'Ambient gas' diaporamas de présentation

Emilio Migneco

Emilio Migneco Erice ISCRA School 2004 Introduction to High energy neutrino astronomy Topics 1) Introduction to high energy neutrino astronomy Motivations for HE neutrino astronomy HE neutrino sources Neutrino telescopes operation principles Backgrounds

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(Some of the possible) Astrophysical origins of high energy cosmic rays

Lawrence Livermore Lab. California, 94550, USA. (Some of the possible) Astrophysical origins of high energy cosmic rays. Diego F. Torres dtorres@igpp.ucllnl.org. www.angelfire.com/id/dtorres. Summary. Plausible sources? Comments on basic observational features of the CR spectrum.

667 views • 43 slides

Physical conditions of the shocked regions in collimated outflows of planetary nebulae

Physical conditions of the shocked regions in collimated outflows of planetary nebulae. Angels Riera (UPC). OUTLINE. Identification: morphology and kinematics. Physical conditions in shocked regions of PNe: NGC 6543, NGC 7009, IC 4634.

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Post Injection Processes in Diesel Engines

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STRONG EXPLOSION MODEL OF GAS DYNAMICS OF A ROCKET PLUME IN THE UPPER ATMOSPHERE

STRONG EXPLOSION MODEL OF GAS DYNAMICS OF A ROCKET PLUME IN THE UPPER ATMOSPHERE. A.G. Molchanov, Yu.V. Platov. Typical value of combustion products pressure on a nozzle exit section of the rocket engine, operating in the upper atmosphere, makes ~ 0.005 MPa. As a pressure

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P RECIPITATION OF HIGH-ENERGY PROTONS AND HYDROGEN ATOMS INTO THE UPPER ATMOSPHERES OF MARS AND VENUS

P RECIPITATION OF HIGH-ENERGY PROTONS AND HYDROGEN ATOMS INTO THE UPPER ATMOSPHERES OF MARS AND VENUS. Valery I. Shematovich Institute of Astronomy, Russian Academy of Sciences.

259 views • 14 slides