✦ LIBER ✦

High resolution observations of solar bursts at 3.7 and 11.1 cm wavelengths

✍ Scribed by C. E. Alissandrakis; M. R. Kundu

Publisher: Springer
Year: 1975
Tongue: English
Weight: 657 KB
Volume: 41
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00152963

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Radio interferometric observations of so

Radio interferometric observations of solar bursts at 3.7 and 11.1 cm wavelengths

✍ M. R. Kundu; P. E. Angerhofer 📂 Article 📅 1979 🏛 Springer 🌐 English ⚖ 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 polarimetry of the Sun a

High resolution polarimetry of the Sun at 3.7 and 11.1 cm wavelengths

✍ Kenneth R. Lang 📂 Article 📅 1977 🏛 Springer 🌐 English ⚖ 341 KB

Fine structure of a solar active region

Fine structure of a solar active region at 3.7 and 11.1 cm wavelengths

✍ M. R. Kundu; R. H. Becker; T. Velusamy 📂 Article 📅 1974 🏛 Springer 🌐 English ⚖ 698 KB

The three-element interferometer of the National Radio Astronomy Observatory was used to observe the Sun at 3.7 and 11.1 cm wavelengths during the period June 5-9, 1973. The baselines of the interferometer were 900, 1800 and 2700 meters, with maximum angular resolution of 3" at 3.7 and 9" at 11.1 cm

Fine structure of a solar flare region a

Fine structure of a solar flare region at 3.7 and 11.1 cm wavelengths

✍ M. R. Kundu; T. Velusamy; R. H. Becker 📂 Article 📅 1974 🏛 Springer 🌐 English ⚖ 273 KB

On June 9, 1973, a flare associated burst was observed with the NRAO 3-element interferometer at 3.7 and 11.1 cm wavelength. The burst was of 'gradual rise and fall' type. Comparing the fringe amplitudes at 3.7 cm to the visibility computed for model flare regions we found that the precursor data ar

High resolution observations of the chro

High resolution observations of the chromosphere at mm and cm wavelengths

✍ M. Simon 📂 Article 📅 1971 🏛 Springer 🌐 English ⚖ 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

High spatial resolution observations of

High spatial resolution observations of solar flares at 3.3 mm wavelength

✍ M.R. Kundu; S.M. White; W.J. Welch; J.H. Bieging 📂 Article 📅 1991 🏛 Elsevier Science 🌐 English ⚖ 498 KB