The problem of producing the hard X-ray burst at the onset of solar flares may be thought of in terms of the problem of producing the non-thermal electrons which emit the X-rays via bremsstrahlung. Electron acceleration to relativistic energies without similar ion acceleration is difficult to achiev
✦ LIBER ✦
Identification of the hard X-ray pulse in the flare of September 11–12, 1968
✍ Scribed by J. Vorpahl; H. Zirin
- Book ID
- 104646329
- Publisher
- Springer
- Year
- 1970
- Tongue
- English
- Weight
- 362 KB
- Volume
- 11
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
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