Chris / Proba
This web page describes the CHRIS/PROBA satellite sensor

CHRIS/PROBA ACQUISITIONS

CHRIS (Compact High Resolution Imaging Spectrometer) is a physically compact payload as its name implies (weighing under 15 kg) and operates in the 'push-broom' mode. Its main applications will be in environmental monitoring, forestry inventory and precision farming.

From a 600 km orbit, CHRIS can image the Earth in a 14 km swath with a spatial resolution of 18 m (this is somewhat variable as the altitude varies around the orbit). Using PROBA's agile steering capabilities in along and across track directions enables observation of selectable targets well outside the nominal field of view of 1.3º. Images will generally be acquired in sets of 5, these being taken at along track angles of ± 55 degrees, ± 36 degrees, and as close to nadir as possible.

CHRIS operates over the visible/near infrared band from 400 nm to 1050 nm and can operate in 63 spectral bands at a spatial resolution of 36m, or with 18 bands at full spatial resolution. Spectral sampling varies from 2-3 nm at the blue end of the spectrum, to about 12 nm at 1050nm. Sampling is about 7nm near the red edge (~690-740nm). The instrument is very flexible and different sets of bands can be used for different applications.

Figure 2.1. Illustration of how CHRIS can hold a target in view by using PROBA's pitch control.


Key Characteristics:

Spatial sampling interval
18m on ground at nadir
Image area
14 km X 14 km (748 X 748 pixels)
Number of images
Nominal is 5 downloads at different view angles
Data per image(for a 14x14 km2)
131 Mbits
Spectral range
410nm to 1050 nm
Number of spectral bands
19 bands at a spatial resolution of 18m
63 bands at a spatial resolution of 36m
Spectral resolution
1.3 nm @ 410nm to 12 nm @ 1050nm (i.e it varies across the spectrum)

 

Programmable operation:

Across track pixel size
18m or 36m
Along track pixel size
finest resolution is 18m but can be made coarser by changing the integration time
Spectral
variable bandwidth and band location
Digitisation
12 bits
Signal-to-noise ratio
200 @ a target albedo of 0.2

Table 2.1. Key characteristics of CHRIS/PROBA.

-55°

+55°

-36°

+36°  

 

Figure 2.2. The different five CHRIS-PROBA acquired images (16/07/04) overlaped to LANDSAT image (17/07/04) over the Barrax test site studied during SPARC-2004 campaign.

 CHRIS-PROBA programmed acquisitions:

 Table 2.2. CHRIS-PROBA acquisition programmed during the SEN2FLEX Mission 1 campaign

Date

Time

Satellite Zenith Angle

Solar Zenith Angle

29 May

11:29

-20

19

5 June

11:12

16

20

6 June

11:24

-10

19

 

 Table 2.3. CHRIS-PROBA acquisition programmed during the SEN2FLEX Mission 2 campaign.

Date

Time

Satellite Zenith Angle

Solar Zenith Angle

10 July

11:25

-17

 

17 July

11:08

20

 

 

Figure 2.3. CHRIS/PROBA quicklook from the image acquired at 20/05/2005.

For more information, please visit the CHRIS-on-PROBA Mission Web Page:

http://www.chris-proba.org.uk

 



•• by GPDS GroupUniversity of Valencia (Spain) ••
•• Last Updated: July 29th - 14:40h LT ••