Results 251 to 260 of about 1,071,863 (291)
A deep learning framework for instrument-to-instrument translation of solar observation data. [PDF]
Nat CommunJarolim R +3 more
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Hybrid solar photovoltaic conversion and water desalination via quad-band fano-resonant optical coatings and superwicking cooling. [PDF]
Light Sci ApplWei R, Xu T, Ma M, Elkabbash M, Guo C.
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Electrostatic solitary wave modeling in lunar wake plasma. [PDF]
Sci RepSingh K, Varghese SS, Kourakis I.
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Highly Active Oxygen Evolution Integrating with Highly Selective CO<sub>2</sub>-to-CO Reduction. [PDF]
Nanomicro LettWang C, Geng L, Bi Y.
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Solar Physics, 1985
The future of solar physics is founded on the existing fundamental unsolved problems in stellar physics. Thus, for instance, the physics of stellar interiors has been called into serious question by the very low-measured neutrino flux. The 71Ga neutrino detection experiment is the next step in unravelling this mystery.
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The future of solar physics is founded on the existing fundamental unsolved problems in stellar physics. Thus, for instance, the physics of stellar interiors has been called into serious question by the very low-measured neutrino flux. The 71Ga neutrino detection experiment is the next step in unravelling this mystery.
openaire +2 more sources
Solar oscillations and the physics of the solar interior
2008The variety and precision of the observed frequencies of solar oscillations allow a detailed investigation of the foundations of computations of stellar models. This is of obvious importance to our understanding of the structure of other stars of moderate mass.
Jørgen Christensen-Dalsgaard +1 more
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2020
Solar physics is one of the liveliest branches of astrophysics at the current time, with many major advances that have been stimulated by observations from a series of space satellites and ground-based telescopes as well as theoretical models and sophisticated computational experiments.
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Solar physics is one of the liveliest branches of astrophysics at the current time, with many major advances that have been stimulated by observations from a series of space satellites and ground-based telescopes as well as theoretical models and sophisticated computational experiments.
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A Discussion on the physics of the solar atmosphere - Physics of the solar atmosphere
Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1976A summary is given on recent results on the physics of the quiet solar atmosphere, and active regions. This includes: solar rotation, velocity fields and waves, magnetic field concentration, the transition region, coronal magnetic field structure, and prominences.
H. Rosenberg +3 more
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Solar physics with LOFAR [PDF]
2014 XXXIth URSI General Assembly and Scientific Symposium (URSI GASS), 2014 LOFAR is a novel radio telescope for the frequency range of 10–250 MHz. It consists of antenna fields that are arranged as a dense core near Exloo and remote stations all over the Netherlands, and international stations that span baselines up to 1000 km across Europe.
Frank Breitling, G. Mann, C. Vocks
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Physics of the Solar Corona [PDF]
, 1964 Abstract : Progress for the year included uncompleted analysis of 1966 eclipse plates for evidence of a difference in the chemical content of coronal condensations from that in the corona in general, continued work toward interpretation of the gradient of the emission-line features in the corona, the discovery of a linear relationship between flare ...
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