Two-engine aircraft suitable for large areas
One- and two-engine aircraft dedicated to smaller areas
Ultralight and cheap platforms for small areas with short processing time
Helicopters dedicated to linear objects
UAVs as support for field measurements
We are currently implementing projects all over Europe using our own fleet of 8 aircraft. During the high season, the number of planes and helicopters in the air grows even up to 12. Each of them is equipped with appropriate navigation, stabilisation and sensor mounting systems.
Our base, as well as hangar and office infrastructure, is located at the Rzeszów Jasionka Airport.
We use three large-format photogrammetric cameras – from Hexagon and Vexcel.
Medium-format cameras, with matrices above 50 MPix, are mounted, either individually or as various integrated sets, on most of our aerial platforms.
Currently, we own more than twenty medium-format cameras.
Our adventure with ALS was from the very beginning associated with Riegl – and we have carried it on ever since. We currently own seven systems made by this company.
Our scanners also work with hyperspectral, thermal, oblique and vertical cameras in multi-sensor configurations.
Since 2015, we have been collecting hyperspectral data with the help of a unique configuration of 3 HySpex scanners by the Norwegian company, NEO. This translates into high spatial resolution data for the full spectral range of. 400 – 2500 nm.
For aerial thermography, we use thermal cameras working within LWIR and MWIR bands. Precisely stabilized lenses and cooled sensor allow detecting temperatures with an accuracy of 1°C, and the ultra-fast matrix, even if not stabilized, produces sharp and clear images. High resolution above 1MPix ensures even 10-cm GSD, where the accuracy an orthophoto amounts to 1 pixel. With a set of several cameras we are able to obtain both vertical and oblique imagery in one flight.
It happens quite often that our projects involve mapping of hard-to-reach areas. To support field measurements and increase flexibility we have been using unmanned aerial vehicles (UAVs).
Multisensor aerial platform is our original design for simultaneous recording of hyperspectral and lidar data, and high-resolution RGB imagery. Our platform gets constantly expanded in order to find room for more sensors – we are already carrying out flight campaigns with an extra thermal camera.
The applied idea of instrument fusion guarantees a synergy between complementary types of data. Products that we deliver are based on data from the multisensor platform and comprehensive analyses aided by data fusion.
The platform was created as part of the R&D project: ‘The innovative approach supporting monitoring of non-forest Natura 2000 habitats, using remote sensing methods’, cofounded by the National Centre for Research and Development in Poland as part of the BIOSTRATEG II strategic program for research and development work ‘Natural environment, agriculture and forestry’.
Constellation | SuperView |
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Spatial resolution |
0,5 m - PAN band 2 m - MS bands |
Spectral bands |
PAN: 450-890 nm Blue: 450-520 nm Green: 520-590 nm Red: 630-690 nm Near-infrared: 770-890 nm |
Radiometric resolution | 11 bit |
Revisit time | daily |
Swath width | 12 km |
The number of satellites | 4 |
Constellation | Jilin |
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Spatial resolution |
0,5 m - PAN band 2 m - MS bands |
Spectral bands |
PAN: 450-800 nm Blue: 450-510 nm Green: 510-580 nm Red: 630-690 nm Near-infrared: 770-895 nm |
Radiometric resolution | 12 bit |
Revisit time | daily (together with Jilin Stereo and Jilin GXA) |
Swath width | 136 km |
The number of satellites | 2 |
Constellation | GaoFen |
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Spatial resolution |
0.65 m - PAN band 2.6 m - MS bands |
Spectral bands |
PAN: 450-900 nm Blue: 450-520 nm Green: 520-590 nm Red: 630-690 nm Near-infrared: 770-890 nm |
Radiometric resolution | 10 bit |
Revisit time | 5 days |
Swath width | 20 km |
The number of satellites | 1 |
Constellation | Jilin |
---|---|
Spatial resolution |
0.72 m - PAN band 2.88 m - MS bands |
Spectral bands |
PAN: 500-800 nm Blue: 450-520 nm Green: 520-600 nm Red: 630-690 nm Near-infrared: 700-800 nm |
Radiometric resolution | 10 bit |
Revisit time | daily (together with Jilin Stereo and EarthScanner) |
Swath width | 11.6 km |
The number of satellites | 1 |
Constellation | Jilin |
---|---|
Spatial resolution |
0.75 m - PAN band 3 m - MS bands |
Spectral bands |
PAN: 450-900 nm Blue: 450-510 nm Green: 510-580 nm Red: 630-690 nm Near-infrared: 7700-895 nm |
Radiometric resolution | 12 bit |
Revisit time | daily (together with Jilin GXA and EarthScanner) |
Swath width | 40 km |
The number of satellites | 2 |
Constellation | Jilin |
---|---|
Spatial resolution |
0.92/1.21 m - Night Image Color Video & Stereo |
Radiometric resolution | 8 bit |
Revisit time | 3 times per day |
Swath width | 11x4.5 km/19x4.5 km/14.4x6 km |
The number of satellites | 9 |
Constellation | Jilin |
---|---|
Spatial resolution |
0.98 / 1.06 m - PAN band 3.92/4.24 m - MS bands |
Spectral bands |
PAN: 470-700 nm Blue: 450-510 nm Green: 510-580 nm Red: 630-690 nm Near-infrared: 770-895 nm |
Radiometric resolution | 12 bit |
Revisit time | Two times a day |
Swath width | 17/18.5 km |
The number of satellites | 10 |
Constellation | GaoFen |
---|---|
Spatial resolution |
0.8 m - PAN band 3.24 m - MS bands |
Spectral bands |
PAN: 450-900 nm Blue: 450-520 nm Green: 520-590 nm Red: 630-690 nm Near-infrared: 770-890 nm |
Radiometric resolution | 10 bit |
Revisit time | 5 days |
Swath width | 45 km |
The number of satellites | 1 |
Constellation | GaoFen |
---|---|
Spatial resolution |
2 m - PAN band 8 /16 m - MS bands |
Spectral bands |
PAN: 450-900 nm Blue: 450-520 nm Green: 520-590 nm Red: 630-690 nm Near-infrared: 770-890 nm |
Radiometric resolution | 10 bit |
Revisit time | daily |
Swath width | 60/830/850 km |
The number of satellites | 5 |
Constellation | ZY Tri |
---|---|
Spatial resolution |
2.1 m - PAN band 5.8 m - MS bands |
Spectral bands |
PAN: 500-800 nm Blue: 450-520 nm Green: 520-590 nm Red: 630-690 nm Near-infrared: 770-800 nm |
Radiometric resolution | 10 bit |
Revisit time | 3 days |
Swath width | 51 km |
The number of satellites | 3 |
Constellation | CBERS |
---|---|
Spatial resolution |
5 m - PAN band 10 m - MS bands 80 m - TIR band |
Spectral bands |
PAN: 510-730 nm Green: 520-590 nm Red: 630-690 nm Near-infrared: 770-890 nm TIR: 10.4-12.5 nm |
Radiometric resolution | 10 bit |
Revisit time |
3 days 26 days (TIR band) |
Swath width | 120 km |
The number of satellites | 1 |
Constellation | Jilin |
---|---|
Spatial resolution |
5 m - bands B0~B6 (nadir) 10 m - bands B7~B12 (nadir) 20 m - bands B13~B19 (nadir) 3 m - bands B3~B5 (nadir) 100 m - bands SW1~SW4, MWIR (nadir) 150 m - band LWIR |
Spectral bands |
B0-B19: 450-1040nm SW1:1195-1225nm; SW2:1360-1390nm; SW3:1550-1590nm; SW4:1610-1690nm; MWIR:3700nm~4950nm; LWIR: 7500nm~13500nm |
Radiometric resolution |
B0~B19: 12 bits; SW1~4,MWIR,LWIR: 14bit |
Revisit time | 2 days |
Swath width | 110 km |
The number of satellites | 2 |
Constellation | GaoFen |
---|---|
Spatial resolution | 1/3/5/10/25/50 m |
Polarization | HH VV HV VH |
Radiometric resolution | 8 bit |
Revisit time | 3 days |
Swath width | 10 - 650 km |
The number of satellites | 1 |
Constellation | GaoFen |
---|---|
Spatial resolution |
50m PAN & MS, 400m MW |
Spectral bands |
PAN: 450-900 nm Blue: 450-520 nm Green: 520-600 nm Red: 630-690 nm Near-infrared: 760-890 nm Mid-wave infrared: 35000-41000 nm |
Radiometric resolution | 16 bit |
Revisit time | 20 s (shooting interval) |
Swath width | 400 km |
The number of satellites | 1 |
Instrument | Dove | Dove-R | SuperDove |
---|---|---|---|
Constellation | PlanetScope | PlanetScope | PlanetScope |
Spatial resolution | 3,7 m MS | 3,7 m MS | 3,7 m MS |
Spectral bands |
Blue: 455 - 515 nm Green: 500 - 590 nm Red: 590 - 670 nm NIR: 780 - 860 nm |
Blue: 464 - 517 nm Green: 547 - 585 nm Red: 650 - 682 nm NIR: 846 - 888 nm |
Coastal Blue 431-452 nm* Blue: 465-515 nm Green I: 513. - 549 nm Green II: 547. - 583 nm* Yellow: 600-620 nm* Red: 650 - 680 nm Red-Edge: 697 - 713 nm NIR: 845 - 885 nm (* after) |
Radiometric resolution | 12 bit | ||
Revisit time | daily | ||
Swath width | 24 km x 8 km | 24 km x 16 km | 32.5 km x 19.6 km |
The number of satellites | 130 |
Instrument | SkySat 1-2 | SkySat 3-15 | SkySat 16-21 | ||||||
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Constellation | SkySat | SkySat | SkySat | ||||||
Spatial resolution |
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Spectral bands |
PAN: 450 - 900 nm Blue: 450 - 515 nm Green: 515 - 595 nm Red: 605 - 695 nm NIR: 740 - 900 nm |
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Radiometric resolution | 16 bit | ||||||||
Revisit time | 4-5 days | ||||||||
Swath width | 5.9 km | ||||||||
The number of satellites | 21 |
Constellation | RapidEye |
---|---|
Spatial resolution |
6.5 m MS, 5 m for ortho |
Spectral bands |
Blue: 440-510 nm Green: 520-590 nm Red: 630-685 nm Red-Edge: 690-730 nm Near-infrared: 760-850 nm |
Radiometric resolution | 12 bit |
Revisit time | daily* *off-nadir |
Swath width | 77 km |
The number of satellites | 5 |
In order to efficiently obtain field data, bearing in mind the need for very precise measurements, we came up with our ownsystem supporting data collection - Nautilus. It consists of a field capture equipment, database and reporting module. Each set has a special antenna that helps locate objects in the area with a centimetre-level accuracy.
The system can be adjusted to specific collections and measure desired parameters which are entered in the form of dictionary-based attributes by the operator. It also allows for creation of photographic documentation. All captured data is transferred in real time to the online database where it is collected, stored and verified. Quality control is also real-time, thanks to dedicated programming solutions (mainly proprietary code in Python and SQL). Thanks to this solution, all errors are reported back straight to the operator and can be immediately corrected, before the field campaign is finished.
We configured our system so that it can work round the clock.
Our multipurpose web platform for publication and analysis of collected data has been successfully used in both urban and natural environment.
Its biggest advantages are:
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