Ineke De Moortel, Isobel Falconer and Robert Stack explore the achievements and influence of Hannes Alfvén, in particular his seminal Monthly Notices paper of 1947 on the heating of the solar corona.Publisher PDFNon peer reviewe
The solar corona, the tenuous outer atmosphere of the Sun, is orders of magnitude hotter than the so...
The grant funded a three year project to investigate the role of Alfvén waves as a possible mechanis...
Alfven waves emanating from the chromosphere have been suggested as a possible driver of coronal hea...
Ineke De Moortel, Isobel Falconer and Robert Stack explore the achievements and influence of Hannes ...
We have recently passed the 75th anniversary of one of the most important results in solar and space...
<p>A study of Alfvén waves in coronal loops and their role in the heating of the solar corona.</p
The discovery of magnetohydrodynamic waves was a major breakthrough in plasma physics and its applic...
The Sun’s outer coronal layer exists at a temperature of millions of kelvins, much hotter than the s...
Absorption of Alfvén waves is considered to be the main mechanism of heating in the solar corona. It...
Although heating of the solar atmosphere has been a subject of research for half-century, there is s...
Heating of magnetized plasma by propagation of Alfven waves is calculated as a function of spectral ...
The steady, supersonic outflow from the Sun we call the solar wind was first posited in the 1950s an...
Many scientific theories have been proposed in the hopes of better understanding the coronal heating...
Wave effects in a two-fluid model for the solar corona and wind are studied. Heating and acceleratio...
The Sun’s outer coronal layer exists at a temperature of millions of kelvins, much hotter than the ...
The solar corona, the tenuous outer atmosphere of the Sun, is orders of magnitude hotter than the so...
The grant funded a three year project to investigate the role of Alfvén waves as a possible mechanis...
Alfven waves emanating from the chromosphere have been suggested as a possible driver of coronal hea...
Ineke De Moortel, Isobel Falconer and Robert Stack explore the achievements and influence of Hannes ...
We have recently passed the 75th anniversary of one of the most important results in solar and space...
<p>A study of Alfvén waves in coronal loops and their role in the heating of the solar corona.</p
The discovery of magnetohydrodynamic waves was a major breakthrough in plasma physics and its applic...
The Sun’s outer coronal layer exists at a temperature of millions of kelvins, much hotter than the s...
Absorption of Alfvén waves is considered to be the main mechanism of heating in the solar corona. It...
Although heating of the solar atmosphere has been a subject of research for half-century, there is s...
Heating of magnetized plasma by propagation of Alfven waves is calculated as a function of spectral ...
The steady, supersonic outflow from the Sun we call the solar wind was first posited in the 1950s an...
Many scientific theories have been proposed in the hopes of better understanding the coronal heating...
Wave effects in a two-fluid model for the solar corona and wind are studied. Heating and acceleratio...
The Sun’s outer coronal layer exists at a temperature of millions of kelvins, much hotter than the ...
The solar corona, the tenuous outer atmosphere of the Sun, is orders of magnitude hotter than the so...
The grant funded a three year project to investigate the role of Alfvén waves as a possible mechanis...
Alfven waves emanating from the chromosphere have been suggested as a possible driver of coronal hea...
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