2020
DOI: 10.18520/cs/v118/i3/383-391
|View full text |Cite
|
Sign up to set email alerts
|

Lunar Near Surface Plasma Environment from Chandrayaan-2 Lander Platform:RAMBHA-LP payload

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1

Citation Types

0
2
0

Year Published

2023
2023
2024
2024

Publication Types

Select...
5
1

Relationship

0
6

Authors

Journals

citations
Cited by 7 publications
(2 citation statements)
references
References 0 publications
0
2
0
Order By: Relevance
“…The plasma (solar wind) electron density decreases by 20%-30% near the surface within type A and B sheaths. These predictions could be validated through the LP (i.e., RAMBHA payload) measurements on board Ch3 (Manju et al 2020).…”
Section: Resultsmentioning
confidence: 99%
“…The plasma (solar wind) electron density decreases by 20%-30% near the surface within type A and B sheaths. These predictions could be validated through the LP (i.e., RAMBHA payload) measurements on board Ch3 (Manju et al 2020).…”
Section: Resultsmentioning
confidence: 99%
“…The interaction of sheathaccelerated, unidirectional positive ions determines the anisotropic etching on silicon substrates [2]. The charging of satellites in zero-gravity conditions [7], plasma thrusters [8,9], surface creation of negative ions in neutral beam sources [10], plasma diagnostics [11][12][13][14][15], plasma confinement [16], and dust particle interaction [17,18] are other examples where sheath physics finds relevance. As a result, a number of theoretical [19][20][21][22][23][24][25][26][27][28] and experimental investigations [29][30][31][32][33] have been carried out to understand the nature of the sheath regions that are typically formed in low-temperature laboratory plasmas.…”
Section: Introductionmentioning
confidence: 99%