Reconnection nanojets in the solar corona

Patrick Antolin*, Paolo Pagano, Paola Testa, Antonino Petralia, Fabio Reale

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

47 Citations (Scopus)
4 Downloads (Pure)


The solar corona is shaped and mysteriously heated to millions of degrees by the Sun’s magnetic field. It has long been hypothesized that the heating results from a myriad of tiny magnetic energy outbursts called nanoflares, driven by the fundamental process of magnetic reconnection. Misaligned magnetic field lines can break and reconnect, producing nanoflares in avalanche-like processes. However, no direct and unique observations of such nanoflares exist to date, and the lack of a smoking gun has cast doubt on the possibility of solving the coronal heating problem. From coordinated multi-band high-resolution observations, we report on the discovery of very fast and bursty nanojets, the telltale signature of reconnection-based nanoflares resulting in coronal heating. Using state-of-the-art numerical simulations, we demonstrate that the nanojet is a consequence of the slingshot effect from the magnetically tensed, curved magnetic field lines reconnecting at small angles. Nanojets are therefore the key signature of reconnection-based coronal heating in action.
Original languageEnglish
JournalNature Astronomy
Early online date21 Sept 2020
Publication statusE-pub ahead of print - 21 Sept 2020


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