Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...55..195d&link_type=abstract
Solar Physics, vol. 55, Nov. 1977, p. 195-209. Research supported by the International Astronomical Union
Astronomy and Astrophysics
Astronomy
6
Decametric Waves, Noise Storms, Solar Radio Bursts, Solar Spectra, Type 3 Bursts, Fine Structure, Position (Location), Radio Astronomy, Solar Activity Effects
Scientific paper
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.
de La Noë Jérôme
Gergely Tomas E.
No associations
LandOfFree
The spectrum and position of solar noise storms at decameter wavelengths does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The spectrum and position of solar noise storms at decameter wavelengths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The spectrum and position of solar noise storms at decameter wavelengths will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1133093