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coreyjcochrane · Mar 19, 2024 · 80ac536 · 80ac536
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diff --git a/.doctrees/environment.pickle b/.doctrees/environment.pickle
diff --git a/.doctrees/functions.doctree b/.doctrees/functions.doctree
diff --git a/.doctrees/readme.doctree b/.doctrees/readme.doctree
diff --git a/functions.html b/functions.html
@@ -1702,25 +1702,29 @@ <h3><a class="reference internal" href="#functions.GetModelOpts" title="function
 </li>
 <li><dl class="simple">
 <dt><code class="docutils literal notranslate"><span class="pre">Jupiter</span></code>:</dt><dd><ul>
-<li><p><code class="docutils literal notranslate"><span class="pre">1</span></code>: VIP4 model from Connerney et al. (1998) <a class="reference external" href="https://doi.org/10.1029/97JA03726">https://doi.org/10.1029/97JA03726</a> +
+<li><p><code class="docutils literal notranslate"><span class="pre">1</span></code>: VIP4 model from Connerney et al. (1998) <a class="reference external" href="https://doi.org/10.1029/97JA03726">https://doi.org/10.1029/97JA03726</a>
+(using more precise values from Connerney (2007)
+<a class="reference external" href="https://doi.org/10.1016/B978-044452748-6.00159-0">https://doi.org/10.1016/B978-044452748-6.00159-0</a>) + analytical approximation of
 Connerney et al. (1981) current sheet model <a class="reference external" href="https://doi.org/10.1029/JA086iA10p08370">https://doi.org/10.1029/JA086iA10p08370</a></p></li>
 <li><p><code class="docutils literal notranslate"><span class="pre">2</span></code>: O6 model from Connerney (1992) <a class="reference external" href="https://core.ac.uk/download/pdf/83644007.pdf">https://core.ac.uk/download/pdf/83644007.pdf</a> +
 Khurana (1997) current sheet model <a class="reference external" href="https://doi.org/10.1029/97JA00563">https://doi.org/10.1029/97JA00563</a></p></li>
 <li><p><code class="docutils literal notranslate"><span class="pre">3</span></code>: VIP4 model with O6 model dipole moment orientation + associated current sheet
 model, together from Khurana and Schwarzl (2005) <a class="reference external" href="https://doi.org/10.1029/2004JA010757">https://doi.org/10.1029/2004JA010757</a></p></li>
 <li><p><code class="docutils literal notranslate"><span class="pre">4</span></code>: JRM09 model from Connerney et al. (2018) <a class="reference external" href="https://doi.org/10.1002/2018GL077312">https://doi.org/10.1002/2018GL077312</a>
-+ Connerney et al. (2020) current sheet model <a class="reference external" href="https://doi.org/10.1029/2020JA028138">https://doi.org/10.1029/2020JA028138</a></p></li>
++ analytical version of Connerney et al. (2020) current sheet model
+<a class="reference external" href="https://doi.org/10.1029/2020JA028138">https://doi.org/10.1029/2020JA028138</a></p></li>
 <li><p><code class="docutils literal notranslate"><span class="pre">5</span></code>: JRM09 model from Connerney et al. (2018) <a class="reference external" href="https://doi.org/10.1002/2018GL077312">https://doi.org/10.1002/2018GL077312</a>
-+ Connerney et al. (1981) current sheet model <a class="reference external" href="https://doi.org/10.1029/JA086iA10p08370">https://doi.org/10.1029/JA086iA10p08370</a>
-This model combination is as applied in Vance et al. (2021)
-<a class="reference external" href="https://doi.org/10.1029/2020JE006418">https://doi.org/10.1029/2020JE006418</a></p></li>
-<li><p><code class="docutils literal notranslate"><span class="pre">6</span></code>: VIP4 model from Connerney et al. (1998) <a class="reference external" href="https://doi.org/10.1029/97JA03726">https://doi.org/10.1029/97JA03726</a> +
-Khurana (1997) current sheet model <a class="reference external" href="https://doi.org/10.1029/97JA00563">https://doi.org/10.1029/97JA00563</a> This model
-combination is as applied in Seufert et al. (2011)
-<a class="reference external" href="https://doi.org/10.1016/j.icarus.2011.03.017">https://doi.org/10.1016/j.icarus.2011.03.017</a></p></li>
++ analytical approximation of Connerney et al. (1981) current sheet model
+<a class="reference external" href="https://doi.org/10.1029/JA086iA10p08370">https://doi.org/10.1029/JA086iA10p08370</a>. This model combination is as applied in
+Vance et al. (2021) <a class="reference external" href="https://doi.org/10.1029/2020JE006418">https://doi.org/10.1029/2020JE006418</a></p></li>
+<li><p><code class="docutils literal notranslate"><span class="pre">6</span></code>: VIP4 model from Connerney et al. (1998) <a class="reference external" href="https://doi.org/10.1029/97JA03726">https://doi.org/10.1029/97JA03726</a>
+(using more precise values from Connerney (2007)
+<a class="reference external" href="https://doi.org/10.1016/B978-044452748-6.00159-0">https://doi.org/10.1016/B978-044452748-6.00159-0</a>) + Khurana (1997) current sheet
+model <a class="reference external" href="https://doi.org/10.1029/97JA00563">https://doi.org/10.1029/97JA00563</a> This model combination is as applied in
+Seufert et al. (2011) <a class="reference external" href="https://doi.org/10.1016/j.icarus.2011.03.017">https://doi.org/10.1016/j.icarus.2011.03.017</a></p></li>
 <li><p><code class="docutils literal notranslate"><span class="pre">7</span></code> (or <code class="docutils literal notranslate"><span class="pre">0</span></code>): JRM33 model from Connerney et al. (2021)
-<a class="reference external" href="https://doi.org/10.1029/2021JE007138">https://doi.org/10.1029/2021JE007138</a> + Connerney et al. (2020) current sheet model
-<a class="reference external" href="https://doi.org/10.1029/2020JA028138">https://doi.org/10.1029/2020JA028138</a>.</p></li>
+<a class="reference external" href="https://doi.org/10.1029/2021JE007138">https://doi.org/10.1029/2021JE007138</a> + analytical version of Connerney et al. (2020)
+current sheet model <a class="reference external" href="https://doi.org/10.1029/2020JA028138">https://doi.org/10.1029/2020JA028138</a></p></li>
 </ul>
 </dd>
 </dl>
@@ -2224,15 +2228,16 @@ <h3><a class="reference internal" href="#modelCoeffs.GetGaussCoeffs" title="mode
 <li><dl class="simple">
 <dt><code class="docutils literal notranslate"><span class="pre">Jupiter</span></code></dt><dd><ul>
 <li><p><code class="docutils literal notranslate"><span class="pre">'MagFldJupiterVIP4'</span></code>: “New models of Jupiter’s magnetic field constrained by the
-Io flux tube footprint.” <a class="reference external" href="https://doi.org/10.1029/97JA03726">https://doi.org/10.1029/97JA03726</a>
-(Voyager–Io footprint–Pioneer degree 4 model.)</p></li>
+Io flux tube footprint.” <a class="reference external" href="https://doi.org/10.1029/97JA03726">https://doi.org/10.1029/97JA03726</a> (Voyager–Io flux tube
+footprint–Pioneer degree 4 model.) The values we use are the more precise ones
+reported in “Planetary Magnetism” <a class="reference external" href="https://doi.org/10.1016/B978-044452748-6.00159-0">https://doi.org/10.1016/B978-044452748-6.00159-0</a></p></li>
 <li><p><code class="docutils literal notranslate"><span class="pre">'MagFldJupiterGSFCO4'</span></code>: “The main magnetic field of Jupiter.”
 <a class="reference external" href="https://doi.org/10.1029/JA081i016p02917">https://doi.org/10.1029/JA081i016p02917</a> The PlanetMag implementation is based on the
 update to System III (1965) conventions by Connerney (1992):
 <a class="reference external" href="https://core.ac.uk/download/pdf/83644007.pdf">https://core.ac.uk/download/pdf/83644007.pdf</a>. The model is named GSFC O4 after the
 institution where it was developed (Goddard Spaceflight Center, GSFC) and that it
 includes up to the octupole (degree 3) coefficients from a degree 4 expansion.</p></li>
-<li><p><code class="docutils literal notranslate"><span class="pre">'MagFldJupiterGSFCO6'</span></code>: Coefficients as repoted in “Magnetic Fields of the Outer
+<li><p><code class="docutils literal notranslate"><span class="pre">'MagFldJupiterGSFCO6'</span></code>: Coefficients as reported in “Magnetic Fields of the Outer
 Planets.” <a class="reference external" href="https://doi.org/10.1007/s11214-009-9621-7">https://doi.org/10.1007/s11214-009-9621-7</a>, though originally described in
 Connerney (1992): <a class="reference external" href="https://core.ac.uk/download/pdf/83644007.pdf">https://core.ac.uk/download/pdf/83644007.pdf</a>. Also developed at
 GSFC, this model includes the octupole coefficients from a degree 6 expansion, hence

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