A numerical model of cometary dust coma structures - Application to comet 9P/Tempel 1

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Volume 512 (March-April 2010)

A&A, 512 (2010) A60

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Table 1:

Observations Logs.
Date	r (AU)	$\Delta$ (AU)	PsAng ( $^\circ$ )	A ( $^\circ$ )	B ( $^\circ$ )	D ( $^\circ$ )	E ( $^\circ$ )	F ( $^\circ$ )	G ( $^\circ$ )	I ( $^\circ$ )
2005-Jul.-19	1.512461	0.978627	109	40	110	180	225	ND	285	330
2005-Jul.-26	1.520488	1.024132	108	45	108	185	225	250	285	330
2005-Aug.-02	1.531667	1.073375	107	55	108	175	210	ND	285	335
2005-Aug.-08	1.543674	1.118653	106	45	105	185	230	260	285	335

Notes. Identification of the coma structures as shown in Figs. 3 and 4. The given position angles refer to the center lines of the structures and may have an uncertainty of maximum $\pm10^\circ$ . North = 0 $^\circ$ , East = +90 $^\circ$ . PsAng is the position of the extended Sun-Comet vector. ND = not detected.

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