✦ LIBER ✦

Height of the slowly varying component of radio emission at 9.1 cm during the Quiet Sun Years

✍ Scribed by A. C. Riddle

Publisher: Springer
Year: 1969
Tongue: English
Weight: 226 KB
Volume: 6
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00150950

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

The slowly varying component of the sola

The slowly varying component of the solar radio emission around 1 cm wavelength

✍ Atsushi Tsuchiya 📂 Article 📅 1969 🏛 Springer 🌐 English ⚖ 378 KB

Slowly varying component spectrum of the

Slowly varying component spectrum of the solar radio emission at millimetre wavelengths

✍ V. A. Efanov; A. G. Kislyakov; I. G. Moiseev 📂 Article 📅 1972 🏛 Springer 🌐 English ⚖ 476 KB

The spectrum of the slowly varying compo

The spectrum of the slowly varying component of solar radio emission at wavelengths of 3.3 mm – 21 cm

✍ A. Tlamicha 📂 Article 📅 1968 🏛 Springer 🌐 English ⚖ 190 KB

The spectrum and diameter of the source of the S-component emission (McMath Plage No. 244) observed on March 4, 1968 has been investigated at 3.3 ram, 4.3 ram, 8.5 mm, 2 cm, 9.1 cm, 21 cm, and 43 cm wavelengths.

Observations on the slowly varying compo

Observations on the slowly varying component of solar radio emission at decameter wavelengths

✍ Ch. V. Sastry; R. K. Shevgaonkar; M. N. Ramanuja 📂 Article 📅 1983 🏛 Springer 🌐 English ⚖ 491 KB

Meter wavelength observations of the qui

Meter wavelength observations of the quiet sun and the slowly varying component during declining phase of the solar cycle

✍ P. Lantos; C.E. Alissandrakis 📂 Article 📅 1994 🏛 Elsevier Science 🌐 English ⚖ 407 KB

Observations and interpretation of the s

Observations and interpretation of the slowly varying component of solar radio emission at decameter wavelengths

✍ Ch. V. Sastry; K. S. Dwarkanath; R. K. Shevgaonkar; V. Krishan 📂 Article 📅 1981 🏛 Springer 🌐 English ⚖ 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