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

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Table 4:

Variability and location of the emission peaks at 6-cm wavelength (Sect. 4).
	EAST LOBE	WEST LOBE
CML ( $^\circ$ )	Emission peak $\lambda_{\rm III}$ ( $^\circ$ )	Emission Peak $\lambda_{\rm III}$ ( $^\circ$ )
070	Increase^* $160 \pm\Delta\varphi$	Decrease $340 \pm\Delta\varphi$
120	Decrease^* $210 \pm\Delta\varphi$	Increase $030 \pm\Delta\varphi$
250	Decrease $340 \pm\Delta\varphi$	Increase^* $160 \pm\Delta\varphi$
270	Increase $000 \pm\Delta\varphi$	Decrease^* $180 \pm\Delta\varphi$
300	Stable $030 \pm\Delta\varphi$	Increase^* $210 \pm\Delta\varphi$
340	Decrease $070 \pm\Delta\varphi$	Increase^* $250 \pm\Delta\varphi$

^* Side of the planet where the significant changes were located.

Source LaTeX | All tables | In the text

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