2006
DOI: 10.1029/2006gl027633
|View full text |Cite
|
Sign up to set email alerts
|

Runaway breakdown in the Jovian atmospheres

Abstract: Using detailed Monte Carlo calculations, the properties of runaway breakdown in the atmospheres of the four gas giant planets in our solar system are investigated, and the runaway avalanche lengths and average runaway electron kinetic energies are presented as a function of atmospheric electric field strengths. The runaway breakdown threshold field for the Jovian atmospheres is found to be 10 times smaller than the conventional breakdown field when hydrometeors are present, compared to 3 times smaller for Eart… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

2
24
0
1

Year Published

2008
2008
2020
2020

Publication Types

Select...
5
3
1

Relationship

0
9

Authors

Journals

citations
Cited by 26 publications
(27 citation statements)
references
References 38 publications
2
24
0
1
Order By: Relevance
“…These issues are addressed in other parts of this manuscript. We can however indicate, in agreement with Dwyer et al (2006), that under similar conditions runaway breakdown is more likely to occur on the gas giants than conventional breakdown when compared to Earth or the other planets.…”
Section: Implications For Planetary Atmospheressupporting
confidence: 88%
“…These issues are addressed in other parts of this manuscript. We can however indicate, in agreement with Dwyer et al (2006), that under similar conditions runaway breakdown is more likely to occur on the gas giants than conventional breakdown when compared to Earth or the other planets.…”
Section: Implications For Planetary Atmospheressupporting
confidence: 88%
“…4a-c where the avalanche time, mean energy, and spread in energy, are plotted as a function of the scaled electric field (E/N ) in Td, respectively. One key result is that the avalanche time is smaller for Jupiter than for Earth by large factors at low E/N and by factors of 2-3 at high E/N , in agreement with the findings of Dwyer et al (2006). The indication again is that runaway breakdown initiates more easily and proceeds faster on the gas giants for the same applied electric field.…”
Section: Runaway Breakdown Regimesupporting
confidence: 84%
“…Experimental evidence as well as Monte-Carlo calculations suggest that the electric field strength in the clouds is much lower than the threshold electric field required to initiate electrical breakdown (Marshall et al 2005;Dwyer et al 2006;Stolzenburg et al 2007). This inhibits the application of the breakdown discharge process to explain the numerous lightning discharges observed during the active period of a thunderstorm.…”
Section: Thunderstorms and Gcr Induced Dischargesmentioning
confidence: 97%