Titlebook: Solar Magnetic Phenomena; Proceedings of the 3 Arnold Hanslmeier,Astrid Veronig,Mauro Messerotti Conference proceedings 2005 Springer Scien

Entropion

Simultaneous Visible and IR Spectropolarimetry of the Quiet Sun observed area, showing intrinsic magnetic fields of kG (traced by visible lines) co-existing with sub-kG fields (traced by infrared lines). We also found . profiles with opposite polarity in the visible and the IR in 25% of the pixels under study (8% of the area).

不如乐死去

和蔼

X-Ray and H,Emission of the 20 Aug 2002 Flare*off evolution is interpreted as a possible gap in energies of electrons injected into the X-ray thick-target source and those of the background plasma. Fast changes of H. intensities were found to be located away from the X-ray sources in the beginning of the H. flare.

你敢命令

arrhythmic

痛苦一下

Solar Flares — Observations and Theoryd temporal evolution common to most flares are summarized, including basic physical processes underlying the described phenomena. Various classification schemes are presented as an introduction to the overview of the actual physical comprehension of the solar flare phenomenon. Basic theoretical conc

Congregate

Coronal Mass Ejections and Magnetic Helicityds or thousands of km s. from the Sun. As CMEs are the primary cause of space weather disturbances, we need to understand their underlying cause(s) in order to be able to predict them. After an overview of their basic properties based on multi-wavelength and multi-instrument data, including optical,

谈判

High Energy Radiation from the Sun addresses observations and theory of high energy radiation from the sun, with the emphasis almost entirely on hard X-rays (HXR) from flares but with brief mention of γ-rays and of nonthermal processes in the non-flaring sun. Following an outline of hard X-ray instrumentation, some relevant plasma p

Eviction

表示向下

Eight Years of Soho: Some Highlightse hot and dynamic atmosphere, to the solar wind and its interaction with the interstellar medium. Analysis of the helioseismology data from SOHO has provided the first images of structures and flows below the Sun’s surface and has shed new light on a number of structural and dynamic phenomena in the