We were selective as to our approach to research activities, and devoted primary attention to two investigations concerning the global behavior of atomic hydrogen in the Earth's upper atmosphere. We derive the thermospheric concentration of H by applying the condition of charge-exchange equilibrium between hydrogen and oxygen atoms and ions to in-situ measurements of F-region composition and temperature from the series of Atmosphere Explorer (AE) aeronomy satellites. Progress and accomplishments on these chosen research projects are summarized
Long latitude distributions of atmospheric neutral hydrogen were derived at Venus for the period 197...
Understanding the influence of the solar cycle variation on the Earth\u27s upper atmosphere is impor...
Understanding the influence of the solar cycle variation on the Earth\u27s upper atmosphere is impor...
Experimental results, based on Explorer 32 data, on the density, temporal variation, and distributio...
Thermospheric model based on Explorer 32 hydrogen ion density measurements including periodic variat...
Diurnal variations of atomic hydrogen in thermosphere derived from Explorer 32 data and correlated w...
We investigate atomic hydrogen (H) variability from the mesopause to the upper thermosphere, on time...
Coincident ground- and satellite-based geocoronal hydrogen emission data are presented, along with f...
Coincident ground- and satellite-based geocoronal hydrogen emission data are presented, along with f...
Neutral hydrogen distribution, and relative and absolute concentration, in transition region between...
We will discuss work in progress to better understand solar cyclic and climatic influences on hydrog...
We will discuss work in progress to better understand solar cyclic and climatic influences on hydrog...
Atomic oxygen (O) and atomic hydrogen (H) in the mesopause region are critical species, governing ch...
Latitudinal variations in H and He ion distribution in upper ionosphere observed by OGO 2 and 4 sate...
Observations made by the neutral mass spectrometer on board the polar orbiting OGO-6 satellite are g...
Long latitude distributions of atmospheric neutral hydrogen were derived at Venus for the period 197...
Understanding the influence of the solar cycle variation on the Earth\u27s upper atmosphere is impor...
Understanding the influence of the solar cycle variation on the Earth\u27s upper atmosphere is impor...
Experimental results, based on Explorer 32 data, on the density, temporal variation, and distributio...
Thermospheric model based on Explorer 32 hydrogen ion density measurements including periodic variat...
Diurnal variations of atomic hydrogen in thermosphere derived from Explorer 32 data and correlated w...
We investigate atomic hydrogen (H) variability from the mesopause to the upper thermosphere, on time...
Coincident ground- and satellite-based geocoronal hydrogen emission data are presented, along with f...
Coincident ground- and satellite-based geocoronal hydrogen emission data are presented, along with f...
Neutral hydrogen distribution, and relative and absolute concentration, in transition region between...
We will discuss work in progress to better understand solar cyclic and climatic influences on hydrog...
We will discuss work in progress to better understand solar cyclic and climatic influences on hydrog...
Atomic oxygen (O) and atomic hydrogen (H) in the mesopause region are critical species, governing ch...
Latitudinal variations in H and He ion distribution in upper ionosphere observed by OGO 2 and 4 sate...
Observations made by the neutral mass spectrometer on board the polar orbiting OGO-6 satellite are g...
Long latitude distributions of atmospheric neutral hydrogen were derived at Venus for the period 197...
Understanding the influence of the solar cycle variation on the Earth\u27s upper atmosphere is impor...
Understanding the influence of the solar cycle variation on the Earth\u27s upper atmosphere is impor...