Modeling the Center-to-limb Systematic in Normal-mode Coupling Measurements
Solar meridional circulation (MC), which manifests as poleward flow near the surface, is a relatively weak flow. While MC has been measured through various local helioseismic techniques, there is a lack of consensus about the nature of the depth profile and location of return flow, owing to its smal...
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| Main Authors: | Samarth G. Kashyap, Shravan M. Hanasoge |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad9476 |
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