Relevant bibliographies by topics / LISA space mission

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'LISA space mission'

Author: Grafiati
Published: 28 September 2024
Last updated: 31 July 2025

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Journal articles on the topic "LISA space mission"

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McNAMARA, PAUL W. "THE LISA PATHFINDER MISSION." International Journal of Modern Physics D 22, no. 01 (2013): 1341001. http://dx.doi.org/10.1142/s0218271813410010.

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Laser Interferometer Space Antenna (LISA) Pathfinder (formerly known as SMART-2) is a European Space Agency mission designed to pave the way for the joint ESA/NASA LISA mission by testing in flight the critical technologies required for space borne gravitational wave detection; it will put two test masses in a near-perfect gravitational free-fall and control and measure their motion with unprecedented accuracy. This is achieved through technology comprising inertial sensors, high precision laser metrology, drag-free control and an ultra precise micro-Newton propulsion system. LISA Pathfinder (
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Schuldt, Thilo, Klaus Döringshoff, Markus Oswald, Evgeny V. Kovalchuk, Achim Peters, and Claus Braxmaier. "Absolute laser frequency stabilization for LISA." International Journal of Modern Physics D 28, no. 12 (2019): 1845002. http://dx.doi.org/10.1142/s0218271818450025.

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The LISA space mission requires laser frequency pre-stabilization of the 1064[Formula: see text]nm laser sources. While cavity-based systems are the current baseline, laser frequencies stabilized to a hyperfine transition in molecular iodine near 532[Formula: see text]nm are a possible alternative. Several setups with respect to space applications were developed, putting special emphasis on compactness and mechanical and thermal stability of the optical setup. Vibration testing and thermal cycling were performed. These setups show frequency noise below 20[Formula: see text]Hz/[Formula: see tex
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Hechler, F., and W. M. Folkner. "Mission analysis for the Laser Interferometer Space Antenna (LISA) mission." Advances in Space Research 32, no. 7 (2003): 1277–82. http://dx.doi.org/10.1016/s0273-1177(03)90332-2.

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Racca, Giuseppe D., and Paul W. McNamara. "The LISA Pathfinder Mission." Space Science Reviews 151, no. 1-3 (2009): 159–81. http://dx.doi.org/10.1007/s11214-009-9602-x.

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Banks, Michael. "Europe gives green light to LISA gravitational-wave mission." Physics World 37, no. 3 (2024): 13i. http://dx.doi.org/10.1088/2058-7058/37/03/16.

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RÜEDIGER, ALBRECHT. "Detecting gravitational waves with ground and space interferometers – with special attention to the space project ASTROD." International Journal of Modern Physics D 11, no. 07 (2002): 963–94. http://dx.doi.org/10.1142/s0218271802002505.

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The existence of gravitational waves is the most prominent of Einstein's predictions that has not yet been directly verified. The space projects LISA and (partially) ASTROD share their goal and principle of operation with the ground-based interferometers currently under construction: the detection and measurement of gravitational waves by laser interferometry. Ground and space detection differ in their frequency ranges, and thus the detectable sources. Towards low frequencies, ground-based detection is limited by seismic noise, and yet more fundamentally by 'gravity gradient noise', thus cover
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Ruiz-Rocha, Krystal, Kelly Holley-Bockelmann, Karan Jani, Michela Mapelli, Samuel Dunham, and William Gabella. "A Sea of Black Holes: Characterizing the LISA Signature for Stellar-origin Black Hole Binaries." Astrophysical Journal 981, no. 1 (2025): 27. https://doi.org/10.3847/1538-4357/adad6b.

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Abstract Observations by the LIGO, Virgo, and KAGRA (LVK) detectors have provided new insights into the demographics of stellar-origin black hole binaries (sBHBs). A few years before gravitational-wave signals from sBHB mergers are recorded in the LVK detectors, their early coalescence will leave a unique signature in the ESA/NASA mission Laser Interferometer Space Antenna (LISA). Multiband observations of sBHB sources between the LISA and LVK detectors opens an unprecedented opportunity to investigate the astrophysical environment and multimessenger early alerts. In this study, we report the
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Smetana, Adam. "Background for gravitational wave signal at LISA from refractive index of solar wind plasma." Monthly Notices of the Royal Astronomical Society: Letters 499, no. 1 (2020): L77—L81. http://dx.doi.org/10.1093/mnrasl/slaa155.

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ABSTRACT A strong indication is presented that the space-based gravitational antennas, in particular the Laser Interferometer Space Antenna (LISA) concept introduced in 2017 in response to the ESA call for L3 mission concepts, are going to be sensitive to a strong background signal interfering with the prospected signal of gravitational waves. The false signal is due to variations in the electron number density of the solar wind, causing variations in the refractive index of plasma flowing through interplanetary space. As countermeasures, two solutions are proposed. The first solution is to de
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Martens, Waldemar, and Eric Joffre. "Trajectory Design for the ESA LISA Mission." Journal of the Astronautical Sciences 68, no. 2 (2021): 402–43. http://dx.doi.org/10.1007/s40295-021-00263-2.

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AbstractThe three Laser Interferometer Space Antenna (LISA) spacecraft are going to be placed in a triangular formation in an Earth-trailing or Earth-leading orbit. They will be launched together on a single rocket and transferred to that science orbit using Solar Electric Propulsion. Since the transfer Δv depends on the chosen science orbit, both transfer and science orbit have been optimised together. For a thrust level of 90 mN, an allocation of 1092 m/s per spacecraft is sufficient for an all-year launch in 2034. For every launch month a dedicated science orbit is designed with a corner an
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Dei Tos, Diogene A., Mirco Rasotto, Florian Renk, and Francesco Topputo. "LISA Pathfinder mission extension: A feasibility analysis." Advances in Space Research 63, no. 12 (2019): 3863–83. http://dx.doi.org/10.1016/j.asr.2019.02.035.

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Dissertations / Theses on the topic "LISA space mission"

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Bogenstahl, Johanna. "Interferometry for the space mission LISA Pathfinder." Thesis, University of Glasgow, 2010. http://theses.gla.ac.uk/1696/.

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VIDANO, SIMONE. "Drag-free control design for the LISA space mission." Doctoral thesis, Politecnico di Torino, 2022. http://hdl.handle.net/11583/2957738.

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Rivas, García Francisco. "Thermo-optical and thermo-elastic effects onboard the LISA Pathfinder mission." Doctoral thesis, Universitat Autònoma de Barcelona, 2019. http://hdl.handle.net/10803/669444.

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Colcombet, Paul. "Étude de photorécepteurs sous irradiation de protons, électrons et rayons gamma pour la mission LISA." Electronic Thesis or Diss., Université Côte d'Azur, 2024. http://www.theses.fr/2024COAZ5022.

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Programmée pour 2035, la mission LISA (Laser Interferometer Space Antenna), pilotée par l'Agence spatiale européenne (ESA), marquera une première en devenant le premier détecteur spatial d'ondes gravitationnelles. Opérant dans la gamme des basses fréquences de 0,1 mHz à 1 Hz inaccessible aux détecteurs terrestres, LISA ouvrira une nouvelle fenêtre sur notre univers et une nouvelle ère dans l'étude de la cosmologie. Le design de LISA présente trois vaisseaux formant un triangle équilatéral de 2,5 millions de km de côté, suivant la Terre dans son orbite autour du Soleil. Au cœur du fonctionnemen
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Roubeau-Tissot, Amaël. "Interférométrie à dérive de fréquence pour la mesure de la lumière parasite sur l'instrument spatial LISA." Electronic Thesis or Diss., Université Côte d'Azur, 2024. http://www.theses.fr/2024COAZ5036.

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LISA (Laser Interferometer Space Antenna) est un interféromètre spatial dédié à la détection des ondes gravitationnelles dans la gamme de fréquence [20 µHz-1 Hz], actuellement en développement (phase B). Ce projet international géré par l'ESA sera composé d'une constellation de trois satellites en formation triangulaire, chacun d'entre eux émettant deux faisceaux laser vers les deux autres satellites. Il y a donc au total 6 liens laser, et 6 unités, appelées MOSA (Moving Optical Sub-Assembly) chargées d'émettre et de recevoir les faisceaux, et de réaliser la mesure des variations de distance i
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Books on the topic "LISA space mission"

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A Good Night For Ghosts A Merlin Mission. Random House Books for Young Readers, 2009.

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Book chapters on the topic "LISA space mission"

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Mee, Nicholas. "Lovely LISA." In The Cosmic Mystery Tour. Oxford University Press, 2019. http://dx.doi.org/10.1093/oso/9780198831860.003.0005.

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The European Space Agency (ESA) has plans to build a space-based gravitational wave detector known as LISA. The recent LISA Pathfinder mission has demonstrated that the technology required for LISA will be sufficiently sensitive to detect gravitational waves. LISA will detect events that are invisible to LIGO and other Earth-based gravitational wave detectors. These include the mergers of distant supermassive black holes.
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Westwood, Lisa, Beth Laura O’Leary, and Milford Wayne Donaldson. "Legal Frameworks for Historic Preservation." In The Final Mission. University Press of Florida, 2017. http://dx.doi.org/10.5744/florida/9780813062464.003.0007.

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“Legal Frameworks for Historic Preservation” provides an overview of the various federal and international laws and guidelines for historic preservation of culture, and explains how preservation of space heritage sites like those noted in the book can fit into that system. Particular attention is paid to the World Heritage List, the United Nations, the National Register of Historic Places, and the National Historic Landmark programs, in terms of the criteria for inclusion in them. The authors make the case for the overarching significance of space heritage sites within this context by referrin
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Carr, Michael H. "Future Mars Exploration." In Water On Mars. Oxford University PressNew York, NY, 1996. http://dx.doi.org/10.1093/oso/9780195099386.003.0009.

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Abstract Missions are the lifeblood of planetary science. Unfortunately, planetary missions are expensive and because they are expensive only a few nations or agencies have independent planetary exploration programs. At the time of this writing the list was restricted to four: the United States, Russia, Japan, and the European Space Agency. To lay out a rational, step-by-step program for the exploration of Mars is not difficult, but the likelihood of such a plan being followed is small. Because the missions are expensive, their approval requires support of a much broader constituency than the
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Boswell, Matthew, and Antony Rowland. "Witness in the Light Stage." In Virtual Holocaust Memory. Oxford University PressNew York, 2023. http://dx.doi.org/10.1093/oso/9780197645390.003.0004.

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Abstract This chapter centers on a Dimensions in Testimony interview with the Holocaust survivor Eva Schloss, the posthumous stepsister of Anne Frank. We begin by exploring the dynamics of the extended question-and-answer format, before discussing three different written accounts that Schloss gave of her Holocaust experiences at different times in her life. We discuss the influence of Schloss’s book for young adults, The Promise (2006), while noting that the project’s aim of making Holocaust testimony available to future generations of young people means that Schloss censors out some of the mo
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Conference papers on the topic "LISA space mission"

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Stebbins, Robin. "LISA Mission Tutorial." In LASER INTERFEROMETER SPACE ANTENNA: 6th International LISA Symposium. AIP, 2006. http://dx.doi.org/10.1063/1.2405016.

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Folkner LISA Team, W. M. "The LISA mission design." In The second international laser interferometer space antenna symposium (LISA) on the detection and observation of gravitational waves in space. AIP, 1998. http://dx.doi.org/10.1063/1.57401.

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Pireaux, S., B. Chauvineau, T. Régimbau, and J. Y. Vinet. "Relativistic approach of the LISA mission." In LASER INTERFEROMETER SPACE ANTENNA: 6th International LISA Symposium. AIP, 2006. http://dx.doi.org/10.1063/1.2405070.

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Ortega-Ruiz, J. A., A. Conchillo, X. Xirgu, and C. Boatella. "Mission Critical Software in LISA Pathfinder." In LASER INTERFEROMETER SPACE ANTENNA: 6th International LISA Symposium. AIP, 2006. http://dx.doi.org/10.1063/1.2405119.

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Karlen, L., S. Kundermann, N. Torcheboeuf, et al. "Laser System for the LISA Mission." In Applications of Lasers for Sensing and Free Space Communications. OSA, 2019. http://dx.doi.org/10.1364/lsc.2019.lm3b.2.

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Bortoluzzi, D., L. Baglivo, M. Benedetti, et al. "Test-Mass Release Phase Ground Testing for the LISA Pathfinder Mission." In LASER INTERFEROMETER SPACE ANTENNA: 6th International LISA Symposium. AIP, 2006. http://dx.doi.org/10.1063/1.2405098.

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Nappo, F., D. Desiderio, A. Franzoso, et al. "Experience and design drivers for the Inertial Sensor on the LISA Pathfinder Mission." In LASER INTERFEROMETER SPACE ANTENNA: 6th International LISA Symposium. AIP, 2006. http://dx.doi.org/10.1063/1.2405096.

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Montemurro, F., W. Fichter, M. Schlotterer, and S. Vitale. "Control Design of the Test Mass Release Mode for the LISA Pathfinder Mission." In LASER INTERFEROMETER SPACE ANTENNA: 6th International LISA Symposium. AIP, 2006. http://dx.doi.org/10.1063/1.2405103.

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Preston, Alix, Rachel J. Cruz, J. Ira Thorpe, et al. "Dimensional Stability of Hexoloy SA® Silicon Carbide and Zerodur™ Materials for the LISA Mission." In LASER INTERFEROMETER SPACE ANTENNA: 6th International LISA Symposium. AIP, 2006. http://dx.doi.org/10.1063/1.2405071.

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Stacey, Jonathan, Geoffrey P. Barwood, Alessio Spampinato, et al. "Laser frequency stabilisation for the LISA mission using a cubic cavity." In International Conference on Space Optics — ICSO 2022, edited by Kyriaki Minoglou, Nikos Karafolas, and Bruno Cugny. SPIE, 2023. http://dx.doi.org/10.1117/12.2691441.

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Reports on the topic "LISA space mission"

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Borgeaud, Maurice, Jonathan Bamber, Anny Cazenave, et al. Earth Observation Groundbreaking Science Discoveries. ESA, 2025. https://doi.org/10.5270/essc-esa-eo-groundbreaking-science-2025.

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This document was prepared by the Earth Sciences Panel of the European Space Sciences Committee in response to the ESA contract 500104016 entitled “Ground-breaking science discoveries and successes enabled by ESA Earth Observation satellites”. This brochure showcases 12 ground-breaking scientific discoveries and successes enabled by the programme. These are divided into 3 cases for each of the 4 main thematic domains of the Earth sciences: atmosphere, ocean, land, and polar regions. The criteria used to define a “groundbreaking science discovery” include a clear “elevator pitch”, the “degree o
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