TY  CONF
TI  The impact of technical constraints on the possibility of resolving the pulsar magnetosphere by observing its scintillations
KW  scattering; pulsars: individual: B1237+25; ISM: general; techniques: high angular resolution; methods: data analysis
JO  Modern astronomy: from the Early Universe to exoplanets and black holes
AU  Fadeev, E..
AU  Andrianov, A..
AU  Burgin, M..
AU  Popov, M..
AU  Rudnitskiy, A..
AU  Smirnova, T..
AU  Soglasnov, V..
PY  2024
PB  Special Astrophysical Observatory of the Russian Academy of Sciences