[PDF] Top 20 Atomic data for the astrophysics : Fe XII soft X-ray lines.
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Atomic data for the astrophysics : Fe XII soft X-ray lines.
... We kept the scaling parameters for the n = 4 the same, and ob- tained those for the n = 5, 6, which are listed in Table 1. This was done to try and keep similar energies (and ordering of the levels) for the n = 4 levels. ... See full document
10
Atomic data for astrophysics: improved collision strengths for Fe VIII
... of Fe ...EUV lines observed in the solar corona by the Hinode EUV Imaging ...main soft X-ray and extreme ultraviolet (EUV) transitions, using the present atomic ...that ... See full document
9
Atomic data for astrophysics : Ni XI.
... the lines, and its value is ...all lines should be closely ...emission lines, but are equivalent to the usual single line ratio plots, where the theoretical ratio of two emission lines is ... See full document
7
Atomic data for astrophysics : Fe IX
... too low, being closer to a quiet Sun rather than a coronal con- densation (which is normally associated with active regions), so we revisited other density diagnostics from the same ob- servation. The only other reliable ... See full document
11
Benchmarking atomic data for astrophysics : Si III
... iii lines have a different temperature ...of lines, obtained with the present level populations, the CHIANTI ...iii lines, an understanding of the temperature structure of the lower atmosphere for ... See full document
11
Atomic data for astrophysics : Ni XII
... Å lines would be well separated in the high-resolution solar spectrum of Behring et ...the lines listed by Ryabtsev (1979) would not be observable in the low- density solar corona, but the 2–31 transition ... See full document
8
Atomic data for astrophysics : Fe X soft x-ray lines
... Similar discrepancies between Malinovsky et al. (1980) and our results are present for the other lines in the same transi- tion array. The differences between our results and Malinovsky et al. (1980) in the ... See full document
10
X-ray spectra of the Fe-L complex
... the Fe-L has been partially lifted by the advent of follow- up ...for Fe xvii by Aggarwal et ...other Fe-L species (Witthoeft et al. 2006 for Fe xviii , Butler & Badnell 2008 for Fe ... See full document
29
Electron Proton Pairing at High Temperatures, Solar Flares, and the FIP Effect
... emit soft X-ray ...spectral lines of the kind given by Equation (13) and then look for them in the soft X-ray line data from ...spectral lines at different ... See full document
11
Calculation of Atomic Data and Gain Coefficient for XUV & Soft X Ray Laser Emission from Ge XXIII
... offering the potential for laser emission in the spectral region between 12 and 53 nm from the Ge XXIII ion. This class of lasers can be achieved under the suitable conditions of pumping power as well as electron den- ... See full document
25
Atomic data for the x-ray lines of Fe viii and Fe ix
... et al. (2000) data have been benchmarked by Del Zanna (2009) using Hinode EUV Imaging Spectrometer (EIS, see Culhane et al. 2007) observations, measurements found in the literature, and laboratory plates from B.C. ... See full document
10
CIELO-RGS : a catalogue of soft X-ray ionized emission lines
... High-resolution X-ray spectroscopy has the potential to reveal the physics of the plasma state that accounts for much of the material in the observable ...The X-ray band contains the inner- ... See full document
23
Al0.52In0.48P avalanche photodiodes for soft X-ray spectroscopy
... for X-ray spectroscopy but they have limitations that wide band gap de- tectors are ...temperature X-ray detection and comprehensive reviews can be found in [1, ...SiC X-ray de- ... See full document
13
Dedicated polarimeter design for hard x-ray and soft gamma-ray astronomy
... real data, this unpolarized distribution would be determined by simulations rather than by direct ...raw data in this fashion do we clearly see the cos 2 η modulation pattern that is expected (the third ... See full document
13
Experimental and density functional study of Mn doped Bi2Te3 topological insulator
... ordered atomic structure of the QLs suggests that in regions with increased Mn concentration Mn also substitutes Te– in addition to the predicted more energetically favorable Bi atomic positions, as has ... See full document
15
RETROPERITONEAL ABSCESSES-CASE REPORTS
... leucocytosis. X-ray abdomen showed a soft tissue shadow in the left iliac fossa with scoliosis and an indistinct psoas shadow on the ...tests, X-ray chest, ... See full document
6
Multiwavelength studies of ultra-soft X-ray AGN
... its soft X-ray emission m ay be found in ...hard X-ray com ponent is detected in the C3 ...the lines have similar profiles, but the continua are flatter th an seen in the USS ... See full document
199
Soft X-ray emission lines from a relativistic accretion disk in MCG-6-30-15 and Mrk 766
... PN data of MCG − 6-30-15 shows that a power-law slope of Γ ∼ ...excess soft emission below ∼ 1 ...observed soft X-ray flux, however, is in the form of C, N, and O emission ...hard ... See full document
7
Experimental and density functional study of Mn doped Bi 2 Te 3 topological insulator
... ordered atomic structure of the QLs suggests that in regions with increased Mn concentration Mn also substitutes Te– in addition to the predicted more energetically favorable Bi atomic positions, as has ... See full document
9
The X-ray spectrum of the Seyfert I galaxy Markarian 766: Dusty warm absorber or relativistic emission lines?
... the soft X-ray spectrum of bright ...absorption lines arising in material with a range of ionisation states ...emission lines of O VIII , N VII and C VI broadened by relativistic motion ... See full document
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