From 0389c17a68bcb8956e75ed332f0f60dd830ab69d Mon Sep 17 00:00:00 2001 From: Paul Wright Date: Sun, 16 May 2021 11:43:37 -0700 Subject: [PATCH] added colab link --- readme.md | 5 +++++ 1 file changed, 5 insertions(+) diff --git a/readme.md b/readme.md index 931881c..47d2cb8 100644 --- a/readme.md +++ b/readme.md @@ -3,6 +3,11 @@ DeepEM: A Deep Learning Approach for DEM Inversion *by Paul Wright et al* [![DOI](https://zenodo.org/badge/155842845.svg)](https://zenodo.org/badge/latestdoi/155842845) +[![Open In Colab](https://colab.research.google.com/assets/colab-badge.svg)](https://colab.research.google.com/github/spaceml-org/helionb-sdoml/blob/main/notebooks/02_temperature_maps_2018/temperature_maps_colab.ipynb) + +May 2021: This work is available to be run (free-of-charge) on Google Colab (link above) using data on the Google Cloud Platform, courtesy of @spaceml-org (https://github.com/spaceml-org/helionb-sdoml/tree/main/notebooks/02_temperature_maps_2018) + +--- The intensity observed through optically-thin SDO/AIA filters (94 Å, 131 Å, 171 Å, 193 Å, 211 Å, 335 Å) can be related to the temperature distribution of the solar corona (the differential emission measure; DEM) as