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Background radiation diffuse emission

There is also considerable variety in the astronomical goals. Seven experiments are devoted primarily to far Infrared surveys, seven to measurements of the cosmic background radiation, four to high resolution mapping and photometry, one to measurement of diffuse emission in the near Infrared, five to solar brightness, polarization, and spectra, and one to planetary spectra,... [Pg.156]

Polycyclic aromatic hydrocarbons (PAHs) Hydrocarbons in complex chains and agglomerated rings thought to be responsible for the diffuse emission Unes observed in dust nebulae in the near-infrared. These molecules form the lowest-mass end of the dust distribution and are responsible for ubiquitous diffuse emission in the 1- to 25-fxm galactic background radiation. [Pg.2]

See other pages where Background radiation diffuse emission is mentioned: [Pg.375]    [Pg.376]    [Pg.247]    [Pg.2]    [Pg.2]    [Pg.155]    [Pg.81]    [Pg.82]    [Pg.4]    [Pg.52]    [Pg.6105]    [Pg.6104]    [Pg.102]    [Pg.193]    [Pg.6]    [Pg.63]    [Pg.344]   
See also in sourсe #XX -- [ Pg.2 ]

See also in sourсe #XX -- [ Pg.2 ]



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Background emission

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Diffuse background

Diffuse background radiation

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