Titlebook: Cosmical Magnetism; D. Lynden-Bell Book 1994 Springer Science+Business Media Dordrecht 1994 Scale.astronomy.magnetosphere.quasar.relativis

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書目名稱Cosmical Magnetism影響因子(影響力)




書目名稱Cosmical Magnetism影響因子(影響力)學(xué)科排名




書目名稱Cosmical Magnetism網(wǎng)絡(luò)公開度




書目名稱Cosmical Magnetism網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Cosmical Magnetism被引頻次




書目名稱Cosmical Magnetism被引頻次學(xué)科排名




書目名稱Cosmical Magnetism年度引用




書目名稱Cosmical Magnetism年度引用學(xué)科排名




書目名稱Cosmical Magnetism讀者反饋




書目名稱Cosmical Magnetism讀者反饋學(xué)科排名

FLAGR

Introduction: Making the Medicinal Poisoner,ing magnetic features that are usually observed to be present in the photosphere below bright points. The model has three phases: a preinteraction phase in which two opposite polarity photospheric magnetic fragments are unconnected magnetically; an interaction phase when the fragments reconnect in t

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Learning at Home and on the Shop Floor a high temperature of 10.K, and occasionally producing spectacular solar flares. The energy flux needed to balance the losses by radiation or by the solar wind of non-flaring coronal gas ranges between several 10. ergs cm. . . in quiet regions to 10. ergs cm. . . in active regions. Coronal holes do

EXULT

From Globalisation to Industrialisationinfluence the theory of the evolution of Cataclysmic Variables, ii) the instability of the toroidal field component in winds and jets from accretion disks, iii) the importance of poloidal vs toroidal collimation of jets, and iv) what determines the distribution of field strength in the disk from whi

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ungainly

Introduction: The Written Constitution,equences include the formation of weak dipole moment millisecond pulsars by the accretion induced spin-up of strong field neutron stars, the absence of observable spin modulation of the thermal X-ray emission from the surfaces of neutron stars in accreting low mass X-ray binaries (LMXB’s), pulsar pe

instate

Introduction: The Written Constitution,fects need to be taken into account in the equation of motion. When this happens, a quasi-classical description is required, with deterministic trajectories becoming stochastic, because quantum corrections must be considered. In this paper the associated physical processes are discussed, simultaneou

Omniscient

Introduction: The Written Constitution,ments by cosmic-ray spallation on interstellar CNO nuclei. Several solutions have been proposed, including confinement of cosmic rays by a strong magnetic field in the early Galaxy, but none of them is very satisfactory. In this paper I suggest a chemically inhomogeneous model for the halo which may