# 'Number density' presentation slideshows

## Progress Towards Developing a Self-Consistent Model for the Production and Transport of SEPs by CME-Driven Shocks

Progress Towards Developing a Self-Consistent Model for the Production and Transport of SEPs by CME-Driven Shocks. Ilia Roussev, Igor Sokolov, Valeriy Tenishev and Tamas Gombosi University of Michigan Marty Lee, Chee Ng, Allan Tylka, and Jozsef Kóta Collaborators. Objectives. Background:

By paul2
(263 views)

## Lecture 6

Lecture 6. The radiation field and opacity. Review. The main sequence is a mass sequence More massive stars are closer to the top-left (hot and bright). M=30M Sun. M=M Sun. M=0.2M Sun. Radiation intensity.

By raiden
(211 views)

## The volume occupied by any lump of matter is due primarily to it’s atoms’ A ) electron clouds B ) protons C ) nuc

The volume occupied by any lump of matter is due primarily to it’s atoms’ A ) electron clouds B ) protons C ) nuclei D ) other. The mass of matter is due primarily to it’s A ) electron cloud B ) nuclei C ) other. If atoms are mostly empty space ,

By robbin
(128 views)

## QUESTIONS

QUESTIONS. 1. What is the most abundant greenhouse gas in the Earth’s atmosphere? 2. What is the radiative equilibrium temperature of the Earth’s surface at the poles in winter? What prevents this temperature from ever being achieved?

By nara
(177 views)

## On-line Detector Methods…and a peak at possibly better things to come.

On-line Detector Methods…and a peak at possibly better things to come. Theme: being average (and averages generally) suck.

By antione
(109 views)

## Buffer Gas Cooling of atomic and molecular beams

Wenhan Zhu Princeton University 11/06/2007. Buffer Gas Cooling of atomic and molecular beams. Basic idea. The technique relies on thermalization of the species-to-be-trapped via collisions with a cold buffer gas, which serves to dissipate the translational energy of the atoms or molecules.

By doctor
(151 views)

## Update on MISR applications to Shrub Abundance Mapping in Desert Grasslands

Update on MISR applications to Shrub Abundance Mapping in Desert Grasslands. Mark Chopping, Lihong Su, Albert Rango, Debra P.C. Peters, John V. Martonchik, and Andrea Laliberte 3 March 2006. Structure: A Strength of Multiangle Remote Sensing .

By wilfred
(97 views)

## The rate of expansion of Universe

The rate of expansion of Universe. Consider a sphere of radius r=R(t) χ , If energy density inside is ρ c 2  Total effective mass inside is M = 4 πρ r 3 /3 Consider a test mass m on this expanding sphere, For Test mass its Kin.Energy + Pot.E. = const E

By hidi
(101 views)

## Lecture 8: Div(ergence)

Lecture 8: Div(ergence). Consider vector field and. outside. Flux (c.f. fluid flow of Lecture 6) of out of S . inside. e.g, if is the fluid velocity (in m s -1 ), . S. rate of flow of material (in kg s -1 ) out of S

By kynthia
(79 views)

## 1. MEASURES OF ATMOSPHERIC COMPOSITION

1. MEASURES OF ATMOSPHERIC COMPOSITION. WHAT IS THE ATMOSPHERE?. Gaesous envelope surrounding the Earth Mixture of gases, also contains suspended solid and liquid particles ( aerosols) Aerosol = dispersed condensed phase suspended in a gas.

By breindel
(178 views)

## 21cmFAST A Fast, Semi-Numerical Simulation of the High-Redshift 21cm Signal

21cmFAST A Fast, Semi-Numerical Simulation of the High-Redshift 21cm Signal. Mesinger, Furlanetto , & Cen (2010). Andrei Mesinger Princeton University. Motivation. We know next to nothing about high-z --> ENORMOUS parameter space to explore

By flann
(308 views)

## Introduction to the Physics of Saturation

Introduction to the Physics of Saturation. Yuri Kovchegov The Ohio State University. Outline. General concepts Classical gluon fields, parton saturation Quantum (small-x) evolution Linear BFKL evolution Non-linear BK and JIMWLK evolution Recent progress (selected topics)

By becka
(122 views)

## Introduction to the Physics of Saturation

Introduction to the Physics of Saturation. Yuri Kovchegov The Ohio State University. Outline. Preamble Review of saturation physics/CGC. Classical fields Quantum evolution More recent progress at small-x Running coupling corrections NLO BFKL/BK/JIMWLK corrections Conclusions.

By nakia
(80 views)

## 3.2 Spatial distribution differences

A Comparison of Extratropical Cyclones in Recent Reanalyses. 1 Introduction

By rowdy
(106 views)

## Yuk Yung, Peter Gao , Xi Zhang, David Crisp, and Charles G. Bardeen DPS 44 October 17 th , 2012

Generation of Aerosol Particles via Nucleation of Meteoric Dust and Cloud Upwelling in the Upper Haze of Venus. Yuk Yung, Peter Gao , Xi Zhang, David Crisp, and Charles G. Bardeen DPS 44 October 17 th , 2012. Observations: The Upper Haze is variable on the order of days .

By ofira
(92 views)

## Weak lensing of CMB from cosmic (super-)strings

9/28/2011 JGRG21 @ Tohoku U. Weak lensing of CMB from cosmic (super-)strings. Daisuke Yamauchi. ICRR, U Tokyo. w ith A. Taruya (U Tokyo, RESCEU), T. Namikawa (U Tokyo), K. Takahashi (Kumamoto U), Y. Sendouda ( Hirosaki U) , C.M. Yoo (YITP). Introduction. CMB lensing .

By bozica
(155 views)

## Selected literatures introduction about gas-liquid flow in microchannels

Selected literatures introduction about gas-liquid flow in microchannels. Reporter: Zhang Weihua Supervisor: Professor Xin Feng. Contents. Fundamentals. Flow patterns Mixer geometry Pressure drop. Fundamentals. Flow patterns.

By shaw
(176 views)

## Physical analogies between solar chromosphere and earth’s ionosphere

Japan-Norway Symposium on Space Science in Polar Region . June 5-6, 2012 Oslo . Physical analogies between solar chromosphere and earth’s ionosphere. Hiroaki Isobe (Kyoto University).

By dot
(129 views)

## Holographic QCD in the medium

Holographic QCD in the medium . Chanyong Park ( CQUeST ) @ LHC Physics Workshop (2010.08.11). Ref. B. H. Lee, CP and S.J. Sin, JHEP 0907 (2009) 087. CP, Phys. Rev. D81, (2010) 045009. K. Jo, B. H. Lee, CP and S.J. Sin, JHEP 1006 (2010) 022. 1. AdS /CFT correspondence

By brigit
(138 views)

## S. Shibata 柴田 　晋平 Yamagata Univ. 山形大学 Department of Phys 物理学科

＠ FAN3 22 June 2012. The Structure of the Pulsar Magnetosphere via Particle Simulation. S. Shibata 柴田 　晋平 Yamagata Univ. 山形大学 Department of Phys 物理学科. Aim of our numerical study. via particle simulation, the main problems to be challenged are.

By mikkel
(137 views)

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