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 42

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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Latest News

News

Dr. Thomas Immel

Mission Operations Update #3

Winds and UV products all published

The MIGHTI 2.1 Line-of-Sight winds and 2.2 Cardinal winds have been updated to v4 and are now available out to November 13 2020. The version resolves a disagreement between the green and red winds that became apparent in the June 2020 timeframe, and extends the set.

Some gaps will be apparent in this set and they are due to 3 things, that the image below describes.

Data gaps in v4 winds

Data excluded for Lunar contamination are recoverable, and will be processed with new L1 files and v5 L2 processing early next year. Data absent during the star tracker anomaly were not taken. Data excluded for solar contamination are partially recoverable, and will be addressed to the degree possible with new L1 files and v5 L2 processing early next year. An example link is reported below.

ftp://icon-science.ssl.berkeley.edu/pub/LEVEL.2/MIGHTI/yyyy/ddd/ZIP/ICON_L2-2_MIGHTI_yyyy-mm-dd_v04r00?.ZIP

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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