Titlebook: Recent Advances in the Understanding of Solar Flares; Proceedings of the U S. R. Kane,Y. Uchida,H. S. Hudson Conference proceedings 1983 Sp

stripper

书目名称Recent Advances in the Understanding of Solar Flares影响因子(影响力)




书目名称Recent Advances in the Understanding of Solar Flares影响因子(影响力)学科排名




书目名称Recent Advances in the Understanding of Solar Flares网络公开度




书目名称Recent Advances in the Understanding of Solar Flares网络公开度学科排名




书目名称Recent Advances in the Understanding of Solar Flares被引频次




书目名称Recent Advances in the Understanding of Solar Flares被引频次学科排名




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书目名称Recent Advances in the Understanding of Solar Flares年度引用学科排名




书目名称Recent Advances in the Understanding of Solar Flares读者反馈




书目名称Recent Advances in the Understanding of Solar Flares读者反馈学科排名

fluoroscopy

Solar Flare X-ray Spectra from the P78-1 Spacecraftdiagnostics used in interpreting the spectra are summarized, and the origin of the thermal soft X-ray emitting plasma is discussed in light of the P78-1 results, earlier data, and numerical simulations of magnetic flux tubes heated to solar flare temperatures.

服从

Energetic Electrons as an Energy Transport Mechanism in Solar Flaresrticular through the diagnostics of both the Fe Kα feature and optically thin transition region lines such as OV. Finally, we discuss the relative roles of electron and proton heating in γ-ray flare events.

创作

哺乳动物

Solar Instruments on the P78-1 Spacecraftuilt by the Aerospace Corporation and the Naval Research Laboratory. The hard X-ray spectrometers were built by the Aerospace Corporation and the white light coronagraph was supplied by the Naval Research Laboratory. Most of these instruments are still returning data.

运气

Magnetic Theories of Solar Flaresm, or emerging flux. The second type is thought to be the result of an eruptive MHD instability that is either spontaneous or triggered from outside. After the eruption the magnetic field lines that have been blown open reconnect back down in a way that has now been simulated numerically.

majestic

Non-Thermal and Non-Equilibrium Effects in Soft X-ray Flare Spectra-state. A search of suitable complex flares with multiple impulsive features has shown indications of soft X-ray line intensity anomalies, consistent with the presence of a non-thermal electron component.

颂扬本人

Transport and Containment of Plasma, Particles and Energy within Flaresture at the time of a flare and a complex and changing magnetic topology during the course of a flare. The rocket data are examined for constraints on flare cooling, within the context of simple loop models. These results form a basis for comments on the limitations of simple loop models for flares.

Annotate

Thermal Evolution of Flare Plasmaursts is confirmed by the observation of an electron temperature increase at the time interval of hard X-ray spikes and a quantitative comparison between thermal energy content and hard X-ray energy input. Non-thermal electrons of 10 keV < E < 30 keV energy may play an important role in pre- and post-burst phases.

Deduct

Upper Limits on the Total Radiant Energy of Solar Flarespulsive emission; for a gradual component, about 4 x 10. ergs total radiant energy. The limits lie about an order of magnitude higher than the total radiant energy estimated from the various known emission components, suggesting that no heretofore unknown dominant component of flare radiation exists.