The Very Large Array (VLA) and the Nancay Radioheliograph (NR) can be used in the 1990s to provide unique observations of the quiescent and active corona. The combined data can specify the evolution and magnetic structure at a variety of heights in the quiescent corona, from compact to extended structures such as loops, streamers and coronal holes. The scientific potential of simultaneous VLA-NR research is illustrated by observations of solar noise storms with hitherto unavailable resolution in space (VLA) and time (NR). Unique information will also be provided for other types of solar bursts, leading to an improved understanding of solar activity during the coming maximum.
High resolution VLA-Nancay observations of the sun
Advances in Space Research ; 8 , 11 1
1988-01-01
Sonstige
Keine Angabe
Englisch
High resolution VLA-Nancay observations of the sun
Elsevier | 1989
|The Nancay multifrequency radioheliograph: New observations
Elsevier | 1989
|SETI at the Nançay radiotelescope
Elsevier | 1983
|WIND/3DP and Nancay Radioheliograph Observations of Solar Energetic Electron Events
British Library Conference Proceedings | 2003
|WIND-3DP and Nancay radioheliograph observations of solar energetic electron events
Online Contents | 2003
|