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- Publications
- Influence
Nanoflares and the solar X-ray corona
- E. N. Parker
- Physics
- 1 July 1988
Observations of the sun with high time and spatial resolution in UV and X-rays show that the emission from small isolated magnetic bipoles is intermittent and impulsive, while the steadier emission… Expand
THE STELLAR WIND REGIONS
- E. N. Parker
- Physics
- 1 July 1961
Abstract : WITH CLASS G main sequence and M-giant stars are given for various interst llar environments. The supersonic wind from a class G star undergoes a shock transition to subsonic flow at a… Expand
Cosmic-Ray Modulation by Solar Wind
- E. N. Parker
- Physics
- 15 June 1958
This chapter focuses on cosmic-ray modulation by solar wind. The hydrodynamic outflow of gas from the Sun as observed by Biermann results in a reduction of the cosmic-ray intensity in the inner solar… Expand
Why Do Stars Emit X Rays
- E. N. Parker
- Physics
- 1 July 1987
The Sun was the first observed x‐ray star. In 1948 rocket‐borne instruments, carried out of the terrestrial atmosphere for only a few minutes at a time, detected solar x rays. Then in April 1960… Expand
Comment on ``Current Paths in the Corona and Energy Release in Solar Flares''
- E. N. Parker
- Physics
- 1 November 1996
The dynamical behavior of an electrically conducting fluid containing a magnetic field B is described by Newton's and Maxwell's equations directly in terms of the momentum density, Reynolds stress,… Expand
The Acceleration of Particles to High Energy
- E. N. Parker
- Physics
- 1976
The common occurrence, and often spectacular consequence, of fast particles in active astrophysical bodies has attracted the attention of physicists for more than four decades. The acceleration… Expand
The occasional reversal of the geomagnetic field
- E. N. Parker
- Physics
- 1 November 1969
Cyclonic convective cell fluctuation and nonuniform core rotation effects on reversal of geomagnetic field, investigating fossil magnetism