The spectrum and position of solar noise storms at decameter wavelengths
| Autor: | J. De La Noe, T. E. Gergely |
|---|---|
| Rok vydání: | 1977 |
| Předmět: |
Physics
Solar flare Astrophysics::High Energy Astrophysical Phenomena Astronomy Balmer series Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Solar physics symbols.namesake Space and Planetary Science symbols Arecibo Observatory Emission spectrum Spectrograph Astrophysics::Galaxy Astrophysics Noise (radio) Radio astronomy |
| Zdroj: | Solar Physics. 55:195-209 |
| ISSN: | 1573-093X 0038-0938 |
| Popis: | Decametric storm radiation during the period July-August 1970 has been observed simultaneously with a high sensitivity spectrograph at Arecibo Observatory and with the log-periodic, swept-frequency array of the Clark Lake Radio Observatory. The observations complement each other; different types of fine structure emissions can be easily identified on the spectrograph records and their position can be determined from the swept-frequency recordings. The relative positions of the different emissions which have been observed during the storms are studied. Four distinct sources appear to be present. The continuum emission, the type I bursts and the flare-related type III's are all emitted at different locations. The storm type III bursts, type IIIb's and drift pairs overlap in position, but appear at different locations than the previously mentioned sources. |
| Databáze: | OpenAIRE |
| Externí odkaz: |
|
Full text from SpringerLink