权益分类	功能权益	普通用户	{{item.name}}会员
{{category.name}}	{{benefitItem.name}}

Balloon Observations of Gamma-ray Glows from Thunderstorms

雷暴伽马射线的气球观测

基本信息

批准号：
1618457
负责人：
Joseph Dwyer
金额：
$ 50.05万
依托单位：
University of New Hampshire
依托单位国家：
美国
项目类别：
Standard Grant
财政年份：
2016
资助国家：
美国
起止时间：
2016-10-01 至 2020-09-30
项目状态：
已结题

来源：
https://www.nsf.gov/awardsearch/showAward?AWD_ID=1618457&HistoricalAwards=false
关键词：
Balloon Observations Gamma ray Glows

项目摘要

Thunderstorms are high-energy environments consisting of electric fields and radiation sources. Gamma-ray emissions from thunderstorms are known as gamma-ray glows and are often terminated by lightning. However, there have been few observations of gamma-ray glows, and little is known about how and where they are created and how they may relate to the initiation of lightning. This project will combine new observations and computer modeling to better understand this phenomena. The main aspect of the project will be the deployment of gamma-ray sensors on balloons that will be flown into thunderstorms to collect data. A potential impact of the project is through the improved understanding of lightning initiation, which may eventually lead to better warnings and lightning safety. Multiple students would be involved in the project, thereby training the next generation of scientists.The research team will conduct balloon-based observations of gamma-ray glows. The work will improve upon a prior design of a balloon-borne instrument that detects gamma-ray glows using Geiger counters by incorporating an inorganic scintillator and a slow electric field measurement. Thirty flights are planned over the course of the proposal period from central Florida. The data, along with Monte Carlo simulations of gamma-ray propagation, would be used to: 1) Determine the frequency of gamma-ray glows and their relationship to thunderstorm meteorology and lightning, 2) Determine source mechanism(s) for gamma-ray glows, 3) Determine discharge currents produced by gamma-ray glows in the source regions, 4) Constrain electric fields present in glow source regions/lightning initiation regions and determine durations of high fields occurring before lightning, 5) Determine relationship between glows, lightning and TGFs.

雷暴是由电场和辐射源组成的高能环境。雷暴释放的伽马射线被称为伽马射线辉光，通常被闪电终止。然而，对伽马射线辉光的观测很少，而且对它们是如何和在哪里产生的以及它们如何与闪电的起源有关知之甚少。这个项目将联合收割机结合新的观察和计算机建模来更好地理解这种现象。该项目的主要方面将是在气球上部署伽马射线传感器，这些气球将飞入雷暴中收集数据。该项目的一个潜在影响是通过提高对闪电启动的理解，这可能最终导致更好的预警和闪电安全。多名学生将参与该项目，从而培养下一代科学家。研究小组将进行基于气球的伽马射线辉光观测。这项工作将改进先前设计的球载仪器，检测伽马射线辉光使用盖革计数器，结合无机闪烁体和缓慢的电场测量。计划在提案期间从佛罗里达中部起飞30次航班。这些数据连同伽马射线传播的蒙特卡罗模拟沿着将用于：1）确定伽马射线辉光的频率及其与雷暴气象和闪电的关系，2）确定伽马射线辉光的源机制，3）确定伽马射线辉光在源区产生的放电电流，4）约束辉光源区/闪电起始区的电场，确定闪电前高场出现的持续时间; 5）确定辉光、闪电和TGFs之间的关系。