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i think you mean 'What is the free spectral range?' it is the range in which orders of are not overlapping. see http://www.shimadzu.com/products/opt/oh80jt0000001ux4.html hope it was some help for you

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Classification of stars according to color?

Stars can be classified into different spectral types based on their color, which is related to their surface temperature. The classification system uses the letters O, B, A, F, G, K, and M to represent the range of temperatures from hottest (blue/white) to coolest (red). This sequence is known as the spectral sequence or spectral types.


You observe the same spectral line in two stars that are identical in every way except that one rotates faster than the other How does the spectral line differ between the two?

The spectral line in the star that rotates faster will be broader due to the Doppler effect caused by the varying speeds of rotation on different parts of the star. The faster rotation creates a wider range of velocities contributing to the broadening of the spectral line compared to the slower rotating star.


Does the spectral type surface temperature and color all describe the same basic characteristic of a star?

Yes, spectral type, surface temperature, and color are related descriptors of a star's characteristics. Spectral type categorizes stars based on their surface temperature and characteristics of their spectra, with each type corresponding to a specific temperature range and color. So, they all provide insights into a star's surface temperature and related properties.


What does spectral disturbance mean?

Spectral disturbance refers to irregularities or variations in the frequency composition of a signal or phenomenon. In the context of data analysis or signal processing, it often indicates anomalies, interference, or noise that can affect the reliability or accuracy of measurements or observations. Spectral disturbance can be identified through spectral analysis techniques such as Fourier transforms.


Who created the three laws dealing with the creation of various spectra?

Niels Bohr proposed the three laws regarding the creation of various spectra. These laws are used to explain the spectral lines of hydrogen and other elements.

Related Questions

What is its spectral range?

Spectral range refers to the range of wavelengths of electromagnetic radiation that a device or instrument can detect or measure. The specific spectral range can vary greatly depending on the type of device or instrument being used, such as visible light, ultraviolet, infrared, etc.


The Maximum spectral response of the germanium and silicon is in the?

The maximum spectral response of germanium is in the infrared region, while the maximum spectral response of silicon is in the visible light region. Germanium has a broader spectral response range compared to silicon.


Why FMCW radar has better range resolution than CW radar?

FM CW radar sweeps the Radio Frequency over time. Time in Radar equates to range and results in a high spectral density at every range. CW radar has a much lower spectral density and does not code range with frequency in the same way.


Two stars of the same spectral class must have the same what?

Two stars of the same spectral class must have the same temperature and color. This classification system groups stars based on their temperature, with each spectral class representing a specific range of temperatures.


What type of electromagnetic waves are your eyes sensitive to?

Those in the range of spectral wavelengths labeled "visible light".


Why are spectral interferences more common in icp-oes than in aas?

Spectral interferences are more common in ICP-OES than in AAS because ICP-OES uses a wider range of wavelengths, increasing the likelihood of overlapping spectral lines from different elements, resulting in interferences. In contrast, AAS typically focuses on a single wavelength for analysis, reducing the possibility of spectral interferences.


What determines the range of spectral lines produced during electron transition?

The range of spectral lines produced during electron transition is determined by the energy difference between the initial and final electronic states. This energy difference corresponds to the photon energy of the emitted light, which dictates the wavelength or frequency of the spectral lines observed in the spectrum. Additionally, the atomic structure and electron configuration of the atom also play a role in determining the specific transitions and resulting spectral lines.


What is spectral energy density?

The energy spectral density describes how the energy (or variance) of a signal or a time series is distributed with frequency.You can read more in Wikipedia 'Spectral Density', but you will need good maths to understand it!


What is the temperature of Zeta Andromedae?

Zeta Andromedae has a spectral class of K1 and will therefor have a temperature range of 3,700 -> 5,200 K


How do you say free range in Spanish?

Free range = de granja Free-range chicken = pollo de granja


Classification of stars according to color?

Stars can be classified into different spectral types based on their color, which is related to their surface temperature. The classification system uses the letters O, B, A, F, G, K, and M to represent the range of temperatures from hottest (blue/white) to coolest (red). This sequence is known as the spectral sequence or spectral types.


What is stronger Free range Eggs or Non-Free range Eggs?

free range eggs know that for a fact because i have a farm in flordia