Added esis.data.synth.scene_aia(), a function to download AIA imagery and convert it into a synthetic scene.

.github/workflows/docs.yml

@@ -32,7 +32,7 @@ jobs:
       - name: Set up Python
         uses: actions/setup-python@v5
         with:
-          python-version: '3.11'
+          python-version: '3.12'
 
       - name: Install package
         run: |
@@ -42,6 +42,8 @@ jobs:
           pip install -e .[doc]
 
       - name: Build with Sphinx
+        env:
+          JSOC_EMAIL: "roytsmart@gmail.com"
         run: |
           cd ./docs
           make html

.github/workflows/tests.yml

@@ -14,7 +14,7 @@ jobs:
       fail-fast: false
       matrix:
         os: [ubuntu-latest, windows-latest, macOS-latest]
-        python-version: ["3.11", "3.12"]
+        python-version: ["3.12", "3.13"]
     name: ${{ matrix.os }}, Python ${{ matrix.python-version }} tests
     steps:
       - name: Set Swap Space
@@ -40,6 +40,7 @@ jobs:
       - name: Test with pytest
         env:
           MPLBACKEND: "agg"
+          JSOC_EMAIL: "roytsmart@gmail.com"
         run: |
           pip install pytest pytest-cov
           pytest --cov=. --cov-report=xml --cov-report=html

docs/conf.py

@@ -113,6 +113,10 @@
 
 nbsphinx_execute = 'always'
 
+suppress_warnings = [
+    'nbsphinx',
+]
+
 codeautolink_custom_blocks = {"jupyter-execute": None}
 
 intersphinx_mapping = {

docs/index.rst

@@ -98,6 +98,7 @@ Flight 1 (2019)
 
     reports/point-spread-function
     reports/throughput
+    reports/aia-image-simulation
     reports/level-0
     reports/level-1
 

docs/refs.bib

@@ -85,4 +85,86 @@ @article{Poletto2004
     doi = {10.1364/AO.43.002029},
     abstract = {Performances are presented of three classes of imaging slit spectrometers for extended sources with aberration-corrected gratings. A general analytical expression for minimizing off-axis grating aberrations is obtained, and it is demonstrated that these aberrations are minimized when the spectrometer is operated at a magnification higher than unity. Classical designs with toroidal uniform-line-spaced (TULS) or spherical varied-line-space (SVLS) gratings are compared with a new class of designs that utilize toroidal varied-line-space (TVLS) gratings. Although TULS and SVLS designs with two stigmatic points can be designed to operate at near-unity magnification with excellent on-axis spectral and spatial resolutions, they cannot be made to satisfy the general off-axis condition, and so their off-axis performances are not optimum. On the contrary TVLS designs with two stigmatic points can be operated at almost any magnification, thus satisfying the off-axis condition perfectly. Such designs are suitable for imaging spectrometer observations that require an extended field of view.},
 }
+@ARTICLE{Vernazza1978,
+       author = {{Vernazza}, J.~E. and {Reeves}, E.~M.},
+        title = "{Extreme ultraviolet composite spectra of representative solar features.}",
+      journal = {\apjs},
+     keywords = {Far Ultraviolet Radiation, Line Spectra, Solar Spectra, Spectrum Analysis, Tables (Data), Ultraviolet Spectra, Astronomical Photometry, Solar Corona, Solar Cycles, Solar Physics, Extreme UV:Sun, Solar Spectrum: Line Identifications},
+         year = 1978,
+        month = aug,
+       volume = {37},
+        pages = {485-513},
+          doi = {10.1086/190539},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/1978ApJS...37..485V},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+@dataset{Dere1997,
+       author = {{Dere}, K.~P. and {Landi}, E. and {Mason}, H.~E. and {Monsignori Fossi}, B.~C. and {Young}, P.~R.},
+        title = "{VizieR Online Data Catalog: CHIANTI - An Atomic Database For Emission Lines I. (Dere+ 1997)}",
+ howpublished = {VizieR On-line Data Catalog: J/A+AS/125/149. Originally published in: 1997A\&AS..125..149D},
+         year = 1997,
+        month = apr,
+          eid = {J/A+AS/125/149},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/1997yCat..41250149D},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+@article{Doschek2004,
+    doi = {10.1086/379877},
+    url = {https://doi.org/10.1086/379877},
+    year = {2004},
+    month = {jan},
+    publisher = {},
+    volume = {600},
+    number = {2},
+    pages = {1061},
+    author = {Doschek, G. A. and Feldman, U.},
+    title = {Properties of the Lower Transition Region: The Widths of Optically Allowed and Intersystem Spectral Lines},
+    journal = {The Astrophysical Journal},
+    abstract = {The widths of spectral lines in the ultraviolet (UV) and extreme ultraviolet (EUV) spectral regions that are formed in the solar transition region and corona are usually greater than the optically thin widths due to thermal Doppler broadening calculated under the assumption of ionization equilibrium. Although opacity can explain the widths of some lines, there are a host of optically thin lines for which the excess widths are attributed to nonthermal motions. Interest in these motions for coronal heating theories has led to the measurement and comparison of spectral line profiles/widths throughout the solar UV and EUV spectrum. We find that for the quiet Sun the widths of some optically allowed lower transition region lines, deduced from spectra obtained by the Solar Ultraviolet Measurements of Ultraviolet Radiation (SUMER) spectrometer on the Solar and Heliospheric Observatory (SOHO) spacecraft, are considerably larger than predicted from simply scaling previously measured wavelengths of other lines from the same ion. For example, the O III lines of the multiplet near 834 Å are considerably wider than predicted from the previously measured (from Skylab) width of the optically thin O III 1666.15 Å intersystem line. The excess widths are not due to nonthermal motions, as these are already included in the width of the 1666.15 Å line. In this paper, we analyze the widths of some prominent optically allowed lines and discuss possible causes for discrepancies with previous measurements of intersystem lines.}
+}
+@ARTICLE{Peter1999,
+       author = {{Peter}, H.},
+        title = "{The Chromosphere in Coronal Holes and the Quiet-Sun Network: an HE I (584 {\r{A}}) Full-Disk Scan by SUMER/SOHO}",
+      journal = {\apjl},
+     keywords = {SUN: SOLAR WIND, SUN: CHROMOSPHERE, SUN: CORONA, Sun: Solar Wind, Sun: Chromosphere, Sun: Corona},
+         year = 1999,
+        month = sep,
+       volume = {522},
+       number = {1},
+        pages = {L77-L80},
+          doi = {10.1086/312214},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/1999ApJ...522L..77P},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+@ARTICLE{Lemen2012,
+       author = {{Lemen}, James R. and {Title}, Alan M. and {Akin}, David J. and {Boerner}, Paul F. and {Chou}, Catherine and {Drake}, Jerry F. and {Duncan}, Dexter W. and {Edwards}, Christopher G. and {Friedlaender}, Frank M. and {Heyman}, Gary F. and {Hurlburt}, Neal E. and {Katz}, Noah L. and {Kushner}, Gary D. and {Levay}, Michael and {Lindgren}, Russell W. and {Mathur}, Dnyanesh P. and {McFeaters}, Edward L. and {Mitchell}, Sarah and {Rehse}, Roger A. and {Schrijver}, Carolus J. and {Springer}, Larry A. and {Stern}, Robert A. and {Tarbell}, Theodore D. and {Wuelser}, Jean-Pierre and {Wolfson}, C. Jacob and {Yanari}, Carl and {Bookbinder}, Jay A. and {Cheimets}, Peter N. and {Caldwell}, David and {Deluca}, Edward E. and {Gates}, Richard and {Golub}, Leon and {Park}, Sang and {Podgorski}, William A. and {Bush}, Rock I. and {Scherrer}, Philip H. and {Gummin}, Mark A. and {Smith}, Peter and {Auker}, Gary and {Jerram}, Paul and {Pool}, Peter and {Soufli}, Regina and {Windt}, David L. and {Beardsley}, Sarah and {Clapp}, Matthew and {Lang}, James and {Waltham}, Nicholas},
+        title = "{The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)}",
+      journal = {\solphys},
+     keywords = {Solar corona, Solar instrumentation, Solar imaging, Extreme ultraviolet},
+         year = 2012,
+        month = jan,
+       volume = {275},
+       number = {1-2},
+        pages = {17-40},
+          doi = {10.1007/s11207-011-9776-8},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2012SoPh..275...17L},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+@ARTICLE{Pesnell2012,
+       author = {{Pesnell}, W. Dean and {Thompson}, B.~J. and {Chamberlin}, P.~C.},
+        title = "{The Solar Dynamics Observatory (SDO)}",
+      journal = {\solphys},
+     keywords = {SDO, Solar cycle, Helioseismology, Coronal, Space weather},
+         year = 2012,
+        month = jan,
+       volume = {275},
+       number = {1-2},
+        pages = {3-15},
+          doi = {10.1007/s11207-011-9841-3},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2012SoPh..275....3P},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+
+