Magnetic fields are ubiquitous in astrophysical plasmas. They are responsible for most of the stellar activities and they manifest in numerous ways in the stellar atmospheres. The Sun being our nearest star is the natural ...

Solar coronal heating and the energy/mass flow of the solar wind is one of the unsolved but fundamental problems of solar physics. While it has been well established for decades that the corona and solar wind owe their ...

Ground-based radio observations of the solar corona at low frequencies (< 100 MHz) provide useful information in the height range ≈ 1−2 R☉ above the photosphere which is presently difficult to observe at other regions ...

The outer solar atmosphere, the corona, is known for its million-degree temperature. The mystery surrounding the source of this high temperature is gradually being resolved with various theories, observations and models. ...