Pozyskiwanie i przetwarzanie danych lotniczych i satelitarnych przez zespół badawczy Zakładu Teledetekcji Instytutu Lotnictwa

Czapski, Paweł; Dorosz, K.; Kacprzak, Mariusz; Korniluk, Tomasz; Kotlarz, Jan; Mazur, Anna; Mrowiec, Karol; Mruk, K.; Pieniążek, Janusz; Pośpieszczyk, Agnieszka; Rotchimmel, Karol; Wodziński, Konrad; Zalewska, Natalia

doi:10.15199/50.2016.3.1

Cited by 2 publications

(1 citation statement)

References 4 publications

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“…Over the next few years, the Space Technology Center was established, which in 2017 employs 80 employees implementing projects under four plants. The Department of Remote Sensing is involved in works that include both image acquisition and operational processing [1,2,3,5]. Photographs are made with the use of commercial equipment and the Multispectral System (6-ranges) developed for the needs of the HESOFF project.…”

Section: Meteor 1 Rocket and Meteor 2k Rocketmentioning

confidence: 99%

Space technology at the Institute of Aviation

Loroch

Okniński

Rarata

et al. 2018

TO - PK

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This paper gives a brief summary of the Institute of Aviation's activities in space technology. Review of historical achievements and latest developments are described. Scope of present work of Space Technology Center and key projects are discussed, that include rocket and satellite technologies. Importance of space technologies in Institute of Aviation's development strategy and their crucial role for safety and independence of the state is underlined. Possibilities and future use of the developed technologies are pointed out.

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Section: Meteor 1 Rocket and Meteor 2k Rocketmentioning

confidence: 99%

Space technology at the Institute of Aviation

Loroch

Okniński

Rarata

et al. 2018

TO - PK

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The Possibility of Ultraviolet Enceladus’ Observations from Stratospheric Balloons

Kotlarz¹,

Zalewska

2019

Transactions on Aerospace Research

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Stratospheric balloons are very important sources for space and terrestrial observation experiments in many disciplines. Instruments developed for astrophysical measurements are usually reusable. It is also possible to observe both hemispheres including observations from the polar and equatorial regions for thirty days or even longer. On the other hand the UV atmospheric transmittance window was used for the astrophysical observations less often than visible optical bands. At the end of the 2017 there are a few scientific groups working on near-UV or UV spectrographs and cameras for balloon flights. In this paper we are discussing the possibility of ultraviolet measurement of Enceladus, an icy Saturnian moon, surface reflectance between 200 and 400 nm from the 20-50 km altitudes. At visible and near infrared optical channels Enceladus’ reflectance is very high (near 1.0). This value is consistent with a surface composed of water ice, however at some ultraviolet wavelengths Enceladus reflectance is lower than it would be expected for this type of surface. The scientific research done in the last decade was focused on H2O, NH3, and tholin particles detection on the Enceladus’ surface as a reason of low UV reflectance phenomenon. Continuous observation of Enceladus’ UV reflectance variability from stratospheric balloons may be interesting and may give us the proof of the presence of biomarkers or/and tholin particles.

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Pozyskiwanie i przetwarzanie danych lotniczych i satelitarnych przez zespół badawczy Zakładu Teledetekcji Instytutu Lotnictwa

Cited by 2 publications

References 4 publications

Space technology at the Institute of Aviation

Space technology at the Institute of Aviation

The Possibility of Ultraviolet Enceladus’ Observations from Stratospheric Balloons

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