《Effect of near-earth thunderstorms electric field on the intensity of ground cosmic ray positrons/electrons in Tibet》

  • 来源专题:中国科学院紫金山天文台科技信息监测服务
  • 编译者: zhoubz
  • 发布时间:2016-04-11
  • Monte Carlo simulations are performed to study the correlation between the ground cosmic ray intensity and near-earth thunderstorms electric field at YBJ (4300 m a.s.l., Tibet, China). The variations of the secondary cosmic ray intensity are found to be highly dependent on the strength and polarity of the electric field. In negative fields and in positive fields greater than 600 V/cm, the total number of ground comic ray positrons and electrons increases with increasing electric field strength. And these values increase more obviously when involving a shower with lower primary energy or a higher zenith angle. While in positive fields ranging from 0 to 600 V/cm, the total number of ground comic ray positrons and electrons declines and the amplitude is up to 3.1% for vertical showers. A decrease of intensity occurs for inclined showers in positive fields less than 500 V/cm, which is accompanied by smaller amplitudes. In this paper, the intensity changes are discussed, especially concerning the decreases in positive electric fields. Our simulation results are in good agreement with ground-based experimental results obtained from ARGO-YBJ and the Carpet air shower array. These results could be helpful in understanding the acceleration mechanisms of secondary charged particles caused by an atmospheric electric field.

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  • 《With X-Ray Analysis, an Asteroid Provides a View into Our Solar System’s Past》

    • 来源专题:可再生能源
    • 编译者:武春亮
    • 发布时间:2024-07-01
    • Skip to main content Enter the terms you wish to search for. Search History Organization Chart Work with Us Newsroom Careers Energy.gov Offices National Labs Office of Science Main navigation Office of Science Home About Us About Us Leadership History Honors and Awards Diversity, Equity & Inclusion Energy.gov Home Initiatives Initiatives Advanced and Sustainable Energy Artificial Intelligence and Machine Learning Genomics High Performance Computing Large Scale Scientific Instrumentation Quantum Information Science Mission Mission Science Programs Field Mission Support Office of Project Assessment Science & Innovation Science & Innovation National Labs Universities User Facilities PuRe Data Resources Science Highlights DOE Explains... SBIR/STTR Funding Funding Funding Opportunities Awards Budget Portfolio Analysis and Management System (PAMS) Resources Resources Newsroom Scientific and Technical Information Brochures, Logos, and Information Resources FACA Science HQ FOIA Requests CSC (Chicago and Oak Ridge) FOIA Requests Jobs button button Office of Science With X-Ray Analysis, an Asteroid Provides a View into Our Solar System’s Past June 24, 2024 Office of Science With X-Ray Analysis, an Asteroid Provides a View into Our Solar System’s Past Artwork showing the Hayabusa2 spacecraft retrieving a sample from the surface of the asteroid Ryugu. Image courtesy of Akihiro Ikeshita Imagine opening a time capsule, hoping to learn about the ancient past. Except, instead of a box or a chest, it’s an asteroid that could provide insights into the very dawn of life on Earth. That was the situation that researchers using the Advanced Light Source (ALS) faced. As the ALS is a Department of Energy (DOE) Office of Science user facility, the team that works there sees a lot of unusual items, from materials for solar cells to particles influenced by wildfires. But even for this crew, a sample from an asteroid was unusual. Fortunately, the innovative tools available at the ALS allowed them to support scientists digging into the history of these rocks delivered from space.Just like studying rocks on Earth can tell us about Earth’s early history, studying primitive small bodies such as asteroids, meteorites, and comets can tell us about our solar system’s history. Chondrites are a particularly useful type of meteorite. They are undifferentiated and chemically primitive. The rocks in them trace back to dust and small grains in the early solar system that came together to form a large parent body. A certain type of chondrites (called carbonaceous chondrites) preserve relatively abundant chemicals that are easily vaporized, including carbon and water. These are the building blocks of life on Earth. By studying these preserved materials, scientists can investigate one of humanity's fundamental questions: “Where did we come from?”  The team using the ALS examined a sample from the surface of a carbonaceous-type asteroid, Ryugu. They expected this asteroid to be similar to carbonaceous chondrite meteorites. Ryugu is relatively close to Earth, compared to asteroids in the main belt between Mars and Jupiter. Scientists hypothesize that Ryugu is a rubble-pile asteroid. They think that it formed when an object hit its parent body and then the rocks that were ejected re-coalesced into a new asteroid. After that process, the asteroid moved from the main belt to near-Earth orbit. The Japan Aerospace Exploration Agency (JAXA)’s spacecraft, Hayabusa2, collected samples from two locations on the surface of Ryugu in 2019 and returned them to Earth in 2020. The curatorial work at JAXA found a total of 5.4 g of sample. The agency allocated a small portion of the sample to the Hayabusa2 initial analysis team, consisting of about 400 scientists around the world. Hikaru Yabuta at Hiroshima University led one of six sub-teams of the initial analysis team. Ultrathin sections of the asteroid particles arrived at the ALS at DOE’s Lawrence Berkeley National Laboratory. The ALS allows scientists to precisely identify the elements and molecules inside materials. It uses a particle accelerator to produce extraordinarily bright X-ray beams. Like the X-rays at a doctor’s office, they reveal information about what is inside an object. But instead of just highlighting bones, these X-rays allow scientists to probe the chemical and structural properties of the matter itself. First, the team carefully scanned the sample in long horizontal rows—like text in a book—with X-rays. By measuring how the X-rays change as the scanning happens, scientists could identify individual grains of organic material in the asteroid sample. These grains were tiny – only 100 times bigger than a strand of DNA. Once the scientists identified grains of interest, they used X-rays to reveal the type of chemical bonds in the organic carbon grains. In this case, the researchers used the process to map out the various elements and functional groups (specific arrangements of atoms) in the sample. Based on this analysis, the scientists found four different types of carbon compounds as well as different types of structures. After identifying these materials, the scientists compared them to similar meteorites that they already knew the history of. Piecing together all of this data allowed them to outline a broad history of the asteroid during the early solar system, which formed about 4.6 billion years ago. The chemical compositions of the organic carbon in the samples indicated that Ryugu’s organic matter resulted from the precursors to that matter changing during a chemical reaction with liquid water on the asteroid’s parent body. The isotopes of carbon in the samples reflected that the organic precursors came from the extremely cold environment of space (about -200 °C). The team was the first to prove the direct link between organic matter in the carbonaceous asteroid and the similar organic matter in primitive carbonaceous chondrites (meteorites). There was one type of material notably missing – graphite. Graphite is a familiar form of carbon used in pencil leads. In asteroids, graphite or graphite-like material is a sign that the carbon was formed by radiogenic heating in parent bodies for several million years. The lack of it suggests that the sample collected from the asteroid was never exposed to heat above 390 °F (200 °C).Studying the material from Ryugu wasn’t the first or likely the last time that scientists will use the ALS to take a close look at rocks from space. Researchers used the ALS to analyze dust particles from the comet 81P/Wild 2 collected by NASA’s spacecraft Stardust in 2006. They found that the comet dust contained organic matter. This matter was composed of nitrogen- and oxygen-bearing chemical bonds as well as types of organic matter similar to that observed from the asteroid Ryugu and other chondritic meteorites.These studies demonstrated tools and techniques that have proven useful for analyzing samples like those from NASA’s OSIRIS-REx mission. This mission collected samples from the asteroid Bennu. In the fall of 2023, it returned them to Earth. The agency recently released a catalog of samples for scientists to study.  The ALS and other light sources allow us to draw lines from the earliest history of our solar system to today. Through shedding light on the objects in our current solar system, the DOE Office of Science scientists and user facilities may one day help us better understand how Earth became habitable. Shannon Brescher Shea Shannon Brescher Shea (shannon.shea@science.doe.gov) is the social media manager and senior writer/editor in the Office of Science’s Office of Communications and Public Affairs. more by this author Office of Science U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 (202) 586-5430 Sign Up for Email Updates Twitter Youtube Linkedin An office of About Office of Science Careers & Internships SC Home Contact Energy.gov Resources Budget & Performance Covid-19 Response Directives, Delegations & Requirements FOIA Inspector General Privacy Program Small Business Federal Government The White House USA.gov Vote.gov Web Policies Privacy No Fear Act Whistleblower Protection Notice of EEO Findings of Discrimination Information Quality Open Gov Accessibility Vulnerability Disclosure Program
  • 《Ultrafast and highly sensitive detection of SARS-CoV-2 spike protein by field-effect transistor graphene-based biosensors》

    • 来源专题:现代化工
    • 编译者:武春亮
    • 发布时间:2024-07-30
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(2014 - 2018)Waves Random Media (1991 - 2004) Volume number: Issue number (if known): Article or page number: Nanotechnology Purpose-led Publishing is a coalition of three not-for-profit publishers in the field of physical sciences: AIP Publishing, the American Physical Society and IOP Publishing. Together, as publishers that will always put purpose above profit, we have defined a set of industry standards that underpin high-quality, ethical scholarly communications. We are proudly declaring that science is our only shareholder. ACCEPTED MANUSCRIPT ? The following article is Open access Ultrafast and highly sensitive detection of SARS-CoV-2 spike protein by field-effect transistor graphene-based biosensors Thiago Alonso Alonso Stephan Lacerda Sousa1, Nathalie Almeida2, Fabrício Santos2, Priscilla Filgueiras3, Camila Corsini3, Camila Lacerda4, Thais Silva4, Rafaella F. Q. Grenfell5 and Flavio Plentz2 Accepted Manuscript online 26 July 2024 ? © 2024 The Author(s). Published by IOP Publishing Ltd What is an Accepted Manuscript? DOI 10.1088/1361-6528/ad67e8 Download Accepted Manuscript PDF Figures Skip to each figure in the article Tables Skip to each table in the article References Citations Article data Skip to each data item in the article What is article data? Open science Article metrics 1 Total downloads Submit Submit to this Journal Share this article Article and author information Author e-mailsthiagostephan@gmail.com Author affiliations1 Physics, Technical University of Denmark, Fysikvej B309, Lyngby, Hovedstaden, 2800, DENMARK 2 Physics, Universidade Federal de Minas Gerais, Av. Pres. Ant?nio Carlos, 6627, Pampulha, Belo Horizonte, MG, 31270-901, BRAZIL 3 Funda??o Oswaldo Cruz Instituto René Rachou, Av. Augusto de Lima, 1715, Barro Preto, Belo Horizonte, Minas Gerais, 30190-002, BRAZIL 4 Physics, Universidade Federal de Minas Gerais, Av. Pres. Ant?nio Carlos, 6627, Pampulha, Belo Horizonte, 31270-901, BRAZIL 5 Funda??o Oswaldo Cruz Centro de Pesquisas René Rachou, Rua Professor José Vieira de Mendon?a, 1000, Belo Horizonte, Minas Gerais, 30190-002, BRAZIL ORCID iDsThiago Alonso Alonso Stephan Lacerda Sousa https://orcid.org/0000-0001-8838-3648 Dates Received 13 March 2024 Revised 16 July 2024 Accepted 26 July 2024 Accepted Manuscript online 26 July 2024 Peer review information Method: Single-anonymous Revisions: 1 Screened for originality? Yes Journal RSS Sign up for new issue notifications 10.1088/1361-6528/ad67e8 Abstract The severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2), etiological agent for the coronavirus disease 2019 (COVID-19), has resulted in over 775 million global infections. Early diagnosis remains pivotal for effective epidemiological surveillance despite the availability of vaccines. Antigen-based assays are advantageous for early COVID-19 detection due to their simplicity, cost-effectiveness, and suitability for point-of-care testing (PoCT). This study introduces a graphene field-effect transistor-based biosensor designed for high sensitivity and rapid response to the SARS-CoV-2 spike protein. By functionalizing graphene with monoclonal antibodies and applying short-duration gate voltage pulses, we achieve selective detection of the viral spike protein in human serum within 100 μs and at concentrations as low as 1 fg/mL, equivalent to 8 antigen molecules per μL of blood. Furthermore, the biosensor estimates spike protein concentrations in serum from COVID-19 patients. Our platform demonstrates potential for next-generation PoCT antigen assays, promising fast and sensitive diagnostics for COVID-19 and other infectious diseases. Export citation and abstract BibTeX RIS As the Version of Record of this article is going to be / has been published on a gold open access basis under a CC BY 4.0 licence, this Accepted Manuscript is available for reuse under a CC BY 4.0 licence immediately. Everyone is permitted to use all or part of the original content in this article, provided that they adhere to all the terms of the licence https://creativecommons.org/licences/by/4.0 Although reasonable endeavours have been taken to obtain all necessary permissions from third parties to include their copyrighted content within this article, their full citation and copyright line may not be present in this Accepted Manuscript version. Before using any content from this article, please refer to the Version of Record on IOPscience once published for full citation and copyright details, as permissions may be required. 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