Langmuir-wave Excitation in Solar Wind Magnetic Holes
Magnetic holes (MHs) are structures commonly observed in various space plasma environments throughout the solar system, including the solar wind. These structures are characterized by a localized decrease in magnetic field strength, coincident with an increase in plasma density. Previous observation...
محفوظ في:
| المؤلفون الرئيسيون: | , , , , , , , , , , |
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| التنسيق: | Artigo |
| اللغة: | Inglês |
| منشور في: |
IOP Publishing
2025-01-01
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| سلاسل: | The Astrophysical Journal Letters |
| الموضوعات: | |
| الوصول للمادة أونلاين: | https://doi.org/10.3847/2041-8213/adea4f |
| الوسوم: |
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