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Helium radiation

Figure 5.13 The photoelectron spectrum of water vapour ionizations from the 1b, 3a, and 1b2 orbitals are indicated. Ionizations from the more stable 2a, orbital are not produced by the helium radiation used... Figure 5.13 The photoelectron spectrum of water vapour ionizations from the 1b, 3a, and 1b2 orbitals are indicated. Ionizations from the more stable 2a, orbital are not produced by the helium radiation used...
The ionization energies of electrons in the three highest occupied molecular orbitals of carbon monoxide are 14.0, 16.8 and 19.7 eV. Calculate the kinetic energies in eV of the photoelectrons that will be emitted when CO is irradiated with (a) helium radiation of wavelength 58.4 nm and (b) neon radiation of wavelength 74.2 nm. [Pg.24]

The fixed points in the lTS-90 are given in Tabie 11.39. Platinum resistance thermometers are recommended for use between 14 K and 1235 K (the freezing point of silver), calibrated against the fixed points. Below 14 K either the vapor pressure of helium or a constant-volume gas thermometer is to be used. Above 1235 K radiometry is to be used in conjunction with the Planck radiation law,... [Pg.1215]

Lasers (see Chapter 9) are sources of intense, monochromatic radiation which are ideal for Raman spectroscopy and have entirely replaced atomic emission sources. They are more convenient to use, have higher intensity and are more highly monochromatic for example, the line width at half-intensity of 632.8 nm (red) radiation from a helium-neon laser can be less than 0.05 cm. ... [Pg.122]

It is possible to change the conditions in the helium discharge lamp so that the helium is ionized predominantly to He (He II). The radiation is due mainly to the n = 2 — n = transition of He II (analogous to the first member of the Lyman series of the hydrogen atom in Figure 1.1) at 30.4 nm with an energy of 40.81 cY A thin aluminium foil filter can be used to remove any He I radiation. [Pg.292]

S2-4 Helium burning as additional process for nucleogenesis 19S4 Slow neutron absorption added to stellar reactions 195S-7 Comprehensive theory of stellar synthesis of all elements in observed cosmic abundances 196S 2.7 K radiation detected... [Pg.5]

The eventual resolution of the issue was that argon was fitted into a new group within the table, between the halogens and the alkali metals. In the meantime, the properties were being investigated of a gas first detected in 1868 by Frankland and Lockyer by spectroscopic analysis of solar radiation. Shortly after the argon episode, it was discovered that this gas, appropriately named helium , could be... [Pg.82]


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See also in sourсe #XX -- [ Pg.325 ]




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Helium resonance radiation

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