Volume 648, April 2021
|Number of page(s)||12|
|Section||The Sun and the Heliosphere|
|Published online||13 April 2021|
Multichannel autocalibration for the Atmospheric Imaging Assembly using machine learning
Heliophysics Science Division, NASA, Goddard Space Flight Center, Greenbelt, MD 20771, USA
2 The Catholic University of America, Washington, DC 20064, USA
3 Rosseland Center for Solar Physics, University of Oslo, PO Box 1029 Blindern, 0315 Oslo, Norway
4 Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, 0315 Oslo, Norway
5 Frontier Development Lab, Mountain View, CA 94043, USA
6 SETI Institute, Mountain View, CA 94043, USA
7 Lockheed Martin Solar & Astrophysics Laboratory (LMSAL), Palo Alto, CA 94304, USA
8 Université Paris-Saclay, CNRS, Institut d’astrophysique spatiale, Orsay, France
9 OATML, Department of Computer Science, University of Oxford, Oxford OX1 3QD, UK
10 Department of Computer Science, University of Oxford, Oxford OX1 3QD, UK
11 Department of Engineering Science, University of Oxford, Oxford OX1 3PJ, UK
Accepted: 29 January 2021
Context. Solar activity plays a quintessential role in affecting the interplanetary medium and space weather around Earth. Remote-sensing instruments on board heliophysics space missions provide a pool of information about solar activity by measuring the solar magnetic field and the emission of light from the multilayered, multithermal, and dynamic solar atmosphere. Extreme-UV (EUV) wavelength observations from space help in understanding the subtleties of the outer layers of the Sun, that is, the chromosphere and the corona. Unfortunately, instruments such as the Atmospheric Imaging Assembly (AIA) on board the NASA Solar Dynamics Observatory (SDO), suffer from time-dependent degradation that reduces their sensitivity. The current best calibration techniques rely on flights of sounding rockets to maintain absolute calibration. These flights are infrequent, complex, and limited to a single vantage point, however.
Aims. We aim to develop a novel method based on machine learning (ML) that exploits spatial patterns on the solar surface across multiwavelength observations to autocalibrate the instrument degradation.
Methods. We established two convolutional neural network (CNN) architectures that take either single-channel or multichannel input and trained the models using the SDOML dataset. The dataset was further augmented by randomly degrading images at each epoch, with the training dataset spanning nonoverlapping months with the test dataset. We also developed a non-ML baseline model to assess the gain of the CNN models. With the best trained models, we reconstructed the AIA multichannel degradation curves of 2010–2020 and compared them with the degradation curves based on sounding-rocket data.
Results. Our results indicate that the CNN-based models significantly outperform the non-ML baseline model in calibrating instrument degradation. Moreover, multichannel CNN outperforms the single-channel CNN, which suggests that cross-channel relations between different EUV channels are important to recover the degradation profiles. The CNN-based models reproduce the degradation corrections derived from the sounding-rocket cross-calibration measurements within the experimental measurement uncertainty, indicating that it performs equally well as current techniques.
Conclusions. Our approach establishes the framework for a novel technique based on CNNs to calibrate EUV instruments. We envision that this technique can be adapted to other imaging or spectral instruments operating at other wavelengths.
Key words: Sun: UV radiation / techniques: image processing / telescopes / Sun: activity / methods: data analysis
© ESO 2021
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