activity
20172025
most citedThe eruption of a small-scale emerging flux rope as the driver of an M-class flare and a coronal mass ejection

38 citations · 68 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2025★ 1 cited

Supergranulation and Poleward Migration of the Magnetic Field at High Latitudes of the Sun

L. P. Chitta, D. Calchetti, J. Hirzberger +26

Magnetoconvection at the solar surface governs the dynamics in the upper solar atmosphere and sustains the heliosphere. Properties of this fundamental process are poorly described…

astro-ph.SR2025★ 9 cited

A magnetic avalanche as the central engine powering a solar flare

L. P. Chitta, D. I. Pontin, E. R. Priest +17

Solar flares are the most powerful, magnetically driven, explosions in the heliosphere. The nature of magnetic energy release in the solar corona that heats the plasma and accelera…

astro-ph.SR2024★ 4 cited

Photospheric Hot Spots at Solar Coronal Loop Footpoints Revealed by Hyperspectral Imaging Observations

L. P. Chitta, M. van Noort, H. N. Smitha +2

Poynting flux generated by random shuffling of photospheric magnetic footpoints is transferred through the upper atmosphere of the Sun where the plasma is heated to over 1 MK in th…

astro-ph.SR2024★ 16 cited

Coronal Heating and Solar Wind Generation by Flux Cancellation Reconnection

D. I. Pontin, E. R. Priest, L. P. Chitta +1

In this paper we propose that flux cancellation on small granular scales ( km) ubiquitously drives reconnection at a multitude of sites in the low solar atmosphere,…

astro-ph.SR2017★ 38 cited

The eruption of a small-scale emerging flux rope as the driver of an M-class flare and a coronal mass ejection

X. L. Yan, C. W. Jiang, Z. K. Xue +6

Solar flares and coronal mass ejections (CMEs) are the most powerful explosions in the Sun. They are major sources of potentially destructive space weather conditions. However, the…