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Article
The He+ λ 4686 line in the low chromosphere
We report an unsuccessful search for the He+ λ 4686 line in the low chromosphere. However, at the location of this line we detect a number of other chromospheric emission lines. This leads us to the conclusion th...
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Article
Theoretical model of flares and prominences
A theoretical model of flare which explains observed quantities in Hα, EUV, soft X-ray and flare-associated solar wind is presented. It is assumed that large mass observed in the soft X-ray flare and the solar...
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Chapter and Conference Paper
Balloon Observation of the F-corona at the 1983 Total Solar Eclipse
A balloon observation of the F-corona in visual and infrared regions was carried out by Japanese and Indonesian teams at the total solar eclipse on June 11, 1983, in Java, Indonesia. For the visual observation...
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Article
Rocket observation of the EUV images of a solar flare and active regions
Images of a flare and active regions were obtained in the extreme ultraviolet emission lines such as CIII 977 Å, Ne VIII 770 Å, and HI Lβ, and hydrogen Lyman continua with a spatial resolution of less than ten se...
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Chapter
Solar Activity
In preparing the present report, which covers the period July 1, 1984, to June 30, 1987, close collaboration has taken place between Commission 10 and 12, the two solar commissions, in order to avoid duplicati...
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Chapter and Conference Paper
Physical conditions in prominences
As a summary of this paper I am presenting a table which is in a very similar format as I have presented in the former IAU colloquium (Hirayama, 1978), and according change was made. Though the present study d...
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Chapter and Conference Paper
Magnetic morphologies of solar flares
We suggest magnetic morphologies for several flares using Hα filter-grams and a flare model of reconnection under an erupting magnetic flux rope (Hirayama, 1974). Here we select those flares which, at first si...
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Chapter and Conference Paper
Solar flare telescope and 10-cm new coronagraph
Two new telescopes were built at the National Astronomical Observatory of Japan, i.e. the Solar Flare Telescope and the 10-cm New Coronagraph. The Solar Flare Telescope was constructed at Mitaka to make observ...
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Chapter
The Soft X-ray Telescope for the SOLAR-A Mission
The Soft X-ray Telescope (SXT) of the SOLAR-A mission is designed to produce X-ray movies of flares with excellent angular and time resolution as well as full-disk X-ray images for general studies. A selection...
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Article
The Soft X-ray Telescope for the SOLAR-A mission
The Soft X-ray Telescope (SXT) of the SOLAR-A mission is designed to produce X-ray movies of flares with excellent angular and time resolution as well as full-disk X-ray images for general studies. A selection...
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Article
The current sheet and Joule heating of a slender magnetic tube in the upper photosphere
Joule heating in a slender magnetic flux tube is investigated. The distribution of the magnetic field and electric sheet current encircling a vertical cylindrical magnetic tube is determined by equating the co...
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Chapter and Conference Paper
Photo-Stimulated Desorption of Ne Metastables from Thin Ne Layers on Solid Ar, Kr, and Xe
Photo-stimulated dcsorplion of Ne melastables(Ne*) from a thin Ne film adsorbed on solid Ar, Kr, and Xe was studied using synchrotron radiation as an excitation source. The excitation which is corresponding to...
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Chapter
Coronal Heating Due to Twisting Faculae of 1 km Radii
We propose a scenario for coronal heating as a result of body Joule heating of a twisting magnetic tube of ≈10 km radius due to anomalous resistivity, whose effective collision frequency is 10-2 times the electro...
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Article
Ion photodesorption from argon multilayers
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Chapter and Conference Paper
Microstructure characterization of the YBa2Cu3O7-y thin films derived from the metal-naphthenates gels coated on SrTiO3(100) and LaAlO3(100) substrates
The thin films of YBa2Cu3O7-y, prepared by chemical solution deposition on SrTiO3(100) and LaAlO3(100) substrates, have been characterized by cross-sectional high-resolution electron microscopy. It is found that ...
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Chapter and Conference Paper
Atomic structure and dopant segregation of [0001] tilt grain boundaries in ZnO bicrystals
Physical properties of ceramics are often changed by presence of grain boundaries (GBs). One possible cause of the change is the grain boundary (GB) itself, because the GB atomic structure is different from th...