Zobrazeno 1 - 10
of 116
pro vyhledávání: '"R. Manso Sainz"'
(Abriged) Blue compact galaxies (BCGs) are low-luminosity, metal-poor, gas-rich objects that form stars at high rates, excellent analogs to the high-redshift star-forming galaxy population. Being low-mass starbursts, they also constitute ideal labora
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e0f874f06c9354f4345cca7d84f1e06c
Publikováno v:
The Astrophysical Journal
We report on spectropolarimetric observations across the Mg II h and k-lines at 2800 angstrom made by the Ultraviolet Spectrometer and Polarimeter onboard the Solar Maximum Mission satellite. Our analysis confirms the strong linear polarization in th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9da38a2bf69ae5d270cc0398ebc69e43
Publikováno v:
The Astrophysical Journal
We carry out a theoretical study of the polarization of the solar Mg II h-k doublet (including its extended wings) and the subordinate UV triplet around 280 nm. These lines are of great diagnostic interest, as they encode information on the physical
We consider the vector emissivity of the polarized radiation transfer in a $\Lambda$-type atomic transition, which we recently proposed in order to account for both CRD and PRD contributions to the scattered radiation. This expression can concisely b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8385470118e45303e6fe876ef8de5ec
http://arxiv.org/abs/1709.00126
http://arxiv.org/abs/1709.00126
We consider the vector emissivity of the polarized radiation transfer in a Λ-type atomic transition, which we recently proposed to account for both complete frequency redistribution (CRD) and partial redistribution (PRD) contributions to the scatter
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::03eb87bd6984ed2f7f599a435c00ad89
http://arxiv.org/abs/1612.03440
http://arxiv.org/abs/1612.03440
We investigated the formation of the Mg II h-k doublet in a weakly magnetized atmosphere (20-100 G) using a newly developed numerical code for polarized RT in a plane-parallel geometry, which implements a recent formulation of partially coherent scat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fc09715c2846f4747bdcac0e6ac82a07
http://arxiv.org/abs/1607.05683
http://arxiv.org/abs/1607.05683
Autor:
Roberto Casini, R. Manso Sainz
We study the effects of Rayleigh and Raman scattering on the formation of polarized spectral lines in a $\Lambda$-type multi-term atom. We fully take into account the partial redistribution of frequency and the presence of atomic polarization in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::01cb76b640aea392b240edab54216144
http://arxiv.org/abs/1602.07173
http://arxiv.org/abs/1602.07173
Publikováno v:
Icarus
Icarus, 2012, 220 (2), pp.1104-1111. ⟨10.1016/j.icarus.2012.07.001⟩
Icarus, Elsevier, 2012, 220 (2), pp.1104-1111. ⟨10.1016/j.icarus.2012.07.001⟩
Icarus, 2012, 220 (2), pp.1104-1111. ⟨10.1016/j.icarus.2012.07.001⟩
Icarus, Elsevier, 2012, 220 (2), pp.1104-1111. ⟨10.1016/j.icarus.2012.07.001⟩
International audience; The conditions of the exosphere of Mercury constitute a prime example of a magnetosphere subject to space weather. We aim at improving the diagnostic of the physical conditions of Na atoms in the exosphere of Mercury, with par
Autor:
Saku Tsuneta, Roberto Casini, Takenori J. Okamoto, Jan Jurcak, Ryoko Ishikawa, L. R. Bellot Rubio, Bruce W. Lites, Kiyoshi Ichimoto, R. Manso Sainz
Publikováno v:
The Astrophysical Journal. 713:450-457
Spectro-polarimetric observations with the Solar Optical Telescope onboard Hinode reveal the emission spectrum of the Fe I 630 nm lines at the solar limb. The emission shell extends for less than 1'' thereby making it extremely difficult to detect fr
Publikováno v:
The Astrophysical Journal. 701:L43-L46
For about a decade, spectro-polarimetry of HeI 10830 has been applied to the magnetic diagnostics of the solar chromosphere. This resonance line is very versatile, as it is visible both on disk and in off-limb structures, and it has a good sensitivit