Changelog#
0.9.2.dev1+g68b6ce7 (2024-09-24)#
Bug Fixes#
Use
reference_date
when constructing an observer coordinate and in place of pullingT_OBS
directly from the header. (#345)
0.9.1 (2024-07-23)#
Bug Fixes#
Fixed Spike issue with data being loaded as floats.
0.9.0 (2024-07-22)#
Breaking Changes#
All inputs and outputs that previously used “counts” or “ct” now use “DN”. (#338)
Minimum version of
sunpy
supported is nowsunpy
6.0.0
0.8.0 (2024-05-11)#
Breaking Changes#
Removed the
aiapy.calibrate.normalize_exposure
function. The same functionality can be achieved by dividing aMap
by the exposure time property,my_map / my_map.exposure_time
. (#182)All the functions in aiapy, that took keywords have been made to only accept them as keyword arguments. This means that you can no longer pass them as positional arguments. (#313)
Removed
setup.cfg
andsetup.py
files, this means you will need to use a modern version of pip (23.0 or above) to install this package now. (#313)Increased the minimum version of Python to 3.10 (#313)
Downgraded warning for Multiple Valid Epochs (
aiapy.util.util._select_epoch_from_correction_table
) to a logging debug message. (#318)
New Features#
Added extra mirrors to fetch files from SSW. (#322)
Documentation#
Cleaned up notes on AIA data preparation and included respiking procedure in the list of steps. (#182)
Transformed the documentation layout. (#318)
Fixed incorrect IDL routine reference in the
aiapy.calibrate.estimate_error
documentation. (#322)Improved the “Requesting specific AIA images from the JSOC” Example to animate and use Fido instead of DRMS. (#323)
Internal Changes#
Catch all
erfa.core.ErfaWarning
that are raised when we convert the times from the error and degradation tables into UTC while making themastropy.time.Time
objects. (#324)
0.7.4 (2023-10-31)#
Bug Fixes#
Fixed mismatch with the sample data downloder.
Fixed theme build to use the new sunpy theme.
0.7.3 (2023-04-05)#
Bug Fixes#
Fixed missing citation. (#177)
0.7.3 (2023-04-05)#
Bug Fixes#
Fixed missing citation. (#177)
0.7.2 (2023-01-18)#
Breaking Changes#
Removed kwargs from
correct_degradation
,degradation
to ensure that the correct keywords are passed into these functions and the function calls that require these keywords. (#170)Several private internal functions now raise
ValueError
instead ofIndexError
, some of these will now be raised to the user when callingcorrect_degradation
, therefore any code that checks for this error type will need updating. (#170)
Bug Fixes#
Documentation#
Added a warning about
register
that it will not return a 4096 by 4096 Map, but most likely a 4094 by 4094 Map. (#170)
Trivial Changes#
Added several tests to ensure that
degradation
works on all wavelengths and the ones it does not, raise the correct error. (#170)
0.7.1 (2022-11-28)#
Bug Fixes#
Change SSW mirror due to the old one being down. (#167)
0.7 (2022-08-04)#
Breaking Changes#
Minimum version of
Python
supported is nowPython
3.8.0. (#159)Minimum version of
sunpy
supported is nowsunpy
4.0.0 LTS. (#159)aiapy.calibrate.register()
use_scipy
keyword has been removed and replaced with amethod
keyword that defaults to usescipy
by default. It is also possible to usescikit-image
oropencv
orcupy
(provided you have either one installed.) (#159)
New Features#
Added a “cupy” method to
aiapy.calibrate.register()
that will use cupy to do the affine_transform. (#159)
0.6.4 (2022-01-14)#
Bug Fixes#
Fixes a bug where columns in the pointing table used to update the pointing information were being converted to masked float values. This bugfix ensures that any column used in the pointing update does not have a mask and any values that are masked are filled with NaN. This bug arises in astropy>=5.0. (#151)
Documentation#
Fixed escaping of characters in equations in multiple docstrings. (#146)
0.6.3 (2021-11-05)#
Bug Fixes#
Fixes a bug in
aiapy.calibrate.update_pointing
concerning how the row in 3-hourly master pointing table is chosen. Previously, the row withT_START
closest toDATE_OBS
was chosen. Now, the row corresponding toT_OBS
greater than or equal toT_START
AND less thanT_STOP
is chosen. (#137)Update the
x0_mp
andy0_mp
keywords when updating the pointing information inaiapy.calibrate.update_pointing
. (#140)
Internal Changes#
In the case where a submap is passed into
aiapy.calibrate.fetch_spikes
, create the full-frame WCS directly from the submap WCS rather than creating an intermediate dummy full-frame map. (#139)
0.6.2 (2021-11-02)#
Bug Fixes#
Fixed a bug in the units on the table returned by
aiapy.calibrate.util.get_pointing_table
. TheX0
andY0
columns were incorrectly being assigned units of arcseconds instead of pixels. (#132)Fixed an off-by-one bug in
aiapy.calibrate.update_pointing
where theCRPIX1
andCRPIX2
keywords were not being properly updated from theX0
andY0
columns in the master pointing table. (#132)
0.6.1 (2021-11-01)#
Bug Fixes#
Fixed a compatibility issue with sunpy>=3.1 in which creating a full-frame WCS in
aiapy.calibrate.fetch_spikes
was throwing an exception. (#126)Added a check on
aiapy.calibrate.update_pointing
so that passing in a submap or a map not at the full AIA resolution, raises an exception. (#127)
0.6.0 (2021-10-27)#
Breaking Changes#
Pin minimum version of Python to 3.7 (#114)
Pin minimum version of sunpy to 3.0.0 LTS.
New Features#
Added a new function
aiapy.util.telescope_number()
that returns the associated telscope number for a given filter wavelength. (#116)Added a new function
aiapy.calibrate.util.get_error_table()
to fetch and parse the table with the associate error parameters. This is used primarily inaiapy.calibrate.estimate_error()
. (#116)Added a new function
aiapy.calibrate.estimate_error()
to calculate the error for a given set of AIA counts and the associated channel. This is an exact port of the IDL functionaia_bp_estimate_error
. (#116)
Bug Fixes#
aiapy.calibrate.update_pointing
now skips updating keywords if the pointing values are missing from the pointing table returned from JSOC. (#120)
0.5.1 (2021-05-24)#
Backwards Incompatible Changes#
Pin sunpy dependency to
<=3.0
to allow for backwards compatibility withsearch_metadata
. (#111)
0.5.0 (2021-04-09)#
Features#
Add a flag to
aiapy.psf.deconvolve()
that sets negative intensity values to zero before performing the deconvolution. (#107)
0.4.0 (2020-12-10)#
Features#
Added a function (
aiapy.util.sdo_location()
) to obtain the SDO location at a given time. (#57)Added a function (
aiapy.calibrate.respike()
) for reinserting hot pixels into level 1 images. (#62)Updated default calibration version to 10. Added test for version 10 (#90)
Bug Fixes#
Updated default calibration version number for degradation correction. Added tests for multiple calibration versions (#74)
Fixed a bug where an out of date calibration epoch was used if there were older duplicate versions available in the same epoch. (#90)
aiapy.calibrate.util.get_pointing_table
now raises a more user-friendlyRuntimeError
if no pointing information can be found during the requested times. Previously it would raise aKeyError
. (#91)aiapy.calibrate.update_pointing
now searches 12 hours either side of the map date for pointing information. This allows for some very rare instances where more than 3 hours elapses between pointing information updates. (#91)
0.3.2 (2020-11-29)#
No significant changes.
0.3.1 (2020-11-15)#
Features#
aiapy.calibrate.register()
now raises a warning if the level number is missing or is greater than 1. (#94)
0.3.0 (2020-10-06)#
Features#
Added a function (
aiapy.calibrate.normalize_exposure
) to normalize an image by its exposure time. (#78)aiapy.calibrate.degradation()
can now acceptTime
objects with length greater than 1. This makes it easier to compute the channel degradation over long intervals. (#80)Citation information for
aiapy
is now available fromaiapy.__citation__
. (#82)The pointing table can now be passed in as a keyword argument to
aiapy.calibrate.update_pointing()
. Added aaiapy.calibrate.util.get_pointing_table()
to retrieve the 3-hour pointing table from JSOC over a given time interval. (#84)
Bug Fixes#
The
CROTA2
keyword update inaiapy.calibrate.update_pointing()
now includes the value ofSAT_ROT
from the FITS header. Previously, the keyword was only being updated withINSTROT
. (#84)
0.2.0 (2020-07-16)#
Features#
Functionality for respiking level 1 images and fetching spike data from JSOC
Updated calibration data now fetched from JSOC to account for instrument degradation
Compatibility fix with sunpy > 2.0.0 which previously caused level 1.5 maps to expand by several pixels
Functionality for fetching the location of SDO in time
0.1.0 (2020-03-31)#
Features#
Update pointing keywords in the header using the 3-hour pointing values from the JSOC
Correct Heliographic Stonyhurst observer location
Register images by removing the roll angle, centering the image, and scaling to a common resolution (i.e. “aia_prep”)
Calculate wavelength response functions for all channels, including time-dependent effects
Account for channel degradation in image correction
Compute the point spread function and deconvolve an image with the point spread function (with optional GPU acceleration)