Temporal Variation of Solar Equatorial Rossby Modes with Azimuthal Orders $6\leq m \leq 10$
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| Autores principales: | , , , , |
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| Formato: | Preprint |
| Publicado: |
2024
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| _version_ | 1866910323040059392 |
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| author | Lekshmi, B. Gizon, Laurent Jain, Kiran Liang, Zhi-Chao Philidet, Jordan |
| author_facet | Lekshmi, B. Gizon, Laurent Jain, Kiran Liang, Zhi-Chao Philidet, Jordan |
| contents | We use nearly two decades of helioseismic data obtained from the GONG (2002-2020) and HMI (2010-2020) ring-diagram pipelines to examine the temporal variations of the properties of individual equatorial Rossby modes with azimuthal orders in the range $6 \le m \le 10$. We find that the mode parameters obtained from GONG and HMI are consistent during the data overlapping period of 2010-2020. The power and the frequency of each mode exhibit significant temporal variations over the full observing period. Using the GONG data during solar cycles 23 and 24, we find that the mode power averaged over $6 \le m \le 10$ shows a positive correlation with the sunspot number ($0.42$), while the averaged frequency shift is anti-correlated ($-0.91$). The anti-correlation between the average mode power and frequency shift is $-0.44$. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2402_05781 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Temporal Variation of Solar Equatorial Rossby Modes with Azimuthal Orders $6\leq m \leq 10$ Lekshmi, B. Gizon, Laurent Jain, Kiran Liang, Zhi-Chao Philidet, Jordan Solar and Stellar Astrophysics We use nearly two decades of helioseismic data obtained from the GONG (2002-2020) and HMI (2010-2020) ring-diagram pipelines to examine the temporal variations of the properties of individual equatorial Rossby modes with azimuthal orders in the range $6 \le m \le 10$. We find that the mode parameters obtained from GONG and HMI are consistent during the data overlapping period of 2010-2020. The power and the frequency of each mode exhibit significant temporal variations over the full observing period. Using the GONG data during solar cycles 23 and 24, we find that the mode power averaged over $6 \le m \le 10$ shows a positive correlation with the sunspot number ($0.42$), while the averaged frequency shift is anti-correlated ($-0.91$). The anti-correlation between the average mode power and frequency shift is $-0.44$. |
| title | Temporal Variation of Solar Equatorial Rossby Modes with Azimuthal Orders $6\leq m \leq 10$ |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2402.05781 |