Basal chromospheric flux and Maunder Minimum-type stars: the quiet-Sun chromosphere as a universal phenomenon

• Published in: Astronomy and astrophysics (Berlin) Vol. 540; p. A130
• Main Authors: Schröder, K.-P., Mittag, M., Pérez Martínez, M. I., Cuntz, M., Schmitt, J. H. M. M.
• Format: Journal Article
• Language: English
• Published: Les Ulis EDP Sciences 01.04.2012
• Subjects: Astronomy; Earth, ocean, space; Exact sciences and technology; plages; stars: activity; stars: chromospheres; Sun: chromosphere; Sun: corona; Sun: dynamo; Sun: faculae; Stellar winds; Soft X radiation; Flux tubes; Sun: corona; Quiet sun; Sun: chromosphere; stars: chromospheres; Giant stars; Surface gravity; Sun: dynamo; Sun:: faculae, plages; K line; Stellar chromospheres; Stellar activity; Magnetic fields; stars: activity; X ray emission; Magnetic polarity; Solar type star
• ISSN: 0004-6361; 1432-0746
• DOI: 10.1051/0004-6361/201118363

Aims. We demonstrate the universal character of the quiet-Sun chromosphere among inactive stars (solar-type and giants). By assessing the main physical processes, we shed new light on some common observational phenomena. Methods. We discuss measurements of the solar Mt. Wilson S-index, obtained by the Hamburg Robotic Telescope around the extreme minimum year 2009, and compare the established chromospheric basal Ca II K line flux to the Mt. Wilson S-index data of inactive (“flat activity”) stars, including giants. Results. During the unusually deep and extended activity minimum of 2009, the Sun reached S-index values considerably lower than in any of its previously observed minima. In several brief periods, the Sun coincided exactly with the S-indices of inactive (“flat”, presumed Maunder Minimum-type) solar analogues of the Mt. Wilson sample; at the same time, the solar visible surface was also free of any plages or remaining weak activity regions. The corresponding minimum Ca II K flux of the quiet Sun and of the presumed Maunder Minimum-type stars in the Mt. Wilson sample are found to be identical to the corresponding Ca II K chromospheric basal flux limit. Conclusions. We conclude that the quiet-Sun chromosphere is a universal phenomenon among inactive stars. Its mixed-polarity magnetic field, generated by a local, “fast” turbulent dynamo finally provides a natural explanation for the minimal soft X-ray emission observed for inactive stars. Given such a local dynamo also works for giant chromospheres, albeit on longer length scales, i.e., l ∝ R/g, with R and g as stellar radius and surface gravity, respectively, the existence of giant spicular phenomena and the guidance of mechanical energy toward the acceleration zone of cool stellar winds along flux-tubes have now become traceable.