Dept. of Theor. Phys., Ulyanovsk State Univ., Ulyanovsk, Russia;
Galaxy; cosmic ray propagation; differential equations; diffusion; fractals; galactic cosmic rays; interstellar matter; Galaxy; cosmic ray reacceleration; diffusion type; fractal-type time-distribution; fractional differential equations; fractional model; fractional operator; interstellar galactic medium; nonuniform time-distribution; secondary acceleration; spatial motion; Acceleration; Cosmic rays; Electric shock; Equations; Fractals; Mathematical model; Signal to noise ratio;
机译:星系群中无线电物质和晕圈的湍流宇宙射线加速
机译:GeV-TeV宇宙射线光谱异常,这是由于银河系中的微弱冲击而重新加速
机译:GeV-TeV宇宙射线光谱异常,这是由于银河系中的微弱冲击而重新加速
机译:星系中宇宙射线传输的分数异常扩散模型
机译:太阳圈中的宇宙射线能量损失和星际再加速。
机译:星系长丝是超高能宇宙射线起源的线索
机译:GeV-TeV宇宙射线光谱异常,这是由于银河系中的微弱撞击而加速
机译:K-Capture宇宙射线辅助和重新加速