Origins of Very Low Helium Abundance Streams Detected in the Solar Wind Plasma
The abundance of helium ( A _He ) in the solar wind exhibits variations typically in the range from 2% to 5% with respect to solar cycle activity and solar wind velocity. However, there are instances where the observed A _He is exceptionally low (<1%). These low- A _He occurrences are detected bo...
| Main Authors: | , , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
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| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad84d6 |