Anomalous UV auroral spectra during a large magnetic disturbance
Technical Report
·
OSTI ID:5178810
Ultraviolet and far-ultraviolet auroral spectra (1100-2900 A) were taken during a very disturbed period (K{sub p} = 7+) on June 2, 1978, by the S3-4 polar-orbiting satellite over the nightside, winter southern hemisphere polar region. The spectra from the equatorward section (-53 to -60 deg. geomagnetic latitude) of the auroral precipitation showed many striking differences from those of the diffuse aurora in other orbits or the poleward section of the diffuse auroral region (-60 to -65 deg. geomagnetic latitude) on the same orbit. The differences are as follows: (1) intensity ratios of the nitrogen atomic lines (1744 A and 2143 A) to the Lyman-Birge-Hopfield (LBH) (3-10) band were 2 instead of 1; (2) intensity ratio of the oxygen line (1356 A) to the LBH (3-10) band was 15 instead of 4; (3) rotational temperature of the Vegard-Kaplan band system was 1000 K instead of 400 K; and (4) effective vibrational temperature of the LBH band system was above 3000 K instead of below 1000 K. These and other characteristics are consistent with the assumption that observed spectra may originate from two different altitude regimes. Emissions from low altitudes (approximately 120 km) were produced by typical keV diffuse auroral-electron precipitation, and those from high altitudes (approximately 200 km) were produced by keV heavy-particle precipitation. The lack of significant enhancement of Lyman-alpha emission indicates a very weak proton precipitation. The authors believe that these low-latitude anomalous ultraviolet spectral features are likely due to the keV ion-atom oxygen precipitation, previously observed by a mass spectrometer at 800 km.
- Research Organization:
- Johns Hopkins Univ., Laurel, MD (USA). Applied Physics Lab.
- OSTI ID:
- 5178810
- Report Number(s):
- AD-A-212289/3/XAB
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640201* -- Atmospheric Physics-- Auroral
Ionospheric
& Magetospheric Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ALTITUDE
AURORAE
BARYONS
CHARGED-PARTICLE PRECIPITATION
DIFFUSION
ELECTROMAGNETIC RADIATION
ELECTRON PRECIPITATION
ELEMENTARY PARTICLES
ELEMENTS
EMISSION SPECTRA
FAR ULTRAVIOLET RADIATION
FERMIONS
HADRONS
MAGNETIC STORMS
MASS SPECTROMETERS
MEASURING INSTRUMENTS
NITROGEN
NONMETALS
NUCLEONS
OXYGEN
PROTONS
RADIATIONS
SPECTRA
SPECTROMETERS
ULTRAVIOLET RADIATION
ULTRAVIOLET SPECTRA
Ionospheric
& Magetospheric Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ALTITUDE
AURORAE
BARYONS
CHARGED-PARTICLE PRECIPITATION
DIFFUSION
ELECTROMAGNETIC RADIATION
ELECTRON PRECIPITATION
ELEMENTARY PARTICLES
ELEMENTS
EMISSION SPECTRA
FAR ULTRAVIOLET RADIATION
FERMIONS
HADRONS
MAGNETIC STORMS
MASS SPECTROMETERS
MEASURING INSTRUMENTS
NITROGEN
NONMETALS
NUCLEONS
OXYGEN
PROTONS
RADIATIONS
SPECTRA
SPECTROMETERS
ULTRAVIOLET RADIATION
ULTRAVIOLET SPECTRA