@article{oai:nagano-nct.repo.nii.ac.jp:00000215,
 author = {NlSHIMURA, Osamu},
 journal = {長野工業高等専門学校紀要},
 month = {Jun},
 note = {application, The cyclotron lines are affected by photon splitting in super-strong magnetized atmospheres(～4.4×10^9 T) into which the power-law-type flux is injected. Since photon splitting occurs in super-strong magnetic field regardless of the existence of the plasma, it will occur over the larger scale than the cyclotron resonant scattering, which is interaction with the electron. We considered the atmospheres consisted of cyclotron resonant scattering predominant and photon splitting predominant regions. The emergent spectra were calculated in the cases of the line formation regions located in the middle and top of the atmosphere. We found that the location of the line formation regions affect the depth of the line. Furthermore, we calculated the emergent spectra in several optical depths of cyclotron resonant scattering predominant region and found that the cyclotron absorption lines become unclear in the higher resonant energies than 200 keV.},
 pages = {73--80},
 title = {The Influence of Photon Splitting on Cyclotron Line Formation in Atmospheres with Distinct Formation Regions},
 volume = {36},
 year = {2002}
}