论文信息 - Authors' Reply to preceding discussion [by E.N. Parker on ‘Hydrodynamic models of the solar corona’] - 字舞流文

Authors' Reply to preceding discussion [by E.N. Parker on ‘Hydrodynamic models of the solar corona’]

F. Scarf | L. M. Noble

[1] W. Axford,et al. TERMINATION OF SOLAR WIND AND SOLAR MAGNETIC FIELD , 1963 .

[2] E. Smith,et al. Interplanetary Magnetic Fields , 1962, Science.

[3] F. Scarf,et al. Hydrodynamic models of the solar corona , 1962 .

[4] W. Axford. The interaction between the solar wind and the Earth's magnetosphere , 1962 .

[5] P. Kellogg. Flow of plasma around the Earth , 1962 .

[6] E. Parker. Kinetic properties of interplanetary matter , 1962 .

[7] E. Parker. Sudden Expansion of the Corona Following a Large Solar Flare and the Attendant Magnetic Field and Cosmic-Ray Effects. , 1961 .

[8] J. W. Chamberlain. Interplanetary Gas. III. a Hydrodynamic Model of the Corona. , 1961 .

[9] D. E. Billings. Distribution of Matter with Temperature in the Emission Corona. , 1959 .

[10] E. Parker. Dynamics of the Interplanetary Gas and Magnetic Fields , 1958 .

[11] S. Chapman. The Viscosity and Thermal Conductivity of a Completely Ionized Gas. , 1954 .

[12] N. Ness,et al. Explorer 10 magnetic field measurements , 1963 .