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Disturbi geomagnetici dovuti a fonti solari e interplanetarie

Disturbi geomagnetici dovuti a fonti solari e interplanetarie

          
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About the Book

Il Sole è la caratteristica più importante del nostro sistema solare. È l'oggetto più grande e contiene circa il 98% della massa totale del sistema solare. Sarebbero necessarie cento nove Terre per passare attraverso il disco del Sole, e il suo interno potrebbe contenere più di 1,3 milioni di Terre. Lo strato visibile esterno del Sole è chiamato fotosfera e ha una temperatura di 6.000°C (11.000°F). Questo strato ha un aspetto screziato a causa delle turbolente eruzioni di energia in superficie. L'energia solare si crea in profondità nel nucleo del Sole. È qui che la temperatura (15.000.000.000° C; 27.000.000° F) e la pressione (340 miliardi di volte la pressione dell'aria terrestre a livello del mare) sono così intense che si verificano reazioni nucleari. Questa reazione fa sì che quattro protoni o nuclei di idrogeno si fondano insieme per formare una particella alfa o un nucleo di elio. La particella alfa è circa lo 0,7 per cento meno massiccia dei quattro protoni. La differenza di massa viene espulsa sotto forma di energia e viene trasportata alla superficie del Sole, attraverso un processo noto come convezione, dove viene rilasciata sotto forma di luce e calore. L'energia generata nel nucleo del Sole impiega un milione di anni per raggiungere la sua superficie.


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Product Details
  • ISBN-13: 9786202623469
  • Publisher: KS Omniscriptum Publishing
  • Publisher Imprint: Sciencia Scripts
  • Height: 229 mm
  • No of Pages: 192
  • Spine Width: 11 mm
  • Width: 152 mm
  • ISBN-10: 6202623462
  • Publisher Date: 24 Feb 2021
  • Binding: Paperback
  • Language: Italian
  • Returnable: N
  • Weight: 290 gr

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