1988
DOI: 10.1007/bf00148595
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Hard X-ray and low-energy gamma-ray spectrometers

Abstract: Basic principles of operation and characteristics of scintillation and semi-conductor detectors used for solar hard X-ray and gamma-ray spectrometers are presented. Scintillation materials such as NaI offer high stopping power for incident gamma rays, modest energy resolution, and relatively simple operation. They are, to date, the most often used detector in solar gamma-ray spectroscopy. The scintillator BGO has higher stopping power than NaI, but poorer energy resolution. The primary advantage of semi-conduc… Show more

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Cited by 12 publications
(7 citation statements)
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“…The rise time of the x‐ray bursts are consistent with the thermal conduction front model [ Batchelor , 1989]. However, the differences between most of the correlations derived from the different hard x‐ray interpretations were insufficient to establish a preference between the thermal and thick‐target processes [ Starr et al , 1988].…”
Section: Energy Input: the Impulsive Phasementioning
confidence: 75%
See 1 more Smart Citation
“…The rise time of the x‐ray bursts are consistent with the thermal conduction front model [ Batchelor , 1989]. However, the differences between most of the correlations derived from the different hard x‐ray interpretations were insufficient to establish a preference between the thermal and thick‐target processes [ Starr et al , 1988].…”
Section: Energy Input: the Impulsive Phasementioning
confidence: 75%
“…Reviews of specific flare topics include the impulsive phase [ Dennis , 1988; Dennis and Schwartz , 1989], multispectral observations [ Walker; 1988], soft x‐ray line emission [ Doschek , 1990], comparisons between solar and stellar flares [ Haisch , 1989b; Mullan , 1989], theories of particle acceleration [ Vlahos , 1989], loop models [ Emslie , 1989], directivity of hard x‐ray and gamma‐ray emission [ Kane , 1987; Vestrand , 1988], lack of observed x‐ray polarization [ Chanan et al , 1988], relations between hard x‐rays and microwaves [ Crannell et al ,1988], and various aspects of flares [ Rust and Batchelor , 1987; Ramaty et al , 1988]. Many of these reviews include discussions of new instruments and the scientific requirements for these instruments (see also Gehrels et al , [1988]).…”
Section: Solar Flaresmentioning
confidence: 99%
“…In X-ray sensors, an indirect X-ray detection type using a scintillator has been developed, but even the NaI scintillator with high absolute fluorescence efficiency possesses the efficiency value of only 13% [1].…”
Section: Introductionmentioning
confidence: 99%
“…However, even for a NaI (Tl) scintillator showing high absolute fluorescence efficiency, this value is only about 13%. 3) For anthracene, the absolute fluorescence efficiency is 5%. 4) For Y 2 SiO 5 and Lu 2 SiO 5 , the absolute fluorescence efficiency is 10% or less.…”
Section: Introductionmentioning
confidence: 99%