At typical protonospheric electron densities, the electron mean free path is long enough that the coefficient of thermal conductivity is no longer given by Spitzer's expression. The effect on the temperature profile of using the corrected expression for conductivity is investigated. The corrected thermal conduction coefficient is density-dependent and has a more complicated temperature dependence than the coefficient applicable to higher density plasmas. The results indicate that the effect is not negligible even under quiet conditions and at low latitudes
Color excesses in B-V are determined indirectly from a study of Stromgren's b-y color for a sample o...
Pictorial data from the Image Dissector Camera System (IDCS) and Temperature-Humidity Infrared Radio...
During relatively quiet times in the period 1964-1968, AE is found to be greater when the interplane...
The performance is discussed of 10-micron mercury-cadmiumtelluride and lead-tin-telluride photodiode...
A self-consistent, two-dimensional, two-component diffusion model is presented to describe the diurn...
Numerical calculations of the generation and propagation of the two important fundamental symmetric ...
Detailed numerical calculations of thermospheric heat sources and sinks are presented and their rela...
The space-time integral of the thermodynamic pressure plays the role of the thermodynamic potential ...
The charge composition of solar cosmic rays were measured during two flares occurring in April and S...
After a preliminary discussion of feasibility, new experimental work with a hydrogen beam is describ...
The flux of secondary protons below 100 MeV in interstellar space is calculated using detailed cross...
It is argued that it is appropriate to consider two correlation lengths for interplanetary magnetic ...
A balloon borne measurement of the cosmic ray electron spectrum from 10 to 200 GeV is reported in wh...
Analysis is presented of data obtained from Nimbus 3 infrared measurements of the Intertropical Conv...
The equations of horizontal motion of the neutral atmosphere between 120 and 500 km are integrated w...
Color excesses in B-V are determined indirectly from a study of Stromgren's b-y color for a sample o...
Pictorial data from the Image Dissector Camera System (IDCS) and Temperature-Humidity Infrared Radio...
During relatively quiet times in the period 1964-1968, AE is found to be greater when the interplane...
The performance is discussed of 10-micron mercury-cadmiumtelluride and lead-tin-telluride photodiode...
A self-consistent, two-dimensional, two-component diffusion model is presented to describe the diurn...
Numerical calculations of the generation and propagation of the two important fundamental symmetric ...
Detailed numerical calculations of thermospheric heat sources and sinks are presented and their rela...
The space-time integral of the thermodynamic pressure plays the role of the thermodynamic potential ...
The charge composition of solar cosmic rays were measured during two flares occurring in April and S...
After a preliminary discussion of feasibility, new experimental work with a hydrogen beam is describ...
The flux of secondary protons below 100 MeV in interstellar space is calculated using detailed cross...
It is argued that it is appropriate to consider two correlation lengths for interplanetary magnetic ...
A balloon borne measurement of the cosmic ray electron spectrum from 10 to 200 GeV is reported in wh...
Analysis is presented of data obtained from Nimbus 3 infrared measurements of the Intertropical Conv...
The equations of horizontal motion of the neutral atmosphere between 120 and 500 km are integrated w...
Color excesses in B-V are determined indirectly from a study of Stromgren's b-y color for a sample o...
Pictorial data from the Image Dissector Camera System (IDCS) and Temperature-Humidity Infrared Radio...
During relatively quiet times in the period 1964-1968, AE is found to be greater when the interplane...