冲击力
发表于 2025-3-25 06:32:45
http://reply.papertrans.cn/24/2383/238292/238292_21.png
Mortal
发表于 2025-3-25 08:47:46
Numerical simulations of shock electron acceleration in solar physics, mainly based on full particle electrostatic and electromagnetic codes. Such codes are appropriate to follow the overall dynamics of the shock itself and to identify the different sources of acceleration and heating of particles in a self-consistent way.
CLIFF
发表于 2025-3-25 11:42:51
http://reply.papertrans.cn/24/2383/238292/238292_23.png
稀释前
发表于 2025-3-25 16:31:27
0075-8450 of magnetic energy releases. The experimental data from groundbased methods of radio astronomy as well as from satellites are also discussed. The book addresses researchers in astrophysics, and planetary science but should also be accessible to graduate students.978-3-662-14002-4978-3-540-49189-7Ser
thrombus
发表于 2025-3-25 21:53:58
https://doi.org/10.1007/978-1-4615-3584-3accurate measurements of geometric parameters (position, altitude, rotation rate), but also the deconvolution of physical parameters (density, temperature, magnetic field) along the line-of-sight, which is most feasible with simultaneous observations in complementary wavelengths, e.g. in soft X-rays, EUV, and radio.
TAIN
发表于 2025-3-26 04:05:10
http://reply.papertrans.cn/24/2383/238292/238292_26.png
Carbon-Monoxide
发表于 2025-3-26 08:10:13
http://reply.papertrans.cn/24/2383/238292/238292_27.png
Felicitous
发表于 2025-3-26 10:08:27
Performance of Natural I/O Applications,ive temperature diagnostic in the range 6.10. to 3.10.K. This SOHO instrument will thus probe the coronal plasma on a global scale, as well as the underlying cooler and turbulent atmosphere. The EIT‘s characteristics and performances are presented, and prospects for coordinated observations with ground-based radio observatories are outlined.
conscience
发表于 2025-3-26 15:46:04
http://reply.papertrans.cn/24/2383/238292/238292_29.png
LUMEN
发表于 2025-3-26 20:32:27
Imaging, stereoscopy, and tomography of the solar corona in soft X-rays and radio,e three-dimensional (3D) reconstruction techniques, such as stereoscopy and tomography. The 3D reconstruction of coronal structures involves not only accurate measurements of geometric parameters (position, altitude, rotation rate), but also the deconvolution of physical parameters (density, tempera