Chromospheric jets around the edges of sunspots

2012/05/07 by R. J. Morton · 1 citation
Computer Science · Physics and Astronomy · #Astro and Planetary Science #Astrobiology #Astronomy #Astrophysics #Chromosphere #Corona (planetary geology) #Magnetic field #Physics #Solar Radiation and Photovoltaics #Solar and Space Plasma Dynamics #Sunspot #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201219137

A&A, In press 2012

openalex publication_date 2012/05/07 · arxiv created 2012/05/11 · arxiv updated 2015/06/05 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims. Evidence is beginning to be put forward that demonstrates the role of the chromosphere in supplying energy and mass to the corona. We aim to assess the role of chromospheric jets in active region dynamics.

Citations

• Sunspots: An overview
• MULTIPLE COMPONENT OUTFLOWS IN AN ACTIVE REGION OBSERVED WITH THE EUV IMAGING SPECTROMETER ONHINODE
• Continuous upflows and sporadic downflows observed in active regions
• ON-DISK COUNTERPARTS OF TYPE II SPICULES IN THE Ca II 854.2 nm AND Hα LINES
• Coronal plasma flows and magnetic fields in solar active regions

Cited by

• Physical properties of a fan-shaped jet backlit by an X9.3 flare
• Small-scale Bright Blobs Ejected from a Sunspot Light Bridge