Publications related to the GRACE Missions (no abstracts)

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Triple mirror assembly in the GRACE Follow-On laser ranging interferometer

Abich, Klaus, Baatzsch, Andreas, Bogan, Christina, Braxmaier, Claus, Danzmann, Karsten, Barranco, Germán Fernández, Gohlke, Martin, Heinzel, Gerhard, Herding, Mark, Hinz, Martin, Kaufer, Marina, Koch, Alexander, Leikert, Thomas, Mahrdt, Christoph, Misfeldt, Malte, Müller, Vitali, Nicklaus, Kolja, Reiche, Jens, Sanjuan, Josep, Schütze, Daniel, Stede, Gunnar, Voss, Kai, Wegener, Henry, and Zimmermann, Marcus, 2025. Triple mirror assembly in the GRACE Follow-On laser ranging interferometer. Physical Review Applied, 24(4):044076, doi:10.1103/7ps8-317c.

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BibTeX

@ARTICLE{2025PhRvP..24d4076A,
       author = {{Abich}, Klaus and {Baatzsch}, Andreas and {Bogan}, Christina and {Braxmaier}, Claus and {Danzmann}, Karsten and {Barranco}, Germ{\'a}n Fern{\'a}ndez and {Gohlke}, Martin and {Heinzel}, Gerhard and {Herding}, Mark and {Hinz}, Martin and {Kaufer}, Marina and {Koch}, Alexander and {Leikert}, Thomas and {Mahrdt}, Christoph and {Misfeldt}, Malte and {M{\"u}ller}, Vitali and {Nicklaus}, Kolja and {Reiche}, Jens and {Sanjuan}, Josep and {Sch{\"u}tze}, Daniel and {Stede}, Gunnar and {Voss}, Kai and {Wegener}, Henry and {Zimmermann}, Marcus},
        title = "{Triple mirror assembly in the GRACE Follow-On laser ranging interferometer}",
      journal = {Physical Review Applied},
         year = 2025,
        month = oct,
       volume = {24},
       number = {4},
          eid = {044076},
        pages = {044076},
     abstract = "{The Gravity Recovery And Climate Experiment (GRACE) Follow-On mission
        was launched on May 22, 2018, to continue monitoring changes in
        the gravity field of the Earth by measuring distance variations
        between two spacecraft that fly 200 km apart in a low-Earth
        polar orbit. The laser ranging interferometer (LRI), a
        technology demonstrator onboard GRACE Follow-On, is the first of
        its kind to perform interspacecraft ranging measurements and has
        shown noise levels of 1 nm/Hz at 100 mHz and 200 pm/Hz at 5 Hz.
        Its development was shared between parties in Germany and the
        United States. A key optical component for the LRI's success is
        the triple mirror assembly (TMA), which acts as a corner-cube
        retroreflector and enables the laser link between the two
        spacecraft. This paper presents the TMA design and
        characterization from the unit level to measurements in orbit.
        The in-orbit measurements furthermore provide the far-field
        intensity distribution of the Gaussian beams exchanged between
        the spacecraft after traveling 200 km. We address lessons
        learned that have influenced the design of the next generations
        of the LRI.}",
          doi = {10.1103/7ps8-317c},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2025PhRvP..24d4076A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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