Immersive Virtual-Reality-Based Streaming Distance Education System for Solar Dynamics Observatory: A Case Study by Joongjae Lee, Jaeheung Surh, Wooseong Choi, Bumjae You

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On the Formation Height of Low-corona and Chromospheric Channels of the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) by Y. Sanjay, S. Krishna Prasad, R. Erdélyi, M. B. Korsós, D. Banerjee, P. S. Rawat

“…The multiwavelength data from the Solar Dynamics Observatory is extensively used in studying the physics of the Sun and its atmosphere. …”
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Heating of Quiescent Coronal Loops Caused by Nearby Eruptions Observed with the Solar Dynamics Observatory and the Solar Upper Transition Region Imager by Leping Li, Hui Tian, Huadong Chen, Hongqiang Song, Zhenyong Hou, Xianyong Bai, Kaifan Ji, Yuanyong Deng

“…In this study, employing data from the Solar Dynamics Observatory (SDO) and Solar Upper Transition Region Imager (SUTRI), we report the heating of quiescent loops associated with nearby eruptions. …”
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Extreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of Science Objectives, Instrument Design, Data Products, and Model Developments by Hock, R., Woodraska, D., Judge, D., Didkovsky, L., Lean, J., Mariska, J., Warren, H., McMullin, D., Chamberlin, P., Bailey, S., Fuller-Rowell, T., Sojka, J., Viereck, R., Woods, T. N., Eparvier, F. G., Jones, A. R., Tobiska, W. K., Berthiaume, Gregory D

“…The Extreme ultraviolet Variability Experiment (EVE) onboard the NASA Solar Dynamics Observatory (SDO) will measure the solar EUV irradiance from 0.1 to 105 nm with unprecedented spectral resolution (0.1 nm), temporal cadence (ten seconds), and accuracy (20%). …”
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Zernike Moments Description of Solar and Astronomical Features: Python Code by Hossein Safari, Nasibe Alipour, Hamed Ghaderi, Pardis Garavand

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Turning Noise Into Data: Characterization of the Van Allen Radiation Belt Using SDO Spikes Data by Spiridon Kasapis, Barbara J. Thompson, Juan V. Rodriguez, Raphael Attie, Gonzalo Cucho‐Padin, Daniel daSilva, Meng Jin, William D. Pesnell

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Handbook of Space and Solar System Exploration in 2010s / by Bower, Keaton, author 648067

“…The Solar Dynamics Observatory ( SDO ) is a NASA mission which will observe the Sun for over five years. …”
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The presence of a systematic error in SDO/HMI data by Rudenko G.V., Dmitrienko I.S.

“…In this paper, we came to the conclusion that there is a systematic error in SDO/HMI (Helioseismic and Magnetic Imager aboard the Solar Dynamics Observatory) vector magnetic data, which reveals itself in a deviation from the radial direction of the knot magnetic fields manifesting themselves on magnetograms in the form of small grains in a strong magnetic field. …”
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3D Reconstruction of Coronal Loops by the Principal Component Analysis by Erwin Verwichte, Valery M. Nakariakov, Giuseppe Nisticò

“…The combination of observations of the Sun from different points of observations in space, thanks to the most recent missions, including the Solar Dynamics Observatory (SDO) and the Solar TErrestrial RElations Observatory (STEREO), allows us to infer information about the geometrical shape of coronal loops in 3D space. …”
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CORONAL JETS AS A CAUSE OF MICROWAVE NEGATIVE BURSTS by I.V. Kuzmenko

“…Analysis of observations in different spectral ranges using images from the Nobeyama radioheliograph and the Solar Dynamics Observatory/Atmospheric Imaging Assembly has shown that the cause of all the three radio emission depressions was the screening of the limb radio source by the material of recurrent coronal jets. …”
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A new Java-based application in solar physics by A. Sarsembayeva, F. Belisarova, M. Odsuren, A. Sarsembay

“…Solar and Heliospheric Observatory, SOHO), numerous perspectives (Solar Terrestrial Relations Observatory, STEREO), and returning a lot of information (Solar Dynamics Observatory, SDO). Specifically, the huge amount of SDO data are accessible only from a few repositories, such type of data as a full-cadence data or full-disk of scientific concern are hard to download, because of their size. …”
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Optimization of Curvilinear Tracing Applied to Solar Physics and Biophysics by Markus J. Aschwanden, Eugene A. Katrukha, Bart De Pontieu

“…Here, we apply an advanced version of this code (OCCULT-2), also, to similar images from the Solar Dynamics Observatory (SDO), to chromospheric H-α images obtained with the Swedish Solar Telescope (SST) and to microscopy images of microtubule filaments in live cells in biophysics. …”
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A center-median filtering method for detection of temporal variation in coronal images by Plowman Joseph

“…Example applications to “EIT waves” (named after EIT, the EUV Imaging Telescope on the Solar and Heliospheric Observatory) and small-scale dynamics are shown, both using 193 Å data from the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory. The technique is found to discriminate EIT waves more cleanly than the running and base difference techniques most commonly used. …”
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Single and Multiwavelength Detection of Coronal Dimming and Coronal Wave Using Faster R-CNN by Zongxia Xie, Chunyang Ji

“…In addition, we have collected and processed a dataset that includes the solar images and event records, where the solar images come from the Atmospheric Imaging Assembly (AIA) of Solar Dynamics Observatory (SDO) and the event records come from Heliophysics Event Knowledgebase (HEK). …”
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Dynamics and Kinematics of the EUV Wave Event on 6 May 2019 by Ramesh Chandra, P. F. Chen, Pooja Devi, Reetika Joshi, Y. W. Ni

“…The event is thoroughly observed with Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO) with high spatio-temporal resolutions. …”
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Wave Reflection in the Solar Atmosphere by Varun Chaturmutha, Bernhard Fleck, Stuart M. Jefferies

“…We present evidence supporting wave reflection in the lower solar chromosphere based on helioseismic analysis of multi-height Doppler data from the Solar Dynamics Observatory/Helioseismic and Magnetic Imager and the Magneto-Optical filters at Two Heights II instrument. …”
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Quasi-Periodic Pulsations in an M-Class Solar Flare by Jun Xu, Zongjun Ning, Dong Li, Fanpeng Shi

“…Based on the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO), we find that the QPPs take place at the same time interval as the flare ribbon separation, and that the QPPs seem to originate from the flare ribbons. …”
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One-Minute Quasi-Periodic Pulsations during an M-Class Solar Flare by Fanpeng Shi, Dong Li, Zongjun Ning

“…Using the data from the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO), the intermittent jets are detected and the interesting fact is that the jets also display one-minute period. …”
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Using Polar Faculae to Determine the Sun’s High-latitude Rotation Rate. II. Simulations and New Measurements by Neil R. Sheeley Jr.

“…Applying this spacetime tracking procedure to magnetic flux elements observed with the Helioseismic Magnetic Imager on the Solar Dynamics Observatory, I obtained a similar rotation profile with a speed of 9.55° day ^−1 and a synodic rotation period of 37.7 days. …”
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Solar active region magnetogram image dataset for studies of space weather by Laura E. Boucheron, Ty Vincent, Jeremy A. Grajeda, Ellery Wuest

“…Abstract In this dataset we provide a comprehensive collection of line-of-sight (LOS) solar photospheric magnetograms (images quantifying the strength of the photospheric magnetic field) from the National Aeronautics and Space Administration’s (NASA’s) Solar Dynamics Observatory (SDO). The dataset incorporates data from three sources and provides SDO Helioseismic and Magnetic Imager (HMI) magnetograms of solar active regions (regions of large magnetic flux, generally the source of eruptive events) as well as labels of corresponding flaring activity. …”
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