Looking for stellar CMEs on different wavelengths

Stellar coronal mass ejections (CMEs) are powerful explosions of plasma and magnetic energy from stars, which can potentially impact the space environment in their astrospheres influencing the development of their planets. The handling of large amounts of observational data (~20TB) is not feasible using desktop computers.

Publikációk

1 - 5 | 8
2026

Stellar flares with Ariel: detection prospects and impacts on exoplanet spectroscopy

K. Vida; B. Seli; B. Edwards
Looking for stellar CMEs on different wavelengths
Tovább
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2026

Sub-second cadence structure of optical flares on AD Leo

B. Schmercz; B. Seli; K. Vida; L. Kriskovics; A. Görgei; K. Oláh; Zs. Regály
Looking for stellar CMEs on different wavelengths
Tovább
Tovább
2026

TESS flares and chromospheric variability in the Pleiades, the Hyades, and Praesepe

A. Görgei; K. Vida; B. Seli; K. Oláh; P. Sági; B. Schmercz; R. M. Roettenbacher; Zs. Kővári
Looking for stellar CMEs on different wavelengths
Tovább
Tovább
2026

What powers the most energetic flares in the Kepler field? Revisiting the superflaring star KIC 2852961

Zs. Kővári; B. Seli; L. Kriskovics; K. Oláh; P. Odert; M. Leitzinger; B. Schmercz; K. Vida; R. Greimel; B. Cseh et al.
Looking for stellar CMEs on different wavelengths
Tovább
Tovább
2025

Magnetic activity on the young Sun: a case study of EK Draconis

A. Görgei; L. Kriskovics; K. Vida; B. Seli; K. Oláh; P. Sági; A. Bódi; S.P. Järvinen; K.G. Strassmeier; A. Pál et al.
Looking for stellar CMEs on different wavelengths
Tovább
Tovább