Journalartikel
Autorenliste: Ilin, Ekaterina; Angus, Ruth; Luger, Rodrigo; Morris, Brett M.; Jehn, Florian U.
Jahr der Veröffentlichung: 2023
Seiten: 4326-4339
Zeitschrift: Monthly Notices of the Royal Astronomical Society
Bandnummer: 523
Heftnummer: 3
ISSN: 0035-8711
eISSN: 1365-2966
Open Access Status: Green
DOI Link: https://doi.org/10.1093/mnras/stad1690
Verlag: Oxford University Press
Abstract:
The distribution of small-scale magnetic fields in stellar photospheres is an important ingredient in our understanding of the magnetism of low-mass stars. Their spatial distribution connects the field generated in the stellar interior with the outer corona and the large scale field, and thereby affects the space weather of planets. Unfortunately, we lack techniques that can locate them on most low-mass stars. One strategy is to localize field concentrations using the flares that occur in their vicinity. We explore a new method that adapts the spot simulation software fleck to study the modulation of flaring times as a function of active latitude. We use empirical relations to construct flare light curves similar to those available from Kepler and the Transiting Exoplanet Survey Satellite (TESS), search them for flares, and use the waiting times between flares to determine the location of active latitudes. We find that the mean and standard deviations of the waiting time distribution provide a unique diagnostic of flaring latitudes as a function of the number of active regions. Latitudes are best recovered when stars have three or less active regions that flare repeatedly, and active latitude widths below 20 deg; when either increases, the information about the active latitude location is gradually lost. We demonstrate our technique on a sample of flaring G dwarfs observed with the Kepler satellite, and furthermore suggest that combining ensemble methods for spots and flares could overcome the limitations of each individual technique for the localization of surface magnetic fields.
Zitierstile
Harvard-Zitierstil: Ilin, E., Angus, R., Luger, R., Morris, B. and Jehn, F. (2023) Flaring latitudes in ensembles of low-mass stars, Monthly Notices of the Royal Astronomical Society, 523(3), pp. 4326-4339. https://doi.org/10.1093/mnras/stad1690
APA-Zitierstil: Ilin, E., Angus, R., Luger, R., Morris, B., & Jehn, F. (2023). Flaring latitudes in ensembles of low-mass stars. Monthly Notices of the Royal Astronomical Society. 523(3), 4326-4339. https://doi.org/10.1093/mnras/stad1690
Schlagwörter
DIFFERENTIAL ROTATION; EARTH-LIKE EXOPLANETS; EJECTION CME ACTIVITY; GROUP SUNSPOT NUMBERS; M DWARFS; methods: statistical; PLANET INTERACTION; SCALE MAGNETIC TOPOLOGIES; SOLAR-TYPE STARS; stars: flare; stars: magnetic field; STELLAR ACTIVITY; X-RAY FLARE