𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Spectrum measurements of the sun near 1 cm wavelength

✍ Scribed by David H. Staelin; Norman E. Gaut; Sara E. Law; Woodruff T. Sullivan

Publisher
Springer
Year
1968
Tongue
English
Weight
80 KB
Volume
3
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Fine structure of the Sun at 1.3 cm wave
Fine structure of the Sun at 1.3 cm wavelength
✍ M. R. Kundu; T. Velusamy πŸ“‚ Article πŸ“… 1974 πŸ› Springer 🌐 English βš– 308 KB

The two-element interferometer at Hat Creek Observatory was used at 1.3 cm wavelength to study the fine structure of the radio emissive regions on the Sun. Observations of the quiet Sun at 1.3 cm show sudden changes in the fringe amplitude and phase, lasting for typically about 5-8 min. Assuming tha

The Ethylene Hot Band Spectrum near 3000
The Ethylene Hot Band Spectrum near 3000 cmβˆ’1
✍ Jos Oomens; JΓΆrg Reuss; Georg Ch. Mellau; Stefan Klee; Iwona Gulaczyk; AndrΓ© Fay πŸ“‚ Article πŸ“… 1996 πŸ› Elsevier Science 🌐 English βš– 547 KB

A new hot band spectrum of ethylene has been recorded from 2970 to 3015 cm 01 at low rotational temperatures in a seeded molecular jet, using vibrational energy transfer from SF 6 to C 2 H 4 . An IR-IR double resonance technique has been applied to pump the lower states and subsequently probe the ho

Determination of the decameter wavelengt
Determination of the decameter wavelength spectrum of the quiet Sun
✍ W. C. Erickson; T. E. Gergely; M. R. Kundu; M. J. Mahoney πŸ“‚ Article πŸ“… 1977 πŸ› Springer 🌐 English βš– 402 KB

The Teepee Tee array of the Clark Lake Radio Observatory has been used to compare the flux of the Sun with that of the sidereal sources Tau A and Vir A at several frequencies in the range 109.0-19.0 MHz. Only the two central banks of the E-W arm of the array were used as elements of a phase switched