Observations of a solar flare and filament eruption in Lyman alpha and X-rays
arXiv:0909.4705 · doi:10.1051/0004-6361/200912651
Abstract
We aim to characterise the appearance and behaviour of a flare and filament ejection which occurred on 8th September 1999 and was observed by TRACE in L-alpha as well as by the Yohkoh Soft and Hard X-ray telescopes. We explore the flare energetics and its spatial and temporal evolution. A correction is applied to the TRACE data to obtain a better estimate of the pure L-alpha signature. The L-alpha power is obtained from a knowledge of the TRACE response function, and the flare electron energy budget is estimated by interpreting Yohkoh/HXT emission in the context of the collisional thick target model.
10 pages, 15 figures
Cited by in corpus (10)
- Detection of flare multi-periodic pulsations in mid-ultraviolet Balmer continuum, Ly-alpha, hard X-ray, and radio emissions simultaneously
- Quasi-periodic pulsation detected in Lyman-alpha emission during solar flares
- Doppler speeds of the hydrogen Lyman lines in solar flares from EVE
- The Response of the Lyman-Alpha Line in Different Flare Heating Models
- Solar Irradiance Variability Due To Solar Flares Observed in Lyman-alpha Emission
- The Lyman-alpha Emission in Solar Flares. I. a Statistical Study on Its Relationship with the 1--8 Å Soft X-ray Emission
- On the Importance of Ca II Photoionisation by the Hydrogen Lyman Transitions in Solar Flare Models
- The Lyman- Emission in a C1.4 Solar Flare Observed by the Extreme Ultraviolet Imager aboard Solar Orbiter
- The role of filament activation in a solar eruption
- Quasi-Periodic Pulsations Detected in Ly and Nonthermal Emissions During Solar Flares