Some ideas are developed concerning solar flares which have been presented earlier by the author (SC~ATZMAN, 1966a). Emphasis is laid on the problem of energy transport; from the energy supply to the region of the optical flare, on the storage of low energy cosmic ray particles in a magnetic bottle
The optical continuum of solar and stellar flares
โ Scribed by M. A. Livshits; O. G. Badalyan; A. G. Kosovichev; M. M. Katsova
- Publisher
- Springer
- Year
- 1981
- Tongue
- English
- Weight
- 967 KB
- Volume
- 73
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
According to one of the most popular classifications, solar flares may be assigned either to the category of small short-lived events, or to the category of large, long-duration two-ribbon (2-R) flares. Even if such a broad division oversimplifies the flare phenomenon, our knowledge of the character
We consider potential sources of infrared (1/t to 1 ram) continuum in solar flares. Several mechanisms should produce detectable fluxes: in the 350/z window for ground-based observations, impulsive emission will arise in synchrotron radiation from 1-10 MeV electrons, and possibly thermal (free-free)
This paper discusses the hydrodynamic modeling offlarmg plasma confined in magnetic loops and its objectives within the broader scope of flare physics. In particular, the Palermo-Harvard model is discussed along with its applications to the detailed fitting of X-ray light curves of solar flares and
A study is made of Lyman continuum observations of solar flares, using data obtained by the Harvard College Observatory EUV spectroheliometer on the Apollo Telescope Mount. We find that there are two main types of flare regions: an overall 'mean' flare coincident with the Ha flare region, and transi