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

A data browser developed by Dr. Yen-Jung Wu here at SSL allows you to make plots of ICON data very quickly, and once the data are plotted provides a quick link to the file at the NASA repository. 

The ICON Project Data Management Plan (PDMP) is available online. This 350 page document was updated for and submitted with the ICON Senior Review proposal.  It describes the content of all data files available on out own FTP site and the NASA SPDF archive.

The ICON Calibration and Measurement Algorithms Document (or CMAD) is also available online. This is a historically prescribed title for a document that is now required of all NASA missions. It is created newly for ICON for the senior review, weighs in at 180 pages, and describes the data processing algorithms used in the ICON Science Data Center.

The first distribution of MIGHTI V5 data published in December 2022 extended to August 2022. This brief entry discusses the work to extend the dataset to the end of data collection.

Version 5 of the MIGHTI thermospheric winds is on its way. We are currently processing all the line of sight winds and once these are approved, will be promoted to the public FTP site and then the NASA archive. This wind product fills some long data gaps bad due to solar contamination. In version 5 the effects of this contamination has been mitigated and most of the data has been recovered. It also un-tethers the zero wind from HWM, using the on-orbit calibration processes to determine zero.