During the 1997 performance period, our work focused on the L-shell X-ray emission from highly charged iron ions in the 10-18 A region. Details of our accomplishments in 1997 are presented in the following. We start by describing the laboratory measurements made and their impact on the X-ray flight program and conclude by an overview of new instrumental capabilities developed for uses in the coming year
For over a decade, the x-ray astrophysics community has enjoyed a fruitful epoch of discovery largel...
The study of the physical conditions within the solar corona and the development of instrumentation ...
A number of topics relating to astrophysical observations that have already been made or are current...
Using the electron beam ion trap EBIT-II facility at Lawrence Livermore National Laboratory, we have...
http://wwwxray.ess.sci.osaka-u.ac.jp/SuzakuMAXI2014/pdf/2014SM_conf_P144-P145.pdfInternational audie...
Using the Electron Beam Ion Trap facility at Lawrence Livermore National Laboratory, we have measure...
We present a comprehensive wavelength survey of Fe L-shell X-ray lines between 7 and 11 {angstrom} m...
International audienceThe electron beam ion trap (EBIT) facility located at the Lawrence Livermore N...
The authors have conducted a systematic study of the dominant x-ray line emission from Fe XVII. Thes...
International audienceThe electron beam ion trap (EBIT) facility located at the Lawrence Livermore N...
International audienceThe electron beam ion trap (EBIT) facility located at the Lawrence Livermore N...
A number of X-ray astronomy satellites are scheduled for launch in the next few years. The Advanced ...
http://wwwxray.ess.sci.osaka-u.ac.jp/SuzakuMAXI2014/pdf/2014SM_conf_P144-P145.pdfInternational audie...
http://wwwxray.ess.sci.osaka-u.ac.jp/SuzakuMAXI2014/pdf/2014SM_conf_P144-P145.pdfInternational audie...
One of the dominant forms of astronomical line emission in the 6 {angstrom} to 18 {angstrom} spectra...
For over a decade, the x-ray astrophysics community has enjoyed a fruitful epoch of discovery largel...
The study of the physical conditions within the solar corona and the development of instrumentation ...
A number of topics relating to astrophysical observations that have already been made or are current...
Using the electron beam ion trap EBIT-II facility at Lawrence Livermore National Laboratory, we have...
http://wwwxray.ess.sci.osaka-u.ac.jp/SuzakuMAXI2014/pdf/2014SM_conf_P144-P145.pdfInternational audie...
Using the Electron Beam Ion Trap facility at Lawrence Livermore National Laboratory, we have measure...
We present a comprehensive wavelength survey of Fe L-shell X-ray lines between 7 and 11 {angstrom} m...
International audienceThe electron beam ion trap (EBIT) facility located at the Lawrence Livermore N...
The authors have conducted a systematic study of the dominant x-ray line emission from Fe XVII. Thes...
International audienceThe electron beam ion trap (EBIT) facility located at the Lawrence Livermore N...
International audienceThe electron beam ion trap (EBIT) facility located at the Lawrence Livermore N...
A number of X-ray astronomy satellites are scheduled for launch in the next few years. The Advanced ...
http://wwwxray.ess.sci.osaka-u.ac.jp/SuzakuMAXI2014/pdf/2014SM_conf_P144-P145.pdfInternational audie...
http://wwwxray.ess.sci.osaka-u.ac.jp/SuzakuMAXI2014/pdf/2014SM_conf_P144-P145.pdfInternational audie...
One of the dominant forms of astronomical line emission in the 6 {angstrom} to 18 {angstrom} spectra...
For over a decade, the x-ray astrophysics community has enjoyed a fruitful epoch of discovery largel...
The study of the physical conditions within the solar corona and the development of instrumentation ...
A number of topics relating to astrophysical observations that have already been made or are current...