1973
DOI: 10.1029/ja078i022p04779
|View full text |Cite
|
Sign up to set email alerts
|

Magnetic field in the very close neighborhood of Mars according to data from the Mars 2 and Mars 3 spacecraft

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
33
0

Year Published

1975
1975
2018
2018

Publication Types

Select...
4
3

Relationship

0
7

Authors

Journals

citations
Cited by 119 publications
(33 citation statements)
references
References 9 publications
0
33
0
Order By: Relevance
“…Thus the shock position chosen by Dolginov et al (1973) stands off further than that given by Valsberg et al (at more than 2350 km instead of 1100 km at the subsolar position). Specifically, for the January 21 passage reported by both groups, in the region of magnetic fluctuations said to lie downstream of the shock, Valsberg et al (1973a) originally reported from the ion energy spectra that the plasma was supersonic and non-thermal.…”
Section: Discussionmentioning
confidence: 62%
See 2 more Smart Citations
“…Thus the shock position chosen by Dolginov et al (1973) stands off further than that given by Valsberg et al (at more than 2350 km instead of 1100 km at the subsolar position). Specifically, for the January 21 passage reported by both groups, in the region of magnetic fluctuations said to lie downstream of the shock, Valsberg et al (1973a) originally reported from the ion energy spectra that the plasma was supersonic and non-thermal.…”
Section: Discussionmentioning
confidence: 62%
“…(iii) The maxima of field and electron density reportedly do not coincide in space (Dolginov et al 1973). …”
Section: Discussionmentioning
confidence: 92%
See 1 more Smart Citation
“…Estimation of the magnetic moment depends on the interpretation of the observed magnetic fields. Dolginov et al (1973Dolginov et al ( , 1976 assumed that the magnetic fields observed with Mars 2, Mars 3 and Mars 5 spacecraft were influenced by an intrinsic magnetic field of Mars and concluded that the magnetic moment was of 2.4-2.5 × 10 22 G·cm 3 . On the other hand, Russell (1978a, b) claimed that magnetic fields observed by Mars-series spacecraft tend to be wrapped around the planet, and proposed an upper limit to the magnetic moment of 2 × 10 21 G·cm 3 .…”
Section: Intrinsic and Crustal Fieldmentioning
confidence: 99%
“…The obstacle to the solar wind flow at Mars has been observed for more than 45 years by several spacecraft. First crossings of the dayside magnetosphere with observations of increasing magnetic field up to ~30 nT (Dolginov et al, ) and ions of lower energy than magnetosheath ions were made by Mars 2 and Mars 3 (called then “ion cushion”; Bogdanov & Vaisberg, ). The ion and magnetic tail at ~7 R М with planetary ions outflow was found on Mars 5 (Dolginov, ; Vaisberg, ).…”
Section: Introductionmentioning
confidence: 99%