Super bolide explosion in the upper atmosphere and possible implications for very low earth orbit satellites: a case study on May 25, 2023

IF 2.4 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
A. A. Pimenta, Oluwasegun M. Adebayo, C. M. Wrasse, R. de Jesus, A. M. Santos, P. P. Batista, V. F. Andrioli, P. R. Fagundes, E. A. Kherani, Siomel Savio, O. F. Olajide
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Abstract

This event is the first documented study in the Brazilian sector regarding a super bolide whose explosion was equivalent to 21 kilotons of TNT (∼8.83 × 10 13 J). The energy released by this event in the altitude range from 96 to 99 km in the upper atmosphere was equivalent to the atomic bomb detonated at an altitude of approximately 550 m over the Nagasaki city, Japan, during World War II. This observation was detected by all-sky images system with a filter in near infrared (NIR) band from 715 to 930 nm, operating at Cachoeira Paulista (22.7°S, 45°W) and lidar observations of the mesospheric sodium and potassium layers, operating at São José dos Campos (23.1°S, 45.9°W), both observatories in Brazil. The all-sky images system showed strong explosion in the mesosphere and a subsequent long-lived meteor train with more than 14 min through the NIR band. On the other hand, the lidar showed that the meteor explosion occurred in an altitude range from 96 to 99 km with the consequent sodium and potassium atoms enhancement on the background layers. Shortly after the fireball explosion, a digisonde operating at Cachoeira Paulista detected a sudden appearance of a sporadic-E layer. Using GNSS data, an analysis of the generation of infrasonic pressure waves excited during meteor explosion is presented. In addition, thermospheric neutral density values obtained with Swarm Satellite B prior to, during, and after 25 May 2023, showed a neutral density peak on 25 May 2023, at ∼ 12 UT, after the super bolide explosion (∼4.5 h later), and reached approximately 0.574 × 10 −12 kg/m 3 , 15% above the average neutral density value prior to event. In this work we present and discuss several features related to this super bolide explosion in the upper atmosphere/ionosphere.
高层大气中的超级火流星爆炸及其对极低地球轨道卫星的可能影响:2023年5月25日的案例研究
这一事件是巴西部门首次记录的关于超级火流星的研究,其爆炸当量相当于21千吨TNT (~ 8.83 × 10 13 J)。在96 ~ 99公里高空释放的能量相当于第二次世界大战期间在日本长崎市上空550米高空引爆的原子弹。该观测是通过在巴西Cachoeira Paulista观测站(22.7°S, 45°W)和o jos dos Campos观测站(23.1°S, 45.9°W)使用近红外(NIR)波段715 ~ 930 nm带滤光片的全天成像系统进行的。通过近红外波段,全天图像系统显示了中间层的强烈爆炸和随后的长寿命流星雨,持续时间超过14分钟。另一方面,激光雷达显示流星爆炸发生在96至99公里的高度范围内,随之而来的钠和钾原子在背景层上增强。在火球爆炸后不久,在卡乔埃拉保利斯塔操作的一个双空探测仪检测到一个偶然的e层突然出现。利用GNSS数据,分析了流星爆炸过程中次声压力波的产生。此外,用Swarm Satellite B在2023年5月25日之前、期间和之后获得的热层中性密度值显示,在2023年5月25日超级火流星爆炸(约4.5 h后)后的~ 12 UT,中性密度达到约0.574 × 10−12 kg/m 3,比事件前的平均中性密度值高出15%。在这项工作中,我们提出并讨论了与高层大气/电离层中超级火流星爆炸有关的几个特征。
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来源期刊
Frontiers in Astronomy and Space Sciences
Frontiers in Astronomy and Space Sciences ASTRONOMY & ASTROPHYSICS-
CiteScore
3.40
自引率
13.30%
发文量
363
审稿时长
14 weeks
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