Results 151 to 160 of about 2,906 (200)
Stimuli-Responsive Afterglow from Luminescent Liquid Crystal Elastomers. [PDF]
Adv MaterYue L, Debije MG, Schenning APHJ.
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Color-tunable ultralong room temperature afterglow in a wide excitation range from ultraviolet to visible light <i>via</i> doping boric acid with polyaromatic hydrocarbons. [PDF]
Chem SciYan S +5 more
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Giant Scintillation Yield Enhancement in Zero-Dimensional Halides by Exciton Confinement Manipulation. [PDF]
Research (Wash D C)Wang Y +10 more
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Investigation of the phosphorescence, persistent decay and structure properties of Eu<sup>2+</sup>: strontium aluminate doped with Nd<sup>3+</sup>, B<sup>3+</sup> or Dy<sup>3</sup>. [PDF]
BMC ChemSawan SEA, Hamdy YM, Khattab RM.
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Butterfly-Shaped Guest Molecules Enable Tunable Room-Temperature Phosphorescence in Host-Guest Doped Systems. [PDF]
Adv Sci (Weinh)Lou Z +5 more
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Science, 1968
Brief stimulation of the upper lip with the tip of a nylon thread frequently produces an "afterglow" sensation that may persist as long as several minutes after cessation of stimulation. The duration of afterglow is increased by strong suggestion, and decreased by vibration of the skin prior to stimulation.
R, Melzack, H, Eisenberg
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Brief stimulation of the upper lip with the tip of a nylon thread frequently produces an "afterglow" sensation that may persist as long as several minutes after cessation of stimulation. The duration of afterglow is increased by strong suggestion, and decreased by vibration of the skin prior to stimulation.
R, Melzack, H, Eisenberg
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2002
Abstract By 1993 most astronomers were convinced, on the basis of the BATSE data and apparently sound theoretical arguments, that gamma-ray bursts occur at cosmological distances, and that they involve relativistic expansion with Lorentz factors of one hundred or more.
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Abstract By 1993 most astronomers were convinced, on the basis of the BATSE data and apparently sound theoretical arguments, that gamma-ray bursts occur at cosmological distances, and that they involve relativistic expansion with Lorentz factors of one hundred or more.
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2011
This chapter focuses on the search for afterglows of gamma-ray bursts (GRBs). In 1996, Peter Mészáros (Pennsylvania State University) and Martin J. Rees (Cambridge University) began developing a detailed theory of afterglows, positing that long-lived emission should be observed at all wavelengths—a panchromatic phenomenon—as a natural consequence of ...
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This chapter focuses on the search for afterglows of gamma-ray bursts (GRBs). In 1996, Peter Mészáros (Pennsylvania State University) and Martin J. Rees (Cambridge University) began developing a detailed theory of afterglows, positing that long-lived emission should be observed at all wavelengths—a panchromatic phenomenon—as a natural consequence of ...
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A short duration afterglow of nitrogen; survey of afterglows
Planetary and Space Science, 1959Abstract When an electron beam of more than 10·5 eV energy traverses low pressure nitrogen the beam is surrounded by a diffuse glow emitting the first positive bands ( 1 ). This light is interpreted as an afterglow. It is attributed to metastable molecules, a 1 Π , which diffuse out of the space occupied by the beam, are thrown by collisions with ...
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