'Balmer' diaporamas de présentation

Quantum Theory, Part I

Quantum Theory, Part I. The Atom Day 5.

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Quanta to Quarks

653 views • 40 slides

electron orbits atomic spectra the Bohr atom

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electron orbits atomic spectra the Bohr atom

365 views • 36 slides

The Prevalence and Properties of Outflowing Galactic Winds at z = 1

The Prevalence and Properties of Outflowing Galactic Winds at z = 1. UC Riverside Astronomy Talk January 27, 2012. Katherine A. Kornei (UCLA). Several important people. Crystal Martin (UCSB). Alice Shapley (UCLA). Alison Coil (UCSD). Galaxies are not closed boxes.

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Ch.4

Ch.4. different profiles, sometimes logarithmic sometimes complex and with variable shape. Broad Line Region. broad lines are important to understand AGN structure for at least two reasons:

486 views • 33 slides

Lecture 4

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Chapter 24

350 views • 18 slides

1 d) Corporate brand in service firms

Corporate Branding KOM5331 Moniza Waheed monizawaheed.upm@gmail.com Rosmiza Bidin rosmiza@upm.edu.my.

306 views • 18 slides

Hydrogen energy levels

Hydrogen energy levels. Paschen. Lyman. Balmer. Hydrogen atomic energy levels. E=hf = hc/ ?. Paschen. Spectra produced by transitions of electrons from upper energy levels to n=3 level. These are in the Infra red region. n=infinity. n=5. -0.54eV -0.85eV -1.5eV -3.4eV -13.6eV.

256 views • 5 slides