Capability of the cassini/huygens PWA-HASI to measure electrical conductivity in Titan

Advances in Space Research

Volumn 28, Issue 10, 2001, Pages 1511-1516

  Molina Cuberos, G J ^a,b   Lopez Moreno J J ^b   Rodrigo, R ^b   Schwingenschuh, K ^a  

^a Austrian Academy of Sciences ^*  (Austria)

^b INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

Author keywords

[No Author keywords available]

Indexed keywords

CARRIER CONCENTRATION; ELECTRIC CONDUCTIVITY; IONOSPHERE; POSITIVE IONS;

ELECTROPHILIC SPECIES;

SPACE RESEARCH;

PLANETARY ATMOSPHERE; TITAN;

EID: 0035659129     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00585-3     Document Type: Article

References (17)

1. Predictions of the electrical conductivity and charging of the aerosols in Titan's atmosphere
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4. Formation of organic molecules on Titan
5. 2 dissociation on Titan
6. Radial intensity gradients of galactic cosmic rays (1972-1995) in the heliosphere
7. The Huygens Atmospheric Structure Instrument (HASI)
8. Vertical distribution of Titan's atmospheric constituents
9. The Huygens Probe: Science, payload and Mission Overview
10. The mobility and concentration of ions and the ionic conductivity in the lower stratosphere
11. Ionization by cosmic rays of the atmosphere of Titan
12. Chemistry of the galactic cosmic rays induced ionosphere of Titan
13. Electrophilic species in the lower ionosphere of Titan
14. Equivalent circuit models, systematic error calculations and measurement range estimation for HASI PWA mutual impedance (MI) probe
15. Ion-ion recombination rates in the Earth's atmosphere