1965
DOI: 10.1088/0370-1328/86/3/304
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Absolute cross sections for simultaneous ionization and excitation of N2by electron impact

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Cited by 41 publications
(7 citation statements)
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“… Aarts et al [1968], Aarts [1970], and Shaw and Campos [1983] utilized the helium emission cross section as a secondary standard while Srivastava and Mirza [1968a, 1968b], and Borst and Zipf [1970] used a standard tungsten lamp for absolute calibration. McConkey and Latimer [1965] and McConkey et al [1967, 1971] used helium, standard iodine lamps, as well as standard tungsten lamps. It should be pointed out that anomalous threshold behavior in the cross section figure of McConkey et al [1967] was attributed to a graphic drawing error.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“… Aarts et al [1968], Aarts [1970], and Shaw and Campos [1983] utilized the helium emission cross section as a secondary standard while Srivastava and Mirza [1968a, 1968b], and Borst and Zipf [1970] used a standard tungsten lamp for absolute calibration. McConkey and Latimer [1965] and McConkey et al [1967, 1971] used helium, standard iodine lamps, as well as standard tungsten lamps. It should be pointed out that anomalous threshold behavior in the cross section figure of McConkey et al [1967] was attributed to a graphic drawing error.…”
Section: Discussionmentioning
confidence: 99%
“…The B 2 Σ u + state, having a lifetime of 60 ∼ 80 ns, has been extensively measured. McConkey and Latimer [1965] measured excitation functions of the (0,0), (0,1) and (0,2) bands of B 2 Σ u + − X 2 Σ g + from threshold to 300 eV and obtained absolute emission cross sections by reference to the helium emission cross section. Subsequently, McConkey et al [1967] extended the measurement to 2000 eV using both standard quartz iodine and tungsten lamps.…”
Section: Introductionmentioning
confidence: 99%
“…The uncertainty in the colour temperature results in a 2 7 % error in the calibration curve. The relative calibration curve is then put on an absolute scale by utilizing the well-established cross sections for the N: 3914 A emission (10,11) and the visible He lines resulting from the excitation of the n ' S levels (12). We estimate an accuracy of 10% for the absolute calibration of the detection system based on the combined uncertainties in the colour temperature of the quartz-iodine lamp and in the benchmark cross sections.…”
Section: Culibrutiotz Of the Detectiotz Systemmentioning
confidence: 99%
“…by electron impact, play an important role in the physics of the plasma torus around Jupiter. The Voyager fly-by missions to Jupiter have revealed intense emissions from ionized sulphur and oxygen species with a peak emission intensity at a distance from the planet that coincides with the orbital radius of Jupiter's satellite 10. It has been suggested (1,2) that the breakup of SO?, which is shot into orbit from active volcanoes on 10 and dissociated and excited by photon and electron impact, is the most likely source of these emissions.…”
Section: Introductionmentioning
confidence: 99%
“…When the 0, integration in Eq. (1) is performed, the result is N (Qn, ) AX = t(X) dp dit dQ f 0 lit X f d 3 r'( T + U cos 2 0,) g (r', p, 6,, X) (N/hc) AX, (3) where g(r', p, 6p, N) 9 7rp 4 sinO,,e(r ', p, N) with T 1 + n 2 2 and U 1 -3n 5 2 . The expression for Nm( Xs N)AX is also given by Eq.…”
Section: Angular Distribution Of the Radiation And The Polarization Fmentioning
confidence: 99%