TO DETERMINE OF RESOLVING POWER OF A DIFFRACTION GRATING BY SPECTROMETER WITH THE HELP OF MERCURY LIGHT SOURCE
TO DETERMINE OF RESOLVING POWER OF A DIFFRACTION GRATING BY SPECTROMETER WITH THE HELP OF MERCURY LIGHT SOURCE

TO DETERMINE OF RESOLVING POWER OF A DIFFRACTION GRATING BY SPECTROMETER WITH THE HELP OF MERCURY LIGHT SOURCE

TO DETERMINE OF RESOLVING POWER OF A DIFFRACTION GRATING BY SPECTROMETER WITH THE HELP OF MERCURY LIGHT SOURCE Specification

  • Type
  • Laboratory Instrument for Optical Experiments
  • Material
  • Heavy-duty Iron Base, Brass Body, Optical Glass Lenses, Polished Grating Holder
  • Size
  • Standard
  • Input Voltage
  • 230V AC, 50 Hz
  • Color
  • Black/Polished Brass & Chrome Finish
  • Dimension (L*W*H)
  • 440 mm x 160 mm x 300 mm (approximate)
  • Capacity
  • Suitable for educational laboratory demonstrations
  • Noise Level
  • Negligible
  • Base
  • Tripod or Heavy Stable Base for Vibration Resistance
  • Light Source Housing
  • Enclosed, with Power Cord and Switch
  • Spectrometer Telescope
  • Achromatic, Adjustable Focus
  • Application
  • Measurement of Resolving Power and Wavelengths through Diffraction
  • Collimator
  • Adjustable with Slit
  • Wavelength Source
  • Mercury Lamp, Multi-line Emission
  • Grating Type
  • Plane Transmission Diffraction Grating
  • Grating Lines Per mm
  • 600 lines/mm
  • Accessories Included
  • Diffraction Grating, Mercury Lamp, Power Cord, Instruction Manual
  • Least Count
  • 0.01 degree
 
 

About TO DETERMINE OF RESOLVING POWER OF A DIFFRACTION GRATING BY SPECTROMETER WITH THE HELP OF MERCURY LIGHT SOURCE



Experience phenomenal optical precision with our customizable setup to determine the resolving power of a diffraction grating using a spectrometer with a mercury light source. This superlative instrument features a plane transmission grating of 600 lines/mm and a multi-line mercury emission lamp, ensuring elite clarity for wavelength analysis. The achromatic, adjustable-focus telescope and heavy-duty, vibration-resistant base provide stability and accuracy. Complete with essential accessories, this best-in-class laboratory instrument is ideal for educational demonstration, research, and advanced optical experimentsdelivering outstanding savings and reliability.

Phenomenal Features & Application Scope

This elite laboratory instrument stands out with extra features such as an achromatic telescope, polished grating holder, and fully enclosed light source housing. Used as a superlative tool for measuring the resolving power and wavelengths, it serves both educational and research sites. Perfectly provisioned for physics laboratories, it facilitates direct comprehension of diffraction phenomena, spectral line separation, and practical optics study, making it the best resource for students and professionals alike.


Packaging, Delivery & Export Market Commitment

Our export market offering ensures your proposal amount includes secure packaging in robust, damage-resistant cartons. Transportation arrangements cater to domestic and international buyers, and typical delivery time is within 10-15 working days. A standard sample is available upon request to help you evaluate the instruments performance before making a bulk purchase. As a reliable distributor, exporter, and supplier, we guarantee swift processing and superior after-sales support across India and beyond.


FAQs of TO DETERMINE OF RESOLVING POWER OF A DIFFRACTION GRATING BY SPECTROMETER WITH THE HELP OF MERCURY LIGHT SOURCE:


Q: How does the spectrometer determine the resolving power of a diffraction grating?

A: The spectrometer analyzes the diffraction patterns produced by the plane transmission grating using the multi-line mercury lamp, allowing precise measurement and comparison of spectral lines. The resolving power is determined by measuring the ability to distinguish closely spaced wavelengths.

Q: What are the main benefits of using this customizable optical setup?

A: This setup offers elite versatility, high accuracy, and superb stabilityenabling in-depth study of diffraction, wavelength measurement, and spectral analysis for both education and laboratory research.

Q: Where can this instrument be effectively utilized?

A: It is designed for physics and optics laboratories, science departments of educational institutions, and research centers that require hands-on experimentation in spectroscopy and diffraction analysis.

Q: What extra features make this laboratory instrument superior?

A: Special features include an achromatic, adjustable-focus telescope, adjustable collimator and slit, vibration-resistant heavy base, enclosed light source housing, and a polished grating holder for reliable and precise performance.

Q: Is a sample available before placing a bulk order?

A: Yes, we offer a sample unit for evaluation, so you can verify its quality and performance prior to confirming your proposal amount and proceeding with larger quantities.

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