首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Effects of dead time losses on terrestrial gamma ray flash measurements with the Burst and Transient Source Experiment
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Effects of dead time losses on terrestrial gamma ray flash measurements with the Burst and Transient Source Experiment

机译:死区时间损失对爆发和瞬态源实验中地面伽马射线闪光测量的影响

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摘要

Measurements from the Burst and Transient Source Experiment (BATSE) instrument on the Compton Gamma Ray Observatory (CGRO) are the only ones where characteristics of single terrestrial gamma ray flashes (TGFs) have been obtained thus far. However, it has been reported that the measurements suffer from significant dead time losses which complicates the analysis and raises question about earlier BATSE studies. These losses are due to the high-intensity flux combined with limitations of the time resolution of the instrument. Since these losses will affect both the spectrum and the temporal distribution of the individual TGFs, results based on BATSE data need to be revisited, including our own. We have therefore developed a Monte Carlo method to study the effects of these dead time losses. We show that the energy spectrum of TGFs becomes softer as the dead time losses increase. We also show that the time delay between the light curves of hard > 300 keV) and soft (E < 300 keV) photons increases significantly as the dead time losses increase. The Monte Carlo approach also enables us to identify the BATSE TGFs where the dead time effects can be corrected. These are the short-duration single-peaked TGFs. Without correcting for dead time losses we find that these short single-peak TGFs have a softer energy spectrum and larger time delay than the multipeaked TGFs. After correcting for dead time losses we perform a new analysis of production altitudes and find that the production altitude is reduced compared to analysis without dead time losses. The new production altitudes combined with dead time losses are also consistent with the apparent large time delays. Our method gives consistent results regarding production altitude and time delays and indicates that the corrected TGF intensities measured by BATSE are 3 to 4 times brighter than the uncorrected measurements would indicate. We also show that the production mechanism of these TGFs has a typical duration of 250 μs.
机译:到目前为止,康普顿伽玛射线天文台(CGRO)上的爆裂和瞬态源实验(BATSE)仪器进行的测量是唯一获得单地面伽玛射线闪光(TGF)特征的测量。然而,据报道,这些测量遭受显着的空载时间损失,这使分析变得复杂,并引起了对早期BATSE研究的质疑。这些损失归因于高强度通量以及仪器时间分辨率的限制。由于这些损失将影响单个TGF的频谱和时间分布,因此需要重新考虑基于BATSE数据的结果,包括我们自己的结果。因此,我们开发了一种蒙特卡洛方法来研究这些停滞时间损失的影响。我们表明,随着停滞时间损失的增加,TGFs的能谱变得更软。我们还表明,随着死区时间损失的增加,硬光> 300 keV)和软光(E <300 keV)的光曲线之间的时间延迟显着增加。蒙特卡洛方法还使我们能够确定可以校正空载时间影响的BATSE TGF。这些是短期的单峰TGF。如果不校正空载时间损失,我们会发现这些短的单峰TGF比多峰TGF具有更软的能谱和更大的时延。校正空载时间损失后,我们对生产高度进行了新的分析,发现与没有空载时间损失的分析相比,生产高度降低了。新的生产高度加上停滞时间损失也与明显的长时间延迟相一致。我们的方法给出了有关生产高度和时间延迟的一致结果,并表明通过BATSE测量的校正后的TGF强度比未校正的测量结果要亮3至4倍。我们还表明,这些TGF的产生机理通常具有250μs的持续时间。

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