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    11. IBIS: Bibliography
    ... Second ATST-EAST Meeting: Magnetic Fields from the Photosphere to the Corona. ... Three-minute wave enhancement in the solar photosphere . 52. ... Dynamics of the solar photosphere with IBIS. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/solar/IBIS/IBIS_biblio.html -- 60.3 Кб -- 13.12.2015
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    12. Terms and Definitions
    ... lower level of the solar atmosphere between the photosphere and the corona. cinders ... A bright region of the photosphere seen in white light, seldom visible except near ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/terms.htm -- 45.4 Кб -- 15.03.1998
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    13. Arcetri Solar Physics Group
    ... High Resolution Solar Studies . Observations of the solar photosphere and chromosphere at high resolutions . Solar Activity . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/solar/ -- 5.8 Кб -- 19.09.2006
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    14. Arcetri Solar Physics Group: High Resolution Studies
    ... to IBIS), can provide insights into the structure of magnetic fields in the chromosphere, a region where both the geometry of the field and its relevance with respect to convective and turbulent motions change dramatically with respect to the photosphere ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/solar/HighRes-2.html -- 6.4 Кб -- 03.06.2003
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    15. Arcetri Solar Physics Group: Solar Activity
    ... Of particular relevance is the measure of the velocity field both in the chromosphere (e.g. in the wings of Hydrogen Balmer lines and Ca II K line) and photosphere. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/solar/solar.activity.html -- 5.6 Кб -- 03.06.2003
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    16. http://www.arcetri.astro.it/~lt/preprints/pianetone/ms.ps.gz
    ... In the inset, we show the comparison between the dereddened broad band photometry (from R to L 0 ; red squares) and the models (practically coincident), photosphere as a dashed line, photosphere plus disk as solid line. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/pianetone/ms.ps.gz -- 649.5 Кб -- 11.09.2007
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    17. http://www.arcetri.astro.it/~lt/preprints/pianetone/gy11.pdf
    ... other (dotted line) to 3R. In the inset we show the comparison between the dereddened broadband photometr y (from R to L ; red squares) and the models (practically coincident): photosphere is shown as a dashed line, photosphere plus disk as a solid line ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/pianetone/gy11.pdf -- 197.3 Кб -- 11.09.2007
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    18. Aldebaran Occultations
    ... Both events were recorded in a narrow CVF filter at 3.55 micron, where the light is expected to come from the stellar photosphere without any contamination by atonic or molecular lines. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/luna/news/aldeb/index.php -- 13.6 Кб -- 04.02.2013
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    19. http://www.arcetri.astro.it/~lt/preprints/g962/g962.ps.gz
    ... photosphere and the free­free and free­bound emission from the ionised gas give the main contribution to the observed emission at 2:2 Їm, this may be the case for component F. On the other hand, in more evolved cases, such as component B, the pointlike ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/g962/g962.ps.gz -- 288.2 Кб -- 11.09.2007
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    20. Programs
    ... Visit of the Astronomy Park . Observations of the solar photosphere and of the sunspots with the Amici telescope . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/outreach/guided-tours/199-outreach/381-programs -- 21.9 Кб -- 11.04.2016
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