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Journal ArticleDOI

Coordinated rocket and satellite measurements of an auroral event, 2. The rocket observations and analysis

TLDR
The results of a coordinated auroral experiment involving the Atmosphere Explorer C satellite and a sounding rocket are reported in this article, where the coordinated measurements are used to infer vertical fluxes of ionization and of electron thermal energy at high altitudes.
Abstract
Results of a coordinated auroral experiment involving the Atmosphere Explorer C satellite and a sounding rocket are reported. Auroral primary electron fluxes and neutral gas densities measured by instruments on the satellite are used in a model calculation of the thermospheric manifestation of the aurora. There is encouraging agreement between the calculated and measured electron density, electron temperature, secondary electron flux, and O I emissions at 5577 and 6300 A. A discrepancy between the calculated and the rocket-measured 3914-A emission profile is discussed in terms of experiment geometry and auroral physics. The coordinated measurements are used to infer vertical fluxes of ionization and of electron thermal energy at high altitudes

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Ultraviolet spectroscopy and remote sensing of the upper atmosphere

TL;DR: A review of the field of airglow analysis can be found in this article, where the basic processes leading to excitation of atomic and molecular energy states are discussed and the current status of knowledge of individual emission features seen in the air glow is examined for the purpose of selecting those species most useful as diagnostics of the state of the upper atmosphere and ionosphere.
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Electron temperatures in the F region of the ionosphere - Theory and observations

TL;DR: The theory and observations relating to electron temperatures in the F region of the ionosphere are reviewed in this paper, and a discussion of the various attempts to compare measured and calculated F region electron temperatures.
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The effect of particle precipitation events on the neutral and ion chemistry of the middle atmosphere: II. Odd hydrogen

TL;DR: In this paper, a one dimensional time-dependent model of the neutral and ion chemistry of the middle atmosphere has been used to examine the production of odd hydrogen (H, OH, and HO2) during charged particle precipitation.
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The auroral 6300 Å emission: Observations and modeling

TL;DR: In this article, a tomographic inversion is used to analyze measurements of the auroral atomic oxygen emission line at 6300 A made by the atmosphere explorer visible airglow experiment.
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The role of metastable species in the thermosphere

TL;DR: The role of these species in the overall thermospheric energy budget and ionization balance is also quantified in this paper, with a major fraction of the kinetic heating of the thermosphere taking place through O(1D).
References
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Journal ArticleDOI

Auroral ionization and excitation by incident energetic electrons

TL;DR: In this paper, the luminosity profiles for the N 2 + 1 N.G. (0, 0) band are predicted for various energy distributions of auroral electrons in the energy range 0.4 to 300 keV.
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A new model for the interaction of auroral electrons with the atmosphere: Spectral degradation, backscatter, optical emission, and ionization

TL;DR: In this paper, a new computational model has been created to describe the interaction of auroral electrons with the atmosphere, which is used to compute energy spectrums, ionization rates, backscatter ratios, and optical emissions associated with different incident electron spectrums.
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Observations and theory of the formation of stable auroral red arcs

M. H. Rees, +1 more
TL;DR: A population of protons with energy of some tens of keV, called the ring current, is found near the equatorial region of the magnetosphere at several earth radii.
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The open‐source neutral‐mass spectrometer on Atmosphere Explorer‐C, ‐D, and ‐E

TL;DR: The open-source mass spectrometer was used to obtain the number densities of the neutral atmospheric gases in the mass range 1 to 48 amu at the satellite location.
Journal ArticleDOI

Analytic Representation of Upper Atmosphere Densities Based on Jacchia's Static Diffusion Models

TL;DR: Modification of mathematical method of Jacchia for satellite drag density of upper atmosphere is discussed in this paper, where the satellite is assumed to be a fixed point in the upper atmosphere of the Earth.
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