Summary of interplanetary and interstellar dust observation by Mars Dust Counter on board NOZOMI

S. Sasaki; E. Igenbergs; H. Ohashi; R. Senger; R. Münzenmayer; W. Naumann; E. Grün; K. Nogami; I. Mann; H. Svedhem

doi:10.1016/j.asr.2006.11.006

Summary of interplanetary and interstellar dust observation by Mars Dust Counter on board NOZOMI

S. Sasaki, E. Igenbergs, H. Ohashi, R. Senger, R. Münzenmayer, W. Naumann, E. Grün, K. Nogami, I. Mann, H. Svedhem

Ehemalige Einrichtungen Engineering and Design

Publikation: Beitrag in Fachzeitschrift › Artikel › Begutachtung

7 Zitate (Scopus)

Abstract

Mars Dust Counter (MDC) is a light-weight dust detector of impact ionization type on board Japanese Mars mission NOZOMI. NOZOMI was launched on July 4th (3rd at UT) 1998. From December 1998 to December 2003 for five years, NOZOMI took eccentric orbits between the Earth's and Mars' orbits. Until April 2002, MDC continuously observed interplanetary dust. MDC has detected nearly 100 doubtless dust impacts. There were observed several high-velocity particles, which are apparently different from Keplerian dust particles gravitationally bound to the sun. Directional analysis showed that MDC has detected several particles of interstellar origin during the cruising phase of NOZOMI.

Originalsprache	Englisch
Seiten (von - bis)	485-488
Seitenumfang	4
Fachzeitschrift	Advances in Space Research
Jahrgang	39
Ausgabenummer	3
DOIs	https://doi.org/10.1016/j.asr.2006.11.006
Publikationsstatus	Veröffentlicht - 2007

Zugriff auf Dokument

10.1016/j.asr.2006.11.006

Andere Dateien und Links

Verknüpfung zur Publikation in Scopus

Dieses zitieren

@article{980cad196db24d3787efc9bd1c8ea4b0,

title = "Summary of interplanetary and interstellar dust observation by Mars Dust Counter on board NOZOMI",

abstract = "Mars Dust Counter (MDC) is a light-weight dust detector of impact ionization type on board Japanese Mars mission NOZOMI. NOZOMI was launched on July 4th (3rd at UT) 1998. From December 1998 to December 2003 for five years, NOZOMI took eccentric orbits between the Earth's and Mars' orbits. Until April 2002, MDC continuously observed interplanetary dust. MDC has detected nearly 100 doubtless dust impacts. There were observed several high-velocity particles, which are apparently different from Keplerian dust particles gravitationally bound to the sun. Directional analysis showed that MDC has detected several particles of interstellar origin during the cruising phase of NOZOMI.",

keywords = "Circumterrestrial dust, Dust detector, Interplanetary dust, Interstellar dust, Meteor stream, NOZOMI",

author = "S. Sasaki and E. Igenbergs and H. Ohashi and R. Senger and R. M{\"u}nzenmayer and W. Naumann and E. Gr{\"u}n and K. Nogami and I. Mann and H. Svedhem",

year = "2007",

doi = "10.1016/j.asr.2006.11.006",

language = "English",

volume = "39",

pages = "485--488",

journal = "Advances in Space Research",

issn = "0273-1177",

publisher = "Elsevier Ltd.",

number = "3",

}

TY - JOUR

T1 - Summary of interplanetary and interstellar dust observation by Mars Dust Counter on board NOZOMI

AU - Sasaki, S.

AU - Igenbergs, E.

AU - Ohashi, H.

AU - Senger, R.

AU - Münzenmayer, R.

AU - Naumann, W.

AU - Grün, E.

AU - Nogami, K.

AU - Mann, I.

AU - Svedhem, H.

PY - 2007

Y1 - 2007

N2 - Mars Dust Counter (MDC) is a light-weight dust detector of impact ionization type on board Japanese Mars mission NOZOMI. NOZOMI was launched on July 4th (3rd at UT) 1998. From December 1998 to December 2003 for five years, NOZOMI took eccentric orbits between the Earth's and Mars' orbits. Until April 2002, MDC continuously observed interplanetary dust. MDC has detected nearly 100 doubtless dust impacts. There were observed several high-velocity particles, which are apparently different from Keplerian dust particles gravitationally bound to the sun. Directional analysis showed that MDC has detected several particles of interstellar origin during the cruising phase of NOZOMI.

AB - Mars Dust Counter (MDC) is a light-weight dust detector of impact ionization type on board Japanese Mars mission NOZOMI. NOZOMI was launched on July 4th (3rd at UT) 1998. From December 1998 to December 2003 for five years, NOZOMI took eccentric orbits between the Earth's and Mars' orbits. Until April 2002, MDC continuously observed interplanetary dust. MDC has detected nearly 100 doubtless dust impacts. There were observed several high-velocity particles, which are apparently different from Keplerian dust particles gravitationally bound to the sun. Directional analysis showed that MDC has detected several particles of interstellar origin during the cruising phase of NOZOMI.

KW - Circumterrestrial dust

KW - Dust detector

KW - Interplanetary dust

KW - Interstellar dust

KW - Meteor stream

KW - NOZOMI

UR - http://www.scopus.com/inward/record.url?scp=34247630573&partnerID=8YFLogxK

U2 - 10.1016/j.asr.2006.11.006

DO - 10.1016/j.asr.2006.11.006

M3 - Article

AN - SCOPUS:34247630573

SN - 0273-1177

VL - 39

SP - 485

EP - 488

JO - Advances in Space Research

JF - Advances in Space Research

IS - 3

ER -

Summary of interplanetary and interstellar dust observation by Mars Dust Counter on board NOZOMI

Abstract

Zugriff auf Dokument

Andere Dateien und Links

Fingerprint

Dieses zitieren