Spectroscopic and Imaging Observations of Spatially Extended Magnetic Reconnection in the Splitting of a Solar Filament Structure
Huidong Hu (1), Ying D. Liu (1, 2), Lakshmi Pradeep Chitta (3),, Hardi Peter (3), Mingde Ding (4) ((1) NSSC, China, (2) UCAS, China, (3) MPS,, Germany, (4) NJU, China)

TL;DR
This study provides the first detailed spectroscopic evidence of magnetic reconnection extending over at least 14,000 km on the Sun, leading to filament splitting and eruption, with bidirectional outflows and high-temperature plasma.
Contribution
It presents high-resolution spectroscopic and imaging observations demonstrating an extended magnetic reconnection region causing filament splitting, a phenomenon not previously confirmed with such spatial detail.
Findings
Reconnection region extends at least 14,000 km
Bidirectional outflows of ~100 km/s observed
Reconnection region temperature exceeds 10 MK
Abstract
On the Sun, Doppler shifts of bidirectional outflows from the magnetic-reconnection site have been found only in confined regions through spectroscopic observations. Without spatially resolved spectroscopic observations across an extended region, the distribution of reconnection and its outflows in the solar atmosphere cannot be made clear. Magnetic reconnection is thought to cause the splitting of filament structures, but unambiguous evidence has been elusive. Here we report spectroscopic and imaging analysis of a magnetic-reconnection event on the Sun, using high-resolution data from the Interface Region Imaging Spectrograph and the Solar Dynamics Observatory. Our findings reveal that the reconnection region extends to an unprecedented length of no less than 14,000 km. The reconnection splits a filament structure into two branches, and the upper branch erupts eventually. Doppler…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Astro and Planetary Science · Stellar, planetary, and galactic studies
