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Review of CIR-related Particle Composition, Charge States, & Energy Spectra

Review of CIR-related Particle Composition, Charge States, & Energy Spectra. Joe Mazur The Aerospace Corporation Glenn Mason Johns Hopkins/APL Joe Dwyer Florida Institute of Technology Mihir Desai Southwest Research Institute. Processes for 1 AU observations of solar material.

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C. Barclay FRAS Blackett Observatory Marlborough College

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Connections from Corona to Geospace

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A New Look at Some Solar Wind Turbulence Puzzles

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A New Look at Some Solar Wind Turbulence Puzzles

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Gas in Protoplanetary Disks

Gas in Protoplanetary Disks. Thomas Henning Max Planck Institute for Astronomy, Heidelberg. Frontiers Science Opportunities with JWST, Baltimore, 2011. Planet Formation: Stages. In presence of gas. In absence of gas. dust. Star & circumstellar (or protoplanetary ) disk. Dynamical

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Energy spectra of suprathermal and energetic ions at low solar activity

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photoelectron energy distribution for 1.6 eV photons

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Publications in Comparative Magnetospheres

Publications in Comparative Magnetospheres. Siscoe, G. L.: Towards a comparative theory of magnetospheres, in Solar System Plasma Physics, Vol. II , edited by C. F. Kennel, L. J. Lanzerotti, and E. N. Parker, North-Holland Publishing Co., 299-402, 1979.

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Phases of the Moon

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Voyager SSG November 3-4, 2011

Voyager Observations of Cosmic Rays in the Heliosheath. F.B. McDonald 1 , A.C. Cummings 2 , E.C. Stone 2 , B.C. Heikkila 3 , N. Lal 3 , W.R. Webber 4 1 Institute for Physical Science and Technology, Univ. of Maryland, College Park, MD, USA

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CISM Science Seminar Oct. 14, 2004

CISM Science Seminar Oct. 14, 2004. Fluid Dynamics of CME Expansion and Propagation. George Siscoe. 1. Statement of problem: Distinction between CME formation and CME propagation. 2. Why is this problem interesting and important?. 3. Relevance to CISM.

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ASTR 1101-001 Spring 2008

ASTR 1101-001 Spring 2008. Joel E. Tohline, Alumni Professor 247 Nicholson Hall [Slides from Lecture11]. Exam #1 Results. Total score composed of two parts: (g1) score on scale-model homework assignment is 25% (g2) score on in-class exam is 75% Where to find scores: g1 at bottom of exam

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39 th COSPAR Scientific Assembly Mysore, INDIA July 14-22, 2012

Voyager In The Distant Heliosheath: Continuing The Quest Of Victor Hess. F.B. McDonald 1 , W.R. Webber 2 , E.C. Stone 3 , A.C. Cummings 3 , B.C. Heikkila 4 , N. Lal 4 1 Institute for Physical Science and Technology, Univ. of Maryland, College Park, MD, USA

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21 - Interstellar Spaceflight

21 - Interstellar Spaceflight. THE PHYSICS OF SPACE TRAVEL (AS WE UNDERSTAND IT). For a spacecraft accelerating at a rate a , the velocity v reached and distance x traveled in a given interval of time t is:. c = speed of light. Accelerating at 1g = 9.8 m/s 2 :.

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Compositional signatures in the mix..

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The terrestrial planets

The terrestrial planets. What is terrestrial planet?. The four inner planets are considered terrestrial planets Terrestrial means made of rock Inner planets have a rocky composition compared to the outer planets. Mercury. Closest planet to the sun 0.39 AU from sun 0 moons

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Finding which solar events made it to interplanetary space

Finding which solar events made it to interplanetary space. Nariaki Nitta (LMSAL). It is important to compare jmaps with movies of images.

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Monday afternoon heliospheric properties of CMEs

Monday afternoon heliospheric properties of CMEs. DL: Alexis Rouillard (GMU/NRL/NASA): CME classification as a discussion starter. Slow CMEs: blobs, in-out pairs, blow-out, 3-part CMEs. All from flux ropes - Nobody actually disagreed officially. Fast CMEs: a more complicated mess.

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Ion Cyclotron Waves in the Inner Heliosphere

Ion Cyclotron Waves in the Inner Heliosphere. L.K. Jian 1 , C.T. Russell 1 , J.G. Luhmann 2 , X. Blanco-Cano 3. 1 IGPP & ESS, UCLA 2 SSL, UCB 3 IG, UNAM. SHINE session: New Questions about ENA, PUI, and ACR.

144 views • 1 slides