The authors utilize line - of - sight (LOS) magnetic field data and
spectral line information obtained by the Helioseismic and Magnetic Imager (HMI) instrument aboard the Solar Dynamics Observatory (SDO).
Not exact matches
The scientists were thus able to transfer the genetic
information from the known fluorescent protein eqFP615 into the DT40 chicken B cell
line in order to produce protein variants of the new infrared marker Amrose with different
spectral properties.
Figures 01 and 02 summarize the
information from IC342's 12CO J = 1 - 0
spectral line data cube.
The dynamics of solar processes can be captured on shorter time scales, and the improved light - gathering capacity of the new telescopes allows us to extract more
information from
spectral lines with higher fidelity and accuracy, especially with respect to magnetic field measurements.