Physics & Astrophysics
Paper Review Records
All Paper Review Records
20 valid samples · Newest publication first
Review days = acceptance date − received date. PDF, DOI, and publisher-page sources are retained.
An Enhanced MIMO-Unet Model for CHASE High Resolution H \(\alpha \) Image Deblurring
AuthorsYoucheng Chu; Haoyuan Zhong; Haoyang Zhang; Qingjian Ni
Affiliations1. School of Computer Science and Engineering, Southeast University, Nanjing, China; 2. Key Laboratory of New Generation Artificial Intelligence Technology and Its Interdisciplinary Applications (Southeast University), Ministry of Education, Nanjing, China
Thermal Non-equilibrium Cycles in a Non-eruptive Pseudo-Streamer
AuthorsClara Froment; Sophie Masson
Affiliations1. LPC2E, OSUC, Univ Orleans, CNRS, CNES, Orleans, France; 2. Sorbonne Université, École polytechnique, Institut Polytechnique de Paris, Université Paris Saclay, Observatoire de Paris, Université PSL, CNRS, Laboratoire de Physique des Plasmas (LPP), Paris, France; 3. Observatoire Radioastronomique de Nançay, Observatoire de Paris, CNRS, PSL, Université d’Orléans, Nançay, France
Exploring Coronal Holes Through K-Band Radio Observations (18 – \(26\text{ GHz}\) ) with INAF Radio Telescopes
AuthorsMarco Marongiu; Giulia Murtas; Alberto Pellizzoni; Sara Mulas; Maria Noemi Iacolina; Simona Righini; Elise Egron; Abimael Xavier Barbosa Amaro; Adriana Marcucci; Massimiliano Oranges; Davide Napolitano; Maddalena Sirigu; Mauro Messerotti; Salvatore Luigi Guglielmino; Alessandra Zanichelli; Vincenzo Andretta; Serena Maria Lezzi; Luca Schirru; Adelaide Ladu; Pierluigi Ortu; Giuseppe Valente; Mauro Pili; Tonino Pisanu; Giampaolo Serra; Alessandro Cabras; Andrea Melis; Pasqualino Marongiu; Alessandro Navarrini; Giuseppe Pupillo; Mattia Mancini; Pietro Zucca
Affiliations1. Cagliari Astronomical Observatory, INAF, Selargius, Italy; 2. Center for Kinetic Plasma Physics, West Virginia University, Morgantown, USA; 3. University of Hawai’i at Mānoa, Honolulu, USA; 4. c/o Cagliari Astronomical Observatory, ASI, Selargius, Italy; 5. Institute of Radio Astronomy, INAF, Bologna, Italy; 6. CNMCA, Italian Air Force, Pomezia, Italy; 7. Department of Environmental Sciences, Informatics and Statistics, Ca’ Foscari University of Venice, Venezia Mestre, Italy; 8. Department of Physics and Astronomy “Augusto Righi”, University of Bologna, Bologna, Italy; 9. Department of Physics, University of Cagliari, Monserrato, Italy; 10. Trieste Astronomical Observatory, INAF, Trieste, Italy; 11. Department of Physics, University of Trieste, Trieste, Italy; 12. Catania Astrophysical Observatory, INAF, Catania, Italy; 13. Capodimonte Astronomical Observatory, INAF, Napoli, Italy; 14. Euro-Mediterranean Center on Climate Change, CMCC Foundation, Lecce, Italy; 15. Central Development Laboratory, NRAO, Charlottesville, USA; 16. SKA Observatory (SKAO), Jodrell Bank Centre for Astrophysics, Macclesfield, UK; 17. ASTRON - The Netherlands Institute for Radio Astronomy, Dwingeloo, The Netherlands
Polarimetric Calibration of the Tunable Magnetograph for the Sunrise III Mission
AuthorsAntonio Campos-Jara; Alberto Álvarez-Herrero; Pilar García Parejo; Daniel Garranzo-García; Pablo Santamarina Guerrero; Francisco Javier Bailén; Alex Feller; Achim Gandorfer; David Orozco Suárez; Jose Carlos del Toro Iniesta
Affiliations1. Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain; 2. Spanish Space Solar Physics Consortium (S³PC); 3. Instituto de Astrofísica de Andalucía (IAA-CSIC), Granada, Spain; 4. Max Planck Institute for Solar System Research (MPS), Göttingen, Germany
On the Relation Between Upflow Velocities and Coronal Non-thermal Velocities as Measured by Hinode/EIS
AuthorsAnna Manou; Miho Janvier; Deborah Baker; Pascal Démoulin; Lidia van Driel-Gesztelyi; Stephanie L. Yardley
Affiliations1. CNRS, Institut d’Astrophysique Spatiale, Université Paris-Saclay, Orsay, France; 2. Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark; 3. European Space Agency, ESTEC, Noordwijk, The Netherlands; 4. Mullard Space Science Laboratory, University College London, Surrey, UK; 5. LIRA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France; 6. Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Budapest, Hungary; 7. Department of Mathematics, Physics and Electrical Engineering, Northumbria University, Newcastle Upon Tyne, UK; 8. Donostia International Physics Center (DIPC), San Sebastián, Spain
The Wide Field Imager (WFI) Instruments for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)
AuthorsGlenn T. Laurent; Craig E. DeForest; Matt N. Beasley; Nicholas F. Erickson; Roy R. Graham; Mary H. Hanson; J. Marcus Hughes; Derek A. Lamb; Reith Nolan; Steve Osterman; Trent Peterson; Michael Shoffner; Kelly D. Smith; Travis Smith; Todd Veach; William L. Wells; Alexander J. Wilson
Affiliations1. Southwest Research Institute, Boulder, USA; 2. Southwest Research Institute, San Antonio, USA
Spatiotemporal Machine-Learning Detection of Coronal Mass Ejections in SOHO/LASCO C2 Images
AuthorsTomasz J. Łaguz; Grzegorz Michałek; Adam A. Zychowicz; Seiji Yashiro
Affiliations1. Astronomical Observatory of the Jagiellonian University, Kraków, Poland; 2. Doctoral School of Exact and Natural Sciences, Jagiellonian University, Kraków, Poland; 3. Catholic University of America, Washington, USA; 4. NASA Goddard Space Flight Center, Greenbelt, USA
Prediction of Solar Activity Using Neutrosophic Fuzzy Time Series: A Study of Yearly and Monthly Hemispherical SSNs
AuthorsGeeta Mathpal; Arvind Bhatt; Rajesh Mathpal; Meenakshi Rana
Affiliations1. Department of Mathematics, School of Sciences, Uttarakhand Open University, Haldwani, India; 2. Department of Physics, School of Sciences, Uttarakhand Open University, Haldwani, India
On Prediction of Solar Wind Speed Large-Scale Structures Using the Solar Full-Disk Multi-Layer Magnetograph - the New Chinese Facility Constructed for the International Meridian Circle Program
AuthorsM. L. Demidov; X. F. Wang; Y. Z. Sun; Y. Y. Deng
Affiliations1. Institute of Solar-Terrestrial Physics of Siberian Branch of Russian Academy of Sciences (ISTP SB RAS), Irkutsk, Russia; 2. National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China; 3. State Key Laboratory of Solar Activity and Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China; 4. School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing, China
The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: An Instrument for SUNRISE III
AuthorsY. Katsukawa; J. C. del Toro Iniesta; S. K. Solanki; M. Kubo; H. Hara; T. Shimizu; T. Oba; Y. Kawabata; T. Tsuzuki; F. Uraguchi; K. Shinoda; T. Tamura; Y. Suematsu; T. Matsumoto; R. T. Ishikawa; Y. Naito; K. Ichimoto; S. Nagata; T. Anan; D. Orozco Suárez; E. Sanchis Kilders; M. Balaguer Jiménez; A. C. López Jiménez; C. Quintero Noda; D. Álvarez García; J. L. Ramos Más; J. P. Cobos Carrascosa; P. Labrousse; B. Aparicio del Moral; A. Sánchez Gómez; D. Hernández Expósito; E. Bailón Martínez; J. M. Morales Fernández; A. Moreno Mantas; A. Tobaruela; I. Bustamante; F. J. Bailén; J. Blanco Rodríguez; J. L. Gasent Blesa; P. Rodríguez Martínez; A. Ferreres; D. Gilabert Palmer; J. Piqueras Carreño; I. Pérez Grande; I. Torralbo; A. Álvarez-Herrero; A. Korpi-Lagg; A. Gandorfer; T. Berkefeld; P. Bernasconi; A. Feller; T. L. Riethmüller; H. N. Smitha; V. Martínez Pillet; B. Grauf; A. Bell; M. Carpenter
Affiliations1. National Astronomical Observatory of Japan, Tokyo, Japan; 2. The Graduate University for Advanced Studies, SOKENDAI, Tokyo, Japan; 3. Department of Astronomy, Graduate School of Science, The University of Tokyo, Tokyo, Japan; 4. Instituto de Astrofísica de Andalucía (IAA-CSIC), Granada, Spain; 5. Spanish Space Solar Physics Consortium, S3PC; 6. Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany; 7. Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, Sagamihara, Japan; 8. Advanced Research Center for Space Science and Technology, Institute of Science and Engineering, Kanazawa University, Kanazawa, Japan; 9. Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Japan; 10. National Institute of Fusion Science, Toki, Japan; 11. Kwasan and Hida Observatory, Kyoto Univ., Takayama, Japan; 12. National Solar Observatory, Makawao, USA; 13. Universitat de Valencia, Burjassot, Spain; 14. Instituto de Astrofísica de Canarias, La Laguna, Spain; 15. Departamento de Astrofísica, Univ. de La Laguna, La Laguna, Spain; 16. Universidad Politécnica de Madrid, Madrid, Spain; 17. Instituto Nacional de Técnica Aeroespacial (INTA), Torrejón de Ardoz, Spain; 18. Institut für Sonnenphysik, Freiburg, Germany; 19. Johns Hopkins Applied Physics Laboratory, Laurel, USA
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