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| HIGH | VISIBLE | LOW | ||||
| GAMMA | XRAY | UV |  | INFRARED | MICROWAVE | RADIOWAVE |
1 The energy of particle travelling through space
 When mass is energized, its particles move and vibrate When some particles attain spin, they become energetic particles Energetic particle distances, and becomes emitted  higher spin farther distance |
 high energy particle escapes |
 low energy particle falls back |
 trapped particle remains |
Visible light and above High energy particle escapes mass Infrared and below Low energy particle is unable to escape mass, falls back Trapped particle remains in mass |
 particle speeds when excited |
 particle slows when resisted |
 when particle slows, it gets closer (clumps) |
 when clumps of particles get big, its mass is visible (cloud, solid) |
I seek refuge in Allah SWT from errors
Only Allah SWT Knows والله أعلم
 Space |  Pulse |  Universe |  Supernova |  Cakerawala |
1 comments on "Particle"
"What is the origin of the solar wind and how is it accelerated to speeds of up to 1.8 million miles per hour? The solar wind fills our entire solar system. When gusts of solar wind arrive at Earth, they can set off dazzling aurora ...
two distinct streams of solar wind: a slow stream travelling at approximately 215 miles per second and a fast stream zipping through space at twice that speed ... the fast wind spews from coronal holes, which are dark, comparatively cool regions on the Sun ... The origins and acceleration mechanisms of the slow solar wind remain mysterious ... As the solar cycle progresses toward its maximum, the structure of the solar wind changes from two-distinct regimes — fast at the poles and slow at the equator — to a mixed, inhomogeneous flow ...
The closed corona refers to regions of the Sun where its magnetic field lines are closed — that is, connected to the solar surface at both ends ... The open corona, on the other hand, refers to regions where the magnetic field lines anchor to the Sun at only one end, stretching out into space on the other, thus creating a highway for solar material to escape into space. Coronal holes — the cooler regions at the source of the fast solar wind — are the habitat of open field lines"
NASA
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