Evidence for short-term variability of Jupiter's decimetric emission from VLA observations

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Table 1:

VLA 2002 observational time schedule and approximate CML coverage (Sect. 2).
Month	Day	Time (UT)	CML range ( $^\circ$ )
October	28 ${\rm th}$	12:00 to 14:30	[345; 75]
November	1 ${\rm st}$	10:00 to 12:10	[154; 232]
November	5 ${\rm th}$	08:00 to 19:30	All
November	8 ${\rm th}$	10:00 to 12:00	[127; 200]
November	10 ${\rm th}$	10:45 to 13:00	[96; 177]
November	11 ${\rm th}$	16:40 to 19:00	[101; 185]
November	21 ${\rm th}$	17:20 to 19:20	[190; 263]
December	4 ${\rm th}$	10:00 to 12:30	[82; 173]
December	11 ${\rm th}$	09:45 to 12:30	[47; 147]

Source LaTeX | All tables | In the text

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