Its uniform motion causes creation of a Parker spiral, which causes distortion of the interplanetary magnetic field.
This phenomenon can be bolstered by ICMEs while the Advanced Composition Explorer was launched in 1997 to find out the constituent particles of this phenomenon.  Its uniform motion causes creation of a Parker spiral, which causes distortion of the interplanetary magnetic field. The slow version of this phenomenon arises from the so-called "streamer belt," which feature closed magnetic loops while the fast version of this phenomenon originates from (*) coronal holes. Wolf-Rayet stars lose ten to the negative 5 solar masses per year due to this phenomenon, which causes comet tails to face away from the sun, and the heliopause is the boundary between the interstellar medium and this stream of plasma. FTP, name this phenomenon in which streams of charged particles are released from the sun's outer layers.
This phenomenon can be bolstered by ICMEs while the Advanced Composition Explorer was launched in 1997 to find out the constituent particles of this phenomenon.  
{solar wind} [or {stellar wind}]