Abstract
view Abstract Citations (102) References (28) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Scaling Law of Solar Coronal Loops Obtained with YOHKOH Kano, Ryouhei ; Tsuneta, Saku Abstract We find a clear correlation among the maximum temperature Tmax (K), the pressure p (dyn cm-2) and the length L (cm) of 32 steady coronal loop structures observed with Yohkoh Soft X-Ray Telescope: Tmax = 3.8 × 104 (pL)1/(5.1±0.5). The best-fit equation, however, systematically deviates from the theoretical scaling law Tmax = 1.4 × 103 (pL)1/3 derived by Rosner, Tucker, & Vaiana. We examine various possibilities for the cause of the discrepancy. Publication: The Astrophysical Journal Pub Date: December 1995 DOI: 10.1086/176547 Bibcode: 1995ApJ...454..934K Keywords: MAGNETOHYDRODYNAMICS: MHD; SUN: CORONA; SUN: X-RAYS; GAMMA RAYS full text sources ADS |
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
