𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Hard X-ray and γ-ray observations of solar flares with the Phebus experiment

✍ Scribed by R. Talon; G. Trottet; N. Vilmer; C. Barat; J. -P. Dezalay; R. Sunyaev; O. Terekhov; A. Kuznetsov

Publisher
Springer
Year
1993
Tongue
English
Weight
954 KB
Volume
147
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Observations of fine time structure in s
Observations of fine time structure in solar flare hard X-ray bursts
✍ K. Hurly; M. Niel; R. Talon; I. V. Estulin; V. Ch. Dolidze 📂 Article 📅 1983 🏛 Springer 🌐 English ⚖ 335 KB

Hard X-ray (ZI00 keY) time histories of solar flares which occurred on 1978 December 4 an@ 1979 February 18 are presented. The first flare was observed by 3 identical instruments from near-earth orbit (Prognoz 7) and interplanetary space (Venera Ii and 12). Fine time structure is present down to t

X-ray observations of stellar coronae an
X-ray observations of stellar coronae and flares: The “SOLAR-Aconnection”
✍ Robert A. Stern 📂 Article 📅 1987 🏛 Springer 🌐 English ⚖ 198 KB

It is now more than ten years since the first x-ray emitting stellar corona was discovered (Catura, Acton, and Johnson 1975). Since then, rapid progress has been made in cataloging the incidence and range of stellar x-ray emission, most notably with the Einstein Observatory (see, eg., reviews by Ste

On the production of hard X-rays in sola
On the production of hard X-rays in solar flares
✍ G. M. Simnett; M. G. Haines 📂 Article 📅 1990 🏛 Springer 🌐 English ⚖ 613 KB

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