Results 211 to 220 of about 31,130 (257)
Searching for ultralight dark matter conversion in solar corona using Low Frequency Array data. [PDF]
Nat CommunAn H, Chen X, Ge S, Liu J, Luo Y.
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LoRa Propagation and Coverage Measurements in Underground Potash Salt Room-and-Pillar Mines. [PDF]
Sensors (Basel)Theissen M, Kianfar A, Clausen E.
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An interstellar mission to test astrophysical black holes. [PDF]
iScienceBambi C.
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Space Science Reviews, 1994
25 years after their discovery, pulsars still pose fundamental problems, in particular when the whole range of their periodsP is considered: 1.56 ms ≤P≤0.09 s. This communication reviews my understanding of the pulsar magnetosphere, windzone, and (coherent) radio emission.
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25 years after their discovery, pulsars still pose fundamental problems, in particular when the whole range of their periodsP is considered: 1.56 ms ≤P≤0.09 s. This communication reviews my understanding of the pulsar magnetosphere, windzone, and (coherent) radio emission.
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Astrophysics, 1995
A new version of the theory of pulsar radio emission is developed for the case of a coaxial rotator. It is based on the electric field that we established [G. S. Sahakian, Astrofizika, 37, 97 (1994)] for the radiation channel (the channel of open magnetic field lines) and on convenient approximations for the electron energy obtained in [G. S.
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A new version of the theory of pulsar radio emission is developed for the case of a coaxial rotator. It is based on the electric field that we established [G. S. Sahakian, Astrofizika, 37, 97 (1994)] for the radiation channel (the channel of open magnetic field lines) and on convenient approximations for the electron energy obtained in [G. S.
openaire +1 more source