Global comparisons of satellite derived SSTs with in-situ observations from the World Ocean database
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Engineering topics
Publications and source records attributed to Armstrong, J..
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This paper describes the new DSN science capability and highlights of the engineering work that lead to its development. It will also discuss experience with operations along with statistics and data quality.
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The first in-flight Doppler tracking measurements performed by LISA will be used to assess its detector performance.
LISA can be considered as six proof masses, pairwise Doppler tracked with one-way optical links.
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LISA (Laser Interferometer Space Antenna) is a proposed mission which will use coherent laser beams exchanged between three remote spacecraft to detect and study low-frequency cosmic gravitational radiation.
Using polarized brightness (pB) measurements made by the High Altitude Observatory (HAO) Mauna Loa Mk III K-coronameter, we investigate the daily changes of path-integrated density at1.15 R-circle dot.
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The Voyager 1/2 plasma wave instruments have observed low-frequency (1.5-4kHz) radio waves apparently generated near the heliopause. The waves are found in two distinct bands.
Ground-based, equal-arm-length laser interferometers are being built to measure high-frequency astrophysical graviatational waves. Because of the arm-length equality, laser light experiences the same delay in each arm and thus phase or frequency noise from the laser itself precisely cancels at the photodetector.