Mapping the solar wind HI outflow velocity in the inner heliosphere by coronagraphic ultraviolet and visible-light observations
We investigated the capability of mapping the solar wind outflow velocity of neutral hydrogen
atoms by using synergistic visible-light and ultraviolet observations. We used polarised …
atoms by using synergistic visible-light and ultraviolet observations. We used polarised …
METIS: a novel coronagraph design for the Solar Orbiter mission
S Fineschi, E Antonucci, G Naletto… - … 2012: Ultraviolet to …, 2012 - spiedigitallibrary.org
METIS (Multi Element Telescope for Imaging and Spectroscopy) METIS, the “Multi Element
Telescope for Imaging and Spectroscopy”, is a coronagraph selected by the European …
Telescope for Imaging and Spectroscopy”, is a coronagraph selected by the European …
Exploring the inner acceleration region of solar wind: A study based on coronagraphic UV and visible light data
A Bemporad - The Astrophysical Journal, 2017 - iopscience.iop.org
This work combined coronagraphic visible light (VL) and UV data to provide with an
unprecedented view of the inner corona where the nascent solar wind is accelerated. The …
unprecedented view of the inner corona where the nascent solar wind is accelerated. The …
Effects of helium ion bombardment on metallic gold and iridium thin films
S Zuccon, E Napolitani, E Tessarolo… - Optical Materials …, 2014 - opg.optica.org
Single layer mirrors have been prepared by evaporating gold and iridium on silicon
substrates. The samples have been exposed to 4 keV He+ ion flux at different total fluences …
substrates. The samples have been exposed to 4 keV He+ ion flux at different total fluences …
Temperature and thermal energy of a coronal mass ejection
A Bemporad - Symmetry, 2022 - mdpi.com
Due to the scarcity of UV–EUV observations of coronal mass ejections (CMEs) far from the
Sun (ie, at heliocentric distances larger than 1.5 R sun) our understanding of the …
Sun (ie, at heliocentric distances larger than 1.5 R sun) our understanding of the …
Morphological and functional modifications of optical thin films for space applications irradiated with low-energy helium ions
MG Pelizzo, AJ Corso, E Tessarolo… - … applied materials & …, 2018 - ACS Publications
Future space missions will operate in increasingly hostile environments, such as those in
low-perihelion solar orbits and Jovian magnetosphere. This exploration involves the …
low-perihelion solar orbits and Jovian magnetosphere. This exploration involves the …
Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test
Context. The determination from coronagraphic observations of physical parameters of the
plasma embedded in coronal mass ejections (CMEs) is of crucial importance for our …
plasma embedded in coronal mass ejections (CMEs) is of crucial importance for our …
Stability of EUV multilayer coatings to low energy alpha particles bombardment
M Nardello, P Zuppella, V Polito, AJ Corso… - Optics …, 2013 - opg.optica.org
Future solar missions will investigate the Sun from very close distances and optical
components are constantly exposed to low energy ions irradiation. In this work we present …
components are constantly exposed to low energy ions irradiation. In this work we present …
Plasma physical parameters along coronal-mass-ejection-driven shocks. I. Ultraviolet and white-light observations
In this work, UV and white-light (WL) coronagraphic data are combined to derive the full set
of plasma physical parameters along the front of a shock driven by a coronal mass ejection …
of plasma physical parameters along the front of a shock driven by a coronal mass ejection …
Empirical relations between the intensities of Lyman lines of H and He+
M Gordino, F Auchère, JC Vial, K Bocchialini… - Astronomy & …, 2022 - aanda.org
Context. Empirical relations between major UV and extreme UV spectral lines are one of the
inputs for models of chromospheric and coronal spectral radiances and irradiances. They …
inputs for models of chromospheric and coronal spectral radiances and irradiances. They …