Zobrazeno 1 - 10
of 87
pro vyhledávání: '"M, Fluri"'
Publikováno v:
64. Kongress der Deutschen Gesellschaft für Gynäkologie und Geburtshilfe e. V..
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e22a17d1873b598cab890a79c27bb8e1
https://doi.org/10.1055/s-0042-1756807
https://doi.org/10.1055/s-0042-1756807
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Microalgae represent a promising resource for nature-derived compounds in different fields of interest. The rigid microalgae cell wall (composed of a polysaccharide and glycoprotein matrix) provides the cells with a formidable defence against harsh e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fb9d464298c1ccda722ec79a0eb54302
https://hdl.handle.net/11475/27590
https://hdl.handle.net/11475/27590
Publikováno v:
Astronomy & Astrophysics. 507:1711-1718
Context. Spectroscopy data in general often deals with an entanglement of spectral line properties, especially in the case of blended line profiles, independently of how high the quality of the data may be. In stellar spectroscopy and spectropolarime
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::426854780d18ad4d23c3738f65416cf7
https://doi.org/10.1051/0004-6361/200912467
https://doi.org/10.1051/0004-6361/200912467
Publikováno v:
Astronomy & Astrophysics. 482:387-395
Context. Lines of diatomic molecules are ideal tools for studying cool stellar atmospheres and the internal structure of sunspots and starspots, given their temperature and pressure sensitivities, which are typically higher than in atomic lines. The
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8022bc86a12be97217440f0ba3c2a2f9
https://doi.org/10.1051/0004-6361:20079300
https://doi.org/10.1051/0004-6361:20079300
Publikováno v:
The Astrophysical Journal. 668:L63-L66
Recent spectropolarimetric observations of Herbig AeBe stellar systems show linear polarization variability with wavelength and epoch near their obscured H-alpha emission. Surprisingly, this polarization is not coincident with the H-alpha emission pe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3e190aa66aaea36f853e6b58c347014d
https://doi.org/10.1086/522425
https://doi.org/10.1086/522425
Publikováno v:
Astronomy & Astrophysics. 475:349-357
Weak entangled magnetic fields with mixed polarity occupy the main part of the quiet Sun. The Zeeman effect diagnostics fails to measure such fields because of cancellation in circular polarization. However, the Hanle effect diagnostics, accessible t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2a19a58ad901bc63b0bc754d3f62b5d2
https://doi.org/10.1051/0004-6361:20078046
https://doi.org/10.1051/0004-6361:20078046
Publikováno v:
Astronomy & Astrophysics. 461:339-349
Context. The second solar spectrum resulting from coherent scattering is a main tool for diagnostics of turbulent magnetic fields on the Sun. Scattering on diatomic molecules plays an important role in forming this spectrum and even dominates in some
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::290e8829ad88552ba0d84f9129cc47df
https://doi.org/10.1051/0004-6361:20066030
https://doi.org/10.1051/0004-6361:20066030
Publikováno v:
Astronomy & Astrophysics. 449:L41-L44
Aims. We compute the linearly polarized spectrum of Ca ii K caused by coherent scattering and exploit the line for chromospheric diagnosis, with particular attention to temperature bifurcation, by comparing the theory with solar observations. Methods
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a0cd0332fdfc6e29499bf66f31d57772
https://doi.org/10.1051/0004-6361:20064832
https://doi.org/10.1051/0004-6361:20064832