Results 191 to 200 of about 2,412 (205)

Electron-Phonon Interactions Facilitating Large Polaron-Related Charge-Carrier Dynamics for Efficient Perovskite Nanocrystal Solar Cells. [PDF]

Adv Sci (Weinh)
Guo W, Dai J, He S, Yang L, He Y, Duan J, Cen H, Yang X, Yuan F, Li J, Wu Z, Manna L, Xi J.   +12 more
europepmc   +1 more source

Occupational exposure to solar ultraviolet radiation among outdoor workers in Lisbon, 2023-first results of the MEAOW study. [PDF]

Front Public Health
Carvalho F, Strehl C, Barroso-Dias J, Castela MM, Gobba F, Lapão LV, Loney T, Maia MR, Modenese A, John SM, Rodrigues A, Pinho C, Bieck C, Tenkate T, Westerhausen S, Wittlich M, Paulo MS.   +16 more
europepmc   +1 more source

Regulating intermolecular interaction of passivators for controllable surface energetics of photovoltaic perovskites. [PDF]

Sci Adv
Jiang X, Xiao Q, Cheng Z, Tian Y, Wang X, Shen J, Deger C, Yavuz I, Zhou J, Li Q, Fan W, Zhang S, Zhang Y, Faheem MB, Qiao Q, Zhang Z, Guo T, Xu X, Lei B, Wang Y, Di D, Xue J, Bi E, Wang R.   +23 more
europepmc   +1 more source

Electrical Properties of ZnO Nanoparticle-Embedded/Polyethylenimine-Functionalized Nitrogen-Doped Graphene Quantum Dot Nanocomposites. [PDF]

ACS Omega
Yıldız İ.
europepmc   +1 more source

Gallium Nitride for Space Photovoltaics: Properties, Synthesis Methods, Device Architectures and Emerging Market Perspectives. [PDF]

Micromachines (Basel)
Drabczyk A, Uss P, Bucka K, Bulowski W, Kasza P, Mazur P, Boguta E, Mazur M, Putynkowski G, Socha RP.   +9 more
europepmc   +1 more source

Extreme Ultraviolet Solar Emission Lines and the Transition Layer between the Chromosphere and the Corona

Extreme Ultraviolet Solar Emission Lines and the Transition Layer between the Chromosphere and the Corona
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Relationship of the nightglow 630.0nm emission intensity to the solar extreme ultraviolet

Journal of Atmospheric and Solar-Terrestrial Physics, 2013
Abstract It is well known that the 630.0 nm nightglow emission intensity at mid latitudes increased more than twofold in periods of maximum sunspot activity. It is assumed that this phenomenon is caused by variations in solar ultraviolet radiation intensity in solar activity cycles ( Fishkova, 1983 ).
I.B. Ievenko, V.N. Alexeyev, S.G. Parnikov   +2 more
exaly   +2 more sources

On the Failure of Standard Emission Measure Analysis for Solar Extreme-Ultraviolet and Ultraviolet Irradiance Spectra

Astrophysical Journal, 1995
We perform emission measure analysis of new and accurate UV (λ > 1200 A) and extreme-ultraviolet (EUV) (λ ≤ 1200 A) irradiance ("Sun-as-a-star") emission-line spectra of the Sun. Our data consist of (1) daily averaged UV irradiances from the SOLSTICE on the UARS spacecraft and (2) EUV irradiances obtained on the same date from a m spectrograph flown on
Thomas N Woods, P Brekke
exaly   +2 more sources

Solar extreme ultraviolet irradiance: Present, past, and future

Journal of Geophysical Research, 2011
J L Lean, Thomas N Woods, Francis G Eparvier   +2 more
exaly  

Solar Observations of High‐Temperature Emission with the Extreme‐Ultraviolet Imaging Spectrometer onHinode

Astrophysical Journal, 2008
Harry P Warren, C M Brown
exaly