1969
DOI: 10.3367/ufnr.0098.196907a.0409
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Physics of interplanetary plasma and laboratory experiments

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Cited by 21 publications
(14 citation statements)
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“…This spatial distribution was observed by Helios 1 and 2 space probes at distances from 0.3 to 1 A.U. from the Sun [20]. It was found that the dust concentration decreases in ecliptic as a function of distance from the Sun as r −1.3 .…”
Section: Characteristics Of the Interplanetary Mediumsupporting
confidence: 57%
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“…This spatial distribution was observed by Helios 1 and 2 space probes at distances from 0.3 to 1 A.U. from the Sun [20]. It was found that the dust concentration decreases in ecliptic as a function of distance from the Sun as r −1.3 .…”
Section: Characteristics Of the Interplanetary Mediumsupporting
confidence: 57%
“…It is acceptable to neglect the interstellar component, taking into account the electromagnetic radiation of the Sun only, even though the interplanetary medium is seen as the entire set of matter and fields which fill interplanetary space inside the Solar system. As the main part of interplanetary matter, we will consider only the solar wind, high-energy charged particles, interplanetary dust, and neutral gas [17][18][19][20][21][22][23][24][25].…”
Section: Characteristics Of the Interplanetary Mediummentioning
confidence: 99%
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