Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Concept Videos

Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

3.4K
Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
3.4K
Atomic Nuclei: Larmor Precession Frequency01:11

Atomic Nuclei: Larmor Precession Frequency

2.6K
The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession,...
2.6K
Inductively Coupled Plasma Atomic Emission Spectroscopy: Principle01:19

Inductively Coupled Plasma Atomic Emission Spectroscopy: Principle

1.5K
Inductively coupled plasma (ICP) is the most widely used plasma source in atomic emission spectroscopy (AES), also known as Inductively Coupled Plasma Optical Emission Spectroscopy (ICP-OES). The ICP source, or torch, consists of three concentric quartz tubes with argon gas flowing through them. A spark from a Tesla coil initiates the ionization of argon, generating a high-temperature plasma.
The ions and electrons produced interact with the fluctuating magnetic field created by a water-cooled...
1.5K
NMR Spectrometers: Radiofrequency Pulses and Pulse Sequences01:17

NMR Spectrometers: Radiofrequency Pulses and Pulse Sequences

1.6K
A pulse is a short burst of radio waves distributed over a range of frequencies that simultaneously excites all the nuclei in the sample. Upon passing a radio frequency pulse along the x-axis, the nuclei absorb energy corresponding to their Larmor frequencies and achieve resonance. This shifts the net magnetization vector from the z-axis toward the transverse plane. This angle of rotation of the magnetization vector, or the flip angle, is proportional to the duration and intensity of the pulse.
1.6K
Atomic Absorption Spectroscopy: Atomization Methods01:25

Atomic Absorption Spectroscopy: Atomization Methods

1.3K
Atomic Absorption Spectroscopy (AAS) atomizes samples through flame atomization or electrothermal atomization. Flame atomization typically involves a nebulizer and spray chamber assembly to combine the sample with a fuel–oxidant mixture, creating a fine aerosol mist that enters a burner. Typically, the fuel and oxidant are combined in an approximately stoichiometric ratio. However, for atoms that are easily oxidized, a fuel-rich mixture may be more advantageous. Only about 5% of the...
1.3K
Inductively Coupled Plasma–Mass Spectrometry (ICP–MS): Overview01:19

Inductively Coupled Plasma–Mass Spectrometry (ICP–MS): Overview

1.6K
In inductively coupled plasma–mass spectrometry (ICP–MS), an inductively coupled plasma (ICP) torch is used as an atomizer and ionizer. Solid samples are dissolved and volatilized before being introduced into the high-temperature argon plasma, while solution samples are nebulized and passed through the high-temperature argon plasma. Plasma dissociates the analytes and ionizes their component atoms to form a mixture of positive ions and molecular species. The positive ions are then...
1.6K

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

Real-Time Observation of Frustrated Ultrafast Recovery from Ionization in Nanostructured SiO_{2} Using Laser-Driven Accelerators.

Physical review letters·2024
Same author

Laser-accelerated electron beams at 1 GeV using optically-induced shock injection.

Scientific reports·2023
Same author

Stabilized Radiation Pressure Acceleration and Neutron Generation in Ultrathin Deuterated Foils.

Physical review letters·2022
Same author

Absolute calibration of Fujifilm BAS-TR image plate response to laser driven protons up to 40 MeV.

The Review of scientific instruments·2022
Same author

Time-resolved study of holeboring in realistic experimental conditions.

Nature communications·2021
Same author

Narrow Bandwidth Gamma Comb from Nonlinear Compton Scattering Using the Polarization Gating Technique.

Physical review letters·2021

Related Experiment Video

Updated: Jan 2, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

15.4K

Intense attosecond pulses carrying orbital angular momentum using laser plasma interactions.

J W Wang1, M Zepf2,3, S G Rykovanov4

  • 1State Key Laboratory of High Field Laser Physics, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, 201800, Shanghai, China. wangjw@siom.ac.cn.

Nature Communications
|December 6, 2019
PubMed
Summary

Intense extreme ultra-violet (XUV) attosecond pulses with orbital angular momentum (OAM) are naturally generated from non-vortex laser beams interacting with a target. This overcomes challenges in producing OAM in high-intensity XUV light.

More Related Videos

Direct Imaging of Laser-driven Ultrafast Molecular Rotation
10:52

Direct Imaging of Laser-driven Ultrafast Molecular Rotation

Published on: February 4, 2017

10.1K
20 mJ, 1 ps Yb:YAG Thin-disk Regenerative Amplifier
10:17

20 mJ, 1 ps Yb:YAG Thin-disk Regenerative Amplifier

Published on: July 12, 2017

11.9K

Related Experiment Videos

Last Updated: Jan 2, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

15.4K
Direct Imaging of Laser-driven Ultrafast Molecular Rotation
10:52

Direct Imaging of Laser-driven Ultrafast Molecular Rotation

Published on: February 4, 2017

10.1K
20 mJ, 1 ps Yb:YAG Thin-disk Regenerative Amplifier
10:17

20 mJ, 1 ps Yb:YAG Thin-disk Regenerative Amplifier

Published on: July 12, 2017

11.9K

Area of Science:

  • * Quantum optics
  • * Laser physics
  • * Attosecond science

Background:

  • * Light beams carrying orbital angular momentum (OAM) offer an extra degree of freedom for coherent light.
  • * Generating OAM beams in the extreme ultra-violet (XUV) at high intensities is challenging using conventional methods like phase plates or gratings.

Purpose of the Study:

  • * To theoretically and numerically demonstrate a novel method for generating intense XUV surface harmonics with OAM.
  • * To investigate the intrinsic dynamics of laser-matter interaction for OAM generation.

Main Methods:

  • * Theoretical and numerical modeling of intense circularly-polarized Gaussian laser beams interacting with a target at normal incidence.
  • * Utilizing the relativistic oscillating mirror mechanism for XUV harmonic generation.
  • * Analyzing the conversion of spin angular momentum to orbital angular momentum during harmonic generation.

Main Results:

  • * Intense surface harmonics carrying OAM are naturally produced from non-vortex laser beams.
  • * The process involves relativistic surface oscillations converting laser pulses to XUV radiation.
  • * Azimuthal and radial dependencies in harmonic generation facilitate the spin-to-orbital angular momentum conversion.

Conclusions:

  • * A new pathway for generating high-intensity XUV attosecond pulses with OAM has been demonstrated.
  • * This method bypasses the need for complex optical elements for OAM beam formation in the XUV spectrum.
  • * The findings open possibilities for advanced applications utilizing OAM-carrying XUV light.