| 2008∼ |
|
*---------*---------*---------*---------*---------*
|
J | |
"Validation of Two MHD Models of the Solar Corona with Rotational Tomography",
Alberto M. Vasquez, Richard A. Frazin, Keiji Hayashi, Igor V.
Sokolov, Ofer Cohen, Ward B. Manchester IV, and Farzad Kamalabadi,
ApJ
(2008) Vol.682, 1328--1337, doi:10.1086/589682 ;
link to ADS
|
J | $ |
"MHD Simulations of the Global Solar Corona around the Halloween Event in 2003
Using the Synchronic Frame Format of the Solar Photospheric Magnetic Field",
Keiji Hayashi, Xue Pu Zhao, and Yang Liu,
JGR
(2008) Vol.113, A07104, doi:10.1029/2007JA012814 ;
link to ADS
|
m | $ |
"An MHD simulation model of the global solar corona with
the time-varying boundary magnetic field based on the measurement data",
Keiji Hayashi,
SPD/AGU joint assembly 2008 (#SH51B-02),
27--30 May 2008 / Fort Lauderdale, FL
|
w | $ |
"MHD simulation of the solar corona using the daily-updated solar surface magnetic field data",
Keiji Hayashi, Xudong Sun, and Yang Liu,
SDO Science Teams Meeting,
25--28 March 2008 / Napa, CA
|
| 2007 |
W | $ |
"From the Sun to the Earth
---
MHD models connecting observable and invisible regions
---
(originally given in Japanese)",
K. Hayashi,
GEMSIS workshop,
26--28 December 2007 / Inuyama, Japan
|
J | |
"IPS tomographic observations of 3D solar wind structure",
Kojima, M., M. Tokumaru, K. Fujiki, K. Hayashi, and B. V. Jackson,
Astronomical and Astrophysical Transactions
(2007) Vol.26, No.6, 467--476 ;
link to ADS
|
m | $ |
"An MHD simulation model of the global solar corona with the time-varying boundary magnetic field
driven with the current at the lower corona",
K. Hayashi,
AGU fall meeting (#SH53A-1072),
10--14 December 2007 / San Francisco, CA
|
m | $ |
"MHD Simulation of The Solar Corona Using The Synchronic Frame Format of
The Solar Magnetic Field and The EIT-based Temperature Map",
K. Hayashi, X. P. Zhao, E. Benevolenskaya, and Y. Liu,
AAS 210th meeting (#91.06),
27--31 May 2007 / Honolulu, HI
|
| 2006 |
m | $ |
"MHD Simulation of the Global Solar Corona Using the Synoptic Frame
of the Photospheric Magnetic Field and Coronal-Base Temperature",
Keiji Hayashi, Xue Pu Zhao, and Elena Benevolenskaya,
AGU fall meeting (#SH23B-0351),
11--15 December 2006 / San Francisco, CA
|
W | $ |
"MHD simulation of solar corona and solar wind and
the sub-Alfvénic boundary treatments to utilize the measurement data",
Keiji Hayashi,
CAWSES International Workshop on Space Weather Modeling (CSWM),
14--17 November 2006, Yokohama, Japan
|
J | $ |
"MHD simulation of two successive interplanetary disturbances
driven by Cone-model parameters in IPS-based solar wind",
K. Hayashi, X. P. Zhao, and Y. Liu,
GRL
(2006) Vol.33 No.20, L20103, doi:10.1029/2006GL027408 ;
link to ADS
|
m | $ |
"The MHD simulation of the solar corona using the synoptic frame map
of the solar photospheric magnetic field and the SOHO/EIT coronal temperature map",
Hayashi, K., Zhao, X. P., and Benevolenskaya, E.,
36th COSPAR Scientific Assembly
(#PSW1-0048-06, PSW1-1MO1P-0150, IT2-0150),
16--23 July 2006 / Beijing, P. R. China
|
m | $ |
"The plasma parameters in the shrinking magnetic flux tubes in the solar corona",
K. Hayashi, X. P. Zhao, and Y. Liu,
AGU 2006 Joint Assembly (#SH43A-03),
23--26 May 2006 / Baltimore, MD
|
J | |
"The 2003 October-November Fast Halo Coronal Mass Ejections and
the Large-Scale Magnetic Field Structures",
Liu, Y., and Hayashi, K.,
ApJ
(2006) Vol.640, 1135--1141, doi:10.1086/500290 ;
link to ADS
|
pW | $ |
"Three-dimensional time-dependent MHD simulation model of the solar corona and solar wind",
Keiji Hayashi,
Proceedings of the International Living With a Star (ILWS) Workshop
(19--24 February 2006 / Goa, India; edited by N. Gopalswamy and A. Bhattacharyya.)
ISBN: 81-87099-40-2, p.124
link to ADS
|
w | $ |
"MHD simulation of the solar corona using the SOHO/MDI magnetograph data",
Keiji Hayashi,
SDO AIA-HMI Science Teams Meeting,
12--17 February 2006 / Monterey, CA
|
J | $ |
"Three-Dimensional Magnetohydrodynamic Simulation of a Global Solar Corona
Using a Temperature Distribution Map Obtained from SOHO EIT Measurements",
Keiji Hayashi, Elena Benevolenskaya, Todd Hoeksema, Yang Liu, and Xue Pu Zhao,
ApJ Letters
(2006) Vol.636, 165--168, doi:10.1086/500127 ;
link to ADS
|
| 2005 |
J | $ |
"Magnetohydrodynamic Simulations of the Solar Corona and Solar Wind
Using a Boundary Treatment to Limit Solar Wind Mass Flux",
Hayashi, K.,
the Astrophysical Journal (ApJ) Supplement Series
(2005) Vol.161, 480--494, doi:10.1086/491791 ;
link to ADS
|
m | $ |
"MHD Simulation of the Global Solar Corona Using
the Synoptic Frame of the Photospheric Magnetic Field",
Keiji Hayashi, Yang Liu, and Xue Pu Zhao,
AGU fall meeting
(#SH11A-0246),
5--9 December 2005 / San Francisco, CA
|
m | $ |
"The MHD simulation on the coronal plasma in radially shrinking open magnetic flux tubes",
Keiji Hayashi, Zhao, X. P., and Poduval, B.,
AAS/AGU Joint Assembly (#SH13A-06),
23--27 May 2005 / New Orleans, LA
(abstract)
|
| 2004 |
m | $ |
"Time-Dependent Three-Dimensional MHD Simulation
of Solar Corona and Solar Wind at Solar Minimum Phase",
Keiji Hayashi, Yang Liu, and Xue Pu Zhao,
AGU fall meeting (#SH13A-1156),
13--17 December 2004 / San Francisco, CA
|
M | $ |
"MHD Simulation Model of the Interplanetary Disturbance Propagation
Following the Flare of 2002 April 17.",
K. Hayashi, Y. Liu, and X. P. Zhao,
American Astronomical Society (AAS) 204th meeting (#62.07),
31 May -- 3 June 2004 / Denver, CO
|
w | $ |
"MHD simulation of solar wind using solar photospheric magnetic field data",
K. Hayashi,
Living With a Star (LWS) Workshop, 22--26 March 2004, Boulder, CO
|
J | |
"Fast Solar Wind after the Rapid Acceleration",
Kojima, M., A. R. Breen, K. Fujiki, K. Hayashi, T. Ohmi, and M. Tokumaru,
JGR
(2004) Vol.109(A4), A04103, doi:10.1029/2003JA010247 ;
link to ADS
|
| 2003 |
m | $ |
"Solar Corona Obtained with MHD Simulation Using Various Boundary Treatments
Based on Characteristic Projection Method",
K. Hayashi, Y. Liu, and X. Zhao,
AGU fall meeting (#SH42B-0524),
8--12 December 2003 / San Francisco, CA
(abstract)
|
m | |
"The Relation Between the Solar Wind Velocity and the Magnetic Conditions of Coronal Holes",
Hirano, M., Kojima, M., Tokumaru, M., Fujiki, K., Ohmi, T., Yamashita, M.,
Hakamada, K., and Hayashi, K.,
AGU fall meeting (#SH21B-0164),
8--12 December 2003 / San Francisco, CA
|
J | |
"Polar low-speed solar wind reappeared at the solar activity maximum of cycle 23",
Ohmi, T., M. Kojima, K. Fujiki, M. Tokumaru, K. Hayashi, and K. Hakamada,
Geophysical Research Letters (GRL)
(2003) Vol.30 No.7, L1409, doi:10.1029/2002GL016347 ;
link to ADS
|
J | |
"How did the solar wind structure change around the solar maximum?
---
From interplanetary scintillation observation",
Fujiki, K., M. Kojima, M. Tokumaru, T. Ohmi, A. Yokobe, K. Hayashi,
D. J. McComas, and H. A. Elliott,
Annales Geophysichae
(2003) Vol.21-6, 1257--1261 ;
link to ADS
|
P | |
"Solar wind velocity structure around the solar maximum
observed by interplanetary scintillation",
Fujiki, K., M. Kojima, M. Tokumaru, T. Ohmi, A. Yokobe, K. Hayashi,
D. J. McComas, and H. A. Elliott,
Solar Wind Ten : AIP Conference Proceedings
(2003) Vol.679, 226--229, doi:10.1063/1.1618583
|
P | $ |
"Basic Results of MHD Tomography Analysis Method for IPS Observation",
Keiji Hayashi, Ken'ichi Fujiki, Masayoshi Kojima, and Munetoshi Tokumaru,
Solar Wind Ten : AIP Conference Proceedings
(2003) Vol.679, 144--147, doi:10.1063/1.1618562 ;
link to ADS
|
P | |
"Solar Cycle Dependence of High-Latitude Solar Wind",
Fujiki, K., M. Kojima, M. Tokumaru, T. Ohmi, A. Yokobe, and K. Hayashi,
Solar Wind Ten : AIP Conference Proceedings
(2003) Vol.679, 141--143, doi:10.1063/1.1618561
|
P | |
"Evidences for Low-speed Streams from Small Coronal Hole",
Tomoaki Ohmi, Masayoshi Kojima, Keiji Hayashi, Atushi Yokobe,
Munetoshi Tokumaru, Ken'ichi Fujiki, and Kazuyuki Hakamada,
Solar Wind Ten : Proceedings of the Tenth International Solar Wind Conference.
(edited by M. Velli, R. Bruno, and F. Malara),
American Institute of Physics (AIP) Conference Proceedings
(2003) Vol.679, 137--140, American Institute of Physics
|
P | |
"Solar wind imaging facility (SWIFT) for space weather research",
Kojima, M., Tokumaru, M., Fujiki, K., Ishida, Y., Ohmi, T., Hayashi, K., and Yamashita, M.
Innovative Telescopes and Instrumentation for Solar Astrophysics :
Proceedings of the International Society for Optical Engineering (SPIE).
(edited by Stephen L. Keil, Sergey V. Avakyan)
(2003) Vol.4853, 121--128
|
M | |
"The 3d Solar Wind Over the Solar Cycle Observed by IPS",
Kojima, M., Bernard, V. J., Ohmi, T., Hick, P., Hayashi, K., Tokumaru, M., and Fujiki, K.
The Sun and the Heliosphere as an Integrated System,
25th meeting of the International Astronomical Union (IAU) Joint Discussion 7,
July 2003 / Sydney, Australia
|
J | $ |
"MHD Tomography Method Using Interplanetary Scintillation Measurement",
Keiji Hayashi, Masayoshi Kojima, Munetoshi Tokumaru, and Ken'ichi Fujiki,
the Journal of Geophysical Research (JGR)
(2003) Vol.108(A3), 1102--1115, doi:10.1029/2002JA009567 ;
link to Astrophysics Data System (ADS) Abstract Service
|
| ∼2002 : some of publications/presentations |
M | $ |
"Heliospheric MHD simulations using IPS solar wind measurement data
(originally given in Japanese)",
Keiji Hayashi,
Astronomical Society of Japan fall meeting,
September 2002 / Miyazaki, Japan
|
W | $ |
"Global Structure of Solar Wind Derived from IPS observational data
and MHD tomography analysis",
Keiji Hayashi,
The Second Japan-Korea-China Joint Workshop on Space Weather (#O-03),
September 2002 / Rikubetsu, Hokkaido, Japan
|
M | $ |
"MHD tomography Using IPS observation",
Keiji Hayashi, Masayoshi Kojima, Munetoshi Tokumaru, and Ken'ichi Fujiki,
American Geophysical Union (AGU) fall meeting (#SH31A-0697),
10--14 December 2001 / San Francisco, CA
(abstract)
|
M | $ |
"The three-dimensional structure of the solar wind determined by
combining the MHD simulation and the IPS observation data",
Keiji Hayashi, Masayoshi Kojima, Munetoshi Tokumaru, and Ken'ichi Fujiki,
the 2001 Japan Geoscience Union Meeting,
June 2001 / Tokyo, Japan
(abstract)
|
m | $ |
"The speed of the solar wind and the solar surface and coronal magnetic field",
Hayashi, K., and Yoshimura, H.,
33rd Committee on Space Research (COSPAR) Scientific Assembly (#PSW1-0073),
16--23 July 2000 / Warsaw, Poland
(abstract)
|