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Merge pull request #152 from sami2py/main
Update develop with release changes
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.. include:: ../CONTRIBUTING.md | ||
.. mdinclude:: ../CONTRIBUTING.md |
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.. _modifications: | ||
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||
Modifications from SAMI2-1.00 | ||
======================================== | ||
============================= | ||
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||
General Updates | ||
--------------- | ||
The calculation for the output step size was adjusted to be closer to the | ||
desired data cadence. | ||
|
||
NRLMSISe-00 | ||
----------- | ||
This version uses the official release of NRLMSISe-00 (with one modification, discussed below). The unmodified version can be found at https://map.nrl.navy.mil/map/pub/nrl/NRLMSIS/NRLMSISE-00/ | ||
This version uses the official release of NRLMSISe-00 (with one modification, | ||
discussed below). The unmodified version can be found at | ||
https://map.nrl.navy.mil/map/pub/nrl/NRLMSIS/NRLMSISE-00/ | ||
|
||
The exospheric neutral temperature can be directly scaled by the user for extreme solar minimum conditions, as discussed by Emmert et al [2010]. This is modified by the ``Tinf_scale`` keyword, and is passed through the namelist as Tinf_scl. | ||
The exospheric neutral temperature can be directly scaled by the user for | ||
extreme solar minimum conditions, as discussed by Emmert et al [2010]. This | ||
is modified by the ``Tinf_scale`` keyword, and is passed through the namelist | ||
as Tinf_scl. | ||
|
||
Photoionization | ||
--------------- | ||
The photoionization rates can be modified by scaling the resultant EUV spectra. Note that this occurs independently of any modifications to the neutral atmosphere through MSIS. See Klenzing et al [2013] for examples. This is modified by the ``euv_scale`` keyword, and is passed through the namelist as euv_scl. | ||
The photoionization rates can be modified by scaling the resultant EUV spectra. | ||
Note that this occurs independently of any modifications to the neutral | ||
atmosphere through MSIS. See Klenzing et al [2013] for examples. This is | ||
modified by the ``euv_scale`` keyword, and is passed through the namelist as | ||
euv_scl. | ||
|
||
ExB Drifts | ||
---------- | ||
Fejer-Scherliess remains the default model for drifts, but the user may now input a series of Fourier coefficients to describe the ExB drifts as a function of local time rather than use the Fejer-Scherliess model. The coefficients are specified by the ``ExB_drifts`` keyword, which are passed into sami2 through the new exb.inp file. The fourier coefficient routine replaces the sine wave triggered when .fejer. = false. | ||
Fejer-Scherliess remains the default model for drifts, but the user may now | ||
input a series of Fourier coefficients to describe the ExB drifts as a function | ||
of local time rather than use the Fejer-Scherliess model. The coefficients are | ||
specified by the ``ExB_drifts`` keyword, which are passed into sami2 through | ||
the new exb.inp file. The fourier coefficient routine replaces the sine wave | ||
triggered when .fejer. = false. | ||
|
||
Horizontal Wind Model | ||
--------------------- | ||
Sami2py uses the HWM-14 model by default. Users may specify HWM93 or HWM07 for comparison through the ``hwm_model`` keyword, which is passed through the namelist as hwm_mod. | ||
Sami2py uses the HWM-14 model by default. Users may specify HWM93 or HWM07 for | ||
comparison through the ``hwm_model`` keyword, which is passed through the | ||
namelist as hwm_mod. |
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numpydoc | ||
ipython | ||
m2r2 | ||
numpydoc |
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matplotlib | ||
netCDF4 | ||
numpy | ||
pandas | ||
xarray | ||
matplotlib | ||
scipy | ||
xarray |
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