Satellite shadows on Jupiter as probes of its upper atmosphere
Photometric profiles of Jupiter shadows cast by large natural satellites used as upper atmosphere probes
Kastner, S. O.↗
Engineering topics
Kastner, S. O.
Publications and source records attributed to Kastner, S. O..
Approximate higher ionization potentials for the heavier elements.
Approximate ionization potentials for high ionization stages of elements with atomic numbers 31 to 92 obtained by binding energy calculations
Kastner, S. O.↗
Spectra of ions in the fluorine I isoelectronic sequence from Sc XIII to Cu XXI.
Spectra study and line classification of ions in fluorine I isoelectronic sequence from Sc XIII to C XXI
Cohen, L.↗
Oscillator strengths for resonance lines of some silicon and sulfur ions.
Si and S ion oscillator strengths for resonance lines in solar spectrum, discussing spin-spin and spin-other orbit interactions
SULFUR↗
Oscillator strengths for resonance lines of some silicon and sulfur ions
Oscillator strengths for resonance lines of sulfur and silicon ions
OSCILLATOR↗
Oscillator strengths for resonance lines of ions in the neon isoelectronic sequence.
Oscillator strengths for extreme UV resonance lines of ions in neon isoelectronic sequence calculated, based on single configurations in intermediate coupling
RADIATION INTENSITY↗
Earth as an occulting disk for study of solar EUV emission heights.
Source distributions of UV and X-ray emission in corona and chromosphere determined from flight of spacecraft-borne instruments into Earth shadow
OCCULTATION↗
Oscillator strengths for resonance lines of ions in the neon isoelectric sequence
Oscillator strengths for extreme ultraviolet resonance lines of ions in neon isoelectronic sequence
NEON↗
On the determination of solar EUV emission altitudes using the earth as an occulting disk
Determination of solar extreme ultraviolet emission altitudes by using earth as occulting disk
ALTITUDE↗
Hydrogen diffusion in the thermosphere by monte carlo method
Monte carlo method applied to hydrogen diffusion in thermosphere
MONTE CARLO METHOD↗