Line profile of H Lyman-beta emission from dissociative excitation of H-2

被引:12
作者
Ajello, JM
Ahmed, SM
Liu, XM
机构
[1] Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA
来源
PHYSICAL REVIEW A | 1996年 / 53卷 / 04期
关键词
D O I
10.1103/PhysRevA.53.2303
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
A high-resolution ultraviolet spectrometer was employed for a measurement of the H Lyman-beta (H L(beta)) emission Doppler line profile at 1025.7 Angstrom from dissociative excitation of H-2 by electron impact. Analysis of the deconvolved line profile reveals the existence of a narrow central peak, less than 30 m Angstrom full width at half maximum (FWHM), and a broad pedestal base about 260 m Angstrom FWHM. Analysis of the red wing of the line profile is complicated by a group of Werner and Lyman rotational lines 160-220 m Angstrom from the line center. Analysis of the blue wing of the line profile gives the kinetic-energy distribution. There are two main kinetic-energy components to the H(3p) distribution: (1) a slow distribution with a peak value near 0 eV from singly excited states, and (2) a fast distribution with a peak contribution near 7 eV from doubly excited states. Using two different techniques, the absolute cross section of H L(beta) is found to be 3.2+/-0.8X10(-19) cm(2) at 100-eV electron impact energy. The experimental cross-section and line-profile results can be compared to previous studies of Ha (6563.7 Angstrom) for principal quantum number n=3 and L(alpha) (1215.7 Angstrom) for n=2.
引用
收藏
页码:2303 / 2308
页数:6
相关论文
共 26 条
[1]  
ABGRALL H, 1993, ASTRON ASTROPHYS SUP, V101, P323
[2]  
ABGRALL H, 1993, ASTRON ASTROPHYS SUP, V101, P273
[3]   THE LYMAN AND WERNER BAND SYSTEMS OF MOLECULAR-HYDROGEN [J].
ABGRALL, H ;
ROUEFF, E ;
LAUNAY, F ;
RONCIN, JY ;
SUBTIL, JL .
JOURNAL OF MOLECULAR SPECTROSCOPY, 1993, 157 (02) :512-523
[4]   SIMPLE ULTRAVIOLET CALIBRATION SOURCE WITH REFERENCE SPECTRA AND ITS USE WITH THE GALILEO ORBITER ULTRAVIOLET SPECTROMETER [J].
AJELLO, JM ;
SHEMANSKY, DE ;
FRANKLIN, B ;
WATKINS, J ;
SRIVASTAVA, S ;
JAMES, GK ;
SIMMS, WT ;
HORD, CW ;
PRYOR, W ;
MCCLINTOCK, W ;
ARGABRIGHT, V ;
HALL, D .
APPLIED OPTICS, 1988, 27 (05) :890-914
[5]   STUDIES OF EXTREME-ULTRAVIOLET EMISSION FROM RYDBERG SERIES OF H-2 BY ELECTRON-IMPACT [J].
AJELLO, JM ;
SHEMANSKY, D ;
KWOK, TL ;
YUNG, YL .
PHYSICAL REVIEW A, 1984, 29 (02) :636-653
[6]   KINETIC-ENERGY DISTRIBUTION OF H(2P) ATOMS FROM DISSOCIATIVE EXCITATION OF H-2 [J].
AJELLO, JM ;
AHMED, SM ;
KANIK, I ;
MULTARI, R .
PHYSICAL REVIEW LETTERS, 1995, 75 (18) :3261-3264
[7]   Line profile of H Lyman alpha from dissociative excitation of H-2 with application to Jupiter [J].
Ajello, JM ;
Kanik, I ;
Ahmed, SM ;
Clarke, JT .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1995, 100 (E12) :26411-26420
[8]   CROSS-SECTIONS FOR PRODUCTION OF H(2P, 2S, 1S) BY ELECTRON COLLISIONAL DISSOCIATION OF H-2 [J].
AJELLO, JM ;
JAMES, GK .
ASTROPHYSICAL JOURNAL, 1991, 371 (01) :422-431
[9]   HUBBLE-SPACE-TELESCOPE GODDARD HIGH-RESOLUTION SPECTROGRAPH H2 ROTATIONAL SPECTRA OF JUPITER AURORA [J].
CLARKE, JT ;
JAFFEL, LB ;
VIDALMADJAR, A ;
GLADSTONE, GR ;
WAITE, JH ;
PRANGE, R ;
GERARD, JC ;
AJELLO, J ;
JAMES, G .
ASTROPHYSICAL JOURNAL, 1994, 430 (01) :L73-L76
[10]   JUPITER DAYGLOW H LY ALPHA EMISSION-LINE PROFILE [J].
CLARKE, JT ;
GLADSTONE, GR ;
BENJAFFEL, L .
GEOPHYSICAL RESEARCH LETTERS, 1991, 18 (11) :1935-1938