What seems even more wonderful is that these spectral colors can be recombined so as to make white light.
"General Science" by Bertha M. Clark
About him, causing his figure to appear gigantic, his shadow grotesque, the yellow gleam of the light shone in spectral coloring.
"Beth Norvell" by Randall Parrish
One of the defects of the light emitted by the incandescent vapor of mercury is its paucity of spectral colors.
"Artificial Light" by M. Luckiesh
The parallel harmony among the spectral colors is blue, violet, and orange.
"The Continental Monthly , Vol. 2 No. 5, November 1862" by Various
The spectral colors are arranged in order along the heavy solid line, and the purples along the heavy dotted line.
"Psychology" by Robert S. Woodworth
Its color was a spectral silvery blue, much like that of the moon when seen in the daytime.
"A Volunteer with Pike" by Robert Ames Bennet
To facilitate comparison, spectral lines and colors are given in Table 4.
"The Nature of Animal Light" by E. Newton Harvey
Each metal has its own number, position, grouping, and color of these spectral lines.
"Curiosities of Heat" by Lyman B. Tefft
In §4 I use colors and model ﬁts to the 9-ﬁlter spectral energy distributions (SEDs) to compute redshifts and classify the EROs as either ellipticals or dusty starbursts.
A Deep Multicolor Survey. VII. Extremely Red Objects and Galaxy Formation
The drawback is that this involves a description of spectral shape in terms of more numbers (the spectral parameters) than just two X-ray colors, and that the correct models are unknown.
A review of rapid X-ray variability in X-ray binaries
Figure 1.1: Left: Spectral evolution of the combined optical ﬂux density of GRB 030329, the associated SN2003dh, and its host galaxy (colored lines) compared to the spectrum of SN1998bw (dashed line).
Gamma-Ray Bursts, Collisionless Shocks and Synthetic Spectra
Spectral properties of the 3D model are rather sensitive to convection too, which results in signiﬁcant differences between photometric colors calculated with the 3D and 1D model atmospheres.
Convection and observable properties of late-type giants
The chosen color corresponds to a spectral class of about M2 and an effective temperature of about 3500 K.
Testing the Disk-Locking Paradigm: An Association Between U-V Excess and Rotation in NGC 2264