๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Past and recent observations of the solar upper atmosphere at vacuum-ultraviolet wavelengths

โœ Scribed by Klaus Wilhelm


Publisher
Elsevier Science
Year
2003
Tongue
English
Weight
542 KB
Volume
65
Category
Article
ISSN
1364-6826

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Observations and interpretation of the s
โœ Ch. V. Sastry; K. S. Dwarkanath; R. K. Shevgaonkar; V. Krishan ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 517 KB

We have observed the slowly varying component of solar radio emission at a frequency of 34.5 MHz with half power beam widths of 26'/40' in the east-west and north-south directions, respectively. It is found that the observed brightness temperatures vary within the limits of 0.3x 106 K to 1.5 x 106 K

Observations of the 7 March, 1970 total
โœ John P. Hagen; Paul N. Swanson; Robert W. Haas; Fred L. Wefer; Raymond W. Vogt ๐Ÿ“‚ Article ๐Ÿ“… 1971 ๐Ÿ› Springer ๐ŸŒ English โš– 992 KB

The 7 March, 1970 total solar eclipse was observed at wavelengths of 3.2 and 8.3 mm; the object being to use the knife edge of the Moon as it passed across the Sun to improve angular resolution on the Sun. This in turn would provide a radial brightness distribution of the Sun with an angular resolut

Observation of the solar soft X-ray comp
โœ Richard G. Teske ๐Ÿ“‚ Article ๐Ÿ“… 1969 ๐Ÿ› Springer ๐ŸŒ English โš– 532 KB

Solar X-rays from 8 .12 ~ have been observed with an ion chamber photometer and fluxes derived from the observations after an assumption concerning the spectral distribution. The time variation of the X-ray flux correlates well with the radio flux, plagc index, and sunspot number. Comparisons of X-r