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Institution

European Space Operations Centre

GovernmentDarmstadt, Germany
About: European Space Operations Centre is a government organization based out in Darmstadt, Germany. It is known for research contribution in the topics: Orbit determination & Satellite. The organization has 309 authors who have published 331 publications receiving 10399 citations. The organization is also known as: ESOC.


Papers
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Journal ArticleDOI
TL;DR: In this article, an analytical meteoroid flux model is presented which extends from 1 to 10 AU and covers a mass range from 10−18 to 1 g. The basic flux curve of the model by Grun et al. (1985, Icarus 62, 244-272.) is modified by an analytical multiplication factor in order to approximate the Meteoroid flux as predicted by the five-populations-model from Divine (1993, J. Geophys. Res. 98(E9), 17,029-17,048).

14 citations

Journal ArticleDOI
TL;DR: In this paper, a structural panel under acoustic loading by supersonic convected turbulence, deriving responses with finite Fourier transforms, was constructed by using a finite-finite Fourier transform.

14 citations

Journal ArticleDOI
TL;DR: Fundamental biases in V-slit sun and pencil-beam infrared Earth sensor measurements are identified and modeled in terms of representative covariances, useful in identifying the best attitude determination intervals and for providing quantitative estimates of the expected error for selected launch configurations.
Abstract: Fundamental biases in V-slit sun and pencil-beam infrared Earth sensor measurements are identified and modeled in terms of representative covariances. Their effects on attitude determination accuracy are assessed by means of covariance transformations following the calculations involved in a realistic attitude estimation process. The results are useful in identifying the best attitude determination intervals and for providing quantitative estimates of the expected error for selected launch configurations. On this basis the most favorable sensor settings can be selected for a given launch window. This is of particular interest for present-day communication satellites equipped with variable sensor mountings which can be adjusted before launch.

14 citations

Journal ArticleDOI
James Ira Thorpe1, Jacob Slutsky1, John G. Baker1, Tyson Littenberg2, Sophie Hourihane1, Sophie Hourihane3, Sophie Hourihane2, Nicole Pagane1, Nicole Pagane4, Petr Pokorny1, Petr Pokorny5, Diego Janches1, Michele Armano6, Heather Audley7, G. Auger8, J. Baird9, Massimo Bassan10, Pierre Binétruy8, M. Born7, Daniele Bortoluzzi11, N. Brandt12, M. Caleno6, Antonella Cavalleri11, A. Cesarini11, A. M. Cruise13, Karsten Danzmann7, M. de Deus Silva6, R. De Rosa, L. Di Fiore14, Ingo Diepholz7, G. Dixon13, Rita Dolesi11, N. Dunbar12, Luigi Ferraioli15, Valerio Ferroni11, E. D. Fitzsimons16, R. Flatscher12, M. Freschi6, C. García Marirrodriga6, R. Gerndt12, Lluis Gesa17, Ferran Gibert11, Domenico Giardini15, R. Giusteri11, Aniello Grado18, Catia Grimani19, J. Grzymisch6, I. Harrison20, Gerhard Heinzel7, M. Hewitson7, Daniel Hollington9, D. Hoyland13, Mauro Hueller11, Henri Inchauspe8, Oliver Jennrich6, Ph. Jetzer21, B. Johlander6, Nikolaos Karnesis7, B. Kaune7, N. Korsakova7, Christian J. Killow22, J. A. Lobo17, Ivan Lloro17, L. Liu11, J. P. López-Zaragoza17, R. Maarschalkerweerd20, Davor Mance15, V. Martín17, L. Martin-Polo6, J. Martino8, F. Martin-Porqueras6, S. Madden6, Ignacio Mateos17, Paul McNamara6, José F. F. Mendes20, L. Mendes6, Miquel Nofrarías17, S. Paczkowski7, Michael Perreur-Lloyd22, Antoine Petiteau8, P. Pivato11, Eric Plagnol8, P. Prat8, U. Ragnit6, Juan Ramos-Castro23, J. Reiche7, D. I. Robertson22, H. Rozemeijer6, F. Rivas17, G. Russano11, P. Sarra, A. Schleicher12, D. Shaul9, Carlos F. Sopuerta17, Ruggero Stanga24, T. J. Sumner9, D. Texier6, C. Trenkel12, Michael Tröbs7, Daniele Vetrugno11, S. Vitale11, Gudrun Wanner7, H. Ward22, Peter Wass9, D. Wealthy12, W. J. Weber11, L. Wissel7, A. Wittchen7, A. Zambotti11, C. Zanoni11, Tobias Ziegler12, Peter Zweifel15, St Drs Operations Team, P. Barela25, Curt Cutler25, Nate Demmons, C. Dunn25, M. Girard25, O. Hsu1, S. Javidnia25, I. Li25, P. Maghami1, C. Marrese-Reading25, J. Mehta25, J. O’Donnell, Andrew Romero-Wolf25, John Ziemer25 
TL;DR: In this article, a new set of data obtained from direct measurements of momentum transfer to a spacecraft from individual particle impacts is presented, which can be used to detect impacts and measure properties such as the transferred momentum, direction of travel, and location of impact on the spacecraft.
Abstract: The zodiacal dust complex, a population of dust and small particles that pervades the solar system, provides important insight into the formation and dynamics of planets, comets, asteroids, and other bodies. We present a new set of data obtained from direct measurements of momentum transfer to a spacecraft from individual particle impacts. This technique is made possible by the extreme precision of the instruments flown on the LISA Pathfinder spacecraft, a technology demonstrator for a future space-based gravitational wave observatory. Pathfinder employed a technique known as drag-free control that achieved rejection of external disturbances, including particle impacts, using a micropropulsion system. Using a simple model of the impacts and knowledge of the control system, we show that it is possible to detect impacts and measure properties such as the transferred momentum, direction of travel, and location of impact on the spacecraft. In this paper, we present the results of a systematic search for impacts during 4348 hr of Pathfinder data. We report a total of 54 candidates with transferred momenta ranging from 0.2 to 230 μNs. We furthermore make a comparison of these candidates with models of micrometeoroid populations in the inner solar system, including those resulting from Jupiter-family comets (JFCs), Oort Cloud comets, Halley-type comets, and asteroids. We find that our measured population is consistent with a population dominated by JFCs, with some evidence for a smaller contribution from Halley-type comets, in agreement with consensus models of the zodiacal dust complex in the momentum range sampled by LISA Pathfinder.

14 citations

Journal ArticleDOI
TL;DR: In this paper, a new efficient parameterization scheme for solar short-wave radiative heating, as a component of the net radiative effects in the atmosphere, is tested in a three-dimensional mesoscale model.
Abstract: A new efficient parameterization scheme for solar short-wave radiative heating, as a component of the net radiative effects in the atmosphere, is tested in a three-dimensional mesoscale model. This model is designed with moist convective processes in mind, so that the radiative parameterization (solar plus thermal infrared) are interactive with the cloud field. Previous work by the authors with only an infrared scheme has demonstrated that cloud-radiation interactions are characterized by strong cloud-top cooling, leading to upper cloud-layer destabilization. The effects of including solar heating are to modulate the strength of the strong infrared cooling, thereby leading to weaker interactions between clouds, radiation, and mesoscale fields. The present study shows that even on the mesoscale and for relatively short time-spans, radiative processes in the presence of clouds are not negligible. As a further step, a simple fractional cloud cover parameterization is introduced and the model response is compared with results omitting this parameterization.

13 citations


Authors

Showing all 312 results

NameH-indexPapersCitations
S. Foley569610888
Anja Rudolph5313717307
José F. F. Mendes5125719604
Johannes Schmetz29853741
Markus Landgraf28862678
Heiner Klinkrad231201777
Ian Harrison22711664
Holger Krag191071081
Marcus Kirsch1643715
R. Maarschalkerweerd14411163
Nicola Policella1464865
Michiel Otten1327539
Jozef C. Van Der Ha1246368
R. Jehn1237387
Andrés Riaguas1014376
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
20231
20226
20217
202010
201914
20189