Geomagnetic disturbances due to solar and interplanetary sources
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- Englisch ausgewählt
59,99 €
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71,90 €
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Beschreibung
Produktdetails
Einband
Taschenbuch
Erscheinungsdatum
07.07.2020
Verlag
LAP LAMBERT Academic PublishingSeitenzahl
184
Maße (L/B/H)
22/15/1,2 cm
Gewicht
292 g
Sprache
Englisch
ISBN
978-620-2-67617-5
The Sun is the most prominent feature in our solar system. It is the largest object and contains approximately 98% of the total solar system mass. One hundred and nine Earths would be required to fit across the Sun's disk, and its interior could hold over 1.3 million Earths. The Sun's outer visible layer is called the photo-sphere and has a temperature of 6,000°C (11,000°F). This layer has a mottled appearance due to the turbulent eruptions of energy at the surface. Solar energy is created deep within the core of the Sun. It is here that the temperature (15,000,000° C; 27,000,000° F) and pressure (340 billion times Earth's air pressure at sea level) is so intense that nuclear reactions take place. This reaction causes four protons or hydrogen nuclei to fuse together to form one alpha particle or helium nucleus. The alpha particle is about 0.7 percent less massive than the four protons. The difference in mass is expelled as energy and is carried to the surface of the Sun, through a process known as convection, where it is released as light and heat. Energy generated in the Sun's core takes a million years to reach its surface.
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