Results 241 to 250 of about 353,818 (294)

Unraveling bulk degradation mechanisms of wide-bandgap perovskite absorbers for tandem applications.

EES Solar
Ongaro C, Othman M, Ballif C, Wolff CM, Hessler-Wyser A.   +4 more
europepmc   +1 more source

Spatial and temporal patterns of vegetation carbon sources/sinks and driving factors in southeastern Xizang from 2000 to 2020. [PDF]

PeerJ
Han J, Meng X, Lin L, Lu J.
europepmc   +1 more source

Thermotropic liquid-assisted interface management enables efficient and stable perovskite solar cells and modules. [PDF]

Nat Commun
Chang Q, Chen R, Yang Y, Huang H, Han X, Huang X, Dai Z, Wu B, Yin J, Li J, Zheng N.   +10 more
europepmc   +1 more source

Multi-stage power-to-water battery synergizes flexible energy storage and efficient atmospheric water harvesting. [PDF]

Nat Commun
Lin H, Song Y, Ding Z, Sui Y, Sui Z, Li F, Zhu J, Wu W.   +7 more
europepmc   +1 more source

Unraveling high-efficiency lead-free perovskite solar cells using a CsSnGeI₃/CsGeI₃ dual absorber and a Cu₂O HTL. [PDF]

Sci Rep
Rahman MF, Rahman M, Hossain MF, Islam MR, Islam S, Ria DD, Benami A, Irfan A, Badi N.   +8 more
europepmc   +1 more source

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Infrared Photometry of Solar Active Regions

International Astronomical Union Colloquium, 2000
AbstractSimultaneous time series of broad-band images of two active regions close to the disk center were acquired at the maximum (0.80μm) and minimum (1.55μm) continuum opacities. Dark faculae are detected in images obtained as weighted intensity differences between both wavelength bands. The elements of quiet regions can be clearly distinguished from
M. Sobotka, M. Vázquez, M. Sánchez Cuberes, J. A. Bonet, A. Hanslmeier   +4 more
openaire   +1 more source

Active Region Evolution and Solar Flux Variations

Solar Physics, 1994
The goal of this study is to relate the changes in the solar radiative output to the growth and decay of magnetic active regions. We will test the assumption that each index of radiation variability is a convolution of an active-region magnetic driving function and a response function.
T. P. Hartsell, P. L. Bornmann
openaire   +1 more source

Abundance determination in solar active region

Advances in Space Research, 1994
An improved method has been developed to evaluate element abundances from emission line intensities of thin plasmas, depending on the differential emission measure (DEM) of the source. Observations made by the Solar EUV Rocket Telescope and Spectrograph (SERTS) Rocket EUV Spectrograph are used to perform a detailed analysis of the DEM distribution for ...
B.C.Monsignori Fossi, M. Landini, R.J. Thomas, W.M. Neupert   +3 more
openaire   +1 more source