✦ LIBER ✦

3D nonlinear wave heating of coronal loops

✍ Scribed by S. Poedts; J. P. Goedbloed

Publisher: Springer Netherlands
Year: 1994
Tongue: English
Weight: 348 KB
Volume: 68
Category: Article
ISSN: 0038-6308
DOI: 10.1007/bf00749123

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Coronal loop heating by Alfvén waves

✍ C. A. De Azevedo; A. G. Elfimov; A. S. De Assis 📂 Article 📅 1994 🏛 Springer 🌐 English ⚖ 536 KB

Heating of coronal loops by fast mode MH

Heating of coronal loops by fast mode MHD waves

✍ Shadia Rifai Habbal; Egil Leer; Thomas E. Holzer 📂 Article 📅 1979 🏛 Springer 🌐 English ⚖ 810 KB

A possible mechanism for the formation and heating of coronal loops through the propagation and damping of fast mode waves is proposed and studied in detail. Loop-like field structures are represented by a dipole field with the point dipole at a given distance below the solar surface. The density of

Coronal loop heating by discrete Alfvén

Coronal loop heating by discrete Alfvén waves

✍ C. A. Azevedo; A. S. Assis; H. Shigueoka; P. H. Sakanaka 📂 Article 📅 1991 🏛 Springer 🌐 English ⚖ 403 KB

We have modeled the solar coronal active loop heating by discrete Alfv6n waves. Discrete Alfv~n waves (DAW) are a new class of Alfv6n waves which can be described by the two-fluid model with finite ion-cyclotron frequency, or the MHD model with plasma current along the magnetic field line as shown b

Observational evidence of continual heat

Observational evidence of continual heating in X-ray emitting coronal loops

✍ M. Gerassimenko; C. V. Solodyna; J. T. Nolte 📂 Article 📅 1978 🏛 Springer 🌐 English ⚖ 617 KB

A 90 s time resolution study of the soft X-ray emission from three active region loops shows the emission to be constant to about two percent over the half hour period of observation. Soft X-ray observations in two wavebands are used to deduce the temperature and density of these loops. The data una

Nonlinear Excitation of Fast Waves by Di

Nonlinear Excitation of Fast Waves by Dispersive Alfvén Waves and Solar Coronal Heating

✍ R. P. Sharma; Sanjay Kumar 📂 Article 📅 2010 🏛 Springer 🌐 English ⚖ 331 KB

Plasma waves caused by transient heat co

Plasma waves caused by transient heat conduction in a coronal loop and anomalous resistivity

✍ T. Takakura 📂 Article 📅 1991 🏛 Springer 🌐 English ⚖ 650 KB

Numerical simulation is made of the transient heat conduction during local heating in a model coronal magnetic loop with an axial electric current. It is assumed that a segment near the top of the normal coronal loop is heated to above 107 K by a sufficiently small heat input as compared with the to