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  • 1
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    Some studies of zonal and meridional wind characteristics at low latitude Indian stations (1985)
    In:  Other Sources
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    Publication Date: 2011-08-19
    Description: At the beginning of the Indian Middle Atmosphere Programme (IMAP), it was decided that the preparation of consolidation reports of already available parameters for the middle atmosphere would be useful. Atmospheric wind data obtained by rockets and balloons constituted one such parameter which had to be consolidated. The present paper summaries the results of this consolidation study. Both zonal and meridional components of winds at four low latitude Indian stations namely Thumba, Shar, Hyderabad, and Balasore, have been analyzed to yield reference wind profiles for each month. The montly mean values have been used to bring out the amplitudes and phases of the annual, semiannual and quasi-biennial oscillations.
    Keywords: GEOPHYSICS
    Type: International Council of Scientific Unions Handbook for MAP, Vol. 18; 4 p
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  • 2
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    The morphology of metallic ions in the upper atmosphere (1980)
    In:  Other Sources
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    Publication Date: 2019-06-28
    Description: Analysis of metallic ion data from a day-night pair of rockets, OGO 6, and the elliptic phases of AE-C and AE-D shows the presence of Fe(+) ions at altitudes above 400 km only at low magnetic latitudes. The detection probability of this ion decreases with altitude, with a maximum over the Atlantic and a minimum over India; the rocket data indicate ions in the E region during the day and on the bottom of the F layer at night. Mg(+) and Fe(+) are the dominant ions below 250 km at all latitudes, but Al(+), Na(+), Si(+), and Ca(+) are also detectable; a correlation was found between solar activity and metallic ion detection probability at low latitudes and high altitudes at night
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 85; Dec. 1
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  • 3
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    Observations of the Helium II 304-A and Helium I 584-A atmospheric dayglow radiation. (1973)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: Two photometers with bandpasses of 170 to 500 and 170 to 800 A were employed to observe dayglow emissions in the extreme ultraviolet (EUV) over an altitude range of 90 to 186 km. The emissions observed with these photometers are identified as resonantly scattered He I 584-A and He II 304-A radiations. At 186 km, 209 plus or minus 70 rayleighs of 584-A and 9.3 plus or minus 3.1 rayleighs of 304-A radiation were measured. These observations are compared with theoretical calculations of resonance scattering of solar emissions from geocoronal He and He(+). Using the Jacchia (1971) atmospheric model for He, it is found that the observed brightness of the 584-A emission requires that the solar 584-A line width be 0.014 plus or minus 0.004 A. In this model the maximum overhead brightness of 584-A dayglow would occur at 900 km, and its magnitude would be 1.9 plus or minus 0.6 kR. The authors' observation of 304-A brightness requires that the overhead column density of the He(+) ions be 4.2 x 10 to the 11th ions/sq cm column. This value is consistent with a constant-density plasmasphere model with a He(+) ion density of 320 ions/cu cm in the plasmasphere.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 78; Mar. 1
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  • 4
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    Zenith angle dependence of the geocoronal Lyman-alpha glow. (1972)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: Review of the observations made on the zenith angle dependence and intensity of the geocoronal hydrogen Lyman-alpha glow by means of one of four extreme ultraviolet photometers flown to an altitude of 264 km on a Nike Tomahawk rocket launched from Thumba, India, in March 1970. The results obtained are compared with Meier and Mange's (1970) theoretical predictions. The possible causes for the discrepancies found are discussed.
    Keywords: GEOPHYSICS
    Type: Planetary and Space Science; 20; Feb. 197
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  • 5
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    The O(+) 834-A dayglow - Satellite observations and interpretation with a radiation transfer model (1983)
    In:  Other Sources
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    Publication Date: 2019-06-28
    Description: The observations were made with the EUV spectrometer on the Air Force satellite STP-78-1. The dayglow intensity was observed at an altitude of 600 km to vary with magnetic latitude from 30 R to 300 R in the near zenith direction (theta - 40 deg) and from 400 R to 500 R in the near nadir direction (theta = 140 deg). The correspondingly large near zenith to near nadir intensity ratio of 0.3-0.65 over much of the dayside is seen as suggesting that the O(+) ions in the topside ionosphere constitute an optically thick medium for resonance scattering of 834-A airglow emission even at this high altitude. The STP 78-1 airglow data are normalized by means of simultaneous measurements of the O(+) density from the Explorer AE-E spacecraft at 460-km altitude near the equator. It is noted that for the ionization excitation of atomic oxygen leading to the production of O(+) atoms in 4P state, a g value of 1.1 x 10 to the -8th/s at zero optical depth is required. The latitudinal distribution of O(+) density derived from the 834-A airglow data reveals a double peak surrounding an equatorial trough (characteristic of the equatorial anomaly) at altitudes below 1000 km and a single peak at the magnetic equator above 1000 km.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research (ISSN 0148-0227); 88; 9271-927
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  • 6
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    An observation of O/+/ 834 A nightglow emission (1974)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: A 40-A resolution spectrometer was employed to measure the extreme ultraviolet nightglow emissions. The spectrometer was flown on a Black Brant V-C rocket, which was launched at 21:08 MST on Feb. 9, 1973, from White Sands Missile Range, New Mexico. The O(+) 834-A emission can be identified in the spectrum and has a brightness of 15 plus or minus 5 R. This emission is probably excited by the conjugate electrons. The data also indicate the presence of some nightglow emission in the 950- to 1050-A region that is still unidentified.
    Keywords: GEOPHYSICS
    Type: Geophysical Research Letters; 1; July 197
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  • 7
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    On the distribution of He+ in the plasmasphere from observations of resonantly scattered He II 304-A radiation (1974)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: The intensity of the He II 304-A radiation in the night sky was measured from a sounding rocket launched from White Sands Missile Range on June 9, 1972. The data obtained on this flight are compared with predictions of theoretical models of the He(+) altitude distribution within the plasmasphere. The observations are not consistent with an isothermal equilibrium model of the helium ion in the plasmasphere, confirming earlier results. The data are best fit by a diffussive equilibrium model of exospheric He(+) having a plasma temperature gradient of 0.5 K per km and a number density at 1600 km of 200,000 He(+) ions per cu cm. In this model the ion densities are calculated without allowance for thermal diffusion. A similar model that allows for thermal diffusion and that has a He(+) number density at 1600 km of 1500 per cu cm and a temperature gradient of 1.2 K per km yields a less satisfactory fit to the observations but is more consistent with in situ satellite observations.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 79; Jan. 1
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  • 8
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    Polarization of the 584- and 304-Angstrom emissions of helium in the geocorona and interplanetary medium (1973)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: The polarization of the 584- and 304-A emissions of helium that have been resonantly scattered in the earth's atmosphere and in the interplanetary medium is discussed. It is shown that in the geocorona the simultaneous measurement of altitude profiles of the 584-A He dayglow intensity and polarization will test the hypothesis that the 584-A dayglow is excited by resonance scattering of sunlight from geocoronal helium. If this is indeed the major source of the 584-A dayglow emission, a simultaneous measurement of the polarization and the altitude profile of the intensity in the exosphere will uniquely determine the helium number density distribution as a function of altitude, and in the thermosphere it will alow a study of nondiffusive equilibrium processes. An attractive feature of this method is that the interpretation does not require a knowledge of the solar 584-A line center flux or line profile.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 78; Dec. 1
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