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- A. Pouquet2 profiles68 · h 62
- S. McIntosh60 · h 47
- T. Metcalfe2 profiles53 · h 54
- P. Mininni50 · h 47
- W. Chaplin2 profiles41 · h 81
- J. Christensen-Dalsgaard3 profiles39 · h 85
- P. Judge36 · h 35
- S. Mathur3 profiles36 · h 64
- R. Casini2 profiles35 · h 28
- Y. Elsworth2 profiles35 · h 64
- Yuhong Fan2 profiles35 · h 36
- H. Kjeldsen2 profiles34 · h 77
- NSF NCAR High Altitude ObservatoryUS515 papers
- Centre National de la Recherche ScientifiqueFR115 papers
- Instituto de Astrofísica de CanariasES105 papers
- University of Colorado BoulderUS101 papers
- Max Planck Institute for Solar System ResearchDE98 papers
- Lockheed Martin (United States)US70 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR66 papers
- National Solar ObservatoryUS63 papers
- Aarhus UniversityDK62 papers
- Center for Astrophysics Harvard & SmithsonianUS62 papers
- Universidad de La LagunaES62 papers
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR59 papers
26 papers · 1 filter
Coronal Densities, Temperatures and Abundances During the 2019 Total Solar Eclipse: The Role of Multi-Wavelength Observations in Coronal Plasma Characterization
G. Del Zanna, J. Samra, A. Monaghan +7
The Airborne Infrared Spectrometer (AIR-Spec) offers an unprecedented opportunity to explore the Near Infra-Red (NIR) wavelength range. It has been flown at two total solar eclipse…
A Machine Learning Enhanced Approach for Automated Sunquake Detection in Acoustic Emission Maps
Vanessa Mercea, Alin Razvan Paraschiv, Daniela Adriana Lacatus +2
Sunquakes are seismic emissions visible on the solar surface, associated with some solar flares. Although discovered in 1998, they have only recently become a more commonly detecte…
Small-scale loops heated to transition region temperatures and their chromospheric signatures in the simulated solar atmosphere
M. Skan, S. Danilovic, J. Leenaarts +2
Recent observations revealed loop-like structures at very small scales visible in observables that sample transition region (TR) and coronal temperatures. Their formation remains u…
Optimal spectral lines for measuring chromospheric magnetic fields
P. Judge, P. Bryans, R. Casini +4
This paper identifies spectral lines from X-ray to infrared wavelengths which are optimally suited to measuring vector magnetic fields as high as possible in the solar atmosphere.…
Data-constrained MHD simulation for the eruption of a filament-sigmoid system in solar active region 11520
Tie Liu, Yuhong Fan, Yingna Su +3
The separation of a filament and sigmoid is observed during an X1.4 flare on July 12, 2012 in solar active region 11520, but the corresponding magnetic field change is not clear. W…
An improved MHD simulation of the 2006 December 13 coronal mass ejection of active region NOAA 10930
Yuhong Fan
We present a magnetohydrodynamic (MHD) simulation of the coronal mass ejection (CME) on 13 December 2006 in the emerging delta-sunspot active region 10930, improving upon a previou…