Suppression of the collisionless tearing mode by flow shear: implications for reconnection onset in the Alfvénic solar wind
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| Main Authors: | , , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866911093448769536 |
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| author | Mallet, A. Eriksson, S. Swisdak, M. Juno, J. |
| author_facet | Mallet, A. Eriksson, S. Swisdak, M. Juno, J. |
| contents | We analyse the collisionless tearing mode instability of a current sheet with a strong shear flow across the layer. The growth rate decreases with increasing shear flow, and is completely stabilized as the shear flow becomes Alfvénic. We also show that in the presence of strong flow shear, the tearing mode growth rate decreases with increasing background ion-to-electron temperature ratio, the opposite behaviour to the tearing mode without flow shear. We find that even a relatively small flow shear is enough to dramatically alter the scaling behaviour of the mode, because the growth rate is small compared to the shear flow across the ion scales (but large compared to shear flow across the electron scales). Our results may explain the relative absence of reconnection events in the near-Sun Alfvénic solar wind observed recently by NASA's Parker Solar Probe. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2412_01796 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Suppression of the collisionless tearing mode by flow shear: implications for reconnection onset in the Alfvénic solar wind Mallet, A. Eriksson, S. Swisdak, M. Juno, J. Space Physics Solar and Stellar Astrophysics Plasma Physics We analyse the collisionless tearing mode instability of a current sheet with a strong shear flow across the layer. The growth rate decreases with increasing shear flow, and is completely stabilized as the shear flow becomes Alfvénic. We also show that in the presence of strong flow shear, the tearing mode growth rate decreases with increasing background ion-to-electron temperature ratio, the opposite behaviour to the tearing mode without flow shear. We find that even a relatively small flow shear is enough to dramatically alter the scaling behaviour of the mode, because the growth rate is small compared to the shear flow across the ion scales (but large compared to shear flow across the electron scales). Our results may explain the relative absence of reconnection events in the near-Sun Alfvénic solar wind observed recently by NASA's Parker Solar Probe. |
| title | Suppression of the collisionless tearing mode by flow shear: implications for reconnection onset in the Alfvénic solar wind |
| topic | Space Physics Solar and Stellar Astrophysics Plasma Physics |
| url | https://arxiv.org/abs/2412.01796 |