Flare physics in solar activity maximum 22 : proceedings of the International Solar-A Science Meeting held at Tokyo, Japan, 23-26 October 1990 : dedicated to the memory of the late professor K. Tanaka
The book reviews the knowledge obtained from ground-based and space-borne solar flare research thus at the same time preparing for the forthcoming mission of the satellite Solar A which will be launched in 1991. Accordinglyone section is devoted to experiments on Solar A. The rest review both theory...
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| Altri autori: | , , |
| Natura: | Livre numérique |
| Lingua: | Anglais |
| Pubblicazione: |
Berlin [etc.] :
Springer
[20..].
Cham : Springer Nature |
| Serie: | Lecture notes in physics
387 |
| Soggetti: | |
| Accesso online: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Nota: |
Autre contribution : E. Hiei Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Flare physics in solar activity maximum 22, proceedings of the International Solar-A Science Meeting held at Tokyo, Japan, 23-26 October 1990, dedicated to the memory of the late professor K. Tanaka, Y. Uchida ... [et al.], eds, Berlin, Springer-Verlag, 1991, 1 vol. (X-360 p.), Lecture notes in physics, 3-540-54383-X • Flare Physics in Solar Activity Maximum 22, Texte imprimé, 9783662138397 • Flare Physics in Solar Activity Maximum 22, Texte imprimé, 9783662138403 |
Sommario:
- General introduction
- In memoriam Katsuo Tanaka
- The sources of solar flares
- The Solar-A mission
- Soft X-ray telescope (SXT)
- The Hard X-ray Telescope(HXT) on board SOLAR-A
- The Solar-A Bragg crystal spectrometer
- The wide band spectrometer on the Solar-A
- The SOLAR-A onboard Data Processor (DP)
- Capabilities and limitations of Solar-A
- Optical observations of flare-productive flux emergence
- Flares appear on the red shift side near the inversion line of the H? Dopplergram
- Small scale active phenomena observed with DST and Huairou magnetogram
- Microflares observed in He I 10830 and their relation to the quiet sun magnetic fields
- HeI 10830Å observations of active regions
- Numerical simulations of ultraviolet and X-ray microflares
- Particle acceleration and the locations of hard X-ray sources
- The controversial relationship between hard X-ray and soft X-ray flares: Causal or non-causal?
- Magnetic morphology of nonthermal electron precipitation during three flares in a highly nonpotential active region
- The role of accelerated ions during the impulsive phase of flares and the production of hard X-rays
- Physical implications of X-ray imaging observations
- Studies of high-energy flare phenomena from simultaneous observations of gamma-rays and energetic particles
- Acceleration of high-energy nuclei as viewed from their chemical composition
- Heating and flows in flares
- Studies of helium-like ion spectra with the SMM flat crystal spectrometer
- X-ray spectra from Hinotori satellite and suprathermal electrons
- Quality improvement of solar flare temperature and density diagnostics derived from BCS spectra
- The beam driven chromospheric evaporation model of large solar flares: a model getting no respect from the sun
- Numerical simulations ofelectron-beam-heated solar flares
- A hydrodynamic thermal model of the impulsive phase of solar flares
- Material flow of a surge flare
- Evolution of hot plasma in flares
- The electron distribution and SXT images of a coronal soft X-ray source
- Interpretation of multi-channel X-ray intensities from solar flares
- Thermodynamic evolution of flares
- Simulation of SXT response to XSST soft X-ray spectrum
- Magnetic morphologies of solar flares
- Theoretical models of solar flares
- The practical application of the magnetic virial theorem
- Maximum energy of semi-infinite magnetic-field configurations
- High-energy particle acceleration during the implosion driven by 3-dimensional X-type current loop coalescence in solar flares
- On mechanisms of solar flares some observational tests by using Solar-A
- Plasma waves caused by transient heat conduction in a coronal loop as a trigger for impulsive solar flares
- Magnetic structures in the corona
- Chromospheric and coronal activities in the quiet sun originating from photospheric 5-minute oscillations
- VLA supporting observations for SOLAR-A
- X-ray observations of global solar activity
- Coronal structures and the sunspot cycle
- Absorption of magnetoacoustic waves in the solar atmosphere with random inhomogeneities of density and magnetic fields
- SXT observations of MHD turbulence in active regions
- Simulated SXT observations of coronal loops
- Max '91/FLARES 22
- Studies of X-Ray flares by project CORONAS
- Solar energetic particle observation by GEOTAIL satellite
- Solar flare telescope and 10-cm new coronagraph
- The MSFC vector magnetograph, eruptive flares, and the Solar-A X-ray images
- Nobeyama radioheliograph
- Millimeter interferometric observations of solar flares during the Solar A mission
- Coronalrestructuring and coronal mass ejections as infrared from interplanetary magnetic flux ropes
- A proposal for a study of the solar wind near the sun by simultaneous observations with SOLAR-A and Kashima 34m antenna
- Search for transient coronal holes by SOLAR-A soft X-ray telescope
- Application of SOLAR-A SXT data to flare and geomagnetic storm forecasting research.