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Related papers: A microwave plasma source for VUV atmospheric phot…

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Analysis of the Cassini Ultraviolet Imaging Spectrometer (UVIS) stellar and solar occultations at Titan to date include 12 species: N$_{2}$ (nitrogen), CH$_{4}$ (methane), C$_{2}$H$_{2}$ (acetylene), C$_{2}$H$_{4}$ (ethylene),…

Astrophysics · Physics 2009-11-13 Mao-Chang Liang , Yuk L. Yung , Donald E. Shemansky

Chemistry in Titan's N2-CH4 atmosphere produces complex organic aerosols. The chemical processes and the resulting organic compounds are still far from understood, although extensive observations, laboratory, and theoretical simulations…

Earth and Planetary Astrophysics · Physics 2022-09-26 Chao He , Joseph Serigano , Sarah M. Horst , Michael Radke , Joshua A. Sebree

Assuming a spherical symmetry, the extreme UV emitted by a very hot source ionizes low pressure molecular hydrogen making a transparent bubble of H II (Protons and electrons). For an increase of radius, intensity of extreme UV and…

General Physics · Physics 2007-07-23 Jacques Moret-Bailly

Shematovich et al. (2003) recently showed plasma induced sputtering in Titan's atmosphere is a source of neutral nitrogen in Saturn's magnetosphere comparable to the photo-dissociation source. These sources form a toroidal nitrogen cloud…

Space Physics · Physics 2015-06-26 H. T. Smith , R. E. Johnson , V. I. Shematovich

A novel kind of electron beam sustained discharge is presented in which a 12keV electron beam is combined with a 2.45GHz microwave power to excite argon gas at atmospheric pressure in a continuous mode of operation. Optical emission…

Plasma Physics · Physics 2015-11-30 T. Dandl , H. Hagn , A. Neumeier , J. Wieser , A. Ulrich

We propose a new scheme of producing intense neutron beam whose yields exceed those of existing facilities by many orders of magnitude. This scheme uses the recently proposed photon beam extracted from circulating quantum ions, which is…

Nuclear Experiment · Physics 2017-12-06 T. Masuda , A. Yoshimi , M. Yoshimura

Extreme ultraviolet (XUV) light sources allow for the probing of bound electron dynamics on attosecond scales, interrogation of high-energy-density matter, and access to novel regimes of strong-field quantum electrodynamics. Despite the…

This paper studies a continuous atmospheric-pressure discharge maintained by focused subterahertz radiation of a 263 GHz gyrotron. A plasma torch propagating towards microwave radiation was sustained on an argon flow exiting a metal gas…

Plasma Physics · Physics 2020-05-20 S. V. Sintsov , A. V. Vodopyanov , M. E. Viktorov , M. V. Morozkin , M. Yu. Glyavin

The IceCube experiment recently detected the first flux of high-energy neutrinos in excess of atmospheric backgrounds. We examine whether these neutrinos originate from within the same extragalactic sources as ultrahigh-energy cosmic rays.…

High Energy Astrophysical Phenomena · Physics 2015-06-12 Matthew D. Kistler , Todor Stanev , Hasan Yuksel

The flat spectrum radio quasar (FSRQ) 4C +21.35 (PKS 1222+216) displays prominent nuclear infrared emission from ~1200 K dust. A 70 -- 400 GeV flare with ~10 min variations during half an hour of observations was found by the MAGIC…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Charles D. Dermer , Kohta Murase , Hajime Takami

Far-ultraviolet (FUV) radiation is a driving source of photochemistry in planetary atmospheres. Proper interpretation of atmospheric observations requires a full understanding of the radiation environment that a planet is exposed to. Using…

Earth and Planetary Astrophysics · Physics 2026-01-09 Patrick R. Behr , Kevin France , Nicholas Kruczek , Nicholas Nell , Brian Fleming , Stefan Ulrich , Girish M. Duvvuri , Amy Louca , Yamila Miguel

Recently, it was suggested that a photospheric component that results from the internal dissipation occurring in the optically thick inner parts of relativistic outflows may be present in the prompt $\gamma$/X-ray emission of gamma-ray…

Astrophysics · Physics 2009-11-13 Xiang-Yu Wang , Zi-Gao Dai

The conceptual design of a compact source of GeV-class muons is presented, based on a plasma based electron-gamma collider. Evaluations of muon flux, spectra and brilliance are presented, carried out with ad-hoc montecarlo simulations of…

It is often stated that the observation of high-energy neutrinos from an astrophysical source would constitute a smoking gun for the acceleration of hadronic cosmic rays. Here, we point out that there exists a purely leptonic mechanism to…

High Energy Astrophysical Phenomena · Physics 2023-05-22 Dan Hooper , Kathryn Plant

This paper describes the development of a pulsed light source using the discharge from an electrode in a medium of various noble gases. This source can be used to aid in the characterization and testing of new vacuum-ultraviolet (VUV)…

Instrumentation and Detectors · Physics 2022-06-01 A. D. McDonald , M. Febbraro , J. Asaadi , C. C Havener

Dust grains in cold circumstellar regions and dark-cloud interiors at 10-20 K are covered by ice mantles. A nonthermal desorption mechanism is invoked to explain the presence of gas-phase molecules in these environments, such as the…

Solar and Stellar Astrophysics · Physics 2014-06-02 G. A. Cruz-Diaz , G. M. Muñoz Caro , Y. -J. Chen , T. -S. Yih

We consider a situation in which a pulsar is formed inside or close to a high density region of a molecular cloud. Right after birth, the pulsar was very active and accelerated hadrons and leptons to very high energies. Hadrons diffuse…

Astrophysics · Physics 2009-11-13 H. Bartko , W. Bednarek

In the past years, EUV lithography scanner systems have entered High-Volume Manufacturing for state-of-the-art Integrated Circuits (IC), with critical dimensions down to 10 nm. This technology uses 13.5 nm EUV radiation, which is…

We report on two types of Raman laser sources emitting in the near and middle ultraviolet spectral ranges by the use of a solarization-resilient gas-filled inhibited-coupling (IC) hollow-core photonic-crystal fiber (HCPCF) with record low…

A new method for the measurement of the muon flux in the deep-sea ANTARES neutrino telescope and its dependence on the depth is presented. The method is based on the observation of coincidence signals in adjacent storeys of the detector.…

High Energy Astrophysical Phenomena · Physics 2012-08-27 ANTARES collaboration