Zobrazeno 1 - 10
of 109
pro vyhledávání: '"Kenneth P. Dere"'
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 268, Iss 2, p 52 (2023)
The CHIANTI atomic database provides sets of assessed data that are used for simulating spectral observations of astrophysical plasmas. This article describes updates that will be released as version 10.1 of the database. A key component of CHIANTI i
Externí odkaz:
https://doaj.org/article/4b7cedb8b148419b9db1c6e06c0d78f7
Quiet Sun electron densities and their uncertainties derived from spectral emission line intensities
Autor:
Kenneth P. Dere
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 496:2334-2345
The goal of this paper is to apply statistical methods to determine electrons densities and their errors from measurements of density-sensitive line intensities in the quiet Sun. Three methods are employed. The first is the use of L-function plots to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::991552079a8b0be9d4dc35738661031c
https://doi.org/10.1093/mnras/staa1645
https://doi.org/10.1093/mnras/staa1645
We present version 10 of the CHIANTI package. In this release, we provide updated atomic models for several helium-like ions and for all the ions of the beryllium, carbon and magnesium isoelectronic sequences that are abundant in astrophysical plasma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5acac5b819e349e7eb9e8b5e7c8c9240
http://arxiv.org/abs/2011.05211
http://arxiv.org/abs/2011.05211
Autor:
Kenneth P. Dere, Will T. Barnes
Publikováno v:
Proceedings of the 16th Python in Science Conference.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::99fd839d9804f0ebb091741ab69b3a6e
https://doi.org/10.25080/shinma-7f4c6e7-011
https://doi.org/10.25080/shinma-7f4c6e7-011
Publikováno v:
Fusion Science and Technology. 63:324-332
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4afe7902e336764e7608be3ada760286
https://doi.org/10.13182/fst13-a16438
https://doi.org/10.13182/fst13-a16438
The CHIANTI atomic database was first released in 1996 and has had a huge impact on the analysis and modeling of emissions from astrophysical plasmas. The database has continued to be updated, with version 8 released in 2015. Atomic data for modeling
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88763549c635dd43cad26b73b28c8351
http://arxiv.org/abs/1512.05620
http://arxiv.org/abs/1512.05620
Publikováno v:
Astronomy & Astrophysics. 498:915-929
Aims. The goal of the CHIANTI atomic database is to provide a set of atomic data for the interpretation of astrophysical spectra emitted by collisionally dominated, high temperature, optically thin sources. Methods. A complete set of ground level ion
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bf6aa1e413752e6354a86e22d9769605
https://doi.org/10.1051/0004-6361/200911712
https://doi.org/10.1051/0004-6361/200911712
Autor:
Kenneth P. Dere
Publikováno v:
Astronomy & Astrophysics. 497:287-290
Aims. In a previous paper, the volumetric plasma filling factor of coronal bright points was determined from spectra obtained with the Extreme ultraviolet Imaging Spectrometer (EIS). The analysis of these data showed that the median plasma filling fa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::aae44e82cbda3945edd59f142aa271e2
https://doi.org/10.1051/0004-6361/200811329
https://doi.org/10.1051/0004-6361/200811329
Autor:
Kenneth P. Dere
Publikováno v:
Astronomy & Astrophysics. 491:561-566
Aims. We determine the volumetric plasma filling factor of coronal bright points. Methods. Rastered spectra of the regions of the quiet Sun were recorded by the Extreme ultraviolet Imaging Spectrometer (EIS) during operations with the Hinode satellit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bf58e8a04523d4bd795db71f4f894e33
https://doi.org/10.1051/0004-6361:200810000
https://doi.org/10.1051/0004-6361:200810000
Autor:
Harry P. Warren, Peter R. Young, Len Culhane, Helen E. Mason, George A. Doschek, John T. Mariska, Tetsuya Watanabe, Kenneth P. Dere
Publikováno v:
Publications of the Astronomical Society of Japan. 59:S707-S712
The Extreme-Ultraviolet Imaging Spectrometer (EIS) on Hinode produces high resolution spectra that can be combined via rasters into monochromatic images of solar structures, such as active regions. Electron temperature and density maps of the structu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0f9afa4b972925359d533a8ea29e11f6
https://doi.org/10.1093/pasj/59.sp3.s707
https://doi.org/10.1093/pasj/59.sp3.s707