Our numerical task is to solve the dispersion relation in complex variables, obtaining the real and imaginary parts of the wave frequency, or as is usually done, of the wave phase velocity [v.sub.ph] = [omega]/[k.sub.z], as functions of the axial wave number, [k.sub.z], at various magnitudes of the velocity shear between the soft X-ray
jet and its environment, [v.sub.0].
The Phase Relation between Sunspot Numbers and Soft X-Ray
Flares, Astrophysics and Space Science 333: pp.
(2005) Luminosity-dependent evolution of soft X-ray
include wavelengths that are shorter than visible light.
It has been reported previously by the authors that soft x-ray
analysis provides a viable alternative testing route to sodium ion testing for superabsorbent amounts in diapers.
Aschenbach et al., "A soft X-ray
image of the Moon," Nature, vol.
NASA's more capable Soft X-ray
Spectrometer (SXS), developed by a team of scientists at NASA's Goddard Space Flight Center in Greenbelt, Maryland, is one of the mission's four scientific instruments.
Astronomers have confirmed that a soft X-ray
glow permeating the sky has two sources: one inside the solar system, one outside.
He further explained that this glow, known as the soft X-ray
diffuse background, was surprisingly bright in the gas-rich central plane of the galaxy, where it should be strongly absorbed and this suggested that the background was a local phenomenon, arising from a bubble of hot gas extending out a few hundred light-years from the solar system in all directions.
NC State physicist Harald Ade, UNC-Chapel Hill chemist Wei You and collaborators from both institutions studied the molecular composition of solar cells to determine what aspects of structures have the most impact on efficiency They used advanced soft x-ray
techniques to describe the orientation of molecules within donor and acceptor materials.
The results from the study of this event were published in December in The Astrophysical Journal article titled "Extraordinary Luminous Soft X-Ray
Transient MAXI J0158-744 as an Ignition of a Nova on a Very Massive O-Ne White Dwarf." This data shares with the world the sighting of an especially bright X-ray emission, named MAXI J0158-744, which provides evidence of the explosion of the star.
Three months later, the rats (4-month-old) were examined by soft X-ray
radiography, micro-computed tomography ([micro]CT), and electron microscopy.