๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Observations of bright coronal points at wavelengths of 5.2 and 1.76 cm

โœ Scribed by V. P. Maksimov; D. V. Prosovetskii; B. B. Krissinel


Book ID
110126198
Publisher
Springer
Year
2001
Tongue
English
Weight
273 KB
Volume
27
Category
Article
ISSN
1063-7737

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Observations of preburst heating and mag
โœ Robert F. Willson ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Springer ๐ŸŒ English โš– 731 KB

The Very Large Array (VLA) has been used at 20 cm wavelength to study the evolution of a burst loop with 4" resolution on timescales as short as 10 s. The VLA observations show that the coronal loop began to heat up and change its structure about 15 rain betbre the eruption of two impulsive bursts.

Radio interferometric observations of so
โœ M. R. Kundu; P. E. Angerhofer ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 219 KB

Several solar active regions were observed during the 1976 vernal equinox with the 3-element interferometer of the National Radio Astronomy Observatory. The element spacings for these observations were 600, 2100, and 2700 m, resulting in maximum angular resolutions of about 3 arc sec at 3.7 cm and 8

High resolution observations of the chro
โœ M. Simon ๐Ÿ“‚ Article ๐Ÿ“… 1971 ๐Ÿ› Springer ๐ŸŒ English โš– 751 KB

High resolution observations of the Sun at 3.3 ram, 3.5 ram, 1.35 cm, and 1.95 cm which were obtained by tracking narrow beam width antennas on the lunar limb as it occulted the Sun are described. The observations indicate that: (1) the region emitting at these wavelengths is very irregular with typ