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    121. http://star.arm.ac.uk/~jgd/outgoing/JOB/ad_pdra.ps
    ... Coronal Hole O iii & Mg ix data of various transient features Further information about Armagh Observatory, and in particular the current Solar Physics re- search programme, may be obtained by consulting the Observatory's web-site http://star.arm.ac.uk ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~jgd/outgoing/JOB/ad_pdra.ps -- 1219.3 Кб -- 17.11.2003
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    122. http://star.arm.ac.uk/preprints/386b.doc
    ... The source of all these geomagnetic effects is the solar plasma that reaches the Earth magnetosphere; this is in the form of high-energy solar particles that may originate from solar flares, eruptive prominences, coronal mass ejections or coronal holes. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/386b.doc -- 776.5 Кб -- 10.02.2003
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    123. http://star.arm.ac.uk/preprints/386b.pdf
    ... The source of all these geomagnetic effects is the solar plasma that reaches the Earth magnetosphere; this is in the form of high-energy solar particles that may originate from solar flares, eruptive prominences, coronal mass ejections or coronal holes. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/386b.pdf -- 146.8 Кб -- 10.02.2003
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    124. http://star.arm.ac.uk/preprints/442.pdf
    ... The temporal series SER150W sequence was run in December 2002 in the North polar region, during a period when the coronal hole at the poles were ill-defined. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/442.pdf -- 254.4 Кб -- 29.04.2005
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    125. http://star.arm.ac.uk/nibulletin/2015/Jan06.html
    ... http://www.dailymail.co.uk/sciencetech/article-2894840/Mystery-sun-s-south-pole-Nasa-reveals-huge-coronal-hole-solar-surface-winds-jet-500-miles-SECOND.html . ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/nibulletin/2015/Jan06.html -- 32.2 Кб -- 06.01.2015
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    126. http://star.arm.ac.uk/~ambn/rad_losses.ps
    ... Solar observational data of active regions, coronal holes, sunspots, `quiescent' regions and flares were also used. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/rad_losses.ps -- 491.9 Кб -- 18.09.1996
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    127. http://star.arm.ac.uk/preprints/419.pdf
    ... spicules may be associacteristic speed given by this formula, a TI travels a distance ated with blinkers, and most probably observed at the boundof 195 km over 20 s, which is the integration time of the aries of unipolar magnetic regions (coronal holes ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/419.pdf -- 153.1 Кб -- 08.03.2004
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    128. http://star.arm.ac.uk/preprints/419.ps
    ... In this context, some spicules may be associ­ ated with blinkers, and most probably observed at the bound­ aries of unipolar magnetic regions (coronal holes). ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/419.ps -- 315.5 Кб -- 08.03.2004
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    129. http://star.arm.ac.uk/~ambn/279jgd.ps
    ... These densities are consistent from the values derived by Doschek et al. (1997) for their quiet Sun observations but approximately a factor of 2--3 higher than their coronal hole results. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/279jgd.ps -- 308.2 Кб -- 20.01.1998
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    130. http://star.arm.ac.uk/preprints/386a.doc
    ... High-energy solar particles originating from flares as well as from other solar activity phenomena (eruptive prominences, CMEs and coronal holes) can produce geomagnetic disturbances on Earth if they arrive at and interact with the magnetosphere. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/386a.doc -- 1698.0 Кб -- 10.02.2003
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