Hello,
I have created a sunpy map using image fits generated using the attached fits file (hsi_image_20141022_140542.fits). The image as generated by hessi package in sswidl is shown attachment "ImageUsingHESSI_IDL.png".
While reading the fits file into sunpy to create the map, I received the following messages:
INFO: Missing metadata for solar radius: assuming the standard radius of the photosphere. [sunpy.map.mapbase]
WARNING: SunpyMetadataWarning: Missing metadata for observer: assuming Earth-based observer.
For frame 'heliographic_stonyhurst' the following metadata is missing: dsun_obs,hglt_obs,hgln_obs
For frame 'heliographic_carrington' the following metadata is missing: crln_obs,crlt_obs,dsun_obs
[sunpy.map.mapbase]
WARNING: IERSStaleWarning: leap-second file is expired. [astropy.utils.iers.iers]
The sunpy map is "SunpyMapFromImageFits.png".
Comparing the two images:
(1) why does the sunpy map "dilute" or "diffuse" some of the structure observed in the sswidl image?
(2) Why are the maximum count flux values different in both the images? the sswidl image has maximum value of 33090, while the sunpy map has ~50000.
Appreciate help in understanding these issues.
Thanks,