Exploring Where Earth's Weather Meets Space Weather

The Ionospheric Connection Explorer (ICON), the newest addition to NASA’s fleet of Heliophysics satellites, launched on October 10, 2019 at 9:59 p.m. EDT. Led by UC Berkeley, scientists and engineers around the world came together to make ICON a reality.

The goal of the ICON mission is to understand the tug-of-war between Earth’s atmosphere and the space environment. In the "no mans land" of the ionosphere, a continuous struggle between solar forcing and Earth’s weather systems drive extreme and unpredicted variability. ICON will investigate the forces at play in the near-space environment, leading the way in understanding disturbances that can lead to severe interference with communications and GPS signals.

Mission Operations News

Mission Operations News

ICON Temperatures Updated to Version 6, Now Available

Colin Triplett 0 46

The MIGHTI temperature product (L2.3) has been updated to version 6 (v06) and is currently available for the full mission on the ICON FTP site and at SPDF. 

With this version update, the MIGHTI-A and MIGHTI-B temperature data are both more rigorously tested to ensure continuity across the solar terminator. Also, the top of the daytime MIGHTI-A temperature profiles is now 135 km, up from 127 km in previous versions. Links to the data products are provided here:

ICON FTP MIGHTI

CDAWeb MIGHTI-A

CDAWeb MIGHTI-B

Prior to using these data, please review the data product documentation here:

ICON FTP Temperature V06 Documentation

RSS

Latest News

News

Karin Hauck
/ Categories: EUV

Rub-A-Dub-Dub, ICON EUV gets a scrub

ICON with its instrument suite illuminated

ICON with its instrument suite illuminated

This photo of ICON provides a nice view of the instrument suite and shows the scrub light source and vacuum plumbing.

In preparation for launch, the ICON EUV instrument recently went through a week long "scrub" activity at the Orbital ATK facility in Gilbert, Arizona. The detector in EUV is a microchannel plate (MCP), and the millions of tiny tubes in the MCP can develop different characteristics during all the testing done on the ground, and overall become less effective. The scrub involves running the detector at high voltage while it is illuminated by a bright EUV light source, which cleans off any molecules that weren’t there at the start of all that testing. When done for a sufficient amount of time (a week, in this case), the detector develops a more uniform and stable amplification, just like when it was new. It’s like a drink from the fountain of youth for the MCP.

This photo of ICON provides a nice view of the instrument suite and shows the scrub light source and vacuum plumbing. There are many reasons for the vacuum system, the first three being:

  • Air is opaque to the EUV light used to illuminate the light source.
  • Air, mainly nitrogen molecules, is what you are trying to scrub off the MCP in the first place.
  • Air, under the high voltage that will be applied to the detector during scrub and in space, breaks down and ionizes, allowing lightning to form. It will come as no surprise to know we don't want lightning on our detector!

[contributed by Will Marchant]

Previous Article Recent media articles featuring ICON and GOLD
Next Article ICON arrives at Vandenberg
Print
2489
ICON skin is based on Greytness by Adammer
Background image, courtesy of NASA, is a derivitave of photograph taken by D. Pettit from the ISS, used under Creative Commons license