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  1. Journal of Astrophysics and Astronomy
  2. Journal of Astrophysics and Astronomy : Volume 27
  3. Journal of Astrophysics and Astronomy : Volume 27, Issue 2-3, June 2006
  4. Mechanisms of coronal heating
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Journal of Astrophysics and Astronomy : Volume 38
Journal of Astrophysics and Astronomy : Volume 37
Journal of Astrophysics and Astronomy : Volume 36
Journal of Astrophysics and Astronomy : Volume 35
Journal of Astrophysics and Astronomy : Volume 34
Journal of Astrophysics and Astronomy : Volume 33
Journal of Astrophysics and Astronomy : Volume 32
Journal of Astrophysics and Astronomy : Volume 31
Journal of Astrophysics and Astronomy : Volume 30
Journal of Astrophysics and Astronomy : Volume 29
Journal of Astrophysics and Astronomy : Volume 28
Journal of Astrophysics and Astronomy : Volume 27
Journal of Astrophysics and Astronomy : Volume 27, Issue 4, December 2006
Journal of Astrophysics and Astronomy : Volume 27, Issue 2-3, June 2006
Preface
Why Study the Sun?
Some recent developments in solar dynamo theory
Helicity of solar active regions from a dynamo model
Nanoflares and heating of the solar corona
Evolving coronal holes and interplanetary erupting stream disturbances
Mechanisms of coronal heating
Spectroscopic studies of solar corona VI: Trend in line-width variation of coronal emission lines with height independent of the structure of coronal loops
Physics of the sun’s hot atmosphere
Magnetic source regions of coronal mass ejections
North-south distribution of solar flares during cycle 23
Initiation of cmes by magnetic flux emergence
Flare ribbon expansion and energy release
Solar x-ray spectrometer (SOXS) mission – Low energy payload – First results
EUV and coronagraphic observations of coronal mass ejections
Enigmatic solar wind disappearance events – Do we understand them?
Transient perturbations and their effects in the heliosphere, the geo-magnetosphere, and the Earth’s atmosphere: Space weather perspective
Space weather effects of coronal mass ejection
Geo-effectiveness of solar wind extremes
The challenge of predicting the occurrence of intense storms
Coronal mass ejections of solar cycle 23
Photospheric, chromospheric and helioseismic signatures of a large flare in super-active region NOAA 10486
Extremely energetic 4B/X17.2 flare and associated phenomena
The flares associated with the dynamics of the sunspots
Design and status of Solar Vector Magnetograph (SVM-I) at Udaipur solar observatory
Research facilities for solar astronomy at ARIES
Data acquisition, control, communication and computation system of solar X-ray spectrometer (SOXS) mission
Observational study of solar magnetic active phenomena
Development of solar scintillometer
Spatial damping of linear compressional magnetoacoustic waves in quiescent prominences
Observational searches for chromospheric G-mode oscillations from CaII H-line observations
The extreme solar activity during october–november 2003
Study of microflares through soxs mission
Study of a large helical eruptive prominence associated with double CME on 21 April 2001
Magnetosonic waveguide model of solar wind flow tubes
Analysis of plasma and field conditions during some intensely geo-effective transient solar/interplanetary disturbances of solar cycle 23
The influence of solar activity on the rainfall over India: Cycle-to-cycle variations
Journal of Astrophysics and Astronomy : Volume 27, Issue 1, March 2006
Journal of Astrophysics and Astronomy : Volume 26
Journal of Astrophysics and Astronomy : Volume 25
Journal of Astrophysics and Astronomy : Volume 24
Journal of Astrophysics and Astronomy : Volume 23
Journal of Astrophysics and Astronomy : Volume 22
Journal of Astrophysics and Astronomy : Volume 21
Journal of Astrophysics and Astronomy : Volume 20
Journal of Astrophysics and Astronomy : Volume 19
Journal of Astrophysics and Astronomy : Volume 18

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Mechanisms of coronal heating

Content Provider Springer Nature Link
Author Verma, S. R.
Copyright Year 2006
Abstract The Sun is a mysterious star. The high temperature of the chromosphere and corona present one of the most puzzling problems of solar physics. Observations show that the solar coronal heating problem is highly complex with many different facts. It is likely that different heating mechanisms are at work in solar corona. Recent observations show that Magnetic Carpet is a potential candidate for solar coronal heating.
Starting Page 113
Ending Page 114
Page Count 2
File Format PDF
ISSN 02506335
Journal Journal of Astrophysics and Astronomy
Volume Number 27
Issue Number 2-3
e-ISSN 09737758
Language English
Publisher Springer India
Publisher Date 2006-01-01
Publisher Institution Indian Academy of Sciences
Publisher Place New Delhi
Access Restriction One Nation One Subscription (ONOS)
Subject Keyword Magnetic field corona Magnetic Carpet magnetic flux Astronomy Astrophysics
Content Type Text
Resource Type Article
Subject Astronomy and Astrophysics Space and Planetary Science
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