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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| 格式: | Final Project |
| 語言: | Indonesia |
| 在線閱讀: | https://digilib.itb.ac.id/gdl/view/57572 |
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