טוען...
Dissipation and heating in solar wind turbulence: from the macro to the micro and back again
The past decade has seen a flurry of research activity focused on discerning the physics of kinetic scale turbulence in high-speed astrophysical plasma flows. By ‘kinetic’ we mean spatial scales on the order of or, in particular, smaller than the ion inertial length or the ion gyro-radius—the spatia...
שמור ב:
| הוצא לאור ב: | Philos Trans A Math Phys Eng Sci |
|---|---|
| Main Authors: | , , |
| פורמט: | Artigo |
| שפה: | Inglês |
| יצא לאור: |
The Royal Society Publishing
2015
|
| נושאים: | |
| גישה מקוונת: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4394685/ https://ncbi.nlm.nih.gov/pubmed/25848077 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2014.0155 |
| תגים: |
הוספת תג
אין תגיות, היה/י הראשונ/ה לתייג את הרשומה!
|