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Paper Title (use style: paper title)
Paper Title (use style: paper title)

... safety threshold) within 30 seconds. This dump rate was chosen based upon a conservative estimate of the time required from removal of the Kirk key at the operator station to entry of the bank enclosure. The dump sizing is also designed to allow several sequential full-energy dumps at 3 minute inter ...
p1,p2,p3 ocr 21st century science
p1,p2,p3 ocr 21st century science

Determination of the levitation limits of dust particles within the
Determination of the levitation limits of dust particles within the

Excitation of molecules in dense clouds
Excitation of molecules in dense clouds

... balance of atoms or molecules, especially those parts of the spectrum where absorption of a photon leads to a significant alteration of the level populations. In many molecules, excitation into an electronically or vibrationally excited state does not lead to emission in the pure rotational lines th ...
Spectral line mapping of the Milky Way
Spectral line mapping of the Milky Way

R&D towards huge liquid argon detectors for nucleon
R&D towards huge liquid argon detectors for nucleon

Diffuse TeV Emission from the Galactic Center
Diffuse TeV Emission from the Galactic Center

Real Properties of Electromagnetic Fields and
Real Properties of Electromagnetic Fields and

Lokal fulltext - Chalmers Publication Library
Lokal fulltext - Chalmers Publication Library

... with a wide range of masses, in proportions approximated by the Salpeter initial mass function (IMF): N (m) ∝ m−2.35 , where N (m) is the number of stars of mass m (Salpeter, 1955). This means that low-mass stars are significantly more numerous than high-mass stars. For example, there are about 225 ...
Astronomy 112: The Physics of Stars Class 9 Notes: Polytropes With
Astronomy 112: The Physics of Stars Class 9 Notes: Polytropes With

Practical Class - Physics and Astronomy
Practical Class - Physics and Astronomy

Quasar feedback revealed by giant molecular outflows
Quasar feedback revealed by giant molecular outflows

... 2004). In addition, both optical and X-ray data have revealed that our line of sight to the active nucleus is heavily obscured, with a measured hydrogen column as high as NH = 2 × 1024 cm−2 (Braito et al. 2004). The quasar Mrk 231 displays clear evidence of powerful ionized outflows by the multiple ...
Neutron Stars – Thermal Emitters
Neutron Stars – Thermal Emitters

スライド 1
スライド 1

... the appearance of peak fluxes at SAMPEX in low Earth orbit . Daily averages of 10–20 MeV electron count rates from SAMPEX 1992 through 2005. A new belt injected during the 29 October 2003 storm appears as a weak enhancement near L = 2 beginning ~ February 2004. Snapshot of the azimuthal component of ...
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Lecture 7 Evolution of Massive Stars on the Main Sequence and

EQUATION OF STATE AND OPACITIES FOR HYDROGEN
EQUATION OF STATE AND OPACITIES FOR HYDROGEN

... According to these studies, an atom moving across the strong magnetic field acquires a constant dipole moment parallel to rc . Those radiative transitions, which were dipole forbidden for an atom at rest because of conservation of the z-projection of the angular momentum, become allowed and should b ...
Hydrogen Peroxide Formation Rates in a PEMFC Anode and Cathode
Hydrogen Peroxide Formation Rates in a PEMFC Anode and Cathode

... Proton exchange membrane fuel cell 共PEMFC兲 technology, owing to its high efficiency, operational flexibility, and superior modularity, has the capability to be the structural and fundamental unit of an impending hydrogen economy. Two main issues that impede its progress toward commercialization are ...
Star Formation and Feedback II: The IMF and the SFR
Star Formation and Feedback II: The IMF and the SFR

... on the correlation. Also note that because we correct for dust temperature when deriving the dust surface density, Σmol should, in principle, also be independent of heating effects. The molecular gas depletion time depends on the scale considered (Figure 2). On the smallest scales considered, r ∼ 12 ...
Cosmology Notes
Cosmology Notes

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High temperature reaction kinetics of CN(v = 0) with C2H4 and
High temperature reaction kinetics of CN(v = 0) with C2H4 and

... from the Maxwell Boltzmann equilibrium for the populations of the v = 0 and v = 1 vibrational levels of OH(X 2 Πi ) radicals were observed in the preflame zone of the methane/oxygen/nitrogen flame by cavity ringdown spectroscopy [12]. More recently, an experimental study employing vacuum ultraviolet ...
Role of column density in the formation of stars
Role of column density in the formation of stars

Non-variable cosmologically distant gamma
Non-variable cosmologically distant gamma

... 10−7 G (so that the initial directions of electrons are not dramatically changed), the resulting gamma-ray synchrotron sources can be quite compact with an angular size as small as 0.1◦ . For cosmologically distant sources embedded in denser (nph ∝ (1 + z)3 ) and more energetic (T ∝ 1 + z) CMBR, pro ...
Introduction to High Energy Density Physics
Introduction to High Energy Density Physics

HEA_Pulsars
HEA_Pulsars

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Microplasma



Microplasmas are plasmas of small dimensions, ranging from tens to thousands of micrometers. They can be generated at a variety of temperatures and pressures, existing as either thermal or non-thermal plasmas. Non-thermal microplasmas that can maintain their state at standard temperatures and pressures are readily available and accessible to scientists as they can be easily sustained and manipulated under standard conditions. Therefore, they can be employed for commercial, industrial, and medical applications, giving rise to the evolving field of microplasmas.
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