Results 81 to 90 of about 6,299 (262)

The abundances of heavy elements in the atmosphere of hyades giant 6 Tauri

open access: yesOdessa Astronomical Publications, 2017
Comparison of synthetic spectrum of the б Tauri photosphere and high quality spectral atlas of this star permit us to identify absorption lines of iron and heavy elements Z ≥ 30 in the observed spectrum.
V. F. Gopka
doaj   +1 more source

Functional Metal Complexes for Solar–Light‐Driven Energy Conversion

open access: yesAdvanced Materials, EarlyView.
This review provides an exhaustive summary of the recent advancements of functional metal complexes in solar‐to‐electrical, ‐chemical, and ‐thermal energy conversion, comprising material categories, design strategies, underlying principles of operation, and identified improvement of performances.
Yanyan Qin   +3 more
wiley   +1 more source

Element Abundances of Solar Energetic Particles and the Photosphere, the Corona, and the Solar Wind

open access: yesAtoms, 2019
From a turbulent history, the study of the abundances of elements in solar energetic particles (SEPs) has grown into an extensive field that probes the solar corona and physical processes of SEP acceleration and transport.
Donald V. Reames
doaj   +1 more source

Solar model with CNO revised abundances

open access: yes, 2004
Recent three-dimensional, NLTE analyses of the solar spectrum have shown a significant reduction in the C, N, O and Ne abundances leading to a Z/X ratio of the order of 0.0177. We have computed solar models with this new mixture in the OPAL opacity tables. The present He abundance we find seems rather consistent with the helioseismic value.
Montalbán, J.   +4 more
openaire   +4 more sources

Solar Abundances: The Reference System [PDF]

open access: yesSymposium - International Astronomical Union, 1991
We summarize the recent critical compilation and analysis of the solar and meteoritic abundances by Anders and Grevesse (1989). We also update a few solar photospheric results and present a detailed discussion of the problem of the solar abundance of iron.
openaire   +1 more source

De Rerum Natura: How Do Halide Perovskites Self‐Heal From Damage?

open access: yesAdvanced Materials, EarlyView.
How can lead‐halide‐perovskites self‐heal after damage from light, heat, mechanical strain, or radiation? We show that reversible chemical defects underly performance losses and recovery, highlighting the roles of halide and proton migration, redox‐driven reactions, and acid‐base equilibria.
Davide Raffaele Ceratti   +2 more
wiley   +1 more source

Elemental Abundances at Coronal Hole Boundaries as a Means to Investigate Interchange Reconnection and the Solar Wind

open access: yesThe Astrophysical Journal
The origin of the slow solar wind is not well understood, unlike the fast solar wind that originates from coronal holes. In situ elemental abundances of the slow solar wind suggest that it originates from initially closed field lines that become open ...
Alexandros Koukras   +2 more
doaj   +1 more source

A Politics of Solar Abundance

open access: yes, 2023
The abolition of fossil fuels requires more than new fuels to power modern pleasures. It also requires new subjectivities. Petro-people need to become solar subjects. Becoming solar subjects, and not just consumers of solar energy, means nurturing solarity as a way of life, a geo-theology.
openaire   +1 more source

Single‐Atom Photocatalyst as Floatable Artificial Leaf for Upcycling Oceanic Plastic Waste

open access: yesAdvanced Materials, EarlyView.
To resolve the catastrophic disaster of oceanic plastic pollution, the novel Ru single atom loaded ZnIn2S4 photocatalysts, in the forms of powder or floatable artificial leaf, were prepared for direct conversion of raw polypropylene plastic into valuable chemicals. The optimized catalyst exhibits exceptional performance, with a total formic/acetic acid
Amin Talebian‐Kiakalaieh   +6 more
wiley   +1 more source

Solar abundances as derived from solar energetic particles [PDF]

open access: yesAIP Conference Proceedings, 1989
Recent studies have shown that there are well defined average abundances of heavy (Z≳2) solar energetic particles (SEPs), with variations in the acceleration and propagation producing a systematic flareâ€toâ€flare fractionation that depends on the charge per unit mass of the ion. Correcting the average SEP abundances for the fractionation yields SEPâ€
openaire   +2 more sources

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