NG004-0032
Multi-Channel Auto-Calibration for the Atmospheric Imaging Assembly instrument with Deep Learning

Tuesday, 15 December 2020
Poster
Souvik Bose1, Luiz Fernando Guedes dos Santos2, Valentina Salvatelli3, Brad Neuberg4, Chun Ming Mark Cheung5, Miho Janvier6, Meng Jin3, Yarin Gal7 and Atılım Güneş Baydin8, (1)University of Oslo, Rosseland Center for Solar Physics, Oslo, Norway, (2)Catholic University of America, Physics, Washington, DC, United States, (3)SETI Institute, Mountain View, CA, United States, (4)SETI Institute, Mountain View, United States, (5)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (6)Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, Orsay, France, (7)University of Oxford, Department of Computer Science, Oxford, United Kingdom, (8)University of Oxford, Department of Engineering Science, Oxford, United Kingdom
Abstract:
Solar activity plays a quintessential role in influencing the interplanetary medium and space-weather around the Earth. Remote sensing instruments on-board heliophysics space missions provide a pool of information about the Sun’s activity, via the measurement of its magnetic field and the emission of light from the multi-layered, multi-thermal and dynamic solar atmosphere. Ultraviolet (UV) and Extreme UV (EUV) wavelength observations from space help in understanding the subtleties of the outer layers of the Sun, namely the chromosphere and the corona. Unfortunately, such instruments, like the Atmospheric Imaging Assembly (AIA) onboard NASA's Solar Dynamics Observatory (SDO), suffer time-dependent degradation, that reduces their sensitivity. Current state-of-the-art calibration techniques rely on periodic sounding rockets which can be infrequent and rather unfeasible for deep-space missions. As a part of the Frontier Development Lab (FDL), we devised a convolutional neural network (CNN) based approach to calibrate or compensate for the concerned degradation, as an alternate to the sounding rocket missions. We use SDO-AIA data for our analysis that aims to perform the auto-calibration by exploiting spatial patterns on the solar surface across multi-wavelength observations. Our results show that CNN based models could comprehensively reproduce the outcomes of the sounding rocket experiments within a reasonable degree of accuracy, indicating that it performs equally well when compared with the current techniques. Furthermore, comparison with a standard “astronomer’s technique” (baseline model) reveal that the CNN approach outperforms it quite significantly. This approach establishes the framework for a novel technique to calibrate (E)UV instruments and advance our understanding of the cross-channel relation between different (E)UV channels thereby paving the way to improved forecasting activities. FDL is a NASA co-operative agreement with SETI institute.