L
L. Wissel
Researcher at Leibniz University of Hanover
Publications - 17
Citations - 937
L. Wissel is an academic researcher from Leibniz University of Hanover. The author has contributed to research in topics: Pathfinder & Computer science. The author has an hindex of 6, co-authored 11 publications receiving 660 citations.
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Journal ArticleDOI
Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results
Michele Armano,Heather Audley,G. Auger,J. Baird,Massimo Bassan,Pierre Binétruy,M. Born,Daniele Bortoluzzi,N. Brandt,M. Caleno,L. Carbone,Antonella Cavalleri,A. Cesarini,Giacomo Ciani,G. Congedo,A. M. Cruise,Karsten Danzmann,M. de Deus Silva,R. De Rosa,M. Diaz-Aguilo,L. Di Fiore,Ingo Diepholz,G. Dixon,Rita Dolesi,N. Dunbar,Luigi Ferraioli,Valerio Ferroni,Walter Fichter,E. D. Fitzsimons,R. Flatscher,M. Freschi,A. F. García Marín,C. García Marirrodriga,R. Gerndt,Lluis Gesa,Ferran Gibert,Domenico Giardini,R. Giusteri,F. Guzmán,Aniello Grado,Catia Grimani,A. Grynagier,J. Grzymisch,I. Harrison,Gerhard Heinzel,M. Hewitson,Daniel Hollington,D. Hoyland,Mauro Hueller,Henri Inchauspe,Oliver Jennrich,Ph. Jetzer,Ulrich Johann,B. Johlander,Nikolaos Karnesis,B. Kaune,N. Korsakova,Christian J. Killow,J. A. Lobo,Ivan Lloro,L. Liu,J. P. López-Zaragoza,R. Maarschalkerweerd,Davor Mance,V. Martín,L. Martin-Polo,J. Martino,F. Martin-Porqueras,S. Madden,Ignacio Mateos,Paul McNamara,José F. F. Mendes,L. Mendes,A. Monsky,Daniele Nicolodi,Miquel Nofrarías,S. Paczkowski,Michael Perreur-Lloyd,Antoine Petiteau,P. Pivato,Eric Plagnol,P. Prat,U. Ragnit,B. Rais,Juan Ramos-Castro,J. Reiche,D. I. Robertson,H. Rozemeijer,F. Rivas,G. Russano,J Sanjuán,P. Sarra,A. Schleicher,D. Shaul,Jacob Slutsky,Carlos F. Sopuerta,Ruggero Stanga,F. Steier,T. J. Sumner,D. Texier,James Ira Thorpe,C. Trenkel,Michael Tröbs,H. B. Tu,Daniele Vetrugno,Stefano Vitale,V Wand,Gudrun Wanner,H. Ward,C. Warren,Peter Wass,D. Wealthy,W. J. Weber,L. Wissel,A. Wittchen,A. Zambotti,C. Zanoni,Tobias Ziegler,Peter Zweifel +118 more
TL;DR: The first results of the LISA Pathfinder in-flight experiment demonstrate that two free-falling reference test masses, such as those needed for a space-based gravitational wave observatory like LISA, can be put in free fall with a relative acceleration noise with a square root of the power spectral density.
Journal ArticleDOI
Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μHz.
Michele Armano,Heather Audley,J. Baird,Pierre Binétruy,M. Born,Daniele Bortoluzzi,E. Castelli,Antonella Cavalleri,A. Cesarini,A. M. Cruise,Karsten Danzmann,M. de Deus Silva,Ingo Diepholz,G. Dixon,Rita Dolesi,Luigi Ferraioli,Valerio Ferroni,E. D. Fitzsimons,M. Freschi,Lluis Gesa,Ferran Gibert,Domenico Giardini,R. Giusteri,Catia Grimani,J. Grzymisch,I. Harrison,Gerhard Heinzel,M. Hewitson,Daniel Hollington,D. Hoyland,Mauro Hueller,Henri Inchauspe,Oliver Jennrich,Ph. Jetzer,Nikolaos Karnesis,B. Kaune,N. Korsakova,Christian J. Killow,J. A. Lobo,Ivan Lloro,L. Liu,J. P. López-Zaragoza,R. Maarschalkerweerd,Davor Mance,N. Meshksar,V. Martín,L. Martin-Polo,J. Martino,F. Martin-Porqueras,Ignacio Mateos,Paul McNamara,José F. F. Mendes,L. Mendes,Miquel Nofrarías,S. Paczkowski,Michael Perreur-Lloyd,Antoine Petiteau,P. Pivato,Eric Plagnol,Juan Ramos-Castro,J. Reiche,D. I. Robertson,F. Rivas,G. Russano,Jacob Slutsky,Carlos F. Sopuerta,T. J. Sumner,D. Texier,James Ira Thorpe,Daniele Vetrugno,Salvatore Vitale,Gudrun Wanner,H. Ward,Peter Wass,Peter Wass,W. J. Weber,L. Wissel,A. Wittchen,Peter Zweifel +78 more
TL;DR: This performance provides an experimental benchmark demonstrating the ability to realize the low-frequency science potential of the LISA mission, recently selected by the European Space Agency.
Journal ArticleDOI
Temperature stability in the sub-milliHertz band with LISA Pathfinder
Michele Armano,Heather Audley,J. Baird,Pierre Binétruy,M. Born,Daniele Bortoluzzi,E. Castelli,Antonella Cavalleri,A. Cesarini,A. M. Cruise,Karsten Danzmann,M. de Deus Silva,Ingo Diepholz,G. Dixon,Rita Dolesi,Luigi Ferraioli,Valerio Ferroni,E. D. Fitzsimons,M. Freschi,Lluis Gesa,Ferran Gibert,Domenico Giardini,R. Giusteri,Catia Grimani,J. Grzymisch,I. Harrison,Gerhard Heinzel,M. Hewitson,Daniel Hollington,D. Hoyland,Mauro Hueller,H. Inchauspé,H. Inchauspé,Oliver Jennrich,Ph. Jetzer,Nikolaos Karnesis,B. Kaune,N. Korsakova,Christian J. Killow,J. A. Lobo,Ivan Lloro,L. Liu,J. P. López-Zaragoza,R. Maarschalkerweerd,Davor Mance,C. Mansanet,V. Martín,L. Martin-Polo,J. Martino,F. Martin-Porqueras,Ignacio Mateos,Paul McNamara,José F. F. Mendes,L. Mendes,N. Meshksar,Miquel Nofrarías,S. Paczkowski,Michael Perreur-Lloyd,Antoine Petiteau,P. Pivato,Eric Plagnol,Juan Ramos-Castro,J. Reiche,D. I. Robertson,F. Rivas,G. Russano,Jose Sanjuan,Jacob Slutsky,Carlos F. Sopuerta,T. J. Sumner,D. Texier,James Ira Thorpe,C. Trenkel,Daniele Vetrugno,S. Vitale,Gudrun Wanner,H. Ward,Peter Wass,D. Wealthy,W. J. Weber,L. Wissel,A. Wittchen,Peter Zweifel +82 more
TL;DR: In this paper, the authors report on the temperature measurements throughout mission operations, characterize the thermal environment, estimate transfer functions between different locations, and report temperature stability (and its time evolution) at frequencies as low as 10'|$\mu$|Hz, where typically values around 1'K'Hz^−1'1/2 were measured.
Journal ArticleDOI
Spacecraft and interplanetary contributions to the magnetic environment on-board LISA Pathfinder
Michele Armano,Heather Audley,J. Baird,Pierre Binétruy,M. Born,Daniele Bortoluzzi,E. Castelli,Antonella Cavalleri,A. Cesarini,A. M. Cruise,Karsten Danzmann,M. de Deus Silva,Ingo Diepholz,G. Dixon,Rita Dolesi,L. Ferraioli,Valerio Ferroni,E.D. Fitzsimons,M. Freschi,Lluis Gesa,Ferran Gibert,D. Giardini,R. Giusteri,Catia Grimani,J. Grzymisch,I. Harrison,M.-S. Hartig,Gerhard Heinzel,Martin Hewitson,Daniel Hollington,D. Hoyland,Mauro Hueller,H. Inchauspe,H. Inchauspe,Oliver Jennrich,Ph. Jetzer,Nikolaos Karnesis,B. Kaune,N. Korsakova,Christian J. Killow,J. A. Lobo,L. Liu,J. P. López-Zaragoza,R. Maarschalkerweerd,D. Mance,V. Martín,L. Martin-Polo,J. Martino,F. Martin-Porqueras,Ignacio Mateos,Paul McNamara,José F. F. Mendes,L. Mendes,N. Meshksar,Miquel Nofrarías,S. Paczkowski,Michael Perreur-Lloyd,Antoine Petiteau,P. Pivato,Eric Plagnol,Juan Ramos-Castro,J. Reiche,F. Rivas,D. I. Robertson,D. Roma-Dollase,G. Russano,Jacob Slutsky,Carlos F. Sopuerta,Tamara Sumner,Daniele Telloni,D. Texier,James Ira Thorpe,C. Trenkel,Daniele Vetrugno,S. Vitale,Gudrun Wanner,H. Ward,Peter Wass,D. Wealthy,W. J. Weber,L. Wissel,A. Wittchen,P. Zweifel +82 more
TL;DR: In this paper, the authors report on the magnetic measurements throughout LISA Pathfinder (LPF) operations and characterize the magnetic environment within the spacecraft, study the time evolution of the magnetic field and its stability down to 20μHz.
Journal ArticleDOI
Measuring the galactic cosmic ray flux with the LISA Pathfinder radiation monitor
Michele Armano,Heather Audley,J. Baird,Pierre Binétruy,M. Born,Daniele Bortoluzzi,E. Castelli,Antonella Cavalleri,A. Cesarini,A. M. Cruise,Karsten Danzmann,M. de Deus Silva,Ingo Diepholz,G. Dixon,Rita Dolesi,Luigi Ferraioli,Valerio Ferroni,N. Finetti,E. D. Fitzsimons,M. Freschi,Lluis Gesa,Ferran Gibert,Domenico Giardini,R. Giusteri,Catia Grimani,J. Grzymisch,I. Harrison,Gerhard Heinzel,M. Hewitson,Daniel Hollington,D. Hoyland,Mauro Hueller,Henri Inchauspe,Oliver Jennrich,Ph. Jetzer,Nikolaos Karnesis,B. Kaune,N. Korsakova,Christian J. Killow,J. A. Lobo,Ivan Lloro,L. Liu,J. P. López-Zaragoza,R. Maarschalkerweerd,Davor Mance,N. Meshskar,V. Martín,L. Martin-Polo,J. Martino,F. Martin-Porqueras,Ignacio Mateos,Paul McNamara,José F. F. Mendes,L. Mendes,Miquel Nofrarías,S. Paczkowski,Michael Perreur-Lloyd,Antoine Petiteau,P. Pivato,E. Plagnol,Juan Ramos-Castro,J. Reiche,D. I. Robertson,F. Rivas,G. Russano,Jacob Slutsky,Carlos F. Sopuerta,T. J. Sumner,D. Texier,James Ira Thorpe,Daniele Vetrugno,S. Vitale,Gudrun Wanner,H. Ward,Peter Wass,Peter Wass,W. J. Weber,L. Wissel,A. Wittchen,Peter Zweifel +79 more
TL;DR: In this article, the authors used the measured deposited energy spectra, in combination with a GEANT4 model, to estimate the galactic cosmic ray differential energy spectrum over the course of the mission.