The SWAP Filter: A Simple Azimuthally Varying Radial Filter for Wide-Field EUV Solar Images
Authors (first, second and last of 8)
Collection
PROBA-2 at Ten Years
At the time of its launch, PROBA2 was an innovative satellite built for in-flight testing, but also carrying two solar instruments with novel technologies. 10 years later, long past its original life expectancy of 2 years, the PROBA2 mission still delivers unique high-quality measurements and images of the Sun. The LYRA and SWAP instruments have paved the way for new and improved solar observations. This Topical Collection is a follow-up of the 2013 Topical Issue and illustrates how PROBA2 data are used in a wide range of solar studies to this day.
Editors
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Elke D'Huys
Royal Observatory of Belgium
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Marie Dominique
Royal Observatory of Belgium
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Matthew J. West
Royal Observatory of Belgium & SwRI
Articles (11 in this collection)
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A Review of the Extended EUV Corona Observed by the Sun Watcher with Active Pixels and Image Processing (SWAP) Instrument
Authors (first, second and last of 10)
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Comparing the Sun Watcher Using Active Pixel System Detector and Image Processing Instrument to the Atmosphere Imaging Assembly Instrument Through Measurements of Polar Coronal Holes
Authors (first, second and last of 5)
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Observation of a Flare and Filament Eruption in Lyman-\(\alpha \) on 8 September 2011 by the PRoject for OnBoard Autonomy/Large Yield Radiometer (PROBA2/LYRA)
Authors (first, second and last of 6)
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Segmentation of Coronal Features to Understand the Solar EUV and UV Irradiance Variability III. Inclusion and Analysis of Bright Points
Authors (first, second and last of 6)
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Automated Detection of Accelerating Solar Eruptions Using Parabolic Hough Transform
Authors (first, second and last of 6)
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Three-Dimensional Reconstructions of Coronal Wave Surfaces Using a New Mask-Fitting Method
Authors (first, second and last of 8)
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Analysis of Large Deflections of Prominence–CME Events during the Rising Phase of Solar Cycle 24
Authors (first, second and last of 10)
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Investigation of the Middle Corona with SWAP and a Data-Driven Non-Potential Coronal Magnetic Field Model
Authors (first, second and last of 5)
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