1-2 |
Atomic energy levels - as derived from the analyses of optical spectra
(flera utgåvor)
|
Charlotte E. Moore
|
1971 |
Engelska |
3 |
Atomic energy levels Vol. 1, The spectra of hydrogen, deuterium, tritium, helium, lithium, beryllium, boron, carbon, nitrogen, oxygen, fluorine, neon, sodium, magnesium, aluminum, silicon, phosphorus, sulfur, chlorine, argon, potassium, calcium, scandium, titanium, and vanadium - as derived from the analyses of optical spectra
|
Charlotte E. Moore
|
1971 |
Engelska |
4 |
Atomic energy levels Vol. 2, The spectra of chromium, manganese, iron, cobolt, nickel, copper, zinc, gallium, germanium, arsenic, selenium, bromine, krypton, rubidium, strontium, yttrium, zirkonium, and niobium - as derived from the analyses of optical spectra
|
Charlotte E. Moore
|
1971 |
Engelska |
5 |
Atomic energy levels Vol. 3, The spectra of molybdenum, technetium, ruthenium, rhodium, palladium, silver, cadmium, indium, tin, antimony, tellurium, iodine, xenon, cesium, barium, lanthanum-hafnium, tantalum, tungsten, rhenium, osmium, iridium, platinum, gold, mercury, thallium, lead, bismuth, polonium, radon and actinium - as derived from the analyses of optical spectra
|
Charlotte E. Moore
|
1971 |
Engelska |
6 |
A multiplet table of astrophysical interest
|
Charlotte E. Moore
|
1972 |
Engelska |
7 |
Atomic energy levels Vol. 2, The spectra of chromium, manganese, iron - as derived from the analyses of optical spectra
|
Charlotte E. Moore
|
1952 |
Engelska |
8 |
Atomic energy levels Vol. 3, The spectra of molybdenum, technetium, ruthenium - as derived from the analyses of optical spectra
|
Charlotte E. Moore
|
1958 |
Engelska |
9 |
The first spectrum of hafnium (Hf 1)
|
William F. Meggers
|
1976 |
Engelska |
10 |
The solar spectrum 2935Å to 8770Å - second revision of Rowland's preliminary table of solar spectrum wavelengths
|
Charlotte E. Moore
|
1966 |
Engelska |
11 |
The solar spectrum 3069Å-2095Å - from the Echelle spectrograph flown in 1961 and 1964 : an extension of Rowland's preliminary table of solar spectrum wavelenghts
|
Charlotte E. Moore
|
1982 |
Engelska |
12 |
Ionization potentials and ionization limits derived from the analysis of optical spectra
|
Charlotte E. Moore
|
1970 |
Engelska |
13 |
Revision of Rowland's preliminary table of solar spectrum wave-lengths with an extension to the present limit of the infra-red
|
Charles E St. John
|
1928 |
Engelska |
14 |
A multiplet table of astrophysical interest P. 2, Finding list of all lines in the table of multiplets
|
Charlotte E. Moore
|
1945 |
Engelska |
15 |
An ultraviolet multiplet table Section 1, The spectra of hydrogen, helium, lithium, beryllium, boron, carbon, nitrogen, oxygen, fluorine, neon, sodium, magnesium, aluminum, silicon, phosphorus, sulfur, chlorine, argon, potassium, calcium, scandium, titanium, and vanadium
|
Charlotte E. Moore
|
1950 |
Engelska |
16 |
An ultraviolet multiplet table Section 2, The spectra of chromium, manganese, iron, cobalt, nickel, copper, zinc, gallium, germanium, arsenic, selenium, bromine, krypton, rubidium, strontium, yttrium, zirconium, and niobium
|
Charlotte E. Moore
|
1952 |
Engelska |
17 |
An ultraviolet multiplet table 3, The spectra of molybdenum, technetium, ruthenium, rhodium, palladium, silver, cadmium, indium, tin, antimony, tellurium, iodine, xenon, cesium, barium, lanthanum; hafnium, tantalum, tungsten, rhenium, osmium, iridium, platinum, gold, mercury, thallium, lead, bismuth, polonium, radon, and radium
|
Charlotte E. Moore
|
1962 |
Engelska |
18 |
An ultraviolet multiplet table 4, Finding list for spectra of the elements hydrogen to niobium (Z=1 to 41)
|
Charlotte E. Moore
|
1962 |
Engelska |
19 |
An ultraviolet multiplet table 5, Finding list for spectra of the elements molybdenum to lanthanum (Z=42 to 57); hafnium to radium (Z=72 to 88)
|
Charlotte E. Moore
|
1962 |
Engelska |