First Steps Towards a New High Resolution Proxy for Paleomagnetic Field Instabilities: Tritiogenic 3He Archived in Speleothems

迈向古磁场不稳定性新高分辨率代理的第一步：三成因 3He 存档于 Speleothems

• 批准号: 1844850
• 负责人: Andrea Balbas
• 金额: $ 26.5万
• 依托单位: Oregon State University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2018
• 资助国家: 美国
• 起止时间: 2018-07-05 至 2021-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1844850&HistoricalAwards=false
• 关键词: First; Steps; Towards; New; Resolution

The terrestrial magnetic field is critical to life on Earth because it shields the planet from harmful cosmic radiation. It also protects technological infrastructure from damage from solar storms. The Earth's magnetic field is generated by organized motions of liquid iron in the Earth's outer core - the geodynamo - by processes that are not fully understood. Key observable features that can be used to inform models of the geodynamo include magnetic field strength and orientation, both of which change over geologic time. Existing records of the temporal variation of magnetic field strength are incomplete and potentially compromised by secondary processes. A potential new archive originates from the protective nature of the field. Cosmic rays continually strike the atmosphere, but their flux is modulated by the magnetic field. Stronger magnetic fields provide greater deflection of cosmic rays from Earth, and weaker fields provide less deflection. The flux of cosmic rays in turn controls the production rate of cosmogenic nuclides - rare isotopes produced when cosmic rays collide with gases in the atmosphere. Several cosmogenic nuclide archives have already been used to establish the history of magnetic field strength. This project will take exploratory steps towards development of a new high temporal resolution archive: the abundance of tritium - a cosmogenic nuclide with a half-life of 12 years - in fluid inclusions trapped in cave deposits of various ages. As an isotope of hydrogen, the post-production behavior of tritium will be controlled by the atmospheric water cycle, and will not suffer the same complications as previously measured cosmogenic nuclide archives of magnetic field strength.The decay product of tritium (3He) will be measured in water pockets that are trapped by stalagmites as they grow. The working hypothesis is that these water inclusions take in tritium in proportion to its production by cosmic rays in the atmosphere via the delivery of local rainwater into the cave system. After entrapment, tritium decays to 3He, which is thereafter retained in the water inclusion until analysis. Stalagmites often have annual bands, and can be dated accurately using U/Th geochronology. Taken together, these ideas suggest stalagmites offer a potential record of geomagnetic field changes with better temporal detail than those provided by alternative methods and with independent sources of potential error. This project will take the first steps for creating such a record by developing the necessary analytical methods and then by analyzing stalagmites that captured atmospheric tritium created by nuclear weapons testing in the latter half of the 20th century to confirm that the putative archive works as expected. Because the atmospheric tritium production from bomb testing is well-documented, the archive will be subjected to a very rigorous test. The two products sought by the end of the proposed work are a) a methodology that can successfully liberate and measure the tritiogenic 3He in speleothems, and b) a confirmation or refutation of the key hypothesis of this proposal: Tritiogenic 3He preserved in water inclusions in speleothems can be measured and will change as a function of the concentration of tritium in local precipitation.

地球磁场对地球上的生命至关重要，因为它保护地球免受有害的宇宙辐射。它还可以保护技术基础设施免受太阳风暴的破坏。地球磁场是由地球外核的液态铁有组织的运动产生的，即地球动力学，其过程尚不完全清楚。可以用来建立地球发电机模型的关键可观测特征包括磁场强度和方向，这两者都随着地质时间的变化而变化。现有的磁场强度随时间变化的记录是不完整的，并且可能受到二次过程的影响。一个潜在的新档案源于该领域的保护性。宇宙射线不断地撞击大气层，但它们的通量受到磁场的调节。较强的磁场会使来自地球的宇宙射线发生较大的偏转，而较弱的磁场则会使偏转较小。宇宙射线的通量反过来控制着宇宙核素的产生速率——当宇宙射线与大气中的气体碰撞时产生的稀有同位素。几个宇宙核素档案已经被用来建立磁场强度的历史。该项目将采取探索性步骤，以开发一种新的高时间分辨率档案：在不同年龄的洞穴沉积物中捕获的流体包裹体中氚的丰度-一种半衰期为12年的宇宙核素。作为氢的同位素，氚的后期生产行为将受到大气水循环的控制，并且不会遭受与先前测量的宇宙核素磁场强度档案相同的复杂性。氚（3He）的衰变产物将在石笋生长过程中被捕获的水袋中测量。可行的假设是，这些水包裹体吸收氚与大气中的宇宙射线通过将当地雨水输送到洞穴系统中产生的氚成比例。在包裹后，氚衰变为3He，然后保留在水包裹体中直到分析。石笋通常有年轮，可以使用U/Th地质年代学准确地确定年代。综上所述，这些观点表明，石笋提供了一种潜在的地磁场变化记录，比其他方法提供的记录具有更好的时间细节，并且具有潜在误差的独立来源。该项目将首先开发必要的分析方法，然后通过分析捕获20世纪后半叶核武器试验产生的大气氚的石笋，以确认假定的档案是否如预期的那样有效，从而迈出创造这种记录的第一步。由于核弹试验产生的大气氚是有案可查的，因此该档案将受到非常严格的测试。在本工作的最后，我们所寻求的两个产物是：a)一种能够成功地释放和测量洞穴中含氚3He的方法；b)对本提案的关键假设的证实或反驳：洞穴中保存在水包裹体中的含氚3He可以被测量，并且会随着当地降水中氚浓度的变化而变化。