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• W2127029333 endingPage "39" @default.
• W2127029333 startingPage "39" @default.
• W2127029333 abstract "We report observations of circularly polarized emission from the solar corona at 77 MHz during the periods 2006 August 11–18, 2006 August 23–29, and 2007 May 16–22 in the minimum phase between the sunspot cycles 23 and 24. The observations were carried out with the east–west one-dimensional radio polarimeter at the Gauribidanur observatory located about 100 km north of Bangalore. Two-dimensional imaging observations at 77 MHz during the same period with the radioheliograph at the same observatory revealed that the emission region co-rotated with the Sun during the three aforementioned periods. Their rotation rates, close to the central meridian on the Sun, are 46, 52, and 49 ± 05 per day, respectively. We derived the radial distance of the region from the above observed rotation rates and the corresponding values are ≈1.24 ± 0.03 R☉ (2006 August 11–18), ≈1.40 ± 0.03 R☉ (2006 August 23–29), and ≈1.32 ± 0.03 R☉ (2007 May 16–22). The estimated lower limit for the magnetic field strength at the above radial distances and periods are ≈1.1, 0.6, and 0.9 G, respectively." @default.
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• W2127029333 date "2011-05-24" @default.
• W2127029333 modified "2023-10-16" @default.
• W2127029333 title "LOW-FREQUENCY OBSERVATIONS OF POLARIZED EMISSION FROM LONG-LIVED NON-THERMAL RADIO SOURCES IN THE SOLAR CORONA" @default.
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• W2127029333 doi "https://doi.org/10.1088/0004-637x/734/1/39" @default.
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