Diagnostic capabilities of spectropolarimetric observations for understanding solar phenomena: I. Zeeman-sensitive photospheric lines

  1. Quintero Noda, C. 1123
  2. Barklem, P.S. 4
  3. Gafeira, R. 56
  4. Ruiz Cobo, B. 23
  5. Collados, M. 23
  6. Carlsson, M. 11
  7. Martínez Pillet, V. 7
  8. Orozco Suárez, D. 5
  9. Uitenbroek, H. 7
  10. Katsukawa, Y. 8
  1. 1 University of Oslo
    info

    University of Oslo

    Oslo, Noruega

    ROR https://ror.org/01xtthb56

  2. 2 Instituto de Astrofísica de Canarias
    info

    Instituto de Astrofísica de Canarias

    Santa Cruz de Tenerife, España

    ROR https://ror.org/03cmntr54

  3. 3 Universidad de La Laguna
    info

    Universidad de La Laguna

    San Cristobal de La Laguna, España

    ROR https://ror.org/01r9z8p25

  4. 4 Uppsala University
    info

    Uppsala University

    Upsala, Suecia

    ROR https://ror.org/048a87296

  5. 5 Instituto de Astrofísica de Andalucía
    info

    Instituto de Astrofísica de Andalucía

    Granada, España

    ROR https://ror.org/04ka0vh05

  6. 6 Universidade de Coimbra
    info

    Universidade de Coimbra

    Coímbra, Portugal

    ROR https://ror.org/04z8k9a98

  7. 7 University of Colorado Boulder
    info

    University of Colorado Boulder

    Boulder, Estados Unidos

    ROR https://ror.org/02ttsq026

  8. 8 National Astronomical Observatory of Japan
    info

    National Astronomical Observatory of Japan

    Mitaka-shi, Japón

    ROR https://ror.org/052rrw050

Journal:
Astronomy and Astrophysics

ISSN: 1432-0746

Year of publication: 2021

Volume: 652

Type: Article

DOI: 10.1051/0004-6361/202037735 SCOPUS: 2-s2.0-85114207713 GOOGLE SCHOLAR
Data source: Scopus