「磁石」としての「惑星」

Similar documents
MTI-HandBook [ : ( ) ] 1 ( km) GPS ( ) GPS Kelley [1989] [2002] 18 MTI c Mesosphere Thermosphere Ionosphere (MTI) Research Group, Japan 2 Rayl

1

200708_LesHouches_02.ppt

(2010 Sep April) Titan s global crater population: A new assessment Neish & Lorenz, PSS in-press Distant secondary craters from Lyot crater, Mar

Microsoft PowerPoint - Fukazawa pptx

Preliminary report on shock remanent magnetization measurement [1] cm 10 cm 8cm 8cm [2] [3] [1] Gattacceca 1 Superconducting

55_1-4_特集4部_2-2.qxd

研究成果報告書

日本海地震・津波調査プロジェクト

T05_Nd-Fe-B磁石.indd


weak ferromagnetism observed on Shimotokuyama and Ayumikotan natural crystals behaves as pre dicted by Dzyaloshinsky and Moriya, while Wagasennin and

草津白根山における地磁気全磁力・自然電位観測

1 a b cc b * 1 Helioseismology * * r/r r/r a 1.3 FTD 9 11 Ω B ϕ α B p FTD 2 b Ω * 1 r, θ, ϕ ϕ * 2 *

0946: : : :30 UT 1004:30 UT global expansion global expansion pseudo breakup pseudo breakup 3 1: Kotzebue UT [Sh

Netsu Sokutei 32 (3) Phase Relations of Minerals and Structure of the Earth's Interior Masaki Akaogi (Received April 2, 2005; Accepted May 11,

Colaprete and Toon , 212 K, 6.2 mbar,.,, 38 (Carr, 1986; Pollack et al., 1987).,, 25% (Gough, 1981)., CO 2. CO 2 CO 2. Pollack et al. (1987

1: : Voyager 1 : Keck 1) : 2) 10 1( ) 15 1/3 50% 3) 1990 adaptive optics ( )

Developement of Plastic Collocation Method Extension of Plastic Node Method by Yukio Ueda, Member Masahiko Fujikubo, Member Masahiro Miura, Member Sum

地質調査総合センター研究資料集, no. 586 日本列島の地殻温度構造と粘弾性構造の 3 次元モデルおよび地殻活動シミュレーションに関する数値データ Digital data of three-dimensional models of thermal and viscoelastic crust

untitled

Spacecraft Propulsion Using Solar Energy Spacecraft with Magnetic Field Light from the Sun Solar Wind Thrust Mirror Solar Sail Thrust production by li

ライトカーブ観測から何がわかるか


Tetsu-to-Hagane Vol. 87 (2001) No. 5 Table 1. Physical properties of particles. (a) side view (b) front view Fig. 1. Experimental apparatus with semic

Fig. 1. Horizontal displacement of the second and third order triangulation points accompanied with the Tottori Earthquake of (after SATO, 1973)

ナトリウムの尾

JHPCN-FINALv04.pdf

Annual Report of the Earth Simulator Center April March 2014 The spherical shell geometry is defined by the radius ratio, χ= r i /r o, where r

日立金属技報 Vol.34

16_.....E...._.I.v2006



Microsoft Word - GPS2017.docx

75 unit: mm Fig. Structure of model three-phase stacked transformer cores (a) Alternate-lap joint (b) Step-lap joint 3 4)

Fig. 3 Flow diagram of image processing. Black rectangle in the photo indicates the processing area (128 x 32 pixels).

第62巻 第1号 平成24年4月/石こうを用いた木材ペレット

Fig. 2 Signal plane divided into cell of DWT Fig. 1 Schematic diagram for the monitoring system

[ 30 p. 1-8 (2012)] / ** *** Numerical Analysis of Metal Transfer Phenomena - critical condition between globular and spray transfer mode - by KADOTA

k = The Last Samurai Tom Cruise [1] Oracle Ken Watanabe (I) has a Bacon number of 2. 1: 6(k 6) (small world p

1) 2 3) 4) 5) [a] Tahara, M., K. Uehira, H. Shimizu, M. Nakada, T. Yamada, K. Mochizuki, M. Shinohara, M. Nishino, R. Hino, H. Yakiwara, H. Miyamachi,

untitled

IPSJ SIG Technical Report Vol.2012-CG-148 No /8/29 3DCG 1,a) On rigid body animation taking into account the 3D computer graphics came

* Meso- -scale Features of the Tokai Heavy Rainfall in September 2000 Shin-ichi SUZUKI Disaster Prevention Research Group, National R

The Phase Behavior of Monooleoylglycerol-Water Systems Mivoshi Oil & Fat Co.. Ltd. Faculty of Science and Technology, Science University of Tokyo Inst

<30365F93C195CA8FDC5F88C092422E696E6464>

Journal of Geography 116 (6) Configuration of Rapid Digital Mapping System Using Tablet PC and its Application to Obtaining Ground Truth

系外惑星大気

mars-cloud_2007_DMseminar-pub.ppt


The faint young Sun paradox Early Mars ( Ga) on Mars wet and warm climate? Valley networks(carr, 1996) The warm climate cannot be sustained (Ka

Fundamental Study on the SOX Gas Sensor Utilizing Beta-Alumina with Sputtered Praseodymium Oxide Thin Films by Shinya YAO1*, Kenji MIYAGAWA1, Shigeru

Vol. 21, No. 2 (2014) W 3 mm SUS304 Ni 650 HV 810 HV Ni Ni Table1 Ni Ni μm SUS mm w 50 mm l 3 mm t 2.2 Fig. 1 XY Fig. 3 Sch

神奈川県西部山北南高感度地震観測井の掘削および孔内検層,Borehole Drilling and Physical Properties of the Yamakita-minami Seismic Observatory in Western Ka

DPA,, ShareLog 3) 4) 2.2 Strino Strino STRain-based user Interface with tacticle of elastic Natural ObjectsStrino 1 Strino ) PC Log-Log (2007 6)

1.7 D D 2 100m 10 9 ev f(x) xf(x) = c(s)x (s 1) (x + 1) (s 4.5) (1) s age parameter x f(x) ev 10 9 ev 2

Study on Application of the cos a Method to Neutron Stress Measurement Toshihiko SASAKI*3 and Yukio HIROSE Department of Materials Science and Enginee

- 4 -

気象学がつくる理科実験.PDF

1 Table 1: Identification by color of voxel Voxel Mode of expression Nothing Other 1 Orange 2 Blue 3 Yellow 4 SSL Humanoid SSL-Vision 3 3 [, 21] 8 325


Microsoft Excelを用いた分子軌道の描画の実習


1

1

hPa ( ) hPa

Jan THE JAPANESE JOURNAL OF ANTIBIOTICS XL-1 Table 1. Outline of administering doses, routes and sampling times *: 4 ml/hr/kg Bacillus subtilis

1


1: A/B/C/D Fig. 1 Modeling Based on Difference in Agitation Method artisoc[7] A D 2017 Information Processing

『広島平和科学』24 (2002) pp


金融機関の資産取引ネットワーク

The Journal of the Japan Academy of Nursing Administration and Policies Vol 12, No 1, pp 49 59, 2008 資料 看護師におけるメンタリングとキャリア結果の関連 Relationship between M

Natural Convection Heat Transfer in a Horizontal Porous Enclosure with High Porosity Yasuaki SHIINA*4, Kota ISHIKAWA and Makoto HISHIDA Nuclear Applie

磁気測定によるオーステンパ ダクタイル鋳鉄の残留オーステナイト定量

食品工学.indb

20 Method for Recognizing Expression Considering Fuzzy Based on Optical Flow

GNSS satellite or Quasar 10m [5] (n 1) 10 6 = K 1 ( P d T ) + K 2( P v T ) + K 3( P v T 2 ) (2) O 1 S G Earth Atmosphere [4] (ray bending) 1 S

/ p p

pp * Yw; Mq 1. 1L 20 cc [1] Sonoluminescence: Light emission from acoustic cavitation bubble. Pak-Kon Choi (Departm

teionkogaku43_527

** Department of Materials Science and Engineering, University of California, Los Angeles, CA 90025, USA) Preparation of Magnetopulmbite Type Ferrite

JAXA-SP indd

1

光学

Abstract This paper concerns with a method of dynamic image cognition. Our image cognition method has two distinguished features. One is that the imag

1..FEM FEM 3. 4.

IHIMU Energy-Saving Principle of the IHIMU Semicircular Duct and Its Application to the Flow Field Around Full Scale Ships IHI GHG IHIMU CFD PIV IHI M

mm mm , ,000 Fig. 1 Locality map of the investigation area NE SW Fi

Fig. 1 Hydrostatic Thrust Bearing Fig. 2 Point loading of elastic half-space

Estimation of Photovoltaic Module Temperature Rise Motonobu Yukawa, Member, Masahisa Asaoka, Non-member (Mitsubishi Electric Corp.) Keigi Takahara, Me


レーザ誘起蛍光法( LIF法) によるピストンの油膜挙動の解析

Core Ethics Vol. : - : : : -

ÿþ


1 2 40/ a M. W. 14, 1990, R. Stevens, Medical Practice in Modern England, Yale University Press, 1966B , 1981F. Honigsba

( )

Hideki MATSUOKA: An Introduction to Small-angle Scattering Fundamental aspects of small-angle scattering technique are duly explained from the very ba

Transcription:

( ) 2014/11/11 -

Outline 1 : 2? 3 ( ) 4

Outline 1 : 2? 3 ( ) 4

( ) S N

?

? ( ). ( ).

:,,, etc.? ( ),, ( ) : ( 800 C)

, ( ), ( ) (, )

( )?

( ) I B v N Q B N F F S S, :

( ) ( ) E Normal Neutral Plane S G H N F Normal Plane of Maximum Induction

?

?

Have any Questions?

Outline 1 : 2? 3 ( ) 4

? 1 2 3...?

? 1 2 3...?

( )... 1 2 ( )?

? 1 2 3...?

: 1650, : 1950

? 1 2 3...?

...?

Have any Questions?

Outline 1 : 2? 3 ( ) 4

?

(1): :!

(2): :

(3):

(1): : 100

(2):?

:?? ( ) :?

(1): :, : 35,

(1):

(2): :???

ガス 氷惑星

(1)

(1)

:, : ( )

??

Have any Questions?

Outline 1 : 2? 3 ( ) 4

: :??

(1) - Barabash, S., 2012: Classes of the solar wind interactions in the solar system. Earth Planets Space, 64, 57--59. - Christensen, U., 2006: A deep dynamo generating Mercury s magnetic field. Nature, 444, 1056--1058. - Dougherty, M. K., Khurana, K. K., Neubauer, F. M., Russell, C. T., Saur, J., Leisner, J. S., Burton, M. E., 2006: Identification of a dynamic atmosphere at Enceladus with the Cassini magnetometer. Science, 311, 1406--1409. - Garrick-Bethell, I., Weiss, B. P., Shuster, D. L., Buz, J., 2009: Early lunar magnetism. Science 323, 356--359. - Heimpel, M., Aurnou, J., Al-Shamali, F., Gomez-Perez, N., 2005: A numerical study of dynamo action as a function of spherical shell geometry. Earth Planet. Sci. Lett. 236, 542--557. - Jia, X., Walker, R. J., Kivelson, M. G., Khurana, K. K., Linker, J. A., 2009: Properties of Ganymede s magnetosphere inferred from improved three-dimensional MHD simulations. J. Geophys. Res. (submitted) - Jia, X., Kivelson, M. G., Khurana, K. K., Walker, R. J., 2010: Magnetic Fields of the Satellites of Jupiter and Saturn. Space Sci. Rev., 152, 271--305. - Khurana, K. K., Kivelson, M. G., Russell, C. T., 2002: Searching for liquid water in Europa by using surface observatories. Astrobiology 2, 93--103. - Khurana, K. K., Russell, C. T., Dougherty, M. K., 2008: Magnetic portraits of Tethys and Rhea. Icarus, 193, 465--474.

(2) - Lang, K. R., 2011: The Cambridge guide to the solar system, Cambridge Univ. Press, Cambridge, 475pp. - Luhmann, J. G., 1995: Plasma interaction with unmagnetized bodies. in Introduction to Space Physics, Eds. Kivelson, M. G., Russell, C. T., Cambridge Univ. Press, Cambridge, pp. 203--226. - Mcfadden, L., Weissman, P. R., Johnson, T. V. (Eds). 2007: Encyclopedia of the Solar system, 2nd Edition, Academic Press, San Diego, 982pp. - Nimmo, F., Stevenson, D. J., 2000: Influence of early plate tectonics on the thermal evolution and magnetic field of Mars. J. Geophys. Res. Planet. 105, 11969--11979. - Russell, C. T., Baker, D. N., Slavin, J. A., 1988: The magnetosphere of Mercury. in Mercury. Eds. Vilas, F., Chapman, C. R., Matthews, M. S., Univ.Arizona Press, Tucson, pp. 514--561. - Schubert, G., Soderlund, K. M., 2011: Planetary magnetic fields: Observations and models. Phys. Earth Planet. Inter., 187, 92--108. - Soderlund, K. M., Aurnou, J. M., 2010: Simulation of an ice giant-style dynamo. American Geophysical Union Fall Meeting 2010. San Francisco. - Stanley, S., Bloxham, J., 2004: Convection-region geometry as the cause of Uranus and Nepturne s magnetic fields. Nature, 428, 151-153.

(3) - Stanley, S., Bloxham, J., Hutchison, W., Zuber, M., 2005: Thin shell dynamo models consistent with Mercury s weak observed magnetic field. Earth Planet. Sci. Lett., 234, 27--38. - Stanley, S., Elkins-Tanton, L., Zuber, M., Parmentier, E. M., 2008: Mars paleomagnetic field as the result of a single-hemisphere dynamo. Science 321, 1822--1825. - Stanley, S., Glatzmaier, G. A., 2010: Dynamo models for planets other than Earth. Space Sci. Rev., 152, 617--649. - Stegman, D. R., Jellinek, A. M., Zatman, S. A., Baumgardner, J. R., Richards, M. A., 2003: An early lunar core dynamo driven by thermochemical mantle convection. Nature 421, 143--146. - Stevenson, D. J., 1983: Planetary magnetic fields. Rep. Progr. Phys. 46, 555--620. - Stevenson, D. J., 2010 : Planetary magnetic fields: achievements and prospects. Space Sce. Rev., 152, 651-664. - Takahashi, F., Matsushima, M., 2006: Dipolar and non-dipolar dynamos in a thin shell geometry with implications for the magnetic field of Mercury. Geophys. Res. Lett. 33, doi:10.1029/2006gl025792. - Vilim, R., Stanley, S., Hauck, S., 2008: Dynamo generation in the presence of iron snow zones: Application to mercury s weak surface field. Eos Trans. AGU 89(53), Fall Meet. Suppl., Abstract U21A-0004

- Magnetic field of an ideal cylindrical magnet with its axis of symmetry inside the image plane, Geek3, http://commons.wikimedia.org/wiki/file:vfpt_cylindrical_magnet_thumb.svg, CC BY-SA 3.0 -,, http://www.sci.hokudai.ac.jp/mineral/index.php/ 1 - A simple electromagnet, consisting of an insulated wire wound around an iron core, Public Domain - Diagram of a solenoid s magnetic field, Geek3 http://commons.wikimedia.org/wiki/file:vfpt_solenoid_correct.svg, CC BY-SA 3.0 - Illustration of the Lorentz force, Pietz, http://commons.wikimedia.org/wiki/file:lorentzkraft_v2.svg, CC BY-SA 3.0 - Seitenlˆˆc3ˆˆa4ufer-Dynamo fˆˆc3ˆˆbcr ein fahrendes Gerˆˆc3ˆˆa4t, Stahlkocher, http://commons.wikimedia.org/wiki/file:bicycle_dynamo.jpg, CC BY-SA 3.0 - Drawing based on w:image:dynamo - commutating plane idealized.jpg, Borb, http://en.wikipedia.org/wiki/image:dynamo_-_commutating_plane_idealized.jpg, CC BY-SA 3.0 Original Ver: http://en.wikipedia.org/wiki/file:dynamo_-_commutating_plane_idealized.jpg - A schematic illustrating the relationship between motion of conducting fluid, organized into rolls by the Coriolis force, and the magnetic field the motion generates. http://commons.wikimedia.org/wiki/file:outer_core_convection_rolls.jpg, Public Domain