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Cool Physics links: Some fun stuff around thermodynamics

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Just because something is cool does not mean it doesn't involve heat.
BTW Please don't confuse 'heat' with internal energy! An object can't "contain an amount of heat", heat is strictly only thermal energy flowing (in transfer) from one body or region to another.

[ARCHIVAL] Gallery: HERA particle collider electron beam analysis

 ARCHIVAL (1999): This content is now considered historical only!

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HERA particle accelerator: electron Beam Loss Monitor lifetime disruption plots
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HERA: Example of electron loss monitor reaction time development for the entire HERA electron storage ring at 12 GeV.
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HERA: Electron ring beam loss monitor count ratio vs beam current, lifetime, and energy
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HERA particle accelerator: custom data analysis application

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HERA particle accelerator: custom data analysis application
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HERA particle accelerator: electron Beam Loss Monitor lifetime disruption plots
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HERA: Electron ring beam loss monitor count ratio vs beam current, lifetime, and energy
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HERA: Example of electron loss monitor reaction time development for the entire HERA electron storage ring at 12 GeV.

HERA particle collider beam dynamics: Maple symbolic worksheet example.

 ARCHIVAL (1995): This content is now considered historical only!
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This Maple worksheet download was exported to PDF via LaTeX from a Maple V worksheet. It shows detailed symbolic calculations and numerical simulations for the electron beam of the HERA (electron-proton synchrotron particle collider)].

[ARCHIVAL] Gallery: A UML Parsing Analysis of an analysis of image formation in the MOST radiotelescope (from 2005)

 ARCHIVAL (2005): This content is now considered historical only!
This page shows (for purposes of historical reference only) an OBSOLETE early attempt at re-appropriating Unified Modeling Language (UML®) for elicitation of model elements using graphical Parsing Analysis.

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MOST: UML: Circularly polarised ring Antenna
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MOST: UML: Feed
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MOST: UML: Waveguide
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MOST: UML: Module
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MOST: UML: Bay
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MOST: UML: Arm
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MOST: UML: synthesis overview
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MOST: UML: top-level
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MOST: UML: Reflector

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MOST: UML: Arm
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MOST: UML: Bay
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MOST: UML: Circularly polarised ring Antenna
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MOST: UML: Feed
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MOST: UML: Module
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MOST: UML: Reflector
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MOST: UML: synthesis overview
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MOST: UML: top-level
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MOST: UML: Waveguide

Reverse-engineering into UML of the TJDO database table structure for the MOST radiotelescope information system application (2004)

 ARCHIVAL (2004): This content is now considered historical only!
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UML Class Diagram
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[ARCHIVAL] Gallery: the MOST radiotelescope in Java and UML

[ARCHIVAL] Gallery: the MOST radiotelescope in Java and UML

 ARCHIVAL (2005): This content is now considered historical only!
Some images and videos from a research project by Webel IT and Dr Darren Kelly involving the Molonglo Observatory Synthesis Telescope (MOST).

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Snapshot from a JSP web application for the MOST radiotelescope
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Reverse-engineering into UML of the TJDO database table structure for the MOST radiotelescope information system application (2004)
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[ARCHIVAL] MOST radiotelescope: Java3D animation: flyby (4.5M)
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MOST radiotelescope: Java3D animation: steering (9.8M)
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Snapshot from a Java3D animation of the MOST radiotelescope

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MOST radiotelescope: Java3D animation: steering (9.8M)
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Reverse-engineering into UML of the TJDO database table structure for the MOST radiotelescope information system application (2004)
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Snapshot from a Java3D animation of the MOST radiotelescope
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Snapshot from a JSP web application for the MOST radiotelescope
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[ARCHIVAL] MOST radiotelescope: Java3D animation: flyby (4.5M)

[ARCHIVAL] Gallery: MOST rotational aperture radiosynthesis figures (1988)

 ARCHIVAL (1988): This content is now considered historical only!
Some key diagrams about the Molonglo Observatory Synthesis Telescope (MOST) extracted from Dr Darren Kelly's honours thesis from 1988 'An analysis of image formation by MOST (Molonglo Observatory Synthesis radioTelescope)' completed at the Department of Astrophysics, School of Physics, University of Sydney.

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Figure 5: The MOST radiotelescope centre fan-beam with field centre at meridian (from 1988)
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Figure 10: the MOST radiotelescope synthesised beam
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Figure 1: MOST radiotelescope "skymap" from observation of a strong point source at field centre
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Figure 2: A diagram of MOST with the numbering system used in this thesis report (1988)
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Figure 3: MOST radiotelescope: A diagram of the coordinate system used in the report (1988)

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Figure 10: the MOST radiotelescope synthesised beam
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Figure 1: MOST radiotelescope "skymap" from observation of a strong point source at field centre
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Figure 2: A diagram of MOST with the numbering system used in this thesis report (1988)
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Figure 3: MOST radiotelescope: A diagram of the coordinate system used in the report (1988)
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Figure 5: The MOST radiotelescope centre fan-beam with field centre at meridian (from 1988)

[ARCHIVAL] Gallery: Scans of Darren Kelly's MOST thesis report from 1988

 ARCHIVAL (1988): This content is now considered historical only!
The PostScript version is lost in time; these scans of the printed honours thesis report for 'An analysis of image formation by MOST (Molonglo Observatory Synthesis radioTelescope)' record the fundamental operations principle of rotational aperture radiosynthesis in the Molonglo Observatory Synthesis Telescope (MOST), as taught to me by staff at the Department of Astrophysics, School of Physics, University of Sydney in 1988.

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03: Contents
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04: Introduction
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01: Cover crest
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00: Cover and title
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02: Abstract

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00: Cover and title
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01: Cover crest
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02: Abstract
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03: Contents
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04: Introduction
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