From fda855deb0dc3e3c1c6118d5e0ad6dafced3857b Mon Sep 17 00:00:00 2001 From: Nick Murphy Date: Sun, 28 Jul 2024 22:01:43 -0400 Subject: [PATCH] Minor notebook update --- docs/source/notebooks/particles-formulary-completed.ipynb | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/docs/source/notebooks/particles-formulary-completed.ipynb b/docs/source/notebooks/particles-formulary-completed.ipynb index 3b6ece2..c2f5f3a 100644 --- a/docs/source/notebooks/particles-formulary-completed.ipynb +++ b/docs/source/notebooks/particles-formulary-completed.ipynb @@ -1091,7 +1091,7 @@ "\n", "When the reconnection layer thickness is shorter than the **ion inertial length**, $d_i ≡ c/ω_{pi}$, collisionless effects and the Hall effect enable reconnection to be fast (Zweibel & Yamada 2009). The inner electron diffusion region has a thickness of about the **electron inertial length**, $d_e ≡ c/ω_{pi}$. (Here, $ω_{pi}$ and $ω_{pe}$ are the ion and electron plasma frequencies.)\n", "\n", - "**Our goal: calculate $d_i$ and $d_e$ to get an idea of how far the MMS spacecraft should be separated from each other to investigate reconnection.**" + "Our goal: calculate $d_i$ and $d_e$ to get an idea of how far the MMS spacecraft should be separated from each other to investigate reconnection." ] }, {