'Magnetic field evolution' diaporamas de présentation

Magnetic field evolution - PowerPoint PPT Presentation

Lecture 5. Population synthesis of NSs

Lecture 5. Population synthesis of NSs

Lecture 5. Population synthesis of NSs. Sergei Popov (SAI MSU). Population synthesis in astrophysics. A population synthesis is a method of a direct modeling of relatively large populations of weakly interacting objects with non-trivial evolution.

★ ★ ★ ★ ★

503 views • 50 slides
Deflections of Ultra High Energy Cosmic Rays by Intergalactic Magnetic Fields

Deflections of Ultra High Energy Cosmic Rays by Intergalactic Magnetic Fields

Deflections of Ultra High Energy Cosmic Rays by Intergalactic Magnetic Fields. Based on astro-ph/0310902 with. Klaus Dolag (Dipartimento di Astronomia - Padova Volker Springel (Max Planck Institute for Astrophysics - Munich) Igor Tkachev (CERN ). Ultra High Energy Cosmic Rays.

★ ★ ★ ★ ★

697 views • 49 slides
Population synthesis of INSs

Population synthesis of INSs

Population synthesis of INSs. Population synthesis in astrophysics. A population synthesis is a method of a direct modeling of relatively large populations of weakly interacting objects with non-trivial evolution.

★ ★ ★ ★ ★

618 views • 48 slides
Spin evolution of NSs

Spin evolution of NSs

Spin evolution of NSs. Evolution of neutron stars. Magneto- rotational. Thermal. Observational appearence of a NS can depend on: Temperature Period Magnetic field Velocity. Evolution of NSs: temperature. Neutrino cooling stage. Photon cooling stage. First papers on the thermal

★ ★ ★ ★ ★

437 views • 43 slides
Observing magnetic fields in star-forming regions

Observing magnetic fields in star-forming regions

Observing magnetic fields in star-forming regions. Jim Cohen. 17 th February 2004. The University of Manchester Jodrell Bank Observatory. Zwolle Workshop. Outline of Talk. Introduction Polarization Mechanisms Zeeman Splitting Maser Regions.

★ ★ ★ ★ ★

537 views • 36 slides
Magnetic field evolution of accreting neutron stars

Magnetic field evolution of accreting neutron stars

Magnetic field evolution of accreting neutron stars. Ya.N. Istomin P.N. Lebedev Physical Institute, Moscow, Russia. Accreting electric current. Depth of penetration into the crust. Critical magnetic field. Superconducting vortices. There exists the minimal magnetic field. Conclusion:

★ ★ ★ ★ ★

132 views • 12 slides

View Magnetic field evolution PowerPoint (PPT) presentations online in SlideServe. SlideServe has a very huge collection of Magnetic field evolution PowerPoint presentations. You can view or download Magnetic field evolution presentations for your school assignment or business presentation. Browse for the presentations on every topic that you want.