Quiz Me ! Cosmic Ray Electron Propagation Cosmic Ray Nucleon Transport Spectral Index Modelling – NGC 891 & NGC 253 Diffuse γ-Ray Modelling.

Slides:



Advertisements
Similar presentations
Introduction to Astrophysics Ronald L. Westra Department Mathematics Maastricht University.
Advertisements

Astronomy and the Electromagnetic Spectrum
25 ii 2011NASM1 Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes Roger Blandford KIPAC Stanford.
Detection of Gamma-Rays and Energetic Particles
Detecting Particles: The Spark Chamber Particle Physics Masterclass Stephen A. Bull Tuesday 24 th April 2007.
Cosmic rays in solar system By: Tiva Sharifi. Cosmic ray The earth atmosphere is bombarded with the energetic particles originating from the outer space.
Terrestrial Gamma-ray Flashes. Gamma Ray Astronomy Beginning started as a small budget research program in 1959 monitoring compliance with the 1963 Partial.
What is High-Energy Astrophysics? What is studied by high-energy astrophysicists: Supernovae Supernovae remnants Pulsars/magnetars Gamma-ray bursts Accreting.
Diffuse Gamma-Ray Emission Su Yang Telescopes Examples Our work.
High Altitude Research Laboratory Astrophysical Sciences Division Bhabha Atomic Research Centre Gulmarg Kashmir. M. A. Darzi.
The Transient Universe: AY 250 Spring 2007 New High Energy Telescopes Geoff Bower.
Gravitational waves LIGO (Laser Interferometer Gravitational-Wave Observatory ) in Louisiana. A laser beam is.
Victor Hess Before making balloon ascents himself, he determined the height at which ground radiation would stop producing ionization (about 500 meters)
Survey of the Universe Greg Snow U Nebraska Lincoln CROP.
07/05/2003 Valencia1 The Ultra-High Energy Cosmic Rays Introduction Data Acceleration and propagation Numerical Simulations (Results) Conclusions Isola.
● What a cosmic ray (CR) and a ultra high energy cosmic ray (UHECR) are? ● What do we know and what we would like to know about them? ● How do we detect.
History 1785 Charles Coulomb, 1900 Elster and Geitel Charged body in air becomes discharged – there are ions in the atmosphere 1912 Victor Hess Discovery.
Survey of the Universe We live in an expanding Universe What’s within 50 Megaparsecs = 150 Million Light Years from us? Why is this distance relevant to.
Cosmic Rays Discovery of cosmic rays Local measurements Gamma-ray sky (and radio sky) Origin of cosmic rays.
LHC ~E -2.7 ~E -3 ankle 1 part km -2 yr -1 knee 1 part m -2 yr -1 T. Gaisser 2005 Nature accelerates particles 10 7 times the energy of LHC! where?how?
High-energy emission from the tidal disruption of stars by massive black holes Xiang-Yu Wang Nanjing University, China Collaborators: K. S. Cheng(HKU),
 Celestial Sphere  Imagine a sphere that surrounds our planet in which all the stars are attached. This sphere is allowed to rotate freely around the.
Cosmic Rays Liz Puchnarewicz Mullard Space Science Laboratory University College London
Sponge: List the six layers of the Earth.. Atmosphere A mixture of gases: N 2 78% O 2 21% Ar0.9% CO %
Nebular Astrophysics.
High-Energy Astrophysics
COSMIC RAYS An Overview Dr. Darrel Smith Department of Physics Embry-Riddle Aeronautical University Prescott, AZ
Chapter 24 Studying the Sun Who is Stan Hatfield and Ken Pinzke.
International research project GALA: Monitoring of high energy gamma-ray astrophysical sources.
Milagro Gus Sinnis Milagro NSF Review July 18-19, 2005 Milagro: A Synoptic VHE Gamma-Ray Telescope Gus Sinnis Los Alamos National Laboratory.
EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens 
At the start of the 20th century scientists became very interested in a puzzling phenomena. There seemed to be rather more radiation in the environment.
Plasma universe Fluctuations in the primordial plasma are observed in the cosmic microwave background ESA Planck satellite to be launched in 2007 Data.
Space Science MO&DA Programs - September Page 1 SS It is known that the aurora is created by intense electron beams which impact the upper atmosphere.
By Dr. A. Mahrous Helwan University - EGYPT By Dr. A. Mahrous Helwan University - EGYPT.
Cosmic Rays GNEP Teacher Workshop Steve Shropshire, July 2007.
Space Environment SSE-120 Please type in your questions and raise your hand so we can answer it during class.
Chapter 9 Our Star, the Sun. What do you think? What is the surface of the Sun like? Does the Sun rotate? What makes the Sun shine?
Discovery of  rays from Star-Forming Galaxies New class of nonthermal sources/gamma-ray galaxies (concept of temperature breaks down at high energies)
Lepton - Photon 01 Francis Halzen the sky the sky > 10 GeV photon energy < cm wavelength > 10 8 TeV particles exist > 10 8 TeV particles exist Fly’s.
Application of neutrino spectrometry
1 High Energy Radiation from Black Holes Gamma Rays, Cosmic Rays, and Neutrinos Chuck Dermer Naval Research Laboratory Govind.
Cosmic rays and solar flares Draw in the back of your book the life cycle of a star.
SN 1987A as a Possible Source of Cosmic Rays with E 0 < eV by Yakutsk EAS Array Data A.V. Glushkov, L.T. Ksenofontov, M.I. Pravdin Yu.G. Shafer Institute.
Characterizing cosmic ray propagation in massive star forming regions: the case of 30 Dor and LMC E. J. Murphy et al. Arxiv:
Earth is surrounded by a mixture of gases known as the Atmosphere
THE OZONE LAYER HOLE.
Diffuse Emission and Unidentified Sources
Where do ultra-high energy cosmic rays come from? No one knows the origin of ultra-high energy cosmic rays. The majority of low-energy cosmic ray particles.
Victor Hess in his balloon (1912). Cosmic Rays Produce Muons in the Atmosphere.
Astroparticle physics with large neutrino detectors  Existing detectors  Physics motivation  Antares project  KM3NeT proposal M. de Jong.
Propagation of CR electrons and the interpretation of diffuse  rays Andy Strong MPE, Garching GLAST Workshop, Rome, 17 Sept 2003 with Igor Moskalenko.
1 Probing MHD Shocks with high-J CO observations: W28F SOFIA Observations 1.W28 is a mature supernova remnant (>2x10 4 yr old) located in the Inner Galaxy.
Gamma-ray Measurements of the distribution of Gas and Cosmic Ray in the Interstellar Space Yasushi Fukazawa Hiroshima University.
Extreme Astrophysics the the > 10 GeV photon energy < cm wavelength > 10 8 TeV particles exist > 10 8 TeV particles exist they should.
Earth’s Atmosphere.
Ching-Yuan Huang (黄庆元) 20 October 2010
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.
Do Now What did you make your content poster on? How does your content poster express they way you interpret that vocabulary word?
 What are Cosmic Rays? A short history What do we know now about CRs  What are Extensive Air Showers? A short history How to detect EAS? Back to CR –
June 19, 2008University of Illinois at Urbana-Champaign 1 Constraining the Low-Energy Cosmic Ray Spectrum Nick Indriolo, Brian D. Fields, Benjamin J. McCall.
Sponge: List the six layers of the Earth.
Hadron Production Measurements
Planetary Discovery in the era of Spacecraft Exploration Xi Zhang
24.1 The Study of Light Electromagnetic Radiation
Electromagnetic spectrum part 2
Shown in this NASA/ESA Hubble Space Telescope image, the supernova remnant, surrounded by inner and outer rings of material, is set in a forest of ethereal,
Electromagnetic spectrum part 2
Chapter 26: Stars and Galaxies
PH3520 / Particle Physics Autumn term 2010 – week 6
Presentation transcript:

Quiz Me ! Cosmic Ray Electron Propagation Cosmic Ray Nucleon Transport Spectral Index Modelling – NGC 891 & NGC 253 Diffuse γ-Ray Modelling

Cosmic rays were first determined to be coming from outer space when … a sharp increase in cosmic rays was observed when E.T. was released in 1982 Michelson & Morley performed their famous experiment in 1887 determining that there was no ether surrounding the earth. Viktor Hess, in 1912, carried ionization chambers to high altitudes and detected an increase in radiation as he ascended. August 7 th, 1912

The project based in Utah & Argentina that, when completed will be the largest cosmic ray detection array ever built, is known as … the Blair Witch project the Manhattan project Pierre Auger project

The highest ever detected energy of a cosmic ray is … ~ 3 [eV] ~ [eV] ~ [eV]

How long are CRs trapped in the Galaxy ? ~ [sec] ~ 20 million [years] ~ Hubble Time

Cosmic rays are caused by … the sun supernova remnants flying monkeys

Large Area TelescopeEGRET Energy Range20 MeV – 300 GeV30 MeV – 10 GeV Peak Effective Area> 8000 cm cm 2 Field of View> 2 sr0.5 sr Angular Resolution < 3.5 o (at 100 MeV) 10 GeV) 5.8 o (at 100 MeV) Point Source Sensitivity< 6·10 -9 cm -2 s cm -2 s -1

boundary between a diffusion dominated and convection dominated regime

solution in the disk

Cosmic rays are responsible for … the expansion of the universe causing cancer among airline passengers aurorae the depletion of the ozone layer New theory predicts the largest ozone hole over Antarctica will occur this month – Cosmic Rays at fault University of Waterloo,Sept., 2008

with