Search Results - "Shiota, D."

Theory and Transport of Nearly Incompressible Magnetohydrodynamic Turbulence by Zank, G. P., Adhikari, L., Hunana, P., Shiota, D., Bruno, R., Telloni, D.

“…The theory of nearly incompressible magnetohydrodynamics (NI MHD) was developed largely in the early 1990s, together with an important extension to…”
Get full text

Theory and Transport of Nearly Incompressible Magnetohydrodynamic Turbulence. IV. Solar Coronal Turbulence by Zank, G. P., Adhikari, L., Hunana, P., Tiwari, S. K., Moore, R., Shiota, D., Bruno, R., Telloni, D.

“…A new model describing the transport and evolution of turbulence in the quiet solar corona is presented. In the low plasma beta environment, transverse…”
Get full text

II. Transport of Nearly Incompressible Magnetohydrodynamic Turbulence from 1 to 75 au by Adhikari, L., Zank, G. P., Hunana, P., Shiota, D., Bruno, R., Hu, Q., Telloni, D.

“…The thermal plasma beta in the solar wind and the solar corona is of the order of and . Zank et al. developed 2D and slab turbulence transport model equations…”
Get full text

Magnetohydrodynamic Simulations for Studying Solar Flare Trigger Mechanism by Muhamad, J., Kusano, K., Inoue, S., Shiota, D.

“…In order to understand the flare trigger mechanism, we conduct three-dimensional magnetohydrodynamic simulations using a coronal magnetic field model derived…”
Get full text

Turbulent Transport in a Three-dimensional Solar Wind by Shiota, D., Zank, G. P., Adhikari, L., Hunana, P., Telloni, D., Bruno, R.

“…Turbulence in the solar wind can play essential roles in the heating of coronal and solar wind plasma and the acceleration of the solar wind and energetic…”
Get full text

Theory and Transport of Nearly Incompressible Magnetohydrodynamics Turbulence. III. Evolution of Power Anistropy in Magnetic Field Fluctuations throughout the Heliosphere by Adhikari, L., Zank, G. P., Telloni, D., Hunana, P., Bruno, R., Shiota, D.

“…A theoretical model that describes the evolution of the power anisotropy in the energy-containing and inertial ranges throughout the heliosphere is developed…”
Get full text

Probing solar wind velocity from simultaneous superior solar conjunction radio science experiments of BepiColombo and Akatsuki missions by Cappuccio, P, Imamura, T, Doria, I, Chiba, S, Stefano, I di, Shiota, D, Asmar, S, Iess, L

“…ABSTRACT A radio link directly probing the inner solar corona offers the possibility to characterize solar wind properties, including velocity, density,…”
Get full text

Twist and Connectivity of Magnetic Field Lines in the Solar Active Region NOAA 10930 by Inoue, S, Kusano, K, Magara, T, Shiota, D, Yamamoto, T. T

“…Twist and connectivity of magnetic field lines in the flare-productive active region NOAA 10930 are investigated in terms of the vector magnetograms observed…”
Get full text

MAGNETIC STRUCTURE PRODUCING X- AND M-CLASS SOLAR FLARES IN SOLAR ACTIVE REGION 11158 by Inoue, S, Hayashi, K, Shiota, D, Magara, T, Choe, G S

“…We study the three-dimensional magnetic structure of the solar active region 11158, which produced one X-class and several M-class flares on 2011 February…”
Get full text

Coronal mass ejection hits mercury: A.I.K.E.F. hybrid-code results compared to MESSENGER data by Exner, W., Heyner, D., Liuzzo, L., Motschmann, U., Shiota, D., Kusano, K., Shibayama, T.

“…Mercury is the closest orbiting planet around the sun and is therefore embedded in an intensive and highly varying solar wind. In-situ data from the MESSENGER…”
Get full text

NONLINEAR FORCE-FREE EXTRAPOLATION OF THE CORONAL MAGNETIC FIELD BASED ON THE MAGNETOHYDRODYNAMIC RELAXATION METHOD by Inoue, S, Magara, T, Pandey, V S, Shiota, D, Kusano, K, Choe, G S, Kim, K S

“…We develop a nonlinear force-free field (NLFFF) extrapolation code based on the magnetohydrodynamic (MHD) relaxation method. We extend the classical MHD…”
Get full text

POLAR FIELD REVERSAL OBSERVATIONS WITH HINODE by SHIOTA, D, TSUNETA, S, SHIMOIO, M, SAKO, N, OROZCO SUAREZ, D, ISHIKAWA, R

“…We have been monitoring yearly variation in the Sun's polar magnetic fields with the Solar Optical Telescope aboard Hinode to record their evolution and…”
Get full text

Predicting Observational Signatures of Coronal Heating by Alfvén Waves and Nanoflares by Antolin, P, Shibata, K, Kudoh, T, Shiota, D, Brooks, D

“…Alfven waves can dissipate their energy by means of nonlinear mechanisms, and constitute good candidates to heat and maintain the solar corona to the observed…”
Get full text

BUILDUP AND RELEASE OF MAGNETIC TWIST DURING THE X3.4 SOLAR FLARE OF 2006 DECEMBER 13 by INOUE, S, SHIOTA, D, YAMAMOTO, T. T, PANDEY, V. S, MAGARA, T, CHOE, G. S

“…We analyze the temporal evolution of the three-dimensional magnetic structure of the flaring active region (AR) NOAA 10930 by using the nonlinear force-free…”
Get full text

A STUDY OF THE HELIOCENTRIC DEPENDENCE OF SHOCK STANDOFF DISTANCE AND GEOMETRY USING 2.5D MAGNETOHYDRODYNAMIC SIMULATIONS OF CORONAL MASS EJECTION DRIVEN SHOCKS by SAVANI, N. P, SHIOTA, D, KUSANO, K, VOURLIDAS, A, LUGAZ, N

“…We perform four numerical magnetohydrodynamic simulations in 2.5 dimensions (2.5D) of fast coronal mass ejections (CMEs) and their associated shock fronts…”
Get full text

Evolution of Coronal Mass Ejection Morphology with Increasing Heliocentric Distance. I. Geometrical Analysis by Savani, N. P, Owens, M. J, Rouillard, A. P, Forsyth, R. J, Kusano, K, Shiota, D, Kataoka, R

“…At launch, coronal mass ejections (CMEs) are often approximated as locally cylindrical objects with circular cross sections. However, CMEs have long been known…”
Get full text

Three-dimensional MHD modeling of the solar wind structures associated with 13 December 2006 coronal mass ejection by Kataoka, R., Ebisuzaki, T., Kusano, K., Shiota, D., Inoue, S., Yamamoto, T. T., Tokumaru, M.

“…A 3‐D magnetohydrodynamic (MHD) simulation is performed to reconstruct the interplanetary propagation of a coronal mass ejection (CME) that occurred on 13…”
Get full text

Internal structure of a coronal mass ejection revealed by Akatsuki radio occultation observations by Ando, H., Shiota, D., Imamura, T., Tokumaru, M., Asai, A., Isobe, H., Päzold, M., Häusler, B., Nakamura, M.

“…A coronal mass ejection (CME) was observed at the heliocentric distance of 12.7 Rυ by radio occultation measurements using the Akatsuki spacecraft. The…”
Get full text

Air shower simulation for WASAVIES: warning system for aviation exposure to solar energetic particles by Sato, T, Kataoka, R, Yasuda, H, Yashiro, S, Kuwabara, T, Shiota, D, Kubo, Y

“…WASAVIES, a warning system for aviation exposure to solar energetic particles (SEPs), is under development by collaboration between several institutes in Japan…”
Get full text

SOLAR RADIO TYPE-I NOISE STORM MODULATED BY CORONAL MASS EJECTIONS by Iwai, K., Miyoshi, Y., Masuda, S., Shimojo, M., Shiota, D., Inoue, S., Tsuchiya, F., Morioka, A., Misawa, H.

“…The first coordinated observations of an active region using ground-based radio telescopes and the Solar Terrestrial Relations Observatory (STEREO) satellites…”
Get full text