What are cosmic rays?
Dr J (Dr Jasmina) is an astronomer and lecturer at the School of Physics and Astronomy explains the connection between cosmic rays, the most energetic particles in the Universe, and supernova remnants (SNRs). Supernova remnants are very likely responsible for creating lower-energy cosmic rays. Active Galactive Nuclei (ie, massive black holes in the centre of active galaxies) are also linked to cosmic rays with higher energies.
Image credits (in order of appearance) and extra info:
Cosmic ray shower, artist's impression. Credit: ASPERA network
The magnetic field along the Galactic plane. Credit: ESA/Planck Collaboration. Acknowledgment: M.-A. Miville-Deschênes, CNRS – Institut d’Astrophysique Spatiale, Université Paris-XI, Orsay, France
http://www.esa.int/spaceinimages/Images/2014/12/The_magnetic_field_along_the_Galactic_plane
Supernova 1987A before and after. Credit: Australian Astronomical Observatory
http://oldweb.aao.gov.au/images/captions/aat050.html
SNR Cassiopeia A. Credit: X-ray: NASA/CXC/SAO; Optical: NASA/STScI; Infrared: NASA/JPL-Caltech/Steward/O.Krause et al.
http://chandra.harvard.edu/photo/2005/casa/
Kepler SNR. Credit: NASA
https://www.nasa.gov/multimedia/imagegallery/image_feature_219.html
SNR N49. Credit: X-ray: (NASA/CXC/Penn State/S.Park et al.); Optical: NASA/STScI/UIUC/Y.H.Chu & R.Williams et al
http://chandra.harvard.edu/photo/2010/n49/
SNR E0102-72. Credit: X-ray (NASA/CXC/SAO); optical (NASA/HST); radio: (ACTA)
Cygnus loop SNR (Veil nebula) in ultraviolet. Credit: NASA/JPL-Caltech
SNR B0509-67.5 Credit: Chandra, NASA, ESA, the Hubble Heritage Team (STScI/AURA), and NASA/CXC/SAO/J. Hughes
SN1006 in X-rays. Credit: Koyama et al., Nature, 378, 255, 1995
http://www-cr.scphys.kyoto-u.ac.jp/research/xray/xray-e.html#SN1006
https://heasarc.gsfc.nasa.gov/docs/objects/heapow/archive/nebulae/asca_sn1006.html
http://imagine.gsfc.nasa.gov/features/satellites/archive/asca_sn1006.html
VERITAS TeV gamma-ray count map of the region around Tycho's SNR, overlaid with X-ray emission from the SNR (black contours) and showing surrounding molecular clouds (magenta lines). Credit: Acciari et al., the Astrophysical Journal 730, L20, 2011
http://veritas.sao.arizona.edu/veritas-science/veritas-results-mainmenu-72/271-could-we-put-in-a-journal-reference-here-
How to make a Cloud Chamber (Cosmic Ray Detector)
https://youtu.be/_qbYvZ-Op4M
Mars with thicker atmosphere in the past and with the current, thinner atmosphere. Credit: NASA/GSFC
http://lasp.colorado.edu/home/wp-content/uploads/2013/04/wetmars_drymars.jpg
Mars rover Curiosity. Credit: NASA/JPL-Caltech
http://mars.nasa.gov/msl/mission/instruments/radiationdetectors/rad/
http://www.sci-news.com/space/science-mars-radiation-measurements-surface-01629.html
What are AGNs?
http://imagine.gsfc.nasa.gov/science/objects/active_galaxies2.html
Видео What are cosmic rays? канала MonashPhysicsAndAstronomy
Image credits (in order of appearance) and extra info:
Cosmic ray shower, artist's impression. Credit: ASPERA network
The magnetic field along the Galactic plane. Credit: ESA/Planck Collaboration. Acknowledgment: M.-A. Miville-Deschênes, CNRS – Institut d’Astrophysique Spatiale, Université Paris-XI, Orsay, France
http://www.esa.int/spaceinimages/Images/2014/12/The_magnetic_field_along_the_Galactic_plane
Supernova 1987A before and after. Credit: Australian Astronomical Observatory
http://oldweb.aao.gov.au/images/captions/aat050.html
SNR Cassiopeia A. Credit: X-ray: NASA/CXC/SAO; Optical: NASA/STScI; Infrared: NASA/JPL-Caltech/Steward/O.Krause et al.
http://chandra.harvard.edu/photo/2005/casa/
Kepler SNR. Credit: NASA
https://www.nasa.gov/multimedia/imagegallery/image_feature_219.html
SNR N49. Credit: X-ray: (NASA/CXC/Penn State/S.Park et al.); Optical: NASA/STScI/UIUC/Y.H.Chu & R.Williams et al
http://chandra.harvard.edu/photo/2010/n49/
SNR E0102-72. Credit: X-ray (NASA/CXC/SAO); optical (NASA/HST); radio: (ACTA)
Cygnus loop SNR (Veil nebula) in ultraviolet. Credit: NASA/JPL-Caltech
SNR B0509-67.5 Credit: Chandra, NASA, ESA, the Hubble Heritage Team (STScI/AURA), and NASA/CXC/SAO/J. Hughes
SN1006 in X-rays. Credit: Koyama et al., Nature, 378, 255, 1995
http://www-cr.scphys.kyoto-u.ac.jp/research/xray/xray-e.html#SN1006
https://heasarc.gsfc.nasa.gov/docs/objects/heapow/archive/nebulae/asca_sn1006.html
http://imagine.gsfc.nasa.gov/features/satellites/archive/asca_sn1006.html
VERITAS TeV gamma-ray count map of the region around Tycho's SNR, overlaid with X-ray emission from the SNR (black contours) and showing surrounding molecular clouds (magenta lines). Credit: Acciari et al., the Astrophysical Journal 730, L20, 2011
http://veritas.sao.arizona.edu/veritas-science/veritas-results-mainmenu-72/271-could-we-put-in-a-journal-reference-here-
How to make a Cloud Chamber (Cosmic Ray Detector)
https://youtu.be/_qbYvZ-Op4M
Mars with thicker atmosphere in the past and with the current, thinner atmosphere. Credit: NASA/GSFC
http://lasp.colorado.edu/home/wp-content/uploads/2013/04/wetmars_drymars.jpg
Mars rover Curiosity. Credit: NASA/JPL-Caltech
http://mars.nasa.gov/msl/mission/instruments/radiationdetectors/rad/
http://www.sci-news.com/space/science-mars-radiation-measurements-surface-01629.html
What are AGNs?
http://imagine.gsfc.nasa.gov/science/objects/active_galaxies2.html
Видео What are cosmic rays? канала MonashPhysicsAndAstronomy
Показать
Комментарии отсутствуют
Информация о видео
Другие видео канала
"Tuning" 2D materials for new computers - Dr Antonija Grubisic-CaboPHS3131 Special Relativity Lecture 6 David PaganinThe complicated lives of disc galaxies - Amelia Fraser McKelvieThe 2016 Robert Street Doctoral Prize in PhysicsAGB outflows shaped by wind-companion interactions - Jolien Malfait (KU Leuven)Introduction to First Year Physics in 2013 at Monash UniversityAngular Momentum IIUsing atomic Lego blocks to create future electronics - Dr Semonti BhattacharyyaConservation of momentumPHS3131 Special Relativity Lecture 5 David PaganinCollisional N-body simulations: black hole binary mergers and my love/hate relationship with FORTRANEwan Cameron: Understanding uncertainties in the photometric decomposition of galaxiesPHS3031 Tutorial #05 Quantum Mechanics - David PaganinSecond Year Physics Studies at Monash (part 2)PhysHooks - PilotBinary Evolution in Multiple-population Gas-enriched Globular Clusters - Mor Rozner (Technion)PHS3031 Tutorial #08 Quantum Mechanics - David PaganinGW190521: The imitation game - Juan Calderon BustilloTheoretical Perspectives on Probing BH Population with Astrometric Satellite Gaia - Minori ShikauchiPublic lecture: meet the Monash team behind the gravitational waves discoveryGreen Chemical Futures construction time lapse