At the time of a total solar eclipse,the spectrum of solar radiation would be:

  • A
    $A$ large number of dark Fraunhofer lines
  • B
    $A$ less number of dark Fraunhofer lines
  • C
    No lines at all
  • D
    All Fraunhofer lines changed into brilliant colours

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The wavelength of the ${K_{\alpha}}$ line for an element of atomic number $43$ is $\lambda$. Then the wavelength of the ${K_{\alpha}}$ line for an element of atomic number $29$ is:

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