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Titlebook: Coronal Magnetic Energy Releases; Proceedings of the C Arnold O. Benz,Albrecht Krüger Conference proceedings 1995 Springer-Verlag Berlin He

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樓主: Washington
51#
發(fā)表于 2025-3-30 11:22:59 | 只看該作者
52#
發(fā)表于 2025-3-30 13:19:00 | 只看該作者
Wavelet Theory and Its Applicationsagnetic energy. Several solar phenomena from bright points to coronal mass ejections are attributed to free magnetic energy apparently available in the corona. The possibility that magnetic energy release is the dominant energy input into the corona is discussed for the Sun with special emphasis on
53#
發(fā)表于 2025-3-30 19:00:09 | 只看該作者
https://doi.org/10.1007/978-1-4615-3584-3e 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
54#
發(fā)表于 2025-3-30 20:45:23 | 只看該作者
Women, Work-Related Stress, and Smokingobservations, which contain a last part of the maximum phase of the solar cycle 22, it was possible to obtain almost every aspect of solar activity at 17 GHz. They include two X-class flares, tens of M-class flares, hundreds of flares from the very initial phase through the late decay phase, or from
55#
發(fā)表于 2025-3-31 04:40:04 | 只看該作者
Summary and Implications for Future ResearchX-ray and microwave emission: gradual hard X-ray and associated radio emission from centimetric to hectometric waves, Moving Type IV bursts, Type II bursts, storm continua and noise storms. The energy budget of suprathermal particles is estimated, possible acceleration sites are investigated, and si
56#
發(fā)表于 2025-3-31 06:06:19 | 只看該作者
Women, Work-Related Stress, and Smoking and in the one case for which we have simultaneous soft and hard X-ray images, they also show compact sources coincident with the radio source. One of the bursts is barely detected in soft X-rays, yet has a moderate 17 GHz flux,.
57#
發(fā)表于 2025-3-31 09:46:29 | 只看該作者
58#
發(fā)表于 2025-3-31 14:33:16 | 只看該作者
Summary and Implications for Future Researchtion of magnetohydrodynamic (i.e., tearing and coalescence) and kinetic currentdriven instabilities, (3) the resulting spatial and temporal scales of energy release, (4) the acceleration of particles in such an environment. The dynamical current sheet model naturally explains fragmentary energy rele
59#
發(fā)表于 2025-3-31 19:30:05 | 只看該作者
Summary and Implications for Future Researchzone. Random movements of the feet of the fibers in the photosphere and emergence of new magnetic flux from the convection zone are responsible for the formation of neutral sheets and magnetic discontinuities inside the active region, which are the sites for magnetic dissipation. A simple model, bas
60#
發(fā)表于 2025-4-1 00:24:27 | 只看該作者
Dissolved Oxygen and Redox Potential,zed compact objects accretion can be modified by repeated magnetic energy storage and release. Further also in the absence of a central magnetosphere, such as around galactic and extragalactic black holes, magnetic flaring activity is possible in a corona on both sides of the disk..Moreover strong o
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