Sky Brightness Evaluation at Concordia Station, Dome C, Antarctica, for Ground-Based Observations of the Solar Corona.

Antarctica Corona Coronagraphy Sky brightness Sun

Journal

Solar physics
ISSN: 0038-0938
Titre abrégé: Sol Phys
Pays: Netherlands
ID NLM: 101659554

Informations de publication

Date de publication:
2022
Historique:
received: 19 10 2021
accepted: 27 01 2022
entrez: 7 3 2022
pubmed: 8 3 2022
medline: 8 3 2022
Statut: ppublish

Résumé

The evaluation of sky characteristics plays a fundamental role for many astrophysical experiments and ground-based observations. In solar physics, the main requirement for such observations is a very low sky brightness value, less than

Identifiants

pubmed: 35250102
doi: 10.1007/s11207-022-01958-x
pii: 1958
pmc: PMC8889400
doi:

Types de publication

Journal Article

Langues

eng

Pagination

29

Informations de copyright

© The Author(s) 2022.

Déclaration de conflit d'intérêts

Disclosure of Potential Conflicts of InterestThe authors declare that there are no conflicts of interest.

Auteurs

Alessandro Liberatore (A)

OATo - Astrophysical Observatory of Turin, INAF - National Institute for Astrophysics, Via Osservatorio 20, 10025 Pino Torinese, To Italy.
Physics Department, University of Torino, Via Pietro Giuria 1, 10125 Torino, Italy.

Gerardo Capobianco (G)

OATo - Astrophysical Observatory of Turin, INAF - National Institute for Astrophysics, Via Osservatorio 20, 10025 Pino Torinese, To Italy.

Silvano Fineschi (S)

OATo - Astrophysical Observatory of Turin, INAF - National Institute for Astrophysics, Via Osservatorio 20, 10025 Pino Torinese, To Italy.

Giuseppe Massone (G)

OATo - Astrophysical Observatory of Turin, INAF - National Institute for Astrophysics, Via Osservatorio 20, 10025 Pino Torinese, To Italy.

Luca Zangrilli (L)

OATo - Astrophysical Observatory of Turin, INAF - National Institute for Astrophysics, Via Osservatorio 20, 10025 Pino Torinese, To Italy.

Roberto Susino (R)

OATo - Astrophysical Observatory of Turin, INAF - National Institute for Astrophysics, Via Osservatorio 20, 10025 Pino Torinese, To Italy.

Gianalfredo Nicolini (G)

OATo - Astrophysical Observatory of Turin, INAF - National Institute for Astrophysics, Via Osservatorio 20, 10025 Pino Torinese, To Italy.

Classifications MeSH