Results 11 to 20 of about 3,067,597 (310)
The infrared solar spectrum contains a wealth of physical data about our Sun, and is explored using modern detectors and technology with new ground-based solar telescopes. The scientific motivation behind exploring these wavelengths is presented, along with a brief look at the rich history of observations here. Several avenues of solar physics research
Penn MJ.
europepmc +8 more sources
ADVANCEMENTS IN SOLAR NEUTRINO PHYSICS [PDF]
We review the results of solar neutrino physics, with particular attention to the data obtained and the analyses performed in the last decades, which were determinant to solve the solar neutrino problem (SNP), proving that neutrinos are massive and oscillating particles and contributing to refine the solar models.
Antonelli, Vito, Miramonti, Lino
openaire +3 more sources
Combining Empirical and Physics-Based Models for Solar Wind Prediction
Solar wind modeling is classified into two main types: empirical models and physics-based models, each designed to forecast solar wind properties in various regions of the heliosphere.
Rob Johnson +3 more
doaj +3 more sources
Review and comparison of MHD wave characteristics at the Sun and in Earth’s magnetosphere
Magnetohydrodynamic (MHD) waves play a crucial role in the plasma processes of stellar atmospheres and planetary magnetospheres. Wave phenomena in both media are known to have similarities and unique traits typical of each system.
Chelpanov M. A. +6 more
doaj +1 more source
Multiwave Siberian Radioheliograph
The article discusses characteristics, fundamental and applied tasks of the Siberian Radioheliograph that is developed at the ISTP SB RAS Radio Astrophysical Observatory and spectropolarimetric complex that measures the total flux of solar radio emission.
Altyntsev A.T. +13 more
doaj +1 more source
Solar neutrinos: Solar physics and neutrino physics [PDF]
Abstract It is shown that the current solar neutrino situation, with results from the Homestake experiment, the Kamiokande experiment, GALLEX and SAGE is unfortunately still ambiguous. The differences between observations and the standard solar theory may still be due to either astrophysical inputs or new neutrino physics.
D.N. Schramm, X. Shi
openaire +1 more source
Turbulent parameters at different heights in the atmosphere. Shack–Hartmann wavefront sensor data
The paper presents the results of studies of wavefront distortions at different heights in the atmosphere. We have used measurement wavefront data to determine optical turbulence parameters along the line of sight of the Large Solar Vacuum Telescope ...
Shikhovtsev A. Y. +5 more
doaj +1 more source
Under the project National Heliogeophysical Complex of the Russian Academy of Sciences, it is planned to create several coherent decameter radars. ISTP SB RAS developed a network of coherent decameter radars well before the start of financing this ...
Berngardt O.I +6 more
doaj +1 more source
Improved equivalent circuit and analytical model for amorphous silicon solar cells and modules [PDF]
An improved equivalent circuit for hydrogenated amorphous silicon (a-Si:H) solar cells and modules is presented. It is based on the classic combination of a diode with an exponential current-voltage characteristic, of a photocurrent source plus a new ...
Platz, R. +10 more
core +2 more sources
Siberian Radioheliograph: first results
Regular observations of active processes in the solar atmosphere have been started using the first stage of the multiwave Siberian Radioheliograph (SRH), a T-shaped 48-antenna array with a 4–8 GHz operating frequency range and a 10 MHz instantaneous ...
Lesovoi S.V. +11 more
doaj +1 more source

