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    1. http://star.arm.ac.uk/~meb/anem/anemometer_Science-1902-WEAD-543-4.pdf
    ... Gannett. :Mr. Bauer told of the expedition now in the field to locate the magnetic North Pole; and Mr. 0. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~meb/anem/anemometer_Science-1902-WEAD-543-4.pdf -- 491.8 Кб -- 24.01.2011
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    2. http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/091107/091107_04.pdf
    ... Magnetic fragment behaviour Note A bipolar region was involved. The magnetic Start of the data set fragments are shaped as an arrow pointing north. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/091107/091107_04.pdf -- 41.0 Кб -- 23.07.2012
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    3. http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/091107/091107_07.pdf
    ... No. 7 Time (UT) 06:38 X-ray BP behaviour Magnetic fragment behaviour A bipolar region is involved. ... Positive fragments locate to the north and negative ones are located to the south. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/091107/091107_07.pdf -- 38.6 Кб -- 23.07.2012
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    4. http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/121107/121107_02.pdf
    ... The growing negative fragments move to the north and keep "ejecting" positive fragments to the south (southeast) until around 06:30 when it move very close to a group of pre-existed positive fragments at "far-north". ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/121107/121107_02.pdf -- 52.0 Кб -- 23.07.2012
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    5. http://star.arm.ac.uk/ssab-workshop/landstreet/Cluster-project.pdf
    ... probably due to magnetic coupling with circumstellar material (accretion disk, stellar wind) · Even young Ap stars (in clusters, associations) have slow rotation, so loss of angular momentum probably occurs in PMS phase (North) · Slowest rotators are ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/ssab-workshop/landstreet/Cluster-project.pdf -- 1193.5 Кб -- 26.03.2008
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    6. http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/091107/091107_05.pdf
    ... No. 5 Time (UT) 06:38 X-ray BP behaviour A BP is present. Magnetic fragment behaviour A bipolar region was involved. ... Negative fragments locate to the north and positive ones to the south. Cancellation occurs. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/091107/091107_05.pdf -- 37.1 Кб -- 23.07.2012
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    7. http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/100109/100109_03.pdf
    ... Another BP emerges Another cancellation site is formed to the north, to the north of the where the positive fragments are more active. location of the previous one. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/100109/100109_03.pdf -- 38.9 Кб -- 23.07.2012
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    8. http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/121107/121107_07.pdf
    ... UT) X-ray BP behaviour 01:21 Magnetic fragment behaviour A simple polarities occurs ... Another one locates at north and become brighter. ... which existed at the beginning of the data set and move a little to the north ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/121107/121107_07.pdf -- 45.7 Кб -- 23.07.2012
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    9. http://star.arm.ac.uk/lectures/landstreet/slides/Lecture-4-stellar-fields-and-phenomena.pdf
    ... magnetic fields and some associated phenomena JD L 01/03/09 Leverhulme Lectures on Stellar Magnetism Sunspot magnetism Hale's discovery opened study of sunspot fields ­ ­ ­ ­ ­ ­ ­ 01/03/09 Sunspots typically have fields of 1- 3 kG Sunspots tend to come ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/lectures/landstreet/slides/Lecture-4-stellar-fields-and-phenomena.pdf -- 1183.1 Кб -- 02.03.2009
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    10. http://star.arm.ac.uk/~ambn/abstract324.html
    ... with the SUMER instrument on SOHO extending from the solar disk to 1.5 R_/odot above the limb in the north polar coronal hole ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~ambn/abstract324.html -- 1.8 Кб -- 08.12.1999
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