Comparison between Laser Ranging Interferometer and K/Ka band Ranging instruments.
<div> <p><span>The GRACE Follow-On mission is the first twin-satellite mission</span><span> equipped with a laser ranging interferometer (LRI) to measure the inter-satellite distance between the pair of satellites. The LRI operates independently of the K/Ka-band interferometer (KBR</span><span>)&#160;and uses</span><span>&#160;wavelengths</span><span>&#160;</span><span>10</span><sup><span>4</span></sup><span>&#160;times</span><span>&#160;shorter than the K-band</span><span>&#160;system.&#160;&#160;</span><span>Released at the end of July 2019, the LRI range data is&#160;</span><span>therefore&#160;</span><span>expected to be of higher accuracy than the KBR and offers the possibility of a better spatial resolution. We compare the LRI and KBR observations of the GRACE-FO mission, from launch to December 2019, to assess the quality of the new LRI system.</span><span>&#160;</span><span>Spectral analysis of the level1B data shows that the noise level of the LRI is 3&#160;</span><span>orders</span><span>&#160;of magnitude smaller than the KBR</span><span>&#160;and that&#160;</span><span>the gravity signal can be detected in the spectral band up to&#160;</span><span>30mHz in the LRI data&#160;</span><span>compared</span><span>&#160;to&#160;</span><span>20mHz</span><span>&#160;</span><span>i</span><span>n</span><span>&#160;the&#160;</span><span>KBR</span><span>&#160;data</span><span>.</span><span>&#160;</span><span>&#160;We compare</span><span>&#160;gravity&#160;</span><span>fields</span><span>&#160;estimated using LRI&#160;</span><span>and KBR and show which parts of the spherical harmonic spectrum are affected by the improved accuracy of the LRI observations.</span></p> </div>