Skip to content

Commit

Permalink
docs: update README.md
Browse files Browse the repository at this point in the history
  • Loading branch information
Beforerr committed Nov 7, 2024
1 parent d4e6765 commit e262cda
Show file tree
Hide file tree
Showing 2 changed files with 44 additions and 36 deletions.
79 changes: 43 additions & 36 deletions README.md
Original file line number Diff line number Diff line change
Expand Up @@ -46,39 +46,46 @@ from discontinuitypy.core import *

<!-- We have developed a pipeline to identify solar wind discontinuities. (Modular, Performant, Scalable) -->

# TODOs

Science part

- Analysis
- [ ] Contribution of discontinuities to the power spectrum
- [ ] Check Datagap
- [ ] Distribution of \|B\| over radius
- [ ] Add error bar
- [ ] More accurate way to obtain the properties of the
discontinuities
- Identifaction
- [ ] Ensemble forest?
- [ ] Smoothing is important?
- [ ] Check change point algorithm
- Features
- [ ] Thickness in N direction
- [ ] Use high resolution data for feature extraction
- Compare with other methods of identifying IDs
- [ ] Verify with other methods of identifying IDs

Code part

- Optimization
- [ ] `dask` for parallel computing instead of `modin`
- [ ] `JAX` library for `numpy` optimization
- [ ] shorten import time
- Refactor
- [x] `process_candidates` to exclude `sat_state` logics
- [x] renaming feature layer `candidates`
- [x] Kedro
- [x] Modular pipelines

### bugs

- [ ] STEREO `B` less than zero (after downsampling?)
# Properties of Discontinuities

Notations:

- $\vec{B}$ : Magnetic field
- $B$ : Magnetic field magnitude

## Outputs

- `b_mag` : mean of magnetic field magnitude across the discontinuity
- `db_over_b` : $|\Delta B|/\bar{B}$ , Change in magnetic field
magnitude over magnetic field magnitude (mean)
- see Fig.14 in Tsurutani and Smith (1979)
- `rotation_angle` : Rotation angle across the discontinuity
- see Fig.12 in Tsurutani and Smith (1979)
- see Fig.11 in Söding et al. (2001)
- `bn_over_b` : $\bar{B}_N/\bar{B}$ : Normal component of magnetic field
over magnetic field magnitude (mean)

<div id="refs" class="references csl-bib-body hanging-indent"
entry-spacing="0">

<div id="ref-sodingRadialLatitudinalDependencies2001" class="csl-entry">

Söding, A., F. M. Neubauer, B. T. Tsurutani, N. F. Ness, and R. P.
Lepping. 2001. “Radial and Latitudinal Dependencies of Discontinuities
in the Solar Wind Between 0.3 and 19 AU and -80$^\circ$ and
+10$^\circ$.” *Annales Geophysicae* 19 (7): 667–80.
<https://doi.org/10.5194/angeo-19-667-2001>.

</div>

<div id="ref-tsurutaniInterplanetaryDiscontinuitiesTemporal1979"
class="csl-entry">

Tsurutani, Bruce T., and Edward J. Smith. 1979. “Interplanetary
Discontinuities: Temporal Variations and the Radial Gradient from 1 to
8.5 AU.” *Journal of Geophysical Research: Space Physics* 84 (A6):
2773–87. <https://doi.org/10.1029/JA084iA06p02773>.

</div>

</div>
1 change: 1 addition & 0 deletions justfile
Original file line number Diff line number Diff line change
Expand Up @@ -13,6 +13,7 @@ publish-qrcode:
publish: pypi-publish quarto-publish

pypi-publish: export
nbdev_readme --path notebooks/index.qmd
pdm publish

test:
Expand Down

0 comments on commit e262cda

Please sign in to comment.