Helmet 发表于 2025-3-21 18:50:28
书目名称Laser Spectroscopy IV影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0581585<br><br> <br><br>书目名称Laser Spectroscopy IV影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0581585<br><br> <br><br>书目名称Laser Spectroscopy IV网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0581585<br><br> <br><br>书目名称Laser Spectroscopy IV网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0581585<br><br> <br><br>书目名称Laser Spectroscopy IV被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0581585<br><br> <br><br>书目名称Laser Spectroscopy IV被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0581585<br><br> <br><br>书目名称Laser Spectroscopy IV年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0581585<br><br> <br><br>书目名称Laser Spectroscopy IV年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0581585<br><br> <br><br>书目名称Laser Spectroscopy IV读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0581585<br><br> <br><br>书目名称Laser Spectroscopy IV读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0581585<br><br> <br><br>stress-test 发表于 2025-3-21 20:47:49
Multiple Coherent Interaction in Optical Separated Fieldsecently elaborated new methods based on the use of Doppler free nonlinear resonances. The methods based on the use of spectroscopy of saturated absorption and two-photon resonances are widely used. The optical resonance widths may be decreased by increasing the time of particle-field interaction.hauteur 发表于 2025-3-22 04:14:52
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Transverse Resonance-Radiation Pressure on Atomic Beams and the Influence of fluctuations demonstrated that ions stored in electromagnetic traps can be cooled using the radiation pressure of nearly-resonant light . We are currently investigating the transverse dipole force of resonance-radiation pressure; an understanding of this type of force is crucial to the construction of optical traps.buoyant 发表于 2025-3-22 13:19:03
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http://reply.papertrans.cn/59/5816/581585/581585_9.pngcraven 发表于 2025-3-23 08:50:18
Theories of Laser Bandwidth Effects in Spectroscopythe simplest of these has been solved. In this talk I will only deal with what I will call the “width change” question. That is, to what extent is the observable spectroscopic linewidth changed if the exciting light has a finite bandwidth of its own?