CHRIS/Proba Meeting Summary - ESA/ESTEC
CHRIS/Proba Meeting Summary - ESA/ESTEC
4-5-July-2000
Synopsis
This meeting brought together the PIs for the CHRIS/Proba mission to
finalise PIs data acquisition requirements and to discuss various
logistical aspects of the mission.
About 50 scientists attended the meeting. The first morning
consisted of overview talks on Proba, on the CHRIS instrument and on
the major scientific aims of the mission - land studies and aerosol
studies. Most of the important discussion centred on the
configuration of the mode of operation of the instrument (no. of views
x no. of bands x spatial resolution), on the data acquisition
schedule, and on the calibration of the instrument (radiometric,
wavelength and other issues).
The afternoon consisted of break-out sessions on aerosol & cal/val studies,
land studies (agriculture), forestry and water quality studies. I
presented two talks in the aerosol & cal/val group ( on behalf of
Grant and Mitchell) and two talks in the land group (on behalf of
Cudahy and Huntington).
The second morning was used by the group leaders (Settle for
aerosols & cal/val; Barnsley for land, Fletcher for forestry, for
the coastal and Lavendar for the inland water group) to
summarise the previous afternoon's discussions and to discuss the issues
raised in the break-out groups amongst the whole group.
The meeting finished at 12:30 on 5 July. A closed session meeting
was held in the afternoon for the Steering Committee to review recommendations and reconsider the
data acquisition plan. PIs were not invited to attend this meeting.
Main Discussion Points
- [1] PIs were asked to complete a Data Acquisition
Details pro-forma and return this to Mike Barnsley. These forms
must be completed by all PIs who have responsibilities for
CHRIS sites. I have done
this for the Grant proposal and given the forms to Mitchell, Cudahy
and Huntington for them to complete.
- [2] The data acquisition schedule will be a complex task and
there are bound to be compromises and restrictions. The nominal
data capture rate is 5 images per day, and this is determined largely
by the availability of power on board Proba. Thus, PIs are unlikely
to get all of their requested image acquisitions.
- [3] The mission lifetime is 12 months. However, it is
anticipated that 4 months will be required for instrument
validation, thus only 8 months of earth imaging will be available.
Preliminary scheduling gives 1282 images for 282 days.
- [4] Wavelength calibration is to be done using the 760 nm
Oxygen absorption feature (A-band), but other possibilities were
discussed (e.g. using Fraunhofer lines or water vapour features).
- [5] Tests sites were designated in 3 categories - core
sites, additional sites and reserve sites. It was hoped that some
rationalisation of these sites would occur due to the paucity of
data acquisitions.
- [6] Sites for calibration apparently have not been considered
in detail previously. At
my urging it was recommended that the images of the Libyan desert and Railroad
valley be acquired for relative and absolute radiometric
calibration. Some animated discussion occurred about the utility
of the Libyan desert site as its BRDF is not measured and there was
some uncertainty concerning the uniformity of the site at 25 m
resolution. Discussion ensued concerning using other satellite
instruments to calibrate CHRIS by imaging the same sites and by
imaging the Greenland ice-sheet, the Antarctic plateau or high,
dense clouds.
- [7] Several band configurations were suggested by various PIs
and all PIs were encouraged to think about band selections
carefully. PIs were discouraged to suggest too many variants as
this would complicate the programming of the instrument. I
suggested that all band configurations should include a water vapour band (936 nm)
and aerosol bands for atmospheric correction. Wavelength
calibration will be done only a few images and the analyses will be
used to correlate the results with the detector temperature. The
detector temperature will then be used on all other images to
characterise the wavelength shifts.
- [8] The pointing accuracy of the instrument was quoted as 0.1
degrees resulting in a pixel location accuracy of ±2 km and satellite
positional errors were thought to be of similar accuracy.
Collocation of the images and absolute navigational accuracy were
issues common to all proposals and these are being addressed.
- [9] Mike Barnsley has agreed to set up four electronic
discussion fora for the mission. The topics will be:- (a)
General, (b) Land applications, (c) Aerosols, and (d) Coastal and
Inland Water. PIs will be informed by email about the address
details of the sites.
- [10] There were uncertainties in knowing the precise number of
days required by the mission operators for data acquisition
programming. Some thought has been given to using weather forecast
information to schedule CHRIS image acquisitions.
- [11] Details of the mission and updates can be found at:
www.chris-proba.org.uk
Fred Prata
6 July, 2000.
File translated from TEX by TTH, version 2.25.
On 11 Jul 2000, 23:53.