| Autor: |
Sheridan, K. V., Labrum, N. R., Payten, W. J., Nelson, G. J., Hill, E. R. |
| Zdroj: |
Solar Physics; February 1983, Vol. 83 Issue: 1 p167-177, 11p |
| Abstrakt: |
The Culgoora radioheliograph has been modified for observing at 327.4 MHz, which is in addition to the three frequencies (43.25, 80, and 160 MHz) previously available. At the new frequency the array beamwidth is 56?, which represents the highest resolution yet available for metre-wavelength solar mapping. |
| Databáze: |
Supplemental Index |
| Externí odkaz: |
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