Titlebook: Solar and Heliospheric Plasma Physics; Proceedings of the 8 George M. Simnett,Constantine E. Alissandrakis,Lou Conference proceedings 1997

Palpate

Flows through the magnetically structured solar atmosphere,represent footpoints of coronal loops. Largescale coronal structures (streamers, jets, post-flare loops, arcades) are linked to photospheric and chromospheric events and give a three-dimensional view of the atmosphere.

ALE

人类的发源

Modulation of solar and stellar activity cycles,r system, for two-dimensional dynamo waves and for a simple global model. Amplitude modulation that leads to grand minima is distinct from modulation associated with changes in the symmetry of the field.

胆大

个阿姨勾引你

SIT

DUCE

Future space instrumentation for solar physics,and a STEREO mission of some form. New particle instruments which can detect solar emissions, such as ACE, will be launched before the year 2000. The ESA Horizon 2000+ program has some medium missions, yet to be defined, which should be devoted to solar studies.

integrated

Baffle

JAMB

Dynamics of flux tubes in the solar atmosphere: Observations, in both the largest and smallest flux tubes, i.e. in sunspots and magnetic elements, is given. Then three such phenomena — the Evershed effect, steady flows in small-scale magnetic features and oscillations in such features — are selected and discussed in detail.