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.
Polarization of solar active regions at 9.5 mm wavelength
โ Scribed by M. R. Kundu; T. P. McCullough
- Publisher
- Springer
- Year
- 1972
- Tongue
- English
- Weight
- 592 KB
- Volume
- 24
- Category
- Article
- ISSN
- 0038-0938
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