On x-ray satellites, relative intensities and line widths

被引:8
|
作者
Parratt, LG [1 ]
机构
[1] Cornell Univ, Ithaca, NY USA
来源
PHYSICAL REVIEW | 1936年 / 50卷 / 07期
关键词
D O I
10.1103/PhysRev.50.598
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
引用
收藏
页码:598 / 602
页数:5
相关论文
共 50 条
  • [21] THE SATELLITES OF THE X-RAY LINE M-BETA
    HIRSH, FR
    PHYSICA, 1950, 16 (04): : 377 - 378
  • [22] Experimental determination of line energies, line widths and relative transition probabilities of the Gadolinium L x-ray emission spectrum
    Wansleben, Matte
    Kayser, Yves
    Hoenicke, Philipp
    Holfelder, Ina
    Waehlisch, Andre
    Unterumsberger, Rainer
    Beckhoff, Burkhard
    METROLOGIA, 2019, 56 (06)
  • [23] RELATIVE INTENSITIES OF THE X-RAY K LINES OF HEAVIER ELEMENTS
    BECKMAN, O
    ARKIV FOR FYSIK, 1955, 9 (06): : 495 - 529
  • [24] RELATIVE INTENSITIES OF CRYSTALLINE X-RAY LINES IN CELLULOSE FIBERS
    HERMANS, PH
    WEIDINGER, A
    JOURNAL OF POLYMER SCIENCE, 1961, 50 (153): : S10 - &
  • [25] X-RAY SATELLITES
    CUE, N
    BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1976, 21 (11): : 1333 - 1333
  • [26] Quantitative extraction of spectral line intensities and widths from x-ray spectra recorded with gated microchannel plate detectors
    Dunham, Greg
    Bailey, J. E.
    Rochau, G. A.
    Lake, P. W.
    Nielsen-Weber, L. B.
    REVIEW OF SCIENTIFIC INSTRUMENTS, 2007, 78 (06):
  • [27] Excitation potential, relative intensities and wave-lengths of the K alpha '' x-ray satellite line
    Parratt, LG
    PHYSICAL REVIEW, 1936, 49 (07): : 0502 - 0507
  • [28] The inner Auger effect and its influence on the intensities and widths of x-ray spectral lines
    Coster, D
    Bril, A
    PHYSICA, 1942, 9 : 84 - 96
  • [29] STUDY OF X-RAY LINE INTENSITIES IN MOLYBDENUM DURING DEFORMATION
    SMIRNOV, BI
    SOVIET PHYSICS-TECHNICAL PHYSICS, 1958, 3 (12): : 2461 - 2463
  • [30] RELATIVE INTENSITIES OF LOW-ENERGY PLASMON SATELLITES IN X-RAY-EMISSION SPECTRA
    SRIVASTAVA, KS
    SINGH, SP
    SHRIVASTAVA, RL
    BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1975, 20 (12): : 1503 - 1503