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- W2108245852 abstract "We carried out radio observations of the solar corona in the frequency range 109–50 MHz during the annular eclipse of 2010 January 15 from the Gauribidanur Observatory, located about 100 km north of Bangalore in India. The radio emission in the above frequency range originates typically in the radial distance range ≈1.2–1.5 R☉ in the undisturbed solar atmosphere. Our analysis indicates that (1) the angular size of the smallest observable radio source (associated with a coronal mass ejection in the present case) is ≈1' ± 03, (2) the source size does not vary with radial distance, (3) the peak brightness temperature of the source corresponding to the above size at a typical frequency like 77 MHz is ≈3 × 109 K, and (4) the coronal magnetic field near the source region is ≈70 mG." @default.
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- W2108245852 date "2011-12-22" @default.
- W2108245852 modified "2023-09-30" @default.
- W2108245852 title "HIGH ANGULAR RESOLUTION RADIO OBSERVATIONS OF A CORONAL MASS EJECTION SOURCE REGION AT LOW FREQUENCIES DURING A SOLAR ECLIPSE" @default.
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- W2108245852 doi "https://doi.org/10.1088/0004-637x/744/2/165" @default.
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