๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

On the mechanism of particle heating and acceleration in the Jovian ionosphere

โœ Scribed by V.E. Shaposhnikov; V.V. Zaitsev

Publisher
Elsevier Science
Year
1993
Tongue
English
Weight
893 KB
Volume
41
Category
Article
ISSN
0032-0633

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

On the Dynamics of the Jovian Ionosphere
On the Dynamics of the Jovian Ionosphere and Thermosphere: III. The Modelling of Auroral Conductivity
โœ George Millward; Steve Miller; Tom Stallard; Alan D. Aylward; Nicholas Achilleos ๐Ÿ“‚ Article ๐Ÿ“… 2002 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 343 KB

Recent work has been concerned with calculating the threedimensional ion concentrations and Pedersen and Hall conductivities within the auroral region of Jupiter for varying conditions of incident electron precipitation. Using the jovian ionospheric model, we present results that show the auroral io

On the Dynamics of the Jovian Ionosphere
On the Dynamics of the Jovian Ionosphere and Thermosphere: I. The Measurement of Ion Winds
โœ Tom Stallard; Steve Miller; George Millward; Robert D. Joseph ๐Ÿ“‚ Article ๐Ÿ“… 2001 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 663 KB

We present profiles of the line-of-sight ionospheric wind velocities in the northern auroral/polar region of Jupiter. Our velocities are derived from the measurement of Doppler shifting of the H + 3 ฮฝ 2 Q(1,0 -) line at 3.953 ยตm. The data for this study were obtained using the facility high-resoluti

On the Dynamics of the Jovian Ionosphere
On the Dynamics of the Jovian Ionosphere and Thermosphere: II. The Measurement of H3+ Vibrational Temperature, Column Density, and Total Emission
โœ Tom Stallard; Steve Miller; George Millward; Robert D. Joseph ๐Ÿ“‚ Article ๐Ÿ“… 2002 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 797 KB

We present the first reported measurements of the intensity of a "hotband" transition for the H + 3 molecular ion in the northern auroral/polar region of Jupiter. This transition is identified as the R(3, 4 + ) line of the (2v 2 (l = 0) โ†’ v 2 ) hotband, with a wavelength of 3.94895 ยตm. This is the f