and its effect on various processes

Slides:



Advertisements
Similar presentations
Tyler Thiele.  Cosmic rays are high energy charged particles, in outer space, that travel at nearly the speed of light and strike the Earth from all.
Advertisements

The Sun The Sun is a star. The Sun is a star. It is 4,500 million years old It is 4,500 million years old It takes 8 minutes for its light to reach.
Cosmic rays in solar system By: Tiva Sharifi. Cosmic ray The earth atmosphere is bombarded with the energetic particles originating from the outer space.
SPACE WEATHER Definition used by the US National Space Weather Plan: Conditions on the Sun and the solar wind, magnetosphere, ionosphere, and thermosphere.
Gravitational waves LIGO (Laser Interferometer Gravitational-Wave Observatory ) in Louisiana. A laser beam is.
Fusion Energy. Source of Energy Before 1940 the Sun’s energy was a mystery.  Chemical reactions:  Gravitational energy:  Nuclear forces: The Sun is.
Integrated Science Chapter 25 Notes
 The visible light we see is only a small amount of energy coming from various objects.  By studying other forms of energy, astronomers can learn more.
Sayfa 1 EP228 Particle Physics Department of Engineering Physics University of Gaziantep Dec 2014 Topic 5 Cosmic Connection Course web page
NASA/NSTA Web Seminar: Radiation – Can’t Live With It, Can’t Live Without It LIVE INTERACTIVE YOUR.
Space Radiation and Fox Satellites 2011 Space Symposium AMSAT Fox.
Nuclear Forces The power behind Stars. Fundamental Forces Gravity –Attractive force governed by mass Electromagnetism –Attractive or repulsive force that.
Solar Wind and Coronal Mass Ejections
Unit 12 – Nuclear Chemistry. Part II Key Terms Alpha decay – spontaneous decay of a nucleus that emits a helium nucleus and energy Beta decay – spontaneous.
NUCLEAR EQUATIONS Alpha Decay An alpha particle looks like a helium atom ( 4 2 He) massatomicmass reduces by 4,the atomic # reduces by 2 Examples: 238.
Space Environment SSE-120 Please type in your questions and raise your hand so we can answer it during class.
Fusion in the Stars Nunez & Panogalinog. Nuclear Fusion in stars is one of the most important reasons which make life on Earth possible! ○ HOW IS THAT.
3-4 Changes in the Nucleus
Cosmic rays at sea level. There is in nearby interstellar space a flux of particles—mostly protons and atomic nuclei— travelling at almost the speed of.
Nuclear Chemistry. Nucleus of an atom contains protons and neutrons Strong forces (nuclear force) hold nucleus together – Protons in nucleus have electrostatic.
Galactic Cosmic Rays (GCRS) Galactic cosmic rays (GCRs) come from outside the solar system but generally from within our Milky Way galaxy. GCRs are atomic.
Cosmic Rays2 The Origin of Cosmic Rays and Geomagnetic Effects.
Nuclear Chemistry. Nuclear Chemistry looks at the number of protons and neutrons in an atom Radioactive Decay = Spontaneous disintegration of a nucleus.
The Sun By: JGilliam The Sun’s CompositionIdentifying Stars Composition ▪ Hydrogen and Helium together make up 99% of the sun’s mass. ▪ 75% of the sun’s.
GROUP 4 Firdiana Sanjaya ( ) Ana Alina ( )
1. What is radioactivity? Radioactivity is the process in which an unstable atomic nucleus emits charged particles and energy. 2. What is a radioisotope?
NUCLEAR CHANGES. Nuclear Radiation Radioactivity: process by which an unstable nucleus emits one or more particles or energy in the form of electromagnetic.
COSMIC RAYS. At the Earth’ Surface We see cascades from CR primaries interacting with the atmosphere. Need to correct for that to understand their astronomical.
What is radiation  A form of energy that can move through empty space.  Transfer of energy by electromagnetic waves.
Some nuclei – usually large ones – are unstable They cannot fit their neutrons and protons into a space small enough that that strong nuclear force can.
Monday, May 4 th m.socrative.com 9bff6d58 Intro to Nuclear Chemistry.
Nuclear Reactions. The atoms of each element behave very differently, but they all have something very important in common. Every atom is made of the.
Chapter 19 Radioactivity
Topic 6 : Atomic and Nuclear Physics.
Atoms: The Building Blocks of Matter
Chemistry Nuclear Chemistry.
The Atomic Nucleus & Radioactive Decay
Nuclear Chemistry.
Geant4 and Microelectronics – Recent Successes, Looming Concerns
Introduction (Atomic and Nuclear Structure-Radioactivity)
The Atomic Nucleus & Radioactive Decay
R. Bucˇık , K. Kudela and S. N. Kuznetsov
Nuclear Chemistry Nuclear chemistry is the study of the properties and reactions of atomic nuclei. Radioactivity- the spontaneous emission of radiation.
Objectives: After completing this module, you should be able to:
Detecting Particles: The Spark Chamber
4-1 Early Ideas of the Atom
Chapter 10 Radioactivity and Nuclear reactions
Earth Chemistry.
NUCLEAR REACTOR MATERIALS
Reviewing Nuclear Chemistry
The Chemistry of the Solar System
PACKET #14: Nuclear Chemistry Reference Table: N and O
Nuclear Chemistry Chapter 21A
NUCLEAR CHEMISTRY.
The Sun.
Nuclear Reactions.
1.1.3 Explain how the sun produces energy which is transferred to the Earth by radiation. Sun’s Energy.
Nuclear Reactions.
The Centre of the Solar System Earth Science 11
Nuclear Reactions.
Radiochemical Methods
Nuclear Physics 243 NMT Dr. Abdo Mansour
Radioactivity Ch. 10.
Fundamental Forces of the Universe
Reviewing Nuclear Chemistry
Nuclear Chemistry Chapter 20.
Earth, Sun Chemistry.
Structure and Properties of Matter Isotopes
Chemistry Unit Two, Day Four.
CORONAL MASS EJECTIONS
Presentation transcript:

and its effect on various processes Сosmic radiation  and its effect on various processes

About cosmic radiation (cosmic rays) Cosmic rays are energetic charged subatomic particles, originating from outer space. They may produce secondary particles that penetrate the Earth's atmosphere and surface . Most primary cosmic rays (those which impact the atmosphere from deep space) are composed of familiar stable subatomic particles that normally occur on Earth, such as protons, atomic nuclei, or electrons. However, a very small fraction are stable particles of antimatter, such as positrons or antiprotons, and the precise nature of this remaining fraction is an area of active research. About 89% of cosmic rays are simple protons or hydrogen nuclei, 10% are helium nuclei or alpha particles, and 1% are the nuclei of heavier elements. These nuclei constitute 99% of the cosmic rays. Solitary electrons (much like beta particles, although their ultimate source is unknown) constitute much of the remaining 1%. The variety of particle energies reflects the wide variety of sources. The origins of these particles range from processes on the Sun (and presumably other stars as well), to as yet unknown physical mechanisms in the farthest reaches of the observable universe.

Changes in atmospheric chemistry Role in ambient radiation Cosmic rays ionize the nitrogen and oxygen molecules in the atmosphere, which leads to a number of chemical reactions. One of the reactions results in ozone depletion. The magnitude of damage, however, is very small compared to the depletion caused by CFCs Role in ambient radiation Cosmic rays constitute a fraction of the annual radiation exposure of human beings on the Earth. For example, the average annual radiation exposure in Australia is 0.3 mSv due to cosmic rays, out of a total of 2.3 mSv

Effect on electronics Cosmic rays have sufficient energy to alter the states of elements in electronic integrated circuits, causing transient errors to occur, such as corrupted data in electronic memory devices, or incorrect performance of CPUs, often referred to as "soft errors" (not to be confused with software errors caused by programming mistakes/bugs). This has been a problem in extremely high-altitude electronics, such as in satellites, but with transistors becoming smaller and smaller, this is becoming an increasing concern in ground-level electronics as well. Studies by IBM in the 1990s suggest that computers typically experience about one cosmic-ray-induced error per 256 megabytes of RAM per month. To alleviate this problem, the Intel Corporation has proposed a cosmic ray detector that could be integrated into future high-density microprocessors, allowing the processor to repeat the last command following a cosmic-ray event.

Significance to space travel Galactic cosmic rays are one of the most important barriers standing in the way of plans for interplanetary travel by crewed spacecraft. Since the intensity of cosmic rays is much larger outside the Earth's atmosphere and magnetic field, it is expected to have a major impact on the design of spacecraft that can safely transport humans in interplanetary space. Cosmic Rays also place a threat to electronics placed aboard outgoing probes. In 2010, a malfunction aboard the Voyager 2 space probe was credited to a single flipped bit, probably caused by a cosmic ray.

Role in lightning Cosmic rays have been implicated in the triggering of electrical breakdown in lightning. It has been proposed that essentially all lightning is triggered through a relativistic process, "runaway breakdown", seeded by cosmic ray secondaries. Subsequent development of the lightning discharge then occurs through "conventional breakdown" mechanisms. Role in climate change A role of cosmic rays directly or via solar-induced modulations in climate change was suggested by E.P.Ney in 1959 and by Robert Dickinson in 1975. In recent years, the idea has been revived most notably by Henrik Svensmark; the most recent IPCC study disputed the mechanism, while the most comprehensive review of the topic to date states: "evidence for the cosmic ray forcing is increasing as is the understanding of its physical principles"

Thank you for your attention =) Link: http://en.wikipedia.org/wiki/Cosmic_radiation Thank you for your attention =)