JOVIAN AND EXOPLANET AURORAL RADIO EMISSION PROFILE IN THE LOW-FREQUENCY RANGE
Earth and giant planets in our Solar System are known to possess an internal magnetic eld and a thick atmosphere that are capable of producing non- thermal low-frequency radio emissions through the Cyclotron Maser Instabili- ty (CMI) mechanism. Particularly for Jupiter, interactions with its sate...
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| Format: | Final Project |
| Language: | Indonesia |
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| Online Access: | https://digilib.itb.ac.id/gdl/view/60917 |
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| Institution: | Institut Teknologi Bandung |
| Language: | Indonesia |