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Natalia Zambrana Prado

University of Paris-Sud

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Linking the Sun to the Heliosphere Using Composition Data and Modelling. A Test Case with a Coronal Jet.

2021 arXiv: Solar and Stellar Astrophysics
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First data for abundance diagnostics with SPICE, the EUV spectrometer on-board Solar Orbiter

2021
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Relative abundance diagnostics with SPICE, the EUV spectrometer on-board Solar Orbiter

2020
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Spectroscopic diagnostics of the elemental composition of the solar corona

2020
- Natalia Zambrana Prado
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Measuring relative abundances in the solar corona with optimised linear combinations of spectral lines.

2019 arXiv: Solar and Stellar Astrophysics
- Natalia Zambrana Prado
- E. Buchlin
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A New Method for Measuring Relative Abundances in the Solar Corona

2018
- Natalia Zambrana Prado
- E. Buchlin
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