stellar studies, which allow the study of how activity evolves and depends on the mass, age, and chemical composition of stars. The result is an illuminating and comprehensive view of stellar magnetic activity. Observational data are interpreted by using the latest models in convective simulations, dynamo theory, outer-atmospheric heating, stellar winds, and angular momentum loss. Researchers are provided with a state-of-the-art review of this exciting field, and the pedagogical style and introductory material make the book an ideal and welcome introduction for graduate students." Ключевые слова: ser, convective envelope, spectral, lac, tube, evolution, outer atmosphere, ddr, sol, red-giant branch, type, active region, ii ux, giant, landi deglinnocenti, i e, te, component, dynamo, function, astron astrophys, greenwich photoheliographic, factor, point, cvn, chromospheric, emergence, concentration, sol phys, constructive interference, pi, rate, astron, content, pyx, magnetic, time, magnetic ?eld, cen, magnetic brake, pc, strength, study, lateral inux, magnetic pressure, region, numerical experiment, yr, taylor theorem, phys, coronal, van driel-gesztelyi, magnetic monopoles, sanchez almeida, relationship, scale, zwaan, result, disperses, fx, completely convective, van rijsbergen, magnetostatic equilibrium, star, coronal condensation, publ, cool, magnetic tension, distribution, spot, gravitational collapse, plage, case, caillault, thermal equilibrium, large, pattern, intersupergranular lane, day, stellar, mass, velocity, plasma, p t, dor, developed, astrophys, sharply bounded, broadband photometry, wilson, active main-sequence, sequence, disk, network, convective zone, ly, highly intermittent, main, temperature, parameter, ohmic diffusion, intergranular lane, schrijver, outer, si iv, random walk, random walks, lorentz force, soft x-rays, nuclear reaction, core, lower-limit, late, corona, grain, vice versa, binary, area, chemically homogeneous, height, hp, turbulent diffusivity, high, electromotive force, heating, von kluber, angular momentum, energy, adv, chromosphere, ht, ?ux, angular-momentum loss, ?ares, g-k-, magnetic braking, range, von steiger, crb, term, spectrum, time scale, san francisco, stellar analog, radiative, random environments, diagram, rapid rotators, fe ix, latitude, nearest neighbor, ha, ii, polarity, photospheric, magnetic grain, opposite-polarity, pressure, soc, cyr, wave, ?ow, force acting, period, structure, convective, active, rev, activity, discussed, density, fully convective, loss, data, rosa, convective collapse, convection, sunspot, ursae majoris, feature, van ballegooijen, solar, eq, photosphere, ?eld, dl dt, rigid rotation, observed, rotation, atmosphere, envelope, collier cameron, increase, model, surface, zone, cycle, wind, weighted preferentially, mx, strong, small, mk, loop, lc iv, emission, roche lobe, tidal bulge, number, momentum deposition, sun, property, change, atmospheric heating, conf, convective motion, bright