Spectroscopy at the solar limb

2011/06/01 by C. Beck, R. Rezaei · 1 citation
Earth and Planetary Sciences · Physics and Astronomy · #Astronomy #Astrophysics #Atmospheric Ozone and Climate #Chromosphere #Doppler effect #Emission spectrum #Geometry #Intensity (physics) #Line (geometry) #Optics #Perpendicular #Physics #Solar and Space Plasma Dynamics #Spectral line #Spectroscopy #Stellar, planetary, and galactic studies #Wavelength #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201014976

11 pages, 11 figures + 3 pages Appendix, accepted by A&A

openalex publication_date 2011/06/01 · arxiv created 2011/06/03 · arxiv updated 2015/05/28 · openalex created_date 2022/10/01 · openalex updated_date 2026/08/05

Abstract

Aims. We present constraints on the thermodynamical structure of the chromosphere from ground-based observations of the Ca ii H line profile near and off the solar limb.

Citations

• FABRY–PÉROT VERSUS SLIT SPECTROPOLARIMETRY OF PORES AND ACTIVE NETWORK: ANALYSIS OF IBIS ANDHINODEDATA
• Physical Properties of Spicules from Simultaneous Spectropolarimetric Observations of He i and Ca ii Lines

Cited by

• The energy of waves in the photosphere and lower chromosphere