Photospheric brightness differences associated with the solar supergranulation-Reference-Cited by-同舟云学术

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Photospheric brightness differences associated with the solar supergranulation

Published:1968-11 Issue:3 Volume:5 Page:309-322
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Beckers Jacques M.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00147143.pdf

Reference15 articles.

1. Beckers, J. M.: 1964, Dissertation, Utrecht (= AFCRL Environmental Research Paper No. 49).

2. Beckers, J. M.: 1966, The Fine Structure of the Solar Atmosphere (ed by K. O. Kiepenheuer), Franz Steiner Verlag, Wiesbaden, p. 56.

3. Beckers, J. M.: 1968, Solar Phys. 3, 258.

4. Blamont, J. E. and Carpentier, G.: 1967, Solar Phys. 1, 180.

5. Edmonds, F. N., Jr.: 1961, Astrophys. J. Suppl. Ser. 6, 357.

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1. Polar Coronal Plumes as Tornado-like Jets;The Astrophysical Journal;2018-10-08

2. The Sun’s supergranulation;Living Reviews in Solar Physics;2018-09-10

3. The Sun’s Supergranulation;Living Reviews in Solar Physics;2010

4. THE INTENSITY PROFILE OF THE SOLAR SUPERGRANULATION;The Astrophysical Journal;2009-11-18

5. Supergranules over the solar cycle;Astronomy & Astrophysics;2008-07-09

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