Analysis of information sources in references of the Wikipedia article "Маса Сонця" in Ukrainian language version.
The fusion cycle that generates energy into the Sun relies on the conversion of hydrogen into helium, which is responsible for a solar mass reduction with a rate of ~−0.67×10−13 per year. On the other hand, the solar wind contribution is more uncertain. The solar cycle significantly influences the solar mass loss rate due to solar wind. Estimates of the mass carried away with the solar wind showed rates between −(2–3)×10−14M☉ per year, whereas numerical simulations of coupled corona and solar wind models provided rates between −(4.2–6.9)×10−14M☉ per year.
The fusion cycle that generates energy into the Sun relies on the conversion of hydrogen into helium, which is responsible for a solar mass reduction with a rate of ~−0.67×10−13 per year. On the other hand, the solar wind contribution is more uncertain. The solar cycle significantly influences the solar mass loss rate due to solar wind. Estimates of the mass carried away with the solar wind showed rates between −(2–3)×10−14M☉ per year, whereas numerical simulations of coupled corona and solar wind models provided rates between −(4.2–6.9)×10−14M☉ per year.
The fusion cycle that generates energy into the Sun relies on the conversion of hydrogen into helium, which is responsible for a solar mass reduction with a rate of ~−0.67×10−13 per year. On the other hand, the solar wind contribution is more uncertain. The solar cycle significantly influences the solar mass loss rate due to solar wind. Estimates of the mass carried away with the solar wind showed rates between −(2–3)×10−14M☉ per year, whereas numerical simulations of coupled corona and solar wind models provided rates between −(4.2–6.9)×10−14M☉ per year.
The fusion cycle that generates energy into the Sun relies on the conversion of hydrogen into helium, which is responsible for a solar mass reduction with a rate of ~−0.67×10−13 per year. On the other hand, the solar wind contribution is more uncertain. The solar cycle significantly influences the solar mass loss rate due to solar wind. Estimates of the mass carried away with the solar wind showed rates between −(2–3)×10−14M☉ per year, whereas numerical simulations of coupled corona and solar wind models provided rates between −(4.2–6.9)×10−14M☉ per year.
The fusion cycle that generates energy into the Sun relies on the conversion of hydrogen into helium, which is responsible for a solar mass reduction with a rate of ~−0.67×10−13 per year. On the other hand, the solar wind contribution is more uncertain. The solar cycle significantly influences the solar mass loss rate due to solar wind. Estimates of the mass carried away with the solar wind showed rates between −(2–3)×10−14M☉ per year, whereas numerical simulations of coupled corona and solar wind models provided rates between −(4.2–6.9)×10−14M☉ per year.
