Correct cadence on AIA and HMI

README.md

@@ -46,7 +46,7 @@ python scripts/main.py --config-name=default experiment.seed=37
 
 | Name 	| Description 	| Granularity & Source 	|
 |---	|---	|---	|
-|  NASA’s Solar Dynamics Observatory (SDO) [Pesnell et al. 2012](https://ui.adsabs.harvard.edu/link_gateway/2012SoPh..275....3P/doi:10.1007/s11207-011-9841-3)  | Three instruments:<br><ul><li>Atmospheric Imaging Assembly (AIA) 2 ultraviolet, 1600 & 1700 Å 7 extreme ultraviolet, 94, 131, 171, 193, 211, 304, and 335 Å.</li><li>Helioseismic and Magnetic Imager (HMI) - visible filtergrams processed into: photospheric Dopplergrams line-of-sight magnetograms vector magnetograms.</li><li>EUV Variability Experiment (EVE) - EUV spectral irradiance from 1 to 1050 Å. MEGS disperse EUV light from full disk of the Sun and corona onto a charge coupled device.</li></ul> | 4096x4096 12 second cadence:<br>AIA - [Lemen et al. 2012](https://ui.adsabs.harvard.edu/link_gateway/2012SoPh..275...17L/doi:10.1007/s11207-011-9776-8).<br>HMI - [Hoeksema et al. 2014](https://ui.adsabs.harvard.edu/link_gateway/2014SoPh..289.3483H/doi:10.1007/s11207-014-0516-8).<br>1024 x 2048: <br>EUV - [Woods et al. 2012](https://ui.adsabs.harvard.edu/link_gateway/2012SoPh..275..115W/doi:10.1007/s11207-009-9487-6).<br>Downsampled 512x512/0.6, 512x512/0.5 arcsec 12 minute cadence for machine learning: [Galvez et al. 2019](https://iopscience.iop.org/article/10.3847/1538-4365/ab1005) via [sdoml.org](sdoml.org). |
+|  NASA’s Solar Dynamics Observatory (SDO) [Pesnell et al. 2012](https://ui.adsabs.harvard.edu/link_gateway/2012SoPh..275....3P/doi:10.1007/s11207-011-9841-3)  | Three instruments:<br><ul><li>Atmospheric Imaging Assembly (AIA) 2 ultraviolet, 1600 & 1700 Å 7 extreme ultraviolet, 94, 131, 171, 193, 211, 304, and 335 Å.</li><li>Helioseismic and Magnetic Imager (HMI) - visible filtergrams processed into: photospheric Dopplergrams line-of-sight magnetograms vector magnetograms.</li><li>EUV Variability Experiment (EVE) - EUV spectral irradiance from 1 to 1050 Å. MEGS disperse EUV light from full disk of the Sun and corona onto a charge coupled device.</li></ul> | 4096x4096 12 second cadence:<br>AIA - [Lemen et al. 2012](https://ui.adsabs.harvard.edu/link_gateway/2012SoPh..275...17L/doi:10.1007/s11207-011-9776-8).<br>HMI - [Hoeksema et al. 2014](https://ui.adsabs.harvard.edu/link_gateway/2014SoPh..289.3483H/doi:10.1007/s11207-014-0516-8).<br>1024 x 2048: <br>EUV - [Woods et al. 2012](https://ui.adsabs.harvard.edu/link_gateway/2012SoPh..275..115W/doi:10.1007/s11207-009-9487-6).<br>Downsampled 512x512/0.6, 512x512/0.5 arcsec 6 (AIA) 12 (HMI) minute cadence for machine learning: [Galvez et al. 2019](https://iopscience.iop.org/article/10.3847/1538-4365/ab1005) via [sdoml.org](sdoml.org). |
 
 ### Models
 | Name 	| Paper	|