This page provides a basic introduction to the interstellar medium (ISM) and the physics needed to understand the main components of the ISM and how astronomers study them. It is designed to be a companion webpage for the WorldWide Telescope tour "The Multiphase ISM." While the tour is aimed at the general public, this website…
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The Multiphase ISM | An introduction to the interstellar medium | multiphaseism.wordpress.com Reviews
https://multiphaseism.wordpress.com
This page provides a basic introduction to the interstellar medium (ISM) and the physics needed to understand the main components of the ISM and how astronomers study them. It is designed to be a companion webpage for the WorldWide Telescope tour "The Multiphase ISM." While the tour is aimed at the general public, this website…
multiphaseism.wordpress.com
The Orion Star-Forming Region | The Multiphase ISM
https://multiphaseism.wordpress.com/2013/05/08/the-orion-star-forming-region
An introduction to the interstellar medium. The Orion Star-Forming Region. May 8, 2013. Energy in the ISM. HII Regions →. Leave a Reply Cancel reply. Enter your comment here. Fill in your details below or click an icon to log in:. Address never made public). You are commenting using your WordPress.com account. ( Log Out. You are commenting using your Twitter account. ( Log Out. You are commenting using your Facebook account. ( Log Out. You are commenting using your Google account. ( Log Out.
Blackbody Radiation | The Multiphase ISM
https://multiphaseism.wordpress.com/2013/05/07/blackbody-radiation
An introduction to the interstellar medium. May 7, 2013. The theoretical blackbody spectrum for an object at various temperatures. Hotter objects emit more total radiation (i.e. they are brighter) and the peak of their spectrum shifts to shorter wavelengths as temperature increases. Understanding Spectral Lines →. Leave a Reply Cancel reply. Enter your comment here. Fill in your details below or click an icon to log in:. Address never made public). Notify me of new comments via email. Shocks in the ISM.
Supernovae | The Multiphase ISM
https://multiphaseism.wordpress.com/2013/05/08/supernovae
An introduction to the interstellar medium. May 8, 2013. Stars will continue to forge elements into heavier elements in their cores via nuclear fusion. Energy in the ISM →. Leave a Reply Cancel reply. Enter your comment here. Fill in your details below or click an icon to log in:. Address never made public). You are commenting using your WordPress.com account. ( Log Out. You are commenting using your Twitter account. ( Log Out. You are commenting using your Facebook account. ( Log Out. Shocks in the ISM.
Energy in the ISM | The Multiphase ISM
https://multiphaseism.wordpress.com/2013/05/08/energy-in-the-ism
An introduction to the interstellar medium. Energy in the ISM. May 8, 2013. As discussed on this. Page, the ISM has multiple components, all of which have different temperatures, densities, and ionization states. As the ISM is a very dynamic environment, clearly it contains nonzero amounts of energy. We are interested in the types of energy stored in the ISM and the relative importance of each component. This is outlined in the pie chart below, adapted from Bruce Draine’s book. Or “nkT” (red ...Green sli...
Jeans Collapse | The Multiphase ISM
https://multiphaseism.wordpress.com/2013/05/08/jeans-collapse
An introduction to the interstellar medium. May 8, 2013. As a simplified case, we consider a spherical cloud of uniform temperature. Consisting of hydrogen and other elements, such that the average mass of a particle is. Is the mass of a hydrogen atom and. Is an enrichment factor). Typically. Using the assumption that the cloud has uniform density to write. So the cloud will collapse if its radius is larger than the Jeans Radius. Produces a Jeans Length. Times the Jeans radius I derived above. Is Newton&...
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Hydrodynamics | A visualization tool of 2D shocks simulations
https://2dshocks.wordpress.com/hydrodynamics
A visualization tool of 2D shocks simulations. An interactive module by Fernando Becerra. Euler equations describe a smooth flow. The equations represent conservation of mass (continuity equation), momentum and energy in the fluid. The set of equations are given by:. Is the total energy density. So far we have three equations and four variables, so we need a forth equation. In the case of a compressible fluid we add an equation of state (EOS) of the type. Which is equivalent to consider constant density).
2013 topical modules | ISM and Star Formation
https://ay201b.wordpress.com/topical-modules/2013-topical-modules
ISM and Star Formation. 8220;The Book”. These modules were produced by the AY 201b students of the Spring 2013 term. For a full description of the module creation process, motivations, and outcomes, see our article arXiv:1308.1908. For a summary of all the modules created in 2013, download the handout. From our May 21st event. Visualizing the Milky Way Project. Visualizing Turbulence in the ISM. Shocks in the ISM–From Simulations to Observations: This module plays with making mock observations of S...
An Overview of the ISM | Landmarks of the ISM
https://ismlandmarks.wordpress.com/an-overview-of-the-ism
Landmarks of the ISM. A tour of some of the most beautiful objects in the interstellar medium and an introduction to what observations at different wavelengths can tell us about them. Skip to primary content. An Overview of the ISM. An Overview of the ISM. What exactly is the interstellar medium (ISM)? In our galaxy that is between the stars. Draine divides all of this ‘stuff’ into seven components:. Or, in more technical terms, small solid particles mixed in with the interstellar gas. To learn even more...
Shocks | A visualization tool of 2D shocks simulations
https://2dshocks.wordpress.com/shocks
A visualization tool of 2D shocks simulations. An interactive module by Fernando Becerra. Shocks by definition are discontinuities in the fluid properties (e.g. density, velocity, pressure). A schematic image is shown in Fig.1, where we can clearly identify the discontinuity as a “shock jump”. The values of the fluid properties change abruptly at that interface. Pressure, energy and density have values. Respectively to the left of the shock, while to the right the values are. Which is basically jets eman...
Simulations | A visualization tool of 2D shocks simulations
https://2dshocks.wordpress.com/simulations
A visualization tool of 2D shocks simulations. An interactive module by Fernando Becerra. What is a numerical simulation? In astrophysics most processes can be described by a set of equations. A simple example are the equations of motion. Take a long time and we are not able to watch the whole process with telescopes. Another interesting example is the formation of the first structures in the Universe. A very famous simulation of large scale structure is the Millenium simulation. Based in an Lagrangian h...
Documentation | A visualization tool of 2D shocks simulations
https://2dshocks.wordpress.com/documentation
A visualization tool of 2D shocks simulations. An interactive module by Fernando Becerra. A zip version of the code is available here. Alternatively you can download pyro2 from its webpage. And add the file interface.py. To the pyro2/ directory. Here a list of programs you need to install before installing pyro2:. The only step needed to install pyro2 is building the fortran source. In order to do that just go to the pyro2/ folder and execute. Running a new simulation. Choose the initial conditions.
The Code | A visualization tool of 2D shocks simulations
https://2dshocks.wordpress.com/code
A visualization tool of 2D shocks simulations. An interactive module by Fernando Becerra. Pyro (from PYthon hydRO) was originally written in 2003-2004 by Michael Zingale. This version was resurrected beginning in 2012 and rewritten for numpy and brought up to date. pyro2. Is a 2D grid-based code mostly written in Python, with a few low-level routines written in Fortran. pyro2 employs a commonly used method to solve numerically the equations in grid-base codes, which is called the finite-volume method.
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Multiphase Computational Fluid Dynamics. Underlying causes for level set deformation. Gradient Augmented Reinitialization Scheme for the Level Set Method. The Multiphase Computational Fluid Dynamics group at University of Wisconsin-Madison. Is led by Professor Mario F. Trujillo. And is associated with the Engine Research Center. 2018 Board of Regents of the University of Wisconsin System.
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Complete List of Studies. DP and Primary Elements. Survey of Flowmeter Users. Volume X: All Flowmeters. Gas and Oil Studies. Gas Flow Core Study. Gas Mod A: Worldwide. Gas Mod B: Mideast. Gas Mod C: Custody Transfer. Gas Mod D: Applications. Gas Mod E: Multiphase. Gas Mod F: LNG. Oil Flow Core Study. Oil Mod A: Worldwide. Oil Mod B: Mideast. Oil Mod C: Custody Transfer. Oil Mod D: Applications. Oil Mod E: Multiphase. Oil Mod F: LNG. Flow and Measurement Articles. Flow, Process, and Energy News. While the...
The Multiphase ISM | An introduction to the interstellar medium
An introduction to the interstellar medium. This page provides a basic introduction to the interstellar medium (ISM) and the physics needed to understand the main components of the ISM and how astronomers study them. It is designed to be a companion webpage for the WorldWide Telescope. Tour “The Multiphase ISM.”. While the tour is aimed at the general public, this website is also intended to provide the interested viewer with a more technically-oriented overview. Introduction: What is the ISM? WHAM (Wisc...
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Hydrants and Hose Reels. Multiphase are Essential Services maintenance specialists who ensure the fire safety compliance of all facilities. When you engage our services we develop an essential services maintenance plan specifically tailored to the needs of your facility in accordance with your Building Occupancy Certificate. Multiphase is multifarious providing numerous services relating to fire safety. All our work complies with Australian Standards, the Building Code of Australia and State Regulations&...
