ANALISIS EVOLUSI KELOMPOK BINTIK MATAHARI DAN PROBABILITAS LEDAKAN MATAHARI KELAS X BERDASARKAN NILAI FRAKTAL KELOMPOK BINTIK MATAHARI AR12192 DAN AR12209

Solar energetic activity, such as solar flare, was produced by the magnetic field on individual sunspots or sunspot groups. The magnetic field on the sunspots is implied from the total area of the spots. Additionally, magnetism can be analyzed using fractal dimension (FD). The evolution of the s...

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Bibliographic Details
Main Author: Ersasiwi Aziza, Shafira
Format: Final Project
Language:Indonesia
Online Access:https://digilib.itb.ac.id/gdl/view/57572
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Institution: Institut Teknologi Bandung
Language: Indonesia