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2 changes: 1 addition & 1 deletion .github/workflows/main.yml
Original file line number Diff line number Diff line change
Expand Up @@ -14,7 +14,7 @@ jobs:
matrix:
os: ["ubuntu-latest", "macos-latest", "windows-latest"]
python-version: ["3.10", "3.11", "3.12", "3.13", "3.14"]
install-extras: ["base", "dmsp_ssj"]
install-extras: ["base", "downloads"]
include:
# Pysat test for only pysat-passing Python version
- python-version: "3.10"
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7 changes: 7 additions & 0 deletions Changelog.rst
Original file line number Diff line number Diff line change
Expand Up @@ -3,6 +3,13 @@ Changelog

Summary of all changes made since the first stable release

1.0.0 (XX-XX-2026)
------------------
* ENH: Added option to download and format AMPERE files
* ENH: Added optional dependencies for AMPERE downloads, as well as all
downloads and all optional dependencies
* DEP: Removed stored AMPERE files

0.7.0 (06-05-2026)
------------------
* ENH: Added the Gussenhoven (1983) model for the EAB
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2 changes: 1 addition & 1 deletion docs/citing.rst
Original file line number Diff line number Diff line change
Expand Up @@ -76,7 +76,7 @@ also includes fits to the R1 and R2 peaks, for those interested.
Electrodynamics Response Experiment, J. Geophys. Res. Space Physics, 120,
doi:10.1002/2015JA021680
* **FAC**: Milan, Stephen (2023). AMPERE R1/R2 FAC radii v2. University of
Leicester. Dataset. https://doi.org/10.25392/leicester.data.22241338.v3
Leicester. Dataset. https://doi.org/10.25392/leicester.data.22241338
* **OCB**: Burrell, A. G., et al. (2020): AMPERE Polar Cap Boundaries,
Ann. Geophys., 38, 481-490, http://doi.org/10.5194/angeo-38-481-2020

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16 changes: 9 additions & 7 deletions docs/ocb_datasets.rst
Original file line number Diff line number Diff line change
Expand Up @@ -46,13 +46,15 @@ AMPERE

OCB data sets can also be obtained from AMPERE (Active Magnetosphere and
Planetary Electrodynamics Response Experiment) R1/R2 Field-Aligned Current (FAC)
boundary data. This data is provided for both hemispheres between 2010-2021,
inclusive. Because there is an offset between the R1/R2 FAC boundary and the
OCB, a correction is required. This correction can be implemented using the
routines in :py:mod:`ocbpy.ocb_correction`.

In the most recent version
(`V2 <https://figshare.le.ac.uk/articles/dataset/AMPERE_R1_R2_FAC_radii_v2/22241338/1>`_)
boundary data. This data may be obtained for both hemispheres between
2010-2024, inclusive, using the downloading and formatting functions in
:py:mod:`ocbpy.boundaries.ampere_r1r2_files`. Because there is an offset
between the R1/R2 FAC boundary and the OCB, a correction is required. This
correction can be implemented using the routines in
:py:mod:`ocbpy.ocb_correction`.

In the most recent
`version <https://figshare.le.ac.uk/articles/dataset/AMPERE_R1_R2_FAC_radii_v2/22241338>`_
of these AMPERE boundary fits, which uses the newly-processed AMPERE data, a fit
for the Heppner-Maynard Boundary (HMB) were also made available. The HMB has
been shown to be related to the equatorward boundary of the auroral oval near
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5 changes: 5 additions & 0 deletions ocbpy/boundaries/__init__.py
Original file line number Diff line number Diff line change
Expand Up @@ -16,3 +16,8 @@
from ocbpy.boundaries import dmsp_ssj_files # noqa F401
except ImportError as ierr:
logger.warning(ierr)

try:
from ocbpy.boundaries import ampere_r1r2_files # noqa F401
except ImportError as ierr:
logger.warning(ierr)
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