Titlebook: Mass Supply and Flows in the Solar Corona; The 2nd SOHO Worksho B. Fleck,G. Noci,G. Poletto Book 1994 Springer Science+Business Media Dordr

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書(shū)目名稱(chēng)Mass Supply and Flows in the Solar Corona影響因子(影響力)




書(shū)目名稱(chēng)Mass Supply and Flows in the Solar Corona影響因子(影響力)學(xué)科排名




書(shū)目名稱(chēng)Mass Supply and Flows in the Solar Corona網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱(chēng)Mass Supply and Flows in the Solar Corona網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




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書(shū)目名稱(chēng)Mass Supply and Flows in the Solar Corona被引頻次學(xué)科排名




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書(shū)目名稱(chēng)Mass Supply and Flows in the Solar Corona讀者反饋




書(shū)目名稱(chēng)Mass Supply and Flows in the Solar Corona讀者反饋學(xué)科排名

Magnitude

緯線(xiàn)

Magnetic Fine Structures in Coronal Loopsnly for short periods of time. The formation of thin current sheets is discussed. It is argued that photospheric magnetic structures (flux tubes) play an important role in the generation of coronal currents.

Jubilation

Small Scale Structures in the Solar Coronawn to be remarkably similar. Particular emphasis is given to observations, potentially feasible with SOHO, that could resolve some of the outstanding issues regarding the role of the small scale magnetic structures in the energy balance and properties of the solar wind.

欺騙手段

Numerical Simulations of Spicule Driving Mechanismsc flux tube. The shocks are initiated due to compression of the tube by the increasing external pressure in the lower chromosphere. Downflow of spicular material depends on radiative cooling and other dissipative processes.

制定

The Chromospheric Network Dynamics as Derived from the Analysis of CA II K and HE I 1083 NM Linesroperties of the main components of the quiet chromosphere: i) the magnetic network, ii) the cell interior. We present a whole set of amplitude spectra near 5 and 3 min periods for the two lines; K3 and He I velocity spectra extending up to 100 mHz are also considered, for the first time.

Flatus

The Coronal Context of Transition Region Explosive Eventshe SOHO spacecraft provides an opportunity to extend this search for the coronal counterparts of the transition region explosive events, as well as to explore the correspondence of explosive events with large scale coronal structures, such as with coronal dark lanes.

Trigger-Point

Flatus

Turbulent Transition in Solar Surgesinstabilities of the MHD tearing jet. Our results confirm that turbulent transition can decelerate the surge, with decay times which compare well with surge data. Furthermore, we find that the turbulent MHD tearing jet forms magnetic field-aligned velocity filaments similar to those often observed in the surge flow field.

Euthyroid