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Comparing the Heliospheric Cataloging, Analysis, and Techniques Service (HELCATS) Manual and Automatic Catalogues of Coronal Mass Ejections Using Solar Terrestrial Relations Observatory/Heliospheric Imager (STEREO/HI) Data
We present the results of a comparative study between automatic and manually compiled coronal mass ejection (CME) catalogues based on observations...
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The Lunar Environment Heliophysics X-ray Imager (LEXI) Mission
The Lunar Environment heliospheric X-ray Imager (LEXI) is a wide field-of-view soft X-ray telescope developed to study solar wind-magnetosphere...
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Automatic Solar Flare Detection Using the Solar Disk Imager Onboard the ASO-S Mission
We present an automated solar flare detection software tool to automatically process solar observed images, detect and track solar flares, and...
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Solar X-ray and EUV imager on board the FY-3E satellite
The solar X-ray and Extreme Ultraviolet Imager (X-EUVI), developed by the Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy...
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A Post-Conjunction Re-Evaluation of the Calibration and Long-term Evolution of the STEREO-A Heliospheric Imagers
In two earlier articles (Tappin, Eyles and Davies in Solar Phys. 290 , 2143,
2015 , and Solar Phys. 292 , 28,2017 ), we used the stellar photometry to...
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Backscattered Solar Lyman-\(\alpha \) Emission as a Tool for the Heliospheric Boundary Exploration
This review summarizes our current understanding of the outer heliosphere and local interstellar medium (LISM) inferred from observations and...
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Super-Resolution of SOHO/MDI Magnetograms of Solar Active Regions Using SDO/HMI Data and an Attention-Aided Convolutional Neural Network
Image super-resolution is an important subject in image processing and recognition. Here, we present an attention-aided convolutional neural network...
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Multi-Spacecraft Observations of an Interplanetary Coronal Mass Ejection Interacting with Two Solar-Wind Regimes Observed by the Ulysses and Twin-STEREO Spacecraft
We present a combined study of a coronal mass ejection (CME), revealed in a unique orbital configuration that permits the analysis of remote-sensing...
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Invited Review: Short-term Variability with the Observations from the Helioseismic and Magnetic Imager (HMI) Onboard the Solar Dynamics Observatory (SDO): Insights into Flare Magnetism
Continuous vector magnetic-field measurements by the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO) allow us to...
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Extracting the Heliographic Coordinates of Coronal Rays Using Images from WISPR/Parker Solar Probe
The Wide-field Imager for Solar Probe (WISPR) onboard Parker Solar Probe (PSP), observing in white light, has a fixed angular field of view,...
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Propagation of coronal mass ejections from the Sun to the Earth
Coronal mass ejections (CMEs), as they can inject a large amounts of mass and magnetic flux into the interplanetary space, are the primary source of...
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On the Differences in the Ambient Solar Wind Speed Forecasting Caused by Using Synoptic Maps from Different Observatories
We consider the problem of forecasting the solar wind speed using not only well-known magnetic field data sets, such as the Wilcox Solar Observatory ...
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Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter
On February 21 and March 21 – 22, 2021, the Extreme Ultraviolet Imager (EUI) onboard Solar Orbiter observed three prominence eruptions. The eruptions...
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Defining the Middle Corona
The middle corona, the region roughly spanning heliocentric distances from 1.5 to 6 solar radii, encompasses almost all of the influential physical...
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Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind
The tendency for low-speed solar wind to show greater spatiotemporal variability and different compositional properties from high-speed wind has led...
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Earth’s Exospheric X-ray Emissions
In this chapter we explore solar wind charge exchange X-ray emission emitted from the Earth’s exosphere, following an interaction between heavy ions...
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Solar Radio Burst Prediction Based on a Multimodal Model
Solar radio bursts are intense radio radiation sources that occur during the energy-release process and represent a hot topic in solar-physics and...
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Comparison of Line-of-Sight Magnetic Field Observed by ASO-S/FMG, SDO/HMI and HSOS/SMAT
The Full-disk MagnetoGraph (FMG) onboard the Advanced Space based Solar Observatory has obtained a series of line-of-sight magnetic-field...
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Generating Photospheric Vector Magnetograms of Solar Active Regions for SOHO/MDI Using SDO/HMI and BBSO Data with Deep Learning
Solar activity is often caused by the evolution of solar magnetic fields. Magnetic field parameters derived from photospheric vector magnetograms of...
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The Eruption of 22 April 2021 as Observed by Solar Orbiter: Continuous Magnetic Reconnection and Heating After the Impulsive Phase
We report on one of the first solar-eruptive events that was simultaneously observed by three of the remote-sensing instruments onboard Solar Orbiter...
