Thermal and non-thermal soft X-ray bursts
β Scribed by M. Landini; B. C. Monsignori Fossi; R. Pallavicini
- Publisher
- Springer
- Year
- 1972
- Tongue
- English
- Weight
- 421 KB
- Volume
- 27
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
β¦ Synopsis
X-ray bursts observed for energies lower than 25 keV are usually interpreted as being produced by a thermal plasma with several million degrees of temperature.
A small number of events recorded at Arcetri by real time telemetry of SOLRAD 9 satellite agrees with a thermal interpretation and gives temperatures ranging between 10 β’ l0 s and 30 β’ 10~K and emission measures, SNe2 dV, between 1047 and 1048 cm -8.
An impulsive event recorded on January 7, 1969 shows an anomalous behaviour. In this case the emission has been attributed to bremsstrahlung radiation from electrons with a power law energy distribution dN = KE-v dE. The values of the spectral index and of the emission measure are given.
A tentative interpretation of the event is suggested and the way to produce non-relativistic electrons with a power law energy distribution is investigated.
π SIMILAR VOLUMES
Processes leading to the excitation of soft X-ray line spectra are discussed in relation to their thermal or non-thermal nature. Through analysis of calcium spectra from the XRP experiment on SMM, it is shown that the ionization balance during the gradual phase of flares is effectively in the steady
Soft X-ray flare data in the wavelength range 2.6-10 A are used to examine the time variation of emission measure and electron temperature. The thermal plasma parameters were derived according to a two-temperature model proposed by Herring and Craig (1973). Estimates of electron density and source v
A semi-empirical model of the soft X-ray source associated with solar flares is presented, based on the results of the two temperature analysis of OSO-5 data obtained by Herring and Craig (1973). The model makes use of a jet of plasma rising from the solar surface as the basic origin of the soft X-r
A simple, analytic model is presented of a hot (> 108 K), thermal hard X-ray source, continuously heated, bounded by ion-acoustic conduction fronts, and expanding in a loop. The model is used to investigate the assumption, made in some published comparisons of this model with data, that the 'rise ti