Spectroscopic evidence of cool plasma in quiet Sun small-scale brightenings detected by HRIEUV on board Solar Orbiter

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. C.4.

Contribution function of the SPICE (left) and EIS (right) lines computed with CHIANTI V10.1, assuming a coronal abundance (Asplund et al. 2021), the recommended ionisation fraction by CHIANTI, and an electron density equal to n_e= 1 × 10⁹ cm⁻³.

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