Magnetospheric Plasmas 201311-13 November, 2013

【Program】
11 Nov (Mon)<So Juicy!>
09:30
K. Khurana
Induced magnetic fields at Europa, Ganymede and Callisto
10:10
P. Brandt
JUICE/Particle Environment Package (PEP): Global imaging and in-situ
observations of the Jovian Magnetosphere and Torus.
10:50<Inner-magnetosphere and ERG>
10:50
L. ChenRecent modeling of Electromagnetic Ion Cyclotron Waves in the Earth's
magnetosphere and their effect of the Earth's Radiation Belt
11:30
<Lunch> & Poster setting-up
Poster viewing
13:30
Y. Miyoshi
Introduction to ERG
14:00K. Keika
Dynamics of heavy ions in the Earth's inner magnetosphere and its contribution to
the global system
14:40

D. Turner
Revelations in radiation belt physics from the new era of multi-constellation
observations
15:20<Break>15:35
M. Usanova
Understanding the role of EMIC waves in radiation belt and ring current
dynamics: Recent Advances
16:15
M. Shoji
Simulation of electromagnetic ion cyclotron triggered emissions: contribution toERG mission
16:55
Y. Omura
Relativistic electron microbursts due to nonlinear pitch angle scattering by EMIC
triggered emissions
17:25

12 Nov (Tue)<Plasma Imaging and Hisaki/SPRINT-A>
09:00
Y. Ezoe
GEO-X : Imaging of Diffuse X-rays from the Earth's Magnetosphere
09:40
I. Yoshikawa
Introduction to Hisaki
10:10
S. Badman
A unique opportunity to discover how energy is transported through Jupiter'smagnetosphere
10:50<Break>11:05

A. Steffl
The Jovian System in the Ultraviolet: Implications for Hisaki and JUICE
11:45
E. Quémerais
Planning Stellar observations in the EUV, a collaboration between EXCEED andPHEBUS/BC
12:25<Lunch>Poster viewing
14:30
R. KraftCoordinated SPRINT-A/Chandra observations of the Jovian Aurora and the Io
Plasma Torus
15:10<M-I coupling and SPRINT-A/EXCEED>
15:10
N. Achilleos
What can observed changes in the size of Jupiter's auroral oval tell us about thechanging conditions at Io?
15:50
L. RayBreaking the azimuthal symmetry in Jupiter’s magnetosphere-ionospherethermosphere coupled system
16:30
Poster viewing<Student-style Party>
13 Nov (Wed)<Magnetic Reconnection and MMS>
09:00
Y. Saito
Introduction to MMS

09:30T. Phan
MMS strategies for capturing key reconnection regions10:10
S. Zenitani
Magnetic diffusion and ion nonlinear dynamics in magnetic reconnection
10:50
Poster viewing<Lunch>13:20
X. JiaGlobal simulations of the two smallest magnetospheres - Ganymede and Mercury
14:00
A. Masters
Magnetic reconnection at a planetary magnetopause: The Mercury-Saturncomparison
14:40<Break>14:55
S. Kawai
Toward predictive simulation of global magnetospheric dynamics: A new highly
accurate numerical method for magnetohydrodynamics
15:35
K. Higashimori
Self-generated turbulence in ion-scale reconnection jets
16:05
K. HirabayashiCollisionless magnetic reconnection under anisotropic MHD approximation
16:35<Adjourn>

【Poster】
NameNO.

Affiliation

Title

1

Keiichiro

Fukazawa

Kyushu Univ.

Simulation of Planetary Magnetosphere toward Exa-flops Computing Era

2

Yuto

Kato

Tohoku Univ.

Effect of the background magnetic field inhomogeneity on generation
processes of whistler-mode chorus and broadband hiss-like emissions

3

KatsuakiHigashimori Univ. of Tokyo

A new approach for phenomena in an extremely high Reynolds number:
Turbulent magnetic reconnection

4

ToshiakiMatsumura Tohoku Univ.

5

YusukeOyama

Univ. of Tokyo

6Shinji

Saito

STEL

Dependence of Frequency Drift Rates of Whistler Chorus Elements for theRelativistic Electron Accelerations

7KenyaShimizu

Univ. of Tokyo・ISAS/JAXA

A study on maintenace and decay of magnetic reconnectin rate

8TohruShimizu

Ehime Univ.

Geotail data analysis to detect three-dimensional features of the
spontaneous fast magnetic reconnection

9TooruSugiyama

JAMSTEC

Co-evolution of upstream waves and accelerated particles
around parallel shocks

10 Hiroyuki

Torii

Ehime Univ.

Sheet current plasma flows to be observed in the three dimensional
spontaneous fast magnetic reconnection

11 Hiroshi

Hasegawa

JAXA/ISAS

A review of magnetopause and boundary layer studies in 2011-2013

12 Tomoaki

Hori

STEL

Evolution of convection vortices associated with sudden impulses observedby SuperDARN

13 Yuichi

KatoSTEL

Statistical analysis of EMIC waves observed by the Akebono satellite in theinner magnetosphere

14 Mariko

Teramoto

ISAS/JAXA

Characteristics of mid-latitude Pi2 pulsations observed by the SuperDARN
radar in North America

15 SatokoYamauchi

Tokyo Inst. of Tech.

Magnetospheric electron injections in quiet conditions

16 Yuichiro

Ezoe

Tokyo Metropolitan Univ.

Lightweight and Compact Soft X-ray Imaging Spectrometer for Future Solar
System Exploration

17 ShuheiHasegawa

STELLong-term variation of plasmasphere observed from the Akebono PWS data

18 Yasumasa Kasaba

Tohoku Univ..

The Radio & Plasma Wave Investigation (RPWI) for JUICE: Contribution planfrom Japan

19 Yasumasa Kasaba

Tohoku Univ.

Ground support observations for and non-planetary targets of JAXASPRINT-A mission

20 MarikoKawamura

Univ. of Tokyo・ISAS/JAXA

A study on the generation mechanisms of the lunar originating ions21 Tomoki

KimuraISAS/JAXA

X-ray spectral model of Io plasma torus for plasma diagnostic

22 Hajime

Kita

Tohoku Univ.

Investigation of the solar UV/EUV heating effect on the Jovian radiation belt
based on radio/infrared observation

23 Hirotaka

Kitagawa

Univ. of Tokyo・ISAS/JAXA

Dependence of Jovian Magnetotail Reconnection on Rotational Phase

24 Daichi

MarunoTohoku Univ.

Occurrence characteristics of Saturn kilometric radiation short-term bursts

25 Takahiro

Mizuguchi

Tohoku Univ.

Study of occurrence processes of the Jovian substorm-like events

26 Masaki

NishinoNagoya Univ.

Type-II entry of solar wind protons into the lunar wake: Effects of magnetic
connection to the night-side surface

27 Fuminori

Tsuchiya

Tohoku Univ.

28 Shinya

Watanabe

Tohoku Univ.

Test particle simulation of interactions between relativistic electrons andobliquely propagating whistler-mode waves
Dynamical pictures of fast magnetic reconnectionmade public by newly highresolution MHD simulations

Pointing control of extreme ultraviolet spectroscope onboard the SPRINT-A
satellite
Study of the plasma density distribution around Ganymede by the Galileo
spacecraft observation