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Observations of ubiquitous compressive waves in the Sun`s
Observations of ubiquitous compressive waves in the Sun`s

... and propagation speed. The observations show that similar structures re-occur in the same regions either continuously or even tens of minutes after previous structures have faded from the field of view (Supplementary Movies S1 and S2), suggesting that the lifetime of the background magnetic field is ...
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Phase behavior of clathrate hydrates: a model for single and

... model uses Eq. (15) to calculate the guest–host interaction energies for the cavity water molecules and water molecules beyond the 9rst shell or cage (Klauda & Sandler, 2002). To include the e)ect of lattice distortion by guests, the water locations for sI guests were obtained from X-ray di)raction ...
The First Galaxies: Assembly under Radiative Feedback from the
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... satisfactory explanation for this phenomenon, but there are some promising models that may account for the observed X-ray emissions. For example, Helling et al. (2011a,b) propose that charge buildup on grains may lead to atmospheric ionization to a degree sufficient to couple the magnetic field to a ...
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Coronene and pyrene (5, 7)-member ring defects: Infrared spectra
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... lines in this area originate from C-H out-of-plane bending motion. It is expected that the undefected molecules show bands near 11.2µm, wherein the peaks of the cations occur at shorter wavelengths, of the anions at longer wavelengths. Our spectra confirm this, even the molecules with defect follow ...
The fuelling of local supermassive black holes
The fuelling of local supermassive black holes

... to see t his picture. are needed to see this picture. ...
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... Many transition metal oxides are active for the ODH but especially vanadium oxide has been investigated due to its high redox activity [2,3,4,5]. It is a heterogeneous catalytic reaction in which the surface of the VOx catalyst reacts with propane to form propene and water. This process follows a re ...
CHEMKIN Tutorials Manual
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... PARAMETER STUDY FACILITY, PARTICLE TRACKING FEATURE, PASR, PLUG, PREMIX, REACTION WORKBENCH, SENKIN, SHOCK, SPIN, SURFACE CHEMKIN, SURFTHERM, TRANSPORT, TWAFER, TWOPNT are all trademarks of Reaction Design or Sandia National Laboratories. All other trademarks are the property of their respective hol ...
The ionized gas in the central region of NGC 5253
The ionized gas in the central region of NGC 5253

... independently modelled for each cube. The spectral regions utilized in the fits were 3650–4060 Å and the whole spectral range for the LR1 and LR2 gratings, respectively. All the main outputs for each spaxel were then reformatted in order to create three cubes per grating with the total, gaseous and ...
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... In all of the nearby galaxies where high resolution observations are possible the molecular gas is largely organized into giant clouds (the so called giant molecular clouds or GMCs) of mass ≈ 104 − 107 M with average densities ∼ 100 H2 molecules per cm3 , separated by a more diffuse intercloud medi ...
An extended X-ray object ejected from the PSR B1259
An extended X-ray object ejected from the PSR B1259

... of the decretion disk heated and expelled from the binary by the interaction with the PW)7 , then its mass would be mcl ∼ 1029 g, much larger than the plausible mass of the disk, mdisk ∼ 1024 − 1026 g (Chernyakova et al. 2014, and references therein), or the mass Ṁ Porb = 6.7 × 1025 (Ṁ /10−8 M /y ...
Acta Polytechnica
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... This is the most energetic event in the Universe since the Big Bang. If two such objects collide with each other, a huge amount of energy may be released and a certain fraction is expected to heat the gas and accelerate particles through shock waves, and induce bulk and turbulent gas motions. Signat ...
The reaction between NH3+ and CH3COOH: a possible process for
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... bicyclopentadiene originating from the Pd precursor. ...
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Vacuum-UV spectroscopy of interstellar ice analogs. I. Absorption
Vacuum-UV spectroscopy of interstellar ice analogs. I. Absorption

... The experiments were performed using the interstellar astrochemistry chamber (ISAC), see Fig. 1. This set-up and the standard experimental protocol were described in Muñoz Caro et al. (2010). ISAC mainly consists of an ultra-high-vacuum (UHV) chamber, with pressure typically in the range P = 34.0 × ...
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Miguel Pereira Santaella

... IR Pumping. HF has a vibrational absorption band at 2.5 μm To be efficient radiation field T > 730 K ...
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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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