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Excitation Mechanism in Laser-Induced Plasma at Atmospheric Air Pressure

Journal of Mathematical and Fundamental Sciences · Vol. 37 No. 1 (2013) · hlm. 1–12

DOI
10.5614/itbj.sci.2005.37.1.1
ISSN
2338-5510, 2337-5760
Terbit
2013-12-31
Penerbit
Directorate for Research and Innovation (DRI) ITB
Bahasa
eng

Abstrak

A special interferometric technique has been devised on the basis of rainbow refractometry without the use of an additional and delicate amplitude-splitting setup. This new technique was used for the characterization of plasma induced by a Q-switched Nd-YAG laser on zinc samples under atmospheric air pressure. An unmistakable signal of the density jump was detected simultaneously with the observation of the emission front signal. It was proved that the emission front and the front of the shock wave coincided and moved together with time at the initial stage of the secondary plasma expansion. However, at a later stage, the emission front began to separate from and left behind the shock wave front propagating in the surrounding air. With the use of zinc sample, the experimental results showed that the separation of the emission front and shock wave front took place at about 4 mm above sample surface for laser energy of 26 mJ. It was also found that the separation time increased by increasing the power density which further supported shock wave model. Analysis of the data of the shock front movement along with the emission characteristics has led us to the conclusion that models other than the shock wave model, such as the gas breakdown model, should be excluded, at least for a zinc sample, as not satisfactorily explaining the excitation process in the secondary plasma generated at atmospheric air pressure of 760 Torr.

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  • Atma Jaya Catholic University of Indonesia
  • University of Indonesia
  • University of Fukui
  • Lambung Mangkurat University
  • Udayana University
  • Binus University
  • Pelita Harapan University
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Rekan penulisOrganisasiArtikel bersama
Kiichiro KagawaUniversity of Fukui4
Eko SusilowatiLambung Mangkurat University2
Mohamad Infrawan Yulianto IchwanAfiliasi tidak diketahui2
Hery SuyantoUdayana University2
Maria Margaretha SuliyantiUniversity of Indonesia2
Rinda HedwigBinus University2
Marincan PardedePelita Harapan University2
Syahrun Nur AbdulmadjidUniversitas Syiah Kuala2
Yong Inn LeeJeonbuk National University2
Iwao KitazimaUniversity of Fukui2
Maria Dara Novi HandayaniAtma Jaya Catholic University of Indonesia1
Hotmaria Agustina PakpahanAfiliasi tidak diketahui1
Ferbian Milas SiswantoAtma Jaya Catholic University of Indonesia1
Rita DewiAtma Jaya Catholic University of Indonesia1
Ian PranandiAfiliasi tidak diketahui1
William WilliamAfiliasi tidak diketahui1
Evi Ulina Margaretha SitumorangAfiliasi tidak diketahui1
Ana Lucia EkowatiAfiliasi tidak diketahui1
Yulia Tanti NarwatiAfiliasi tidak diketahui1

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Sumber metadata: OAI-PMH (metadata jurnal) https://journals.itb.ac.id/index.php/jmfs/oai, pertama di-harvest 9 Nov 2026, terakhir terlihat 9 Nov 2026.
Metadata asli (oai_dc)
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	<dc:title xml:lang="en-US">Excitation Mechanism in Laser-Induced Plasma at Atmospheric Air Pressure</dc:title>
	<dc:creator>Manalu, Jojor Lamsihar</dc:creator>
	<dc:creator>Kurniawan, Koo Hendrik</dc:creator>
	<dc:creator>Lie, Tjung Jie</dc:creator>
	<dc:description xml:lang="en-US">A special interferometric technique has been devised on the basis of rainbow refractometry without the use of an additional and delicate amplitude-splitting setup. This new technique was used for the characterization of plasma induced by a Q-switched Nd-YAG laser on zinc samples under atmospheric air pressure. An unmistakable signal of the density jump was detected simultaneously with the observation of the emission front signal. It was proved that the emission front and the front of the shock wave coincided and moved together with time at the initial stage of the secondary plasma expansion. However, at a later stage, the emission front began to separate from and left behind the shock wave front propagating in the surrounding air. With the use of zinc sample, the experimental results showed that the separation of the emission front and shock wave front took place at about 4 mm above sample surface for laser energy of 26 mJ. It was also found that the separation time increased by increasing the power density which further supported shock wave model. Analysis of the data of the shock front movement along with the emission characteristics has led us to the conclusion that models other than the shock wave model, such as the gas breakdown model, should be excluded, at least for a zinc sample, as not satisfactorily explaining the excitation process in the secondary plasma generated at atmospheric air pressure of 760 Torr.</dc:description>
	<dc:publisher xml:lang="en-US">Directorate for Research and Innovation (DRI) ITB</dc:publisher>
	<dc:date>2013-12-31</dc:date>
	<dc:type>info:eu-repo/semantics/article</dc:type>
	<dc:type>info:eu-repo/semantics/publishedVersion</dc:type>
	<dc:format>application/pdf</dc:format>
	<dc:identifier>https://journals.itb.ac.id/index.php/jmfs/article/view/280</dc:identifier>
	<dc:identifier>10.5614/itbj.sci.2005.37.1.1</dc:identifier>
	<dc:source xml:lang="en-US">Journal of Mathematical and Fundamental Sciences; Vol. 37 No. 1 (2005); 1-12</dc:source>
	<dc:source>2338-5510</dc:source>
	<dc:source>2337-5760</dc:source>
	<dc:language>eng</dc:language>
	<dc:relation>https://journals.itb.ac.id/index.php/jmfs/article/view/280/263</dc:relation>
</oai_dc:dc>