Investigation of mass flows in the transition region and corona in a
... In these models, coronal heating comes from the Joule dissipation of currents produced by the braiding of the magnetic field through photospheric plasma motions; however, details on the origin of the redshifts have not been identified so far. Spadaro et al. (2006) used one-dimensional coronal loop m ...
... In these models, coronal heating comes from the Joule dissipation of currents produced by the braiding of the magnetic field through photospheric plasma motions; however, details on the origin of the redshifts have not been identified so far. Spadaro et al. (2006) used one-dimensional coronal loop m ...
Stability of Organic Cations in Solution
... sublimation temperatures are higher with respect to those characteristic of thin films, due to the much lower surface-tovolume ratio,30 this result fully supports our conclusion about the presence of excess molecular species within the perovskite matrix in the as-received samples. Such extra species ...
... sublimation temperatures are higher with respect to those characteristic of thin films, due to the much lower surface-tovolume ratio,30 this result fully supports our conclusion about the presence of excess molecular species within the perovskite matrix in the as-received samples. Such extra species ...
Chapter 5 Stellar Energy Production
... We have written the CNO sequence as if the (p, γ ) reaction on 12 C were the first step, but it is a closed cycle and we may consider any step to be the initial one. • This implies that any of the carbon, nitrogen, or oxygen isotopes appearing in the cycle may be viewed as a catalyst that serves to ...
... We have written the CNO sequence as if the (p, γ ) reaction on 12 C were the first step, but it is a closed cycle and we may consider any step to be the initial one. • This implies that any of the carbon, nitrogen, or oxygen isotopes appearing in the cycle may be viewed as a catalyst that serves to ...
Pulsed laser deposition of a dense and uniform Au nanoparticles
... trapping in the active layer without increasing its thickness that would inevitably affect the device resistance[ 3]. Particularly suitable for these applications is Au, most likely because the surface plasmon resonance (SPR) can be tuned from the visible (λ ≥ 500nm) to the near IR range by changing ...
... trapping in the active layer without increasing its thickness that would inevitably affect the device resistance[ 3]. Particularly suitable for these applications is Au, most likely because the surface plasmon resonance (SPR) can be tuned from the visible (λ ≥ 500nm) to the near IR range by changing ...
Cosmic Rays 3 - zainab
... of an extensive air shower: one can look for the particles in the pancake directly, or one can look for the Cherenkov light generated by the particles in the atmosphere. The figure below illustrates both techniques. • On the left is an air Cherenkov telescope (ACT). These are large mirrors that focu ...
... of an extensive air shower: one can look for the particles in the pancake directly, or one can look for the Cherenkov light generated by the particles in the atmosphere. The figure below illustrates both techniques. • On the left is an air Cherenkov telescope (ACT). These are large mirrors that focu ...
Low-temperature surface formation of NH3 and HNCO
... phase yet, but its direct derivative, the cyanate ion (OCN− ), has been found in interstellar ices with abundances between 0.3 and 0.6 per cent with respect to water ice. The assignment of solid OCN− is often attributed to either the entire, so-called, XCN band or to a single component (2165 cm−1 ) ...
... phase yet, but its direct derivative, the cyanate ion (OCN− ), has been found in interstellar ices with abundances between 0.3 and 0.6 per cent with respect to water ice. The assignment of solid OCN− is often attributed to either the entire, so-called, XCN band or to a single component (2165 cm−1 ) ...
Low-temperature surface formation of NH3 and HNCO
... phase yet, but its direct derivative, the cyanate ion (OCN− ), has been found in interstellar ices with abundances between 0.3 and 0.6 per cent with respect to water ice. The assignment of solid OCN− is often attributed to either the entire, so-called, XCN band or to a single component (2165 cm−1 ) ...
... phase yet, but its direct derivative, the cyanate ion (OCN− ), has been found in interstellar ices with abundances between 0.3 and 0.6 per cent with respect to water ice. The assignment of solid OCN− is often attributed to either the entire, so-called, XCN band or to a single component (2165 cm−1 ) ...
The First Stars in the Universe - Scientific American
... bang, some bright galaxies and quasars had already appeared, so the first stars must have formed sometime before. When did these first luminous objects arise, and how might they have formed? Many astrophysicists, including Martin Rees of the University of Cambridge and Abraham Loeb of Harvard Univer ...
... bang, some bright galaxies and quasars had already appeared, so the first stars must have formed sometime before. When did these first luminous objects arise, and how might they have formed? Many astrophysicists, including Martin Rees of the University of Cambridge and Abraham Loeb of Harvard Univer ...
Fast Quantum Gates for Neutral Atoms V 85, N 10
... while the atom is in jr典, and thus excites the atomic motion. We treat the deviation of the potential in the excited state from the ground state trapping potential as a perturbation and estimate the probability pt of exciting an atom from the vibrational ground state during the gate operation. We fi ...
... while the atom is in jr典, and thus excites the atomic motion. We treat the deviation of the potential in the excited state from the ground state trapping potential as a perturbation and estimate the probability pt of exciting an atom from the vibrational ground state during the gate operation. We fi ...
© Taganov I
... out of the protogalaxy core formed in the plasma epoch after fragmentation at recombination at planet (PFP) and protoglobularstarcluster (PGC) masses and freezing to solid H-He dark objects as the expanding universe cooled, Fig. 1e. We see from Tadpole that stars form from planets in dense clumps of ...
... out of the protogalaxy core formed in the plasma epoch after fragmentation at recombination at planet (PFP) and protoglobularstarcluster (PGC) masses and freezing to solid H-He dark objects as the expanding universe cooled, Fig. 1e. We see from Tadpole that stars form from planets in dense clumps of ...
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.