Results 131 to 140 of about 72,728 (314)
On the influence of magnetic topology on the propagation of internal gravity waves in the solar atmosphere. [PDF]
Philos Trans A Math Phys Eng Sci, 2021 Vigeesh G, Roth M, Steiner O, Fleck B.
europepmc +1 more source
A Functional 2D Carbon Allotrope Combining Nanoporous Graphene and Biphenylene Segments
Advanced Materials, EarlyView.The synthesis of a novel nanoporous graphene (NPG) is reported with biphenylene segments via thermal fusion of 12‐armchair porous graphene nanoribbons grown on gold surfaces. Characterization using STM, AFM, and DFT reveals low‐defect semiconducting behaviour and tunable band gaps.
Paula Angulo‐Portugal +14 more
wiley +1 more source
Геофизический журнал, 2010 Review of results has been given, which approve the hypothesis that solar cosmic rays (SCR) apparently play an important role in ionization of middle and lower atmosphere and may serve as a physical intermediary in solar-terrestrial climatic ...
L. V. Raichenko
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Solar Surface and Atmospheric Dynamics [PDF]
Space Science Reviews, 2013 ISSI Workshop Microphysics of Cosmic ...
openaire +2 more sources
Opportunities of Semiconducting Oxide Nanostructures as Advanced Luminescent Materials in Photonics
Advanced Materials, EarlyView.The review discusses the challenges of wide and ultrawide bandgap semiconducting oxides as a suitable material platform for photonics. They offer great versatility in terms of tuning microstructure, native defects, doping, anisotropy, and micro‐ and nano‐structuring. The review focuses on their light emission, light‐confinement in optical cavities, and
Ana Cremades +7 more
wiley +1 more source
The Carrying Capacity of the Solar Wind: Applications to Ion Escape
The Astrophysical JournalWe present a physically motivated analytic framework for estimating solar wind mass-loading rates from ion sources using a simplified “particles in a box” (PIB) model.
P. C. Hinton +6 more
doaj +1 more source
Living Reviews in Solar Physics, 2014 The infrared solar spectrum contains a wealth of physical data about our Sun, and is explored using modern detectors and technology with new ground-based solar telescopes.
Matthew J. Penn
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Atmospheric attenuation of solar radiation [PDF]
, 1977 The attenuation of solar radiation by the atmosphere between the heliostat and receiver of a Central Receiver solar energy system has been computed for a number of atmospheric conditions and tower-heliostat distances. The most important atmospheric variable is found to be the atmospheric aerosol content.
openaire +4 more sources
Advanced Materials, EarlyView.In this work, low bandgap (≈1.55 eV) semitransparent perovskite solar cells (ST‐PSCs) having thin (thickness < ≈100 nm) perovskite layers and transparent conductive oxide‐based rear electrodes are fabricated using vacuum‐deposition methods. Two different ST‐PSCs demonstrated a high light utilization efficiency value of 4.2 (PCE: 9.26% and AVT: 45.3 ...
Abhyuday Paliwal +9 more
wiley +1 more source
Replacement and late formation of atmospheric N2 on undifferentiated Titan by impacts
, 2011 Saturn’s moon, Titan, has remarkable surface features—a massive N2 atmosphere and hydrological cycle of CH4—that are often compared with that of Earth^1^. However, the origin and evolution of Titan’s atmosphere remains largely
Toshihiko Kadono +4 more
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