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1 April 2024: Hinode-17/IRIS-15/SPHERE meeting in Bozeman, Montana, July 23-27, 2024 3 Oct 2023: Confronting numerical models of the solar chromosphere and corona with high resolution observations - a RoCS/MUSE/IRIS workshop February 27 to March 2, 2023, Svalbard, Norway Spectral lines represent the richest source of information on the physical properties of the observed plasma, which can be evaluated using plasma diagnostic tools. The most relevant diagnostics provided by the IRIS optically-thin lines are described in the following sections. 1.1. Summary IRIS is the Interface Region Imaging Spectrograph small explorer (NASA Small Explorer-SMEX), a satellite designed to study the solar transition region, i.e., the region between the chromosphere and the corona. IRIS was built for NASA by the Lockheed Martin Solar & Astrophysics Laboratory (LMSAL) in Palo Alto with major contributions from NASA Ames, Smithsonian Astrophysical. IRIS | Interface Region Imaging Spectrograph The primary goal of the Interface Region Imaging Spectrograph (IRIS) explorer is to understand how the solar atmosphere is energized. The IRIS investigation combines advanced numerical modeling with a high resolution UV imaging spectrograph. IRIS will obtain UV spectra and images with high resolution in space (0.33-0.4 arcsec) and time (1-2s. The IRIS team at the Lockheed Martin Solar and Astrophysics Laboratory (LMSAL) created new data cubes consisting of the Hinode/SOT and SDO/AIA images co-aligned with the simultaneous IRIS observations. These datasets all have the same IRIS level 2 FITS format, therefore can be accessed and examined using the IRIS SolarSoft software. During the upcoming ALMA cycle 4 solar observations from December 2016 to April 2017, IRIS will prioritize support of successful ALMA cycle 4 solar observing proposals. Proposers to the ALMA cycle 4 can refer to this message as evidence of IRIS support for their observations. Keep in mind that while IRIS is in eclipse season from early November through mid February, during this time frame IRIS. Lockheed employees with MDI machines: Firefox 17 can be installed from the MDI help portal and should work. IRIS has an open data policy. When you publish work based on IRIS data, please acknowledge IRIS as follows: IRIS is a NASA small explorer mission developed and operated by LMSAL with mission operations executed at NASA Ames Research Center and major contributions to downlink communications funded by ESA and the Norwegian Space Centre. IRIS is the Interface Region Imaging Spectrograph small explorer (NASA Small Explorer- SMEX). The IRIS investigation combines advanced numerical modeling with a high resolution, high throughput multi-channel UV imaging spectrograph fed by a 20 cm UV telescope. The main science goal of IRIS is to understand how the solar atmosphere is energized. IRIS | Interface Region Imaging Spectrograph The standard WCS keywords for specifying the the linear coordinate system (CDELTn, CRPIXn, CRVALn) are used, where n is an integer specifying the dimension of the data (X, Y, lambda). Note that CDELT1 is typically larger than CDELT2 -- the X axis scale is set by the raster step size (generally 2 arcsec), while the Y axis scale is set by the spatial.

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