Coronal heating by waves
Technical Report
·
OSTI ID:6624409
Alfven waves or Alfvenic surface waves carry enough energy into the corona to provide the coronal energy requirements. Coronal loop resonances are an appealing means by which large energy fluxes enter active region loops. The wave dissipation mechanism still needs to be elucidated, but a Kolmogoroff turbulent cascade is fully consistent with the heating requirements in coronal holes and active region loops.
- Research Organization:
- New Hampshire Univ., Durham (USA)
- OSTI ID:
- 6624409
- Report Number(s):
- N-84-13068
- Country of Publication:
- United States
- Language:
- English
Similar Records
Heating of coronal loops by phase-mixid shear Alfven waves
Resonances of coronal loops
MAGNETOHYDRODYNAMIC WAVES AND CORONAL HEATING: UNIFYING EMPIRICAL AND MHD TURBULENCE MODELS
Journal Article
·
Sat Oct 31 23:00:00 EST 1987
· Astrophys. J.; (United States)
·
OSTI ID:5293472
Resonances of coronal loops
Journal Article
·
Tue Jan 31 23:00:00 EST 1984
· Astrophys. J.; (United States)
·
OSTI ID:6747170
MAGNETOHYDRODYNAMIC WAVES AND CORONAL HEATING: UNIFYING EMPIRICAL AND MHD TURBULENCE MODELS
Journal Article
·
Sat Feb 09 23:00:00 EST 2013
· Astrophysical Journal
·
OSTI ID:22167075
Related Subjects
640104* -- Astrophysics & Cosmology-- Solar Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ALFVEN WAVES
ATMOSPHERES
ENERGY TRANSFER
HEATING
HYDROMAGNETIC WAVES
MAGNETIC FIELD CONFIGURATIONS
PHYSICAL PROPERTIES
SOLAR ACTIVITY
SOLAR CORONA
SOLAR WIND
STELLAR ATMOSPHERES
STELLAR CORONAE
THERMAL CONDUCTIVITY
THERMODYNAMIC PROPERTIES
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ALFVEN WAVES
ATMOSPHERES
ENERGY TRANSFER
HEATING
HYDROMAGNETIC WAVES
MAGNETIC FIELD CONFIGURATIONS
PHYSICAL PROPERTIES
SOLAR ACTIVITY
SOLAR CORONA
SOLAR WIND
STELLAR ATMOSPHERES
STELLAR CORONAE
THERMAL CONDUCTIVITY
THERMODYNAMIC PROPERTIES