activity
20122026
most citedThe Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action

112 citations · 664 across the 39 of their papers we have counts for

collaborators
Showing 2023Show all

18 papers · 1 filter

astro-ph.SR2023★ 5 cited

Coronal voids and their magnetic nature

J. D. Nölke, S. K. Solanki, J. Hirzberger +68

Extreme ultraviolet (EUV) observations of the quiet solar atmosphere reveal extended regions of weak emission compared to the ambient quiescent corona. The magnetic nature of these…

astro-ph.SR2023★ 8 cited

Evolution of dynamic fibrils from the cooler chromosphere to the hotter corona

Sudip Mandal, Hardi Peter, Lakshmi Pradeep Chitta +17

Dynamic fibrils (DFs) are commonly observed chromospheric features in solar active regions. Recent observations from the Extreme Ultraviolet Imager (EUI) aboard the Solar Orbiter h…

astro-ph.SR2023★ 77 cited

Picoflare jets power the solar wind emerging from a coronal hole on the Sun

L. P. Chitta, A. N. Zhukov, D. Berghmans +17

Coronal holes are areas on the Sun with open magnetic field lines. They are a source region of the solar wind, but how the wind emerges from coronal holes is not known. We observed…

astro-ph.SR2023

Polarisation of decayless kink oscillations of solar coronal loops

Sihui Zhong, Valery M. Nakariakov, Dmitrii Y. Kolotkov +4

Decayless kink oscillations of plasma loops in the solar corona may contain an answer to the enigmatic problem of solar and stellar coronal heating. The polarisation of the oscilla…

astro-ph.SR2023★ 7 cited

Beyond small-scale transients: a closer look at the diffuse quiet solar corona

J. Gorman, L. P. Chitta, H. Peter +9

Within the quiet Sun corona imaged at 1 MK, much of the field of view consists of diffuse emission that appears to lack the spatial structuring that is so evident in coronal loops…

astro-ph.SR2023★ 16 cited

Fleeting Small-scale Surface Magnetic Fields Build the Quiet-Sun Corona

L. P. Chitta, S. K. Solanki, J. C. del Toro Iniesta +19

Arch-like loop structures filled with million Kelvin hot plasma form the building blocks of the quiet-Sun corona. Both high-resolution observations and magnetoconvection simulation…