Time Evolution of Optical Emission Spectrum of a Hg-HID Lamp Exposed to X-ray
Time variation of optical emission lines for Hg, and other elements detected in a mercury HID lamp before and during X-ray irradiation were analyzed. Various irradiation conditions are causing differences in time dependencies of all Hg spectral line intensities (including that of 253.73 nm resonance...
Saved in:
Published in | Plasma chemistry and plasma processing Vol. 30; no. 4; pp. 449 - 459 |
---|---|
Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
Boston
Springer US
01.08.2010
Springer Verlag |
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | Time variation of optical emission lines for Hg, and other elements detected in a mercury HID lamp before and during X-ray irradiation were analyzed. Various irradiation conditions are causing differences in time dependencies of all Hg spectral line intensities (including that of 253.73 nm resonance line not completely self-absorbed). The X-ray optical depths are smaller in the case of Hg gas compared with burner wall glass. The free electrons generated during X-ray exposure (photoelectrons, Auger electrons) contribute to changes in plasma characteristics (e.g. plasma temperature, density, etc.) in transitory regime. In quasi-stable regime there are practically no differences between electron temperatures for normal and irradiated lamp. A qualitative explanation in the framework of Beer-Lambert law is given. |
---|---|
Bibliography: | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 |
ISSN: | 0272-4324 1572-8986 |
DOI: | 10.1007/s11090-010-9228-5 |