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    131. http://star.arm.ac.uk/~ambn/335jgd.ps
    ... With the launch of SOHO in 1995, the measurements of spectral line widths in different so­ lar features, coronal holes, `quiet' and active regions has been published (Teriaca et al. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/335jgd.ps -- 1207.9 Кб -- 18.04.2000
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    132. http://star.arm.ac.uk/annrep/annrep2003/annrep2003.pdf
    ... revealed for the first time the presence of bi-directional jets and magnetic reconnection occurring at coronal hole boundaries ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/annrep/annrep2003/annrep2003.pdf -- 1755.5 Кб -- 18.05.2004
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    133. http://star.arm.ac.uk/preprints/386a.pdf
    ... 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.pdf -- 219.5 Кб -- 10.02.2003
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    134. http://star.arm.ac.uk/~ambn/341epb.pdf
    ... occurs during the years around 1971, when the aa index has a delayed peak in its activity cycle, probably due to the fast solar wind and recurrent geomagnetic storms produced by near-equatorial coronal holes during the descending phase of the solar cycles ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/341epb.pdf -- 118.6 Кб -- 21.11.2008
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    135. http://star.arm.ac.uk/preprints/436.ps
    ... Coronal oscillations from GIS The long period (P = 10 15 min) slow waves have been observed so far only in open magnetic structures in coronal holes (DeForest & Gurman 1998; Ofman et al. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/436.ps -- 1932.8 Кб -- 18.01.2005
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    136. http://star.arm.ac.uk/preprints/459.pdf
    ... The redshifts have been observed in coronal holes, quiet sun regions, and active regions. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/459.pdf -- 483.6 Кб -- 26.09.2005
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    137. http://star.arm.ac.uk/preprints/459.ps
    ... The red­ shifts have been observed in coronal holes, quiet sun regions, and active regions. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/459.ps -- 2832.4 Кб -- 26.09.2005
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    138. http://star.arm.ac.uk/~ambn/acl_paper_II.ps
    ... The helium lines may appear relatively weak in coronal holes due to a weakening of this enhancement mechanism. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/acl_paper_II.ps -- 613.1 Кб -- 31.05.1996
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    139. http://star.arm.ac.uk/preprints/2015/686.pdf
    ... Uninterrupted space observations with long-time surveys of coronal holes in equatorial and polar regions, available through a dedicated mission such as ADAHELI+, will advance our understanding of where and how the fast solar wind is generated and ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2015/686.pdf -- 1843.7 Кб -- 15.01.2016
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    140. http://star.arm.ac.uk/preprints/488.pdf
    ... In this scenario, the plasma density would b e much higher in the radiation b elts than in the "coronal holes" ab ove the magnetic p oles. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/488.pdf -- 307.2 Кб -- 22.08.2006
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