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SDO AIA and HMI Bz, 2010-05 to 2016-12, two times a day, 256 x 256

frames.tar holds frames/<YYYYMMDDTHHMM>.npz (UT), one file per time at 00:00 and 12:00 UT from May 2010 to December 2016. Each file holds the AIA channels present among aia94, aia131, aia171, aia193, aia211, aia304, aia335, aia1600 and aia1700 (DN/s) and bz, the line-of-sight component of the HMI vector magnetic field (gauss), as 256 x 256 float16 arrays.

Source

SDOML v2: R. Galvez, D. F. Fouhey, M. Jin, A. Szenicer et al., "A Machine-learning Data Set Prepared from the NASA Solar Dynamics Observatory Mission", The Astrophysical Journal Supplement Series 242, 7 (2019); version 2 by M. Jin, P. J. Wright and M. C. M. Cheung, in NASA's Heliophysics Digital Resource Library (https://registry.opendata.aws/sdoml-fdl/). Courtesy of NASA/SDO and the AIA and HMI science teams.

The registry entry reads "There are no restrictions on the use of this data." The HDRL, SDAC and SPDF data use policy (https://spdf.gsfc.nasa.gov/data_use_policy.html) makes the archive's data "public domain and made available with a Creative Commons Zero (CC0) dedication". This derived set is released under CC0 1.0.

Changes from SDOML v2

The frame nearest 00:00 and 12:00 UT of each day (within 10 minutes) was taken from each array, averaged in 2 x 2 blocks from 512 x 512 to 256 x 256 (about 9.6 arcsec per pixel; the solar radius is fixed at 976 arcsec, about 101.7 pixels, with the disk centred at pixel 127.5), clipped to the float16 range and stored as float16. Times with no AIA channel were left out; a channel that is missing at a time is absent from that file.

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