𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Diffuse Component Spectra of Solar Active Regions at Submillimeter Wavelengths

✍ Scribed by Adriana V. R. Silva; Tatiana F. Laganá; C. Guillermo Gimenez De Castro; Pierre Kaufmann; Joaquim E. R. Costa; Hugo Levato; Marta Rovira

Book ID
106532221
Publisher
Springer
Year
2005
Tongue
English
Weight
362 KB
Volume
227
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Polarization of solar active regions at
Polarization of solar active regions at 3.5 millimeter wavelength
✍ M. R. Kundu; T. Gergely 📂 Article 📅 1973 🏛 Springer 🌐 English ⚖ 432 KB

A study of the circular polarization structure of solar active regions has been made from data obtained at 3.5 mm wavelength, using the 36 ft diameter radio telescope of the National Radio Astronomy Observatory at Kitt Peak, Arizona. The angular resolution of the telescope at this wavelength is 1:2.

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