Innovation New Jersey
  • Home
  • Our Coalition
    • Contact Us
  • News
  • Resources
    • State Supports
    • Federal Supports
    • Higher Ed Supports
  • Join Us

Innovation News

Everything Innovation. Everything New Jersey.
Follow us and stay connected.

NJIT Scientists Shed Light on How Solar Blasts Accelerate Particles to Nearly the Speed of Light

12/6/2015

0 Comments

 
Newark, NJ - For scientists studying the impacts of space weather, one of the central mysteries of solar flares – the colossal release of magnetic energy in the Sun’s atmosphere that erupts with the force of millions of hydrogen bombs – is the means by which these explosions produce radiation and accelerate particles to nearly the speed of light within seconds. The most powerful blasts dispatch energized particles that can penetrate Earth’s atmosphere within an hour, disrupting orbiting satellites and electronic communications on the ground.
In an article published in Science magazine this week, “Particle acceleration by a solar flare termination shock,” solar scientists at several institutions, including NJIT, have shed light on an elusive structure known as a termination shock that is believed to play a key role in converting released magnetic energy from flares into kinetic energy in accelerated particles. Through a recent set of observations captured by a large radio telescope, the Jansky Very Large Array, they have imaged a shock and its time evolution during a long-lasting solar flare and demonstrated its role in accelerating particles.

​“Although predicted by theoretical models, this is the first time we have had direct images and movies showing the repeated formation, disruption, and reformation of a termination shock, enabling us to link it directly to particle acceleration,” said Dale Gary, distinguished professor of physics at NJIT and one of the authors of the article. Bin Chen, an astrophysicist at the Harvard Smithsonian Center for Astrophysics who will join NJIT next January, is the article’s lead author.

The powerful shocks occur when high-speed jets expelled from the explosive energy-release site of a solar flare collide with stationary plasma below.  One surprising result is that, occasionally, some jets can disrupt the shock, after which the shock takes time to reform.  During the disruptions, radio and X-ray emission due to accelerated particles is observed to decrease not just at the shock, but throughout the emitting region, showing that the shock is at least partly responsible for accelerating those particles.

The observations were made possible by the ability of the newly enhanced Karl G. Jansky Very Large Array (VLA) in New Mexico to acquire the more than 40,000 individual images per second of observation needed to resolve the rapidly varying emission features produced by the termination shock.  This level of resolved detail allowed the firm identification of the radio source as a shock and revealed its dynamic evolution.  Chen, who took part in significant upgrades of the VLA which made these observations possible, developed the technique to visualize the shock dynamics from the millions of images taken during the event. 

“We have been studying the Sun for many years using observations of its light in a broad range of wavelengths, but we have been unable to observe some of its activities in detail, including those related to particle acceleration,” Chen said. “Radio telescopes, which are now able to capture tens of thousands of images per second through various frequencies, are giving us much more information on what was previously hidden.”

Solar flares erupt when stored magnetic energy is suddenly released and converted to other forms, such as high-energy particles, hot plasma at millions of degrees, intense electromagnetic radiation and plasma eruptions called coronal mass ejections (CMEs). Solar radiation from the primary flare and that generated secondarily from CMEs can affect Earth in many ways.  The high-energy particles can destroy the electronic systems in satellites used in telecommunications, weather forecasting and navigation systems, among other services.  The electromagnetic radiation can interfere directly with communication and navigation signals, ionize the atmosphere, and cause short-wave radio black-outs.  Associated magnetic disturbances can also affect devices on the ground such as power transformers.

The study of flares began in 1859 following what is known as the Carrington Event, a solar flare and associated geomagnetic storm so powerful that it electrified telegraph wires, causing spark discharges that caught paper on fire, caused world-wide magnetic disturbances, and was visible across the globe in the form of auroras. That storm was by some estimates four orders of magnitude stronger than the flare described in the Science article.

“A flare the size of the Carrington event would pose real danger today because of our increasing reliance on susceptible technology,” Gary said. “Big events are difficult to predict, however. We have ways of measuring energy build-up, but sometimes when we think a large flare will occur, the energy dissipates quietly or in a series of smaller events instead. Studies like ours provide better understanding of the fundamental processes occurring in flares, and may one day lead to better predictions.”

NJIT is expanding its own, solar-dedicated radio telescope, the Expanded Owens Valley Solar Array, to observe the Sun every day with many of the same observational capabilities.  Multi-frequency imaging with high frequency and time resolution will become a standard method of studying solar flares in the near future.
“The VLA observes all sorts of astronomical targets and so the amount of time allotted to focus on the Sun amounts to less than a week per year. Owens Valley observes the Sun 24 hours a day,” said Chen, who called the star – “reasonably close” at 93 million miles away – “the best laboratory for studying a broad range of physical processes that occur across the Universe.”
0 Comments



Leave a Reply.

    Do not miss a single innovative moment and sign up for our newsletter!
    Weekly updates


    Categories

    All
    3D Printing
    Academia
    Acquisitions
    Aerospace
    Agriculture
    AIDS
    Algae
    Alumni
    Animals
    Architecture
    Astrophysics
    Autism
    Awards
    Big Data
    Bioethics
    Biofuel
    Biomedical
    BioNJ
    Bioterrorism
    Bit Coins
    Brain Health
    Business
    Camden
    Cancer
    CCollege
    Cellular
    Centenary
    Chemistry
    ChooseNJ
    Climate Change
    Clinical Trials
    Cloud Tech
    Collaboration
    Computing
    Congress
    Coriell
    Council On Innovation
    Crowdfunding
    Cybersecurity
    DARPA
    Defense
    Degree
    Dementia
    Dental Health
    DOC
    DOD
    DOE
    Drew
    Drones
    Drug Creation
    Einstein's Alley
    Electricity
    Energy
    Engineering
    Entrepreneurship
    Environmental
    FAA
    Fairleigh Dickinson
    FDA
    Federal Budget
    Federal Government
    Federal Labs
    Federal Program
    Finance
    Food Science
    Fort Monmouth
    Fuel Cells
    Funding
    Genome
    Geography
    Geology
    Global Competition
    Google
    Governor Christie
    Grant
    Hackensack
    HackensackUMC
    Healthcare
    Health Care
    HHS
    HINJ
    Hospitals
    Immigration
    Incubator
    Infrastructure
    International
    Internet
    Investor
    IoT
    IP
    IT
    Jobs
    Johnson & Johnson
    K-12
    Kean
    Kessler
    Legislation
    Logistics
    Manufacturing
    Medical Devices
    Med School
    Mental Health
    Mentor
    Microorganisms
    Molecular Biology
    Montclair
    NAS
    Neuroscience
    Newark
    New Jersey
    NIFA
    NIH
    NIST
    NJBDA
    NJBIA
    NJ Chemistry Council
    NJCU
    NJDOLWD
    NJEDA
    NJEDge
    NJHF
    NJII
    NJIT
    NJMEP
    NJPAC
    NJPRO
    NJTC
    Nonprofit
    NSF
    OpEd
    Open Data
    OSHE
    OSTP
    Parasite
    Patents
    Paterson
    Patients
    Perth Amboy
    Pharma
    POTUS
    PPPL
    Princeton
    Prosthetics
    Ranking
    Rare Disease
    R&D Council
    Report
    Resiliency
    Rider
    Robotics
    Rowan
    Rutgers
    SBA
    Seton Hall
    Siemens
    Smart Car
    Smart Cities
    Software
    Solar
    Space
    SSTI
    Startup
    State Government
    STEM
    Stevens
    Stockton
    Subatomic
    Supports
    Sustainability
    Taxes
    TCNJ
    Teachers
    Telecom
    Therapy
    Thermodynamics
    Transportation
    Undergraduate
    USEDA
    Verizon
    Video Game
    Virtual Reality
    Water
    WHO
    William Paterson
    Women In STEM
    Workforce Development

Home   Coalition   News   Resources   Events   Join Us
Picture
Innovation New Jersey Coalition
10 West Lafayette Street
Trenton, NJ 08608-2002
609-858-9507