2s-photoionization of magnesium is analyzed for incident energies
ranging up to three times the 2s threshold (96.6 eV). The 3s shake
processes amount to almost 30% of single photoionization. The shake-up
cross section 3s --> 4s exceeds 14% of the single one, and the
conjugate shake-up probability plays an important role in the energy
range up to three times the 2s threshold. The 2s2p(6)3s(2) Auger and
Coster-Kronig rates are calculated, and the 2s(2)2p(5)3s (1)p(o) exit is
found to be favour ed (80% of the total decay), giving rise to the line
MgIII 231.73 Angstrom.
%0 Journal Article
%1 WOS:000166541100023
%A Kochur, AG
%A Petrini, D
%A da Silva, EP
%C 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
%D 2001
%I EDP SCIENCES S A
%J ASTRONOMY & ASTROPHYSICS
%K atomic data; formation} line processes; {atomic
%N 2
%P 248-251
%R 10.1051/0004-6361:20000189
%T 2s-photoionisation of atomic magnesium: Shake processes and
Coster-Kronig radiationless decay
%V 365
%X 2s-photoionization of magnesium is analyzed for incident energies
ranging up to three times the 2s threshold (96.6 eV). The 3s shake
processes amount to almost 30% of single photoionization. The shake-up
cross section 3s --> 4s exceeds 14% of the single one, and the
conjugate shake-up probability plays an important role in the energy
range up to three times the 2s threshold. The 2s2p(6)3s(2) Auger and
Coster-Kronig rates are calculated, and the 2s(2)2p(5)3s (1)p(o) exit is
found to be favour ed (80% of the total decay), giving rise to the line
MgIII 231.73 Angstrom.
@article{WOS:000166541100023,
abstract = {2s-photoionization of magnesium is analyzed for incident energies
ranging up to three times the 2s threshold (96.6 eV). The 3s shake
processes amount to almost 30% of single photoionization. The shake-up
cross section 3s --> 4s exceeds 14% of the single one, and the
conjugate shake-up probability plays an important role in the energy
range up to three times the 2s threshold. The 2s2p(6)3s(2) Auger and
Coster-Kronig rates are calculated, and the 2s(2)2p(5)3s (1)p(o) exit is
found to be favour ed (80% of the total decay), giving rise to the line
MgIII 231.73 Angstrom.},
added-at = {2022-05-23T20:00:14.000+0200},
address = {17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE},
author = {Kochur, AG and Petrini, D and da Silva, EP},
biburl = {https://www.bibsonomy.org/bibtex/2bd0dcfd4b84f1fe1575961bc6d51f3ec/ppgfis_ufc_br},
doi = {10.1051/0004-6361:20000189},
interhash = {ccd80b75b7cdba94e4d7a3bada49d1e9},
intrahash = {bd0dcfd4b84f1fe1575961bc6d51f3ec},
issn = {1432-0746},
journal = {ASTRONOMY & ASTROPHYSICS},
keywords = {atomic data; formation} line processes; {atomic},
number = 2,
pages = {248-251},
publisher = {EDP SCIENCES S A},
pubstate = {published},
timestamp = {2022-05-23T20:00:14.000+0200},
title = {2s-photoionisation of atomic magnesium: Shake processes and
Coster-Kronig radiationless decay},
tppubtype = {article},
volume = 365,
year = 2001
}