1.1k citations
- California Institute of TechnologyUS70 papers
- Queen's University BelfastGB69 papers
- Center for Astrophysics Harvard & SmithsonianUS40 papers
- Centre National de la Recherche ScientifiqueFR40 papers
- Jet Propulsion LaboratoryUS35 papers
- Tsinghua UniversityCN35 papers
- University of California, Santa BarbaraUS32 papers
- Princeton UniversityUS31 papers
- University of California, Los AngelesUS30 papers
- University of ChileCL28 papers
- Nanjing UniversityCN25 papers
- Atacama Large Millimeter Submillimeter ArrayCL24 papers
6 papers · 2 filters
Unravelling the components of a multi-thermal coronal loop using magnetohydrodynamic seismology
S. Krishna Prasad, D. B. Jess, J. A. Klimchuk +1
Coronal loops, constituting the basic building blocks of the active Sun, serve as primary targets to help understand the mechanisms responsible for maintaining multi-million Kelvin…
Chandra Characterization of X-ray Emission in the Young F-Star Binary System HD 113766
C. M. Lisse, D. J. Christian, S. J. Wolk +3
Using Chandra we have obtained imaging X-ray spectroscopy of the 10 to 16 Myr old F-star binary HD 113766. We individually resolve the binary components for the first time in the X…
Multifractal Solar EUV Intensity Fluctuations and their Implications for Coronal Heating Models
Ana Cristina Cadavid, Yeimy J. Rivera, John K. Lawrence +3
We investigate the scaling properties of the long-range temporal evolution and intermittency of SDO/AIA intensity observations in four solar environments: an active region core, a…
Observations and simulations of the Na I D1 line profiles in an M-class solar flare
D. Kuridze, M. Mathioudakis, D. J. Christian +7
We study the temporal evolution of the Na I D1 line profiles in the M3.9 flare SOL2014-06-11T21:03 UT, using high spectral resolution observations obtained with the IBIS instrument…
Solar coronal magnetic fields derived using seismology techniques applied to omnipresent sunspot waves
D. B. Jess, V. E. Reznikova, R. S. I. Ryans +9
Sunspots on the surface of the Sun are the observational signatures of intense manifestations of tightly packed magnetic field lines, with near-vertical field strengths exceeding 6…
Time-dependent suppression of oscillatory power in evolving solar magnetic fields
S. Krishna Prasad, D. B. Jess, R. Jain +1
Oscillation amplitudes are generally smaller within magnetically active regions like sunspots and plage, when compared to their surroundings. Such magnetic features, when viewed in…