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Space-weather HMI Active Region Patch (SHARP)
SHARP stands for Space-weather HMI Active Region Patch. A SHARP is a DRMS series that contains (1) various space-weather quantities calculated from the photospheric vector... -
SHARP Near-Real-Time Data
SHARP Near Real Time data in CCD coordinates. SHARP stands for Space-weather HMI Active Region Patch. A SHARP is a DRMS series that contains (1) various space-weather quantities... -
SHARP Cylindrical-Equal-Area Data
SHARP stands for Space-weather HMI Active Region Patch. A SHARP is a DRMS series that contains (1) various space-weather quantities calculated from the photospheric vector... -
SHARP Near-Real-Time Cylindrical-Equal-Area Data
SHARP Near Real Time data in the Cylindrical Equal Area (CEA) Cartesian coordinate. SHARP stands for Space-weather HMI Active Region Patch. A SHARP is a DRMS series that... -
SDO/HMI Linewidth, 720-Second Data
The linewidth observable refers to the FWHM of the (assumed) Gaussian absorption line profile for the 6173.3 Å line on the surface of the sun. HMI samples the Fe I absorption... -
SDO/HMI Linewidth, 45-Second Data
The linewidth observable refers to the FWHM of the (assumed) Gaussian absorption line profile for the 6173.3 Å line on the surface of the sun. HMI samples the Fe I absorption... -
SDO/HMI Linedepth, 720-Second Data
The HMI Linedepth refers to the difference in intensity between the "true" continuum and intensity at the core of the the Fe I absorption line at 6173.3 Å on the surface of the... -
SDO/HMI Linedepth, 45-Second Data
The HMI Linedepth refers to the difference in intensity between the "true" continuum and intensity at the core of the the Fe I absorption line at 6173.3 Å on the surface of the... -
SDO/HMI line-of-sight Magnetogram, 720-Second Data
Magnetograms are maps of the observed solar magnetic field in the photosphere. The line-of-sight component of the field can be accurately measured as it evolves in time over the... -
SDO/HMI line-of-sight Magnetogram, 45-Second Data
Magnetograms are maps of the observed solar magnetic field in the photosphere. The line-of-sight component of the field can be accurately measured as it evolves in time over the... -
SDO/HMI line-of-sight Dopplergram, 720-Second Data
Dopplergrams are maps of solar surface velocity. The HMI (Camera 2) instrument takes 72 filtergrams to construct a single dopplergram. Six filtergrams are taken in six positions... -
SDO/HMI line-of-sight Dopplergram, 45-Second Data
Dopplergrams are maps of solar surface velocity. The HMI (Camera 2) instrument takes 72 filtergrams to construct a single dopplergram. Six filtergrams are taken in six positions... -
SDO/HMI Continuum, 720-Second Data
The HMI continuum data refers to map of the continuum intensity of the solar spectrum in the region of the Fe I absorption line at 6173 Å on the surface of the sun. HMI samples... -
SDO/HMI Continuum, 45-Second Data
The HMI continuum data refers to map of the continuum intensity of the solar spectrum in the region of the Fe I absorption line at 6173 Å on the surface of the sun. HMI samples... -
SDO/EVE Level 4 Version 8 Data
The Laboratory for Atmospheric and Space Physics in Boulder, Colorado created Level 4 data files for the NASA Solar Dynamics Observatory (SDO) Extreme Ultraviolet Variability... -
SDO/EVE Level 3 Version 8 Data
EVE level 3 data files were created at the Laboratory for Atmospheric and Space Physics in Boulder, Colorado for the NASA Solar Dynamics Observatory (SDO) Extreme Ultraviolet... -
SDO/EVE Level 3 Version 8 Mission-Long Data
EVE level 3 data files were created at the Laboratory for Atmospheric and Space Physics in Boulder, Colorado for the NASA Solar Dynamics Observatory (SDO) Extreme Ultraviolet... -
SDO/EVE Level 2B Version 8 Data
EVE level 2B data files were created at the Laboratory for Atmospheric and Space Physics in Boulder, Colorado for the NASA Solar Dynamics Observatory (SDO) Extreme Ultraviolet... -
SDO/EVE Level 2 Version 8 Data
EVE level 2 data files were created at the Laboratory for Atmospheric and Space Physics in Boulder, Colorado for the NASA Solar Dynamics Observatory (SDO) Extreme Ultraviolet... -
SDO/EVE Level 1 Version 8 Data
The SDO EVE ESP Level 1 data files are created by the Laboratory for Atmospheric and Space Physics in Boulder, Colorado for the NASA Solar Dynamics Observatory (SDO) Extreme...