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The mystery of unidentified infrared emission bands
A family of unidentified infrared emission (UIE) bands has been observed throughout the Universe. The current observed spectral properties of the UIE...
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Finite Resources: Pawsey and the HI-Line, 1948–1960
It is well known that the group at RPL had the equipment and the talent to have achieved one of the ground-breaking discoveries of early radio... -
Effect of Continuum Scattering on the Statistical and Temporal Characteristics of Spectral Line Formation
Some new results from our study of the effect of continuum scattering on different observed characteristics of spectral lines are presented. The main...
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Circumstellar Shell and Emission of the SN 2020tlf Progenitor
AbstractWe investigate the phenomenon of a dense circumstellar (CS) shell and powerful emission of the (type IIP) SN 2020tlf progenitor. Our modeling...
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Temperatures in the Upper Mesosphere and Lower Thermosphere from O2 Atmospheric Band Emission Observed by ICON/MIGHTI
The Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI) was launched aboard NASA’s Ionospheric Connection (ICON)...
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Single photon emission and recombination dynamics in self-assembled GaN/AlN quantum dots
III-nitride quantum dots (QDs) are a promising system actively studied for their ability to maintain single photon emission up to room temperature....
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THz emission with X-mode laser pulses
We propose to investigate the THz emission using laser–plasma interaction, when two X-mode lasers beat and interact with inhomogeneous plasmas. Pulse...
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Detection of green line emission in the dayside atmosphere of Mars from NOMAD-TGO observations
The oxygen emission at 557.7 nm is a ubiquitous component of the spectrum of the terrestrial polar aurora and the reason for its usual green colour
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Defocused imaging-based quantification of plasmon-induced distortion of single emitter emission
Optical properties of single emitters can be significantly improved through the interaction with plasmonic structures, leading to enhanced sensing...
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Features of the Shape of the Emission Spectrum of a Spherical Microresonator with a High Refractive Index Luminescent Shell Due to the Polarization of the Whispering Gallery Modes
AbstractThe effect of the thickness and refractive index of the shell on the amplitudes of lines of the TE and TM polarized whispering gallery modes...
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Temporal Defocusing as a Depth Diagnostic of Submerged Sources of Transient Acoustic Emission from Solar Flares
Helioseismic holography applied to HMI observations of a sunquake associated with the SOL20140207T10:29M1.9 flare hosted by NOAA AR11968 shows the...
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Application of Machine Learning to Determine Electron Temperature in Globus-M2 Tokamak Using the Soft X-Ray Emission Data and the Thomson Scattering Diagnostics Data
AbstractAn important part of high-temperature plasma study is the determination of the electron temperature dynamics in the tokamak plasma. At...
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Multi-millijoule terahertz emission from laser-wakefield-accelerated electrons
High-power terahertz radiation was observed to be emitted from a gas jet irradiated by 100-terawatt-class laser pulses in the laser-wakefield...
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Gamma-ray line from electroweakly interacting non-abelian spin-1 dark matter
We study gamma-ray line signatures from electroweakly interacting non-abelian spin-1 dark matter (DM). In this model, Z 2 -odd spin-1 particles...
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Efficiencies of Emission Excitation and Electron Density Formation in Auroras
AbstractIt is shown that the efficiencies of excitation of optical emissions with λ = 391.4, 557.7, and 630.0 nm, and the efficiency of formation of...
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Modeling of Hydrogen Emission Lines in the Spectrum of UX Ori in Its Bright State and during Eclipses
Abstract—The hydrogen spectrum of the UX Ori-type star is modeled in a bright state and during an eclipse by an opaque dusty fragment of its own...
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Peering into the Milky Way by FAST: II. Ionized gas in the inner Galactic disk revealed by the piggyback line observations of the FAST GPPS survey
As one of the major components of the interstellar medium, the ionized gas in our Milky Way, especially the low-density diffuse component, has not...
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Secondary Emission in Bi2Se3
In this chapter I will present our study of the secondary emissions (radiation) in a prototypical 3D topological insulator (TI) material, Bi2Se3. I... -
Gamma Ray Emission Imaging in the Medical and Nuclear Safeguards Fields
Gamma rays emitted from within an object can reveal information about that object in a non-destructive way, i.e. without physically opening the...