| 저자(한글) |
Yoon, Heesun,Cho, Jungyeon,Kim, Jongsoo |
| 저자(영문) |
|
| 소속기관 |
|
| 소속기관(영문) |
|
| 출판인 |
|
| 간행물 번호 |
|
| 발행연도 |
2016-01-01 |
| 초록 |
Turbulent motions produce density and magnetic field fluctuations. Correlation between density and magnetic field fluctuations are important for interpretation of observations, such as the rotation measure (RM) and dispersion measure (DM). We study the several factors that can affect the correlation between two. In particular, we numerically investigate how the correlation time of driving affects the correlation between density and magnetic field. We perform compressible MHD turbulence simulations at different sonic Mach number and consider two different driving schemes - continuously changing driving and delta-correlated driving. The continuously changing driving results in strong anti-correlation between density and magnetic field when sonic and Alfvenic Mach numbers are similar unity. The delta-correlated driving produces virtually no correlation between two fields. |
| 원문URL |
http://click.ndsl.kr/servlet/OpenAPIDetailView?keyValue=03553784&target=NART&cn=JAKO201615964634939 |
| 첨부파일 |
|
