EGU22-1856, updated on 27 Mar 2022
https://doi.org/10.5194/egusphere-egu22-1856
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

A Study of Small-Scale Brightenings using EUV Data from SPICE on board Solar Orbiter

Jenny Marcela Rodriguez Gomez1,2, Peter Young1, and Therese Kucera1
Jenny Marcela Rodriguez Gomez et al.
  • 1NASA Goddard Space Flight Center, Washington, United States of America (rodriguezgomez@cua.edu)
  • 2The Catholic University of America Washington, D.C. 20064

Recently small-scale solar dynamic features have been observed on the Sun by Solar Orbiter/EUI (Berghmans et al. 2021; Panesar et al. 2021). These events (initially referred to as “campfires”) are small-scale heating events observed mainly in the solar corona. The Spectral Imaging of Coronal Environment (SPICE; SPICE Consortium et al. 2020) is a high-resolution imaging spectrometer that observes the Sun in extreme ultraviolet (EUV) wavelengths. This study uses L2 SPICE data (calibrated images)  to characterize and follow the evolution of these small-scale brightenings. Additionally, we use HRIEUV 174 Å on board Solar Orbiter and Stereo A datasets to have a complementary view of small-scale brightenings during the study period.

How to cite: Rodriguez Gomez, J. M., Young, P., and Kucera, T.: A Study of Small-Scale Brightenings using EUV Data from SPICE on board Solar Orbiter, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-1856, https://doi.org/10.5194/egusphere-egu22-1856, 2022.

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