It’s about a year until ICON launches, and all teams—science, instruments, mission operations and modeling teams—are moving forward with laser focus. There is little time to rest when so much goes into making a NASA satellite ready for launch in June 2017.  Systems need to be tested to ensure they can download and process the data that ICON will be generating nearly continuously, orbit after orbit, in Earth’s upper atmosphere. Current data processing testing is making use of the data that the flight instruments are already producing as they undergo ground testing—it's a great way to see how everything's flowing through the data pipeline.  In fact, the mission and instrument operations teams worked together recently to perform a “day in the life” test with the instruments, where they ran them through a 24 hour long sequence of commands, to simulate what they will do over a full day's worth of orbits.

FUV is continuing its series of successful tests and calibrations at CSL in Belgium. Once all of instrument’s accelerometers have been mounted, the Z-axis vibration test will be conducted. FUV is on schedule for delivery for integration in Utah, early in 2016. 

While the IVM enjoys many years of heritage, the ICON IVM has improvements and modifications that will produce measurements of the plasma drift with unprecedented sensitivity to achieve the ICON science goals. 

The second IVM (IVM-B) fabrication is following closely behind IVM-A and is in the final phases of test and assembly. IVM-B faces in the aft direction on the spacecraft during normal operations, when the remote sensing optical instruments view the northern hemisphere. However, it will be activated during operations when the spacecraft is rotated to allow the optical instruments to view the southern hemisphere.

The preliminary alignment for the Far Ultraviolet Spectrograph (FUV) instrument using visible wavelength light has been completed at Lockheed Martin. The next phase of testing will see the instrument ship to Belgium to complete the alignment in the FUV in a specialized vacuum chamber.

The FUV ICON instrument has an articulating field of view. In order to accommodate this, special machinery is required to rotate the instrument during alignment, testing and calibration while inside the vacuum chamber. Centre Spatial de Liege (CSL) in Belgium will provide this unique ultraviolet vacuum facility.

The design for the FUV instrument is such that the optical system can be focused using visible light and a visible grating, as well as FUV light and grating. This is preferable, since alignment using UV must be performed in a vacuum chamber, which makes it more challenging to conduct the alignment.

Over the past four weeks, the SSL team has been traveling to Lockheed Martin where the instruments’ mirrors were carefully adjusted to achieve best focus and optimum spectral performance at visible wavelengths. The visible wavelengths chosen were suitably scaled to simulate performance at the FUV operating wavelength.

The next phase of testing will see the optics package ship to Centre Spatial de Liege (CSL) in Belgium. After verifying the visible alignments were maintained, and no shifts happened during transport, the UV grating and the two UV cameras will be installed and UV alignment will begin.