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    91. http://star.arm.ac.uk/administration/business-plan/2010-2011/bp2010.pdf
    ... and is aimed at fundamental questions such as how the corona is heated, how the solar wind is driven, and what drives the Sun's ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/administration/business-plan/2010-2011/bp2010.pdf -- 356.1 Кб -- 07.05.2010
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    92. http://star.arm.ac.uk/~ambn/bpremg.ps
    ... Ideal magnetohydrodynamics (MHD) is often a very good approximation of plasma phenomena, like magnetic loops in the solar corona. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/bpremg.ps -- 485.8 Кб -- 20.12.1996
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    93. http://star.arm.ac.uk/preprints/2008/533.pdf
    ... However, it has recently been shown by Santos et al. (2008) that brightenings in the solar corona associated wit h BPs are related with the strongest electric current concentrat ions. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2008/533.pdf -- 2597.2 Кб -- 11.09.2008
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    94. http://star.arm.ac.uk/preprints/432.pdf
    ... It is widely accepted that they are the result of the rapid conversion of a large amount of magnetic energy, previously stored in the solar corona, and dissipated through magnetic reconnections. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/432.pdf -- 378.2 Кб -- 19.09.2005
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    95. http://star.arm.ac.uk/administration/business-plan/2009-2010/bp2009.pdf
    ... and is aimed at fundamental questions such as how the corona is heated, how the solar wind is driven, and what drives the Sun's ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/administration/business-plan/2009-2010/bp2009.pdf -- 353.2 Кб -- 20.04.2009
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    96. http://star.arm.ac.uk/~meb/ras_leaflets2012/Infrared.2012.pdf
    ... This was an adaptation of his carbonbutton microphone for telephones. during the total solar eclipse of 29 July 1878, in Wyoming, he used the tasimeter to measure the temperature of the solar corona. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~meb/ras_leaflets2012/Infrared.2012.pdf -- 308.0 Кб -- 05.03.2012
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    97. http://star.arm.ac.uk/~ambn/na_cool.ps
    ... The Na i ––5890,5896 resonance doublet as chromospheric diagnostics in M dwarfs 5 sities, representative of an ``average'' solar quiet corona, have been multiplied by a factor 10 4 ; the result is shown in Fig. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/na_cool.ps -- 1254.1 Кб -- 20.11.1996
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    98. http://star.arm.ac.uk/~ambn/abstract284.html
    ... We model the solar corona as two-layer isothermal atmosphere, with the lower layer having chromospheric thickness and the temperature and the upper layer having coronal temperature. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~ambn/abstract284.html -- 2.3 Кб -- 29.04.1998
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    99. http://star.arm.ac.uk/annrep/annrep98/Annual-Report-1998.ps
    ... solar physics group at Armagh, with a particular focus on using data from satellites ... to study various aspects of solar activity, including heating of the solar corona ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/annrep/annrep98/Annual-Report-1998.ps -- 324.6 Кб -- 08.05.2000
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    100. http://star.arm.ac.uk/preprints/2015/654.pdf
    ... REFERENCES Adams W. S., Joy A. H., 1917, ApJ, 46, 313 Aschwander M. J., 2004, Physics of the Solar Corona: An introduction. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2015/654.pdf -- 1739.4 Кб -- 05.01.2015
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