Pawel Lejba

Dr. Pawel Lejba

orcid

Research Focus & Metrics

Academic Career Length

20Years (2007-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

View All Publications
4 October 2017 in Earth and Space Science
Verified
Journal Article
Open access
PDF file
DKD. Kucharski
D. Kucharski
GKG. Kirchner
G. Kirchner
JBJ. C. Bennett
J. C. Bennett
MLM. Lachut
M. Lachut
KSKrzysztof Sośnica
Krzysztof Sośnica
TST. Suchodolski
T. Suchodolski
The (TOPography EXperiment) TOPEX/Poseidon (T/P) altimetry mission operated for 13 years before the satellite was decommissioned in January 2006, becoming a large space debris object at an altitude of 1,340 km. Since the end of the mission, the interaction of T/P with the space environment has driven the satellite's spin dynamics. Satellite laser ranging (SLR) measurements collected from June 2014 to October 2016 allow for the satellite spin axis orientation to be determined with an accuracy of 1.7°. The spin axis coincides with the platform yaw axis (formerly pointing in the nadir direction) about which the body rotates in a counterclockwise direction. The combined photometric and SLR data collected over the 11 year time span indicates that T/P has continuously gained rotational energy at an average rate of 2.87 J/d and spins with a period of 10.73 s as of 19 October 2016. The satellite attitude model shows a variation of the cross‐sectional area in the Sun direction between 8.2 m2 and 34 m2. The direct solar radiation pressure is the main factor responsible for the spin‐up of the body, and the exerted photon force varies from 65 μN to 228 μN around the mean value of 138.6 μN. Including realistic surface force modeling in orbit propagation algorithms will improve the prediction accuracy, giving better conjunction warnings for scenarios like the recent close approach reported by the ILRS Space Debris Study Group—an approximate 400 m flyby between T/P and Jason‐2 on 20 June 2017.


1 May 2018 in Advances In Space Research
Verified
Journal Article
Closed access
PLPawel Lejba
Pawel Lejba
TSTomasz Suchodolski
Tomasz Suchodolski
PMPiotr Michałek
Piotr Michałek
JBJacek Bartoszak
Jacek Bartoszak
Stanislaw SchillakStanislaw Schillak
Stanislaw Schillak
SZStanisław Zapaśnik
Stanisław Zapaśnik

23 January 2021 in Sensors
Verified
Journal Article
Open access
PDF file
Stanislaw SchillakStanislaw Schillak
Stanislaw Schillak
PLPawel Lejba
Pawel Lejba
PMPiotr Michałek
Piotr Michałek
The LARES (LAser RElativity Satellite) was built by the Italian Space Agency (ASI) and launched on 13 February 2012 by the European Space Agency. It is intended for studying the Lense–Thirring effect resulting from general relativity as well as for geodynamic studies and satellite geodesy. The satellite is observed by most ground laser stations. The task of this work is to determine the station coordinates and to assess the quality of their determination by comparison with the results from the LAGEOS-1 and LAGEOS-2 satellites. Observation results in the form of normal points (396,105 normal points in total) were downloaded from the EUROLAS Data Center for the period from 29 February 2012 to 31 December 2015. Seven-day orbital arcs were computed by the NASA GSFC GEODYN-II software, determining the coordinates of seventeen selected measuring stations. The average Root Mean Square (RMS) (15.1 mm) of the determined orbits is nearly the same as for LAGEOS (15.2 mm). The stability of the coordinates of each station (3DRMS) is from 9 mm to 46 mm (for LAGEOS, from 5 mm to 15 mm) with the uncertainty of determining the coordinates of 3–11 mm (LAGEOS 2–7 mm). The combined positioning for the LARES + LAGEOS-1 + LAGEOS-2 satellites allows for the stability of 5–18 mm with an uncertainty of 2–6 mm. For most stations, this solution is slightly better than the LAGEOS-only one.

1 January 2007 in Advances In Space Research
Verified
Journal Article
Closed access
PLPawel Lejba
Pawel Lejba
Stanislaw SchillakStanislaw Schillak
Stanislaw Schillak
EWE. Wnuk
E. Wnuk

26 July 2022 in Journal of Space Safety Engineering
Verified
Journal Article
Closed access
ECEmiliano Cordelli
Emiliano Cordelli
AMAndrea Di Mira
Andrea Di Mira
TFTim Flohrer
Tim Flohrer
SSSrinivas Setty
Srinivas Setty
IZIgor Zayer
Igor Zayer
WPWolfgang Promper
Wolfgang Promper