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

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Karin Hauck
/ Categories: Science, Press Release

ICON Co-Investigator Siegmund Wins the 2020 Joseph Weber Award for Astronomical Instrumentation

AAS

The 2020 Joseph Weber Award for Astronomical Instrumentation, awarded for the design, invention, or significant improvement of instrumentation leading to advances in astronomy, goes to Oswald “Ossy” Siegmund (University of California, Berkeley, Space Sciences Laboratory) for his significant and innovative contributions to the technology of photon counting detectors and the impact these instruments have had on advancing our understanding of the universe. His role in developing and continually improving microchannel plate (MCP) detectors has been transformative to a broad range of astrophysical studies. Sensors incorporating MCPs are used in particle detectors and in astronomical instruments spanning X-ray, ultraviolet, and visible wavelengths. Over several decades detector technology directly enabled by Siegmund has been incorporated into numerous NASA, European Space Agency, and Department of Energy projects and has led to fundamental astrophysical discoveries. “

"Calling prize winners to let them know they’ve won an award is by far the best part of this AAS President gig,” says Megan Donahue (Michigan State University). “AAS prizes not only acknowledge the recipients, but also the people who surround and support them. It’s a win-win for the awardees, their institutions, their collaborators, and the AAS — which gets to celebrate the many kinds of excellent work being done in our field.”

Siegmund is a co-Investigator on ICON.

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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