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Study of the effects of neutral gas heating in a radio frequency inductively coupled plasma / Kanesh Kumar Jayapalan

机译:研究射频电感耦合等离子体/ Kanesh Kumar Jayapalan中性气体加热的影响

摘要

A 13.56 MHz, planar coil, inductively coupled plasma reactor was experimentallyudand theoretically characterized; with emphasis on the effects of neutral gas heating onudthe distribution of the H mode magnetic fields of the source coil and the E-H modeudtransition characteristics of the discharge.udThe radially resolved electron density, ne, electron temperature, Te and electronudenergy distribution function (EEDF) were measured using a Langmuir probe at differentudaxial distances above the dielectric plate for 0.03, 0.07 and 0.2 mbar argon pressures.udThe range of ne and Te obtained were (0.065 ± 0.004)-(4.0 ± 0.6) × 1017 m-3 andud(1.38 ± 0.08)-(3.8 ± 0.2) eV assuming Maxwellian distribution. The measured neuddistribution at 0.2 mbar suggested significant influence of neutral gas heating. EEDFudplots showed that the distributions were Maxwellian-like.udThe radially resolved absolute axial magnetic field, |Bz|, and absolute radial magneticudfields, |Br|, were measured using electrostatically compensated magnetic probes in theudappropriate orientations. The fields were measured at different axial distances above theuddielectric plate for the chamber in evacuated condition and for 0.03, 0.07 and 0.2 mbarudargon pressures. R.f. power was set at 180 W. Maximum |Bz| and |Br| fields wereudobtained when the chamber was in evacuated condition with values of (1.507 ± 0.005) ×ud10-4 T and (7.67 ± 0.01) × 10-5 T, respectively.udThe peak E-H mode transition current, Itr and peak H-E mode transition current, Imtudwere measured using a current probe for 0.02-0.2 mbar argon pressures. The minimumudvalue for Itr was (13.5 ± 0.5) A at 0.08 mbar, whereas, the minimum value for Imt wasud(8.3 ± 0.1) A at 0.3 mbar. As pressure is increased, hysteresis between E-H mode andudH-E mode transitions was observed to become more distinct. The line averaged neutral gas temperature, Tn, was measured using a fiber probe withudthe actinometry optical emission spectroscopy (AOES) technique at 0.03, 0.05, 0.07, 0.1udand 0.2 mbar argon pressure for different axial distances above the dielectric plate. R.f.udpower was varied from 100 W to 200 W. The range of Tn obtained wasud(350 ± 30)-(840 ± 30) K.udFor theoretical characterization, two predictive models were used. The first was anudelectromagnetic field model that simulates |Bz| and |Br|, using empirically fitted,udspatially resolved electron density, ne (r, z) and electron temperature, Te (r, z).udSimulations were run for spatially averaged Tn and heuristically fitted, spatiallyuddistributed temperature, Tn (r, z). Tn (r, z) gave the closest agreement to the measuredudmagnetic fields.udThe second model was a power deposition model that simulates Itr and Imt.udSimulations were run for Tn = 300 K and at elevated Tn. Calculations better matched theudmeasured values only when neutral gas heating was considered. The effect of hysteresisudin mode transition of the discharge was also demonstrated using a fitted 3D powerudevolution plot.udThese results indicate that neutral gas heating plays an important role in influencingudplasma parameters. Thus, knowledge of the effects of neutral gas heating is essential inudproviding better understanding of the formation and maintenance of the plasmauddischarge.
机译:实验上理论上表征了13.56 MHz平面线圈电感耦合等离子体反应器;着重于中性气体加热对'过去世“ ” “径向解析的电子密度,ne,电子温度,Te和电子使用Langmuir探针在0.03、0.07和0.2 mbar的氩气压力下,在电介质板上方的不同非轴向距离处测量udenergy分布函数(EEDF)。 ud得到的ne和Te的范围为(0.065±0.004)-(4.0±0.6) )×1017 m-3和 ud(1.38±0.08)-(3.8±0.2)eV(假设麦克斯韦分布)。在0.2毫巴下测得的新分布显示出中性气体加热的显着影响。 EEDF udplots表明分布是麦克斯韦式的。 ud使用静电补偿磁探针在 u合适的方向上测量了径向分辨的绝对轴向磁场| Bz |和绝对径向磁场| Br |。在真空条件下,在真空室上方的 u介电板上方的不同轴向距离处测量了电场,并测量了0.03、0.07和0.2 mbar udargon的压力。 R.f.最大功率| Bz |和| Br |当真空室处于真空状态时,场的场强为(1.507±0.005)× ud10-4 T和(7.67±0.01)×10-5 T. ud峰值EH模式转换电流,Itr和峰值使用电流探针在0.02-0.2 mbar的氩气压力下测量HE模式过渡电流Imt ud。在0.08 mbar时Itr的最小值为(13.5±0.5)A,而在0.3 mbar时,Imt的最小值为 ud(8.3±0.1)A。随着压力增加,观察到E-H模式和udH-E模式转换之间的磁滞变得更加明显。对于电介质板上方的不同轴向距离,使用带有光化学发光发射光谱法(AOES)的光纤探针在0.03、0.05、0.07、0.1 ud和0.2 mbar的氩气压力下使用纤维探针测量线平均中性气体温度Tn。 R.f.udpower在100 W到200 W之间变化。获得的Tn范围为 ud(350±30)-(840±30)K​​.ud。对于理论表征,使用了两个预测模型。第一个是 ud电磁场模型,它模拟| Bz |和| Br |,使用经验拟合的空间分解的电子密度ne(r,z)和电子温度Te(r,z)。 ud对空间平均Tn和启发式拟合的空间 ud分布温度Tn进行了模拟(r,z)。 Tn(r,z)与测得的超磁场最接近。 ud第二个模型是模拟Itr和Imt的功率沉积模型。 ud在Tn = 300 K和升高的Tn下进行仿真。仅当考虑中性气体加热时,计算才能更好地匹配测得的值。还使用拟合的3D功率偏差图证明了放电的滞后 udin模式转变的影响。 ud这些结果表明,中性气体加热在影响 udplasma参数中起着重要作用。因此,了解中性气体加热的影响是必不可少的,它有助于更​​好地理解等离子体放电的形成和维持。

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    Kanesh Kumar Jayapalan;

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