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Solar X-ray Emission and Metre-Wave Radio Bursts

Publications of the Astronomical Society of Australia, 1977
Soft X-ray photographs of the Sun taken from the manned Skylab satellite (Vaiana et al. 1973) gave, not the earliest, but perhaps the most graphic evidence that the solar corona is patchy. During the Skylab mission (May 1973 to February 1974), the solar corona as usually envisaged covered only 80% of the Sun (Bohlin 1977).
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Hard X-Ray Emission in Solar Flares

2021
Michele Piana   +3 more
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Intermediate‐term epochs in solar soft X ray emission

Journal of Geophysical Research: Space Physics, 1983
Observations of the daily 1‐ to 8‐Å solar X ray emission from 1977 to 1981 are analyzed from a terrestrial viewpoint. A high‐resolution method of anharmonic frequency analysis is used to search for discrete frequencies in a finite time series and estimate the frequency, phase, and amplitude of each periodic component.
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Radio and X-Ray Emission Associated with Solar Flares

1965
The observed emission of solar radio waves, X-rays, and energetic particles indicate that processes involving great energies may develop in certain parts of the sun which we identify as the corona. Although radio quanta from the sun have small energies, the circumstances under which they are emitted indicate that they are produced by processes ...
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Molecular engineering of contact interfaces for high-performance perovskite solar cells

Nature Reviews Materials, 2022
Furkan H Isikgor   +2 more
exaly  

Stability challenges for the commercialization of perovskite–silicon tandem solar cells

Nature Reviews Materials, 2023
Leiping Duan, Kylie R Catchpole
exaly  

Minimizing non-radiative recombination losses in perovskite solar cells

Nature Reviews Materials, 2019
Deying Luo, Rui Su, Wei Zhang
exaly  

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