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

Phase Contrast and Differential Interference Contrast Microscopy01:26

Phase Contrast and Differential Interference Contrast Microscopy

15.1K
Phase-Contrast Microscopes
In-phase-contrast microscopes, interference between light directly passing through a cell and light refracted by cellular components is used to create high-contrast, high-resolution images without staining. It is the oldest and simplest type of microscope that creates an image by altering the wavelengths of light rays passing through the specimen. Altered wavelength paths are created using an annular stop in the condenser. The annular stop produces a hollow cone of...
15.1K
Masking and Demasking Agents01:19

Masking and Demasking Agents

4.0K
EDTA titrations may necessitate masking and demasking agents to temporarily protect a particular metal ion in a mixture from the EDTA reaction. These agents facilitate the sequential analysis of the metal ions by forming stable complexes with some—but not all—metal ions during certain steps.
There are many masking agents, such as cyanide, fluoride, triethanolamine, thiourea, and 2,3-bis(sulfanyl)propan-1-ol (formerly 2,3-dimercapto-1-propanol), with the masking agent chosen based on...
4.0K
Phase Changes01:19

Phase Changes

5.6K
Phase transitions play an important theoretical and practical role in the study of heat flow. In melting or fusion, a solid turns into a liquid; the opposite process is freezing. In evaporation, a liquid turns into a gas; the opposite process is condensation.
A substance melts or freezes at a temperature called its melting point and boils or condenses at its boiling point. These temperatures depend on pressure. High pressure favors the denser form of the substance, so typically, high pressure...
5.6K

You might also read

Related Articles

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

Sort by
Same author

Genome-wide identification of SNPs in microRNA genes and the SNP effects on microRNA target binding and biogenesis.

Human mutation·2011
Same author

A case of intimal sarcoma of the pulmonary artery successfully treated with chemotherapy.

International journal of clinical oncology·2011
Same author

Exome sequencing identifies frequent mutation of ARID1A in molecular subtypes of gastric cancer.

Nature genetics·2011
Same author

Energetic salts based on dipicrylamine and its amino derivative.

Chemistry (Weinheim an der Bergstrasse, Germany)·2011
Same author

Biophysical properties of slow potassium channels in human embryonic stem cell derived cardiomyocytes implicate subunit stoichiometry.

The Journal of physiology·2011
Same author

Natural variation of folate content and composition in spinach (Spinacia oleracea) germplasm.

Journal of agricultural and food chemistry·2011

Related Experiment Video

Updated: Mar 25, 2026

Shaping the Amplitude and Phase of Laser Beams by Using a Phase-only Spatial Light Modulator
08:39

Shaping the Amplitude and Phase of Laser Beams by Using a Phase-only Spatial Light Modulator

Published on: January 28, 2019

10.5K

Cascade six-level phase-mask achromatic coronagraph.

Yajun Ge, Qing Cao, Rongfei Hu

    Applied Optics
    |February 25, 2016
    PubMed
    Summary

    A novel six-level phase-mask achromatic coronagraph achieves high starlight suppression. This advanced coronagraph technology stably reduces starlight by 10⁻¹⁰ over a 40% bandwidth.

    Area of Science:

    • Optical Engineering
    • Astronomy
    • Instrumentation

    Background:

    • Coronagraphs are essential for exoplanet detection by blocking starlight.
    • Achieving broadband starlight suppression remains a significant challenge in coronagraph design.

    Purpose of the Study:

    • To propose and analyze a cascade six-level phase-mask achromatic coronagraph (SLPMC).
    • To evaluate the starlight suppression performance of the SLPMC over a wide bandwidth.

    Main Methods:

    • Designing a three-stage SLPMC architecture.
    • Performing optimization analysis on the working wavelength of each phase mask.
    • Simulating starlight suppression in an ideal aberration-free scenario.

    Main Results:

    More Related Videos

    Multimodal Volumetric Retinal Imaging by Oblique Scanning Laser Ophthalmoscopy oSLO and Optical Coherence Tomography OCT
    12:22

    Multimodal Volumetric Retinal Imaging by Oblique Scanning Laser Ophthalmoscopy oSLO and Optical Coherence Tomography OCT

    Published on: August 4, 2018

    9.1K
    High Speed Sub-GHz Spectrometer for Brillouin Scattering Analysis
    13:31

    High Speed Sub-GHz Spectrometer for Brillouin Scattering Analysis

    Published on: December 22, 2015

    15.9K

    Related Experiment Videos

    Last Updated: Mar 25, 2026

    Shaping the Amplitude and Phase of Laser Beams by Using a Phase-only Spatial Light Modulator
    08:39

    Shaping the Amplitude and Phase of Laser Beams by Using a Phase-only Spatial Light Modulator

    Published on: January 28, 2019

    10.5K
    Multimodal Volumetric Retinal Imaging by Oblique Scanning Laser Ophthalmoscopy oSLO and Optical Coherence Tomography OCT
    12:22

    Multimodal Volumetric Retinal Imaging by Oblique Scanning Laser Ophthalmoscopy oSLO and Optical Coherence Tomography OCT

    Published on: August 4, 2018

    9.1K
    High Speed Sub-GHz Spectrometer for Brillouin Scattering Analysis
    13:31

    High Speed Sub-GHz Spectrometer for Brillouin Scattering Analysis

    Published on: December 22, 2015

    15.9K
    • The ideal aberration-free SLPMC achieves an average starlight suppression of approximately 10⁻⁸ over a 40% bandwidth.
    • Optimized SLPMC design stably suppresses starlight to below 10⁻⁸, averaging around 10⁻¹⁰ across the entire 40% bandwidth.

    Conclusions:

    • The proposed SLPMC demonstrates significant potential for high-contrast imaging in astronomy.
    • This coronagraph design offers a viable solution for broadband starlight suppression, crucial for exoplanet studies.