... SN 1006: Pieces of the Cosmic Ray Puzzle . ... Credit: E. Gotthelf ( Columbia University ), ASCA Project, NASA Explanation: Research balloon flights conducted in 1912 by Austrian physicist Victor Hess revealed that the Earth was constantly bombarded by high energy radiation from space - which came to be called "Cosmic Rays" . ... If (as expected) high energy protons are associated with these energetic electrons then supernova remnants like SN 1006 are sources of Hess' puzzling Cosmic Rays . ...

Neutron Monitors ] [ Solar Neutrons ] [ Muon Telescopes ] [ Base Potchefstroom University ] [ Magnetometers ] [ GPS systems ] [ Ionosphere ] [ Related Data ] [ Space Weather ] . ... All Cosmic Ray Stations + InterPlanetary Data: WorldNet . Alma-AtaB (Mt.Tien Shan) DataBase of Kazakhstan Spectrograph Alma-AtaB (Mt.Tien Shan) new . ... Nagoya Muon Telescope and DATA or mail . ... Belgrade Muon Telescopes and DATA or ">mail . ... Real-Time database for Cosmic Ray Anisotropy (DB10) . ...

Main News Phones Research area Brief history Institute Structure Experimental Base Observational data English/Russian . research on the site(Google) . ... 677980 Yakutsk, Russia . ... 7(4112)390400 . Fax: . 7(4112)390450 . ... The Yakutsk Cosmic Ray Spectrograph . ... Phone: +7(4112) 390-455 . Fax: +7(4112) 390-450 . ... The cosmic ray spectrograph is located near Yakutsk . ... cosmic ray intensity in energy range from 2 to 300 Gev . ... ground-based muon telescope . ...

... October 16, 1996 . SN 1006: Pieces of the Cosmic Ray Puzzle . ... Explanation: Research balloon flights conducted in 1912 by Austrian physicist Victor Hess revealed that the Earth was constantly bombarded by high energy radiation from space - which came to be called "Cosmic Rays" . ... If (as expected) high energy protons are associated with these energetic electrons then supernova remnants like SN 1006 are sources of Hess' puzzling Cosmic Rays . ... About APOD | ...

... If two or more spectra have been taken under the same conditions, a very efficient way of removing particle hits from the raw data is to replace pixel values with large deviations from other observations with a local estimator, as done in the command COMBINE/LONG . If multiple images are not available, cosmic ray hits have to be filtered out by a different method. ... where subframe defines the region to filter. ... This step is done twice to remove the hits on the sky on each side of the object. ...

We cannot observe the way the distant universe accelerates cosmic rays or produces energetic photons, but acceleration processes also occur on our Sun , though on a much more moderate scale. ... That is why such events are often missed by cosmic ray detectors near the equator, where the lowest energies are excluded by the Earth's magnetic field. The best detectors for observing solar particles are therefore those sensitive to the lowest energies of the cosmic radiation. ...

... HST . ... Data . ... HST Overview . Overview . ... Phase I Proposing . ... DrizzlePac . ... ACS ETC . ... Note that with MultiDrizzle added to the pipeline (~Sep 2004), image combination (including cosmic ray rejection) will be performed for any type of associated dataset, using the parameters contained in the MDRIZTAB reference files. file_name delivery pedigree comment n4e12511j_crr 04/17/03 INFLIGHT WFC CR-rejection table n4e12510j_crr 04/17/03 INFLIGHT HRC CR-rejection table Copyright | ...

BNO is in Baksan Gorge at the Northern Caucasus . ... The Baksan Underground Scintillation Telescope (BUST) of volume 3000 cubic centimeters at a depth of more 300 m. The mountainous plant ANDYRCHI to register wide air showers located over BUST on the area 5*10 4 square metres. The complex of surface plants KOVER including a large muon detector, a scintillation telescope and a neutrino monitor meant for studying the hard component of cosmic rays and wide air showers. ...

... Magnetic Storms . ... Cosmic Rays . ... Energetic Particles . ... Solar fast Particles . We cannot observe the way the distant universe accelerates cosmic rays or produces energetic photons, but acceleration processes also occur on our Sun , though on a much more moderate scale. ... That is why such events are often missed by cosmic ray detectors near the equator, where the lowest energies are excluded by the Earth's magnetic field. ... Should we be concerned about solar energetic radiation? ...

... Cosmic radiation is capable of depositing significant quantities of energy and momentum in gravitational wave antennas at times which will generally be random with respect to gravitational signals. Such cosmic ray effects may generate noise signals at detectable levels compared to antenna design thresholds at rates of a few per year but, since antennas will not be capable of absorbing all the cosmic ray energy, it should be readily possible to construct vetoing cosmic ray detectors. ...

Cosmic ray intensities (left) compared with predictions (right) from IBEX. The similarity between these observations and predictions as evidenced by the similar color regions supports the local galactic magnetic field direction determined from IBEX observations made from particles at vastly lower energies than the cosmic ray observations shown here. The blue area represents regions of lower fluxes of cosmic rays. ...

... CfA Home . HCO Home . SAO Home . ... Welcome to CfA . CfA History . ... Laboratory Astrophysics . Extreme Astrophysics . ... 617) 495-7210 . ... 617) 495-7044 . ... 617) 495-7265 . ... HEA Research . ... HEA Home Page . CFA/HEA Home Page . ... High Energy Astrophysics Division (HEAD) . Chandra X-ray Center . ... Chandra Cluster Cosmology Project . Chandra Multiwavelength Project (ChaMP) . ... Chandra-Planck Clusters Project . ... CfA Virtual Observatory Project . ...

297 Fax: +39 055 220039 Scientific Career · · · · · · · · · · 2004 - Present: Associate Professor 2014 ­ Present: Professor of Cosmic Ray Physics and Astrophysics , GSSI, L'Aquila September ­ November 2009: Visiting Scientist, Kavli Institute , Santa Barbara, California, USA October 2007 - September 2008: Visiting Scientist, Center for Particle Astrophysics , Fermi National Accelerator Laboratory, Fermilab, USA 2004 - 2006: Visiting Professor of Cosmic ...

Next: Population Synthesis of X-ray Up: Cosmic Rays and Evolution Previous: Supernova Explosions . Immediately after the discovery of pulsars, especially of the Crab pulsar,   it became clear that rapidly rotating NS are copious sources of relativistic particles. ... Figure 37: Evolution of magnetorotational energy of NS in elliptical and spiral galaxies. ...

... It is notoriously difficult to identify weak cosmic ray events in long exposure observations. ... The method is to compare the probability distribution function (PDF) of cosmic ray events between an observation and a dark frame matched in exposure time. We illustrate the basic idea using dark exposures from a Tek 1024 1024 CCD with varying exposure lengths and read-out times. ... Figure: Histogram of cosmic ray events in a two hour dark frame. ... Original PostScript figure (78 kB) . ...

... Science Users Information > Science Activities > Science in Garching > Research Area: COSMOLOGY AND THE EARLY UNIVERSE . ... Research Area: COSMOLOGY AND THE EARLY UNIVERSE . ... Reset view all 3 per page 5 per page 10 per page Sort by Title A-Z Title Z-A Date asc Date desc Research Topics Planets and Star Formation Stellar Structure and Evolution Stellar Populations Evolution of Galaxies and the ISM Cosmology and the Early Universe Scientific Positions Faculty Fellows Scientists Students . ...

NATIONAL ASTRONOMY AND IONOSPHERE CENTER . ... Astronomy . ... Information . Visitor Center . ... The Observatory . ... Research Areas . ... Radio Astronomy is the study of natural radio energy emitted by galaxies, erupting stars, clouds of gas, pulsars and quasars. The Arecibo Radio Telescope enables astronomers to detect the faint radio emissions from these far off regions of the universe. ... This weak radio echo is collected, focused and detected by the Arecibo Telescope. ...

April 4, 2008 (Friday) Maxim Pospelov, Victoria University . ... Fall 2007 . Winter 2008 . Fall 2006 . Winter 2007 . Spring 2007 . ... A new generation cosmic ray detector, the Pierre Auger Observatory, has been designed to study cosmic rays with energy above 10 18 eV and answer the crucial questions of ultra high energy cosmic ray physics. ... Oscillating scalar fields, with an oscillation frequency much greater than the expansion rate, have been proposed as models for dark energy. ...

... About INTEGRAL . INTEGRAL is a European (ESA) Gamma-Ray Observatory Satellite Mission for the study of cosmic gamma-ray sources in the keV to MeV energy range. ... The PROTON launcher injected the satellite into a transfer orbit and INTEGRAL's own propulsion system brought the satellite into its 72 hours eccentric operational orbit with an apogee of 153600 km and an inclination of 52.5 degrees. More details on ESA website dedicated to INTEGRAL mission. 2016 IKI RAN ...

... Staff at the Armagh Observatory carry out research in the following principal areas: . ... Solar System Astronomy , including celestial mechanics, numerical and semi-analytic methods, the origin and dynamical evolution of comets, asteroids and meteorites, the evolution of interplanetary dust; the formation of Edgeworth-Kuiper belt objects, the origin and evolution of planetary systems, and the structure and evolution of extra-solar planetary systems. ... A few highlights from 1998: . ...