関谷実 (Minoru Sekiya) - マイポータル - researchmap

基本情報

所属: 九州大学大学院理学研究院地球惑星科学部門教授

学位: 理学博士

J-GLOBAL ID: 200901036790346958
researchmap会員ID: 1000184566

外部リンク: https://jupiter.geo.kyushu-u.ac.jp/

研究キーワード

2

研究分野

2

MISC

46

Kinetic stability of a melted iron globule during chondrule formation. I. Non-rotating model

Masayuki Uesugi, Minoru Sekiya, Tomoki Nakamura

METEORITICS & PLANETARY SCIENCE 43(4) 717-730 2008年4月
Numerical simulations of the gravitational instability in the dust layer of a protoplanetary disk using a thin disk model

Shigeru Wakita, Minoru Sekiya

ASTROPHYSICAL JOURNAL 675(2) 1559-1575 2008年3月
Two evolutionary paths of an axisymmetric gravitational instability in the dust layer of a protoplanetary disk

Fumiharu Yamoto, Minoru Sekiya

ASTROPHYSICAL JOURNAL 646(2) L155-L158 2006年8月
Two evolutional paths of an axisymmetric gravitational instability in the dust layer of a protoplanetary disk

Fumiharu Yamoto, Minoru Sekiya

Astrophys.J.646:L155-L158,2006 2006年5月8日
Two evolutionary paths of an axisymmetric gravitational instability in the dust layer of a protoplanetary disk

Fumiharu Yamoto, Minoru Sekiya

Astrophysical Journal 646 L155-158 2006年
Motion of iron sulfide inclusions inside a shock-melted chondrule

M Uesugi, T Akaki, M Sekiya, T Nakamura

METEORITICS & PLANETARY SCIENCE 40(7) 1103-1114 2005年7月
Does the gas flow through a porous dust aggregate help its growth in a protoplanetary disk?

M Sekiya, H Takeda

ICARUS 176(1) 220-223 2005年7月
The gravitational instability in the dust layer of a protoplanetary disk: axisymmetric solutions for nonuniform dust density distributions in the direction vertical to the midplane

F Yamoto, M Sekiya

ICARUS 170(1) 180-192 2004年7月
Stabilization of the Shear Instability in a Dust Layer of a Protoplanetary Disk and Possible Formation of Planetesimals due to Gravitational Fragmentation of the Dust Layer

Naoki Ishitsu, Minoru Sekiya

2004年6月2日
The effects of the tidal force on shear instabilities in the dust layer of the solar nebula

N Ishitsu, M Sekiya

ICARUS 165(1) 181-194 2003年9月
The effects of the tidal force on shear instabilities in the dust layer of the solar nebula

N Ishitsu, M Sekiya

ICARUS 165(1) 181-194 2003年9月
Flow in a liquid sphere moving with a hypersonic velocity in a rarefied gas - An analytic solution of linearized equations

M Sekiya, M Uesugi, T Nakamoto

PROGRESS OF THEORETICAL PHYSICS 109(5) 717-728 2003年5月
Acid-susceptive material as a host phase of argon-rich noble gas in the carbonaceous chondrite Ningqiang

T Nakamura, M Zolensky, M Sekiya, R Okazaki, K Naga

METEORITICS & PLANETARY SCIENCE 38(2) 243-250 2003年2月
Deformation and internal flow of a chondrule-precursor molten sphere in a shocked nebular gas

M Uesugi, M Sekiya, T Nakamoto

EARTH PLANETS AND SPACE 55(8) 493-507 2003年
Deformation and internal flow of a chondrule-precursor molten sphere in a shocked nebular gas

Masayuki Uesugi, Minoru Sekiya, Taishi Nakamoto

Earth Planets and Space 55(8) 493-507 2003年
The effects of the tidal force on shear instabilities in the dust layer of the solar nebula

Icarus 165(1) 181-194 2003年
Were planetesimals formed by dust accretion in the solar nebula?

M Sekiya, H Takeda

EARTH PLANETS AND SPACE 55(5) 263-269 2003年
Flow in a liquid sphere moving with a hypersonic velocity in a rarefied gas - An analytic solution of linearized equations

Minoru Sekiya, Masayuki Uesugi, Taishi Nakamoto

Progress of Theoretical Physics 109(5) 717-728 2003年
Cosmic-ray exposure age and heliocentric distance of the parent body of H chondrites Yamato-75029 and Tsukuba

Antarctic Meteorite Research 15,97-113 2002年
Shear instabilities in the dust layer of the solar nebula III. Effects of the Coriolis force

N Ishitsu, M Sekiya

EARTH PLANETS AND SPACE 54(9) 917-926 2002年

もっとみる

書籍等出版物

1

Shear instability of the solar nebula

Primitive solar nebula and origin of planets, Terra Scientific Publishing Company 1993年

所属学協会

2

共同研究・競争的資金等の研究課題

6