Observations of the temporal evolution of Saturn’s stratosphere following the Great Storm of 2010–2011 - I. Temporal evolution of the water abundance in Saturn’s hot vortex of 2011–2013

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Table 1

Summary of the Herschel-PACS observations of Saturn.

Window 1: July 2011

Date	OD	DOY2011	Obs. ID	Δt (s)	λ

2011-07-12 12:40:53	789	192	1342224015	5347	67.09 μm

Window 2: February 2012

Date	OD	DOY2011	Obs. ID	Δt (s)	λ

2012-02-02 00:05:21	994	397	1342238584	3259	66.44 μm
2012-02-02 21:33:59	995	398	1342238616	3259	67.09 μm

Window 3: July–August 2012

Date	OD	DOY2011	Obs. ID	Δt (s)	λ

2012-07-29 16:58:22	1173	576	1342248742	3259	66.44 μm
2012-08-10 17:50:26	1185	588	1342249394	3259	67.09 μm

Window 4: January–February 2013

Date	OD	DOY2011	Obs. ID	Δt (s)	λ

2013-01-30 03:19:45	1357	760	1342262558	3259	66.44 μm
2013-02-02 06:10:01	1360	763	1342262796	3259	67.09 μm

Notes. The given time corresponds to the start of the observation. OD means operational day, DOY2011 is the day number since 2011-01-01, Δt is the total integration time and λ the water line central wavelength.

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