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- Cooperative Institute for Research in Environmental SciencesUS23 papers
- University of Colorado BoulderUS18 papers
- National Oceanic and Atmospheric AdministrationUS17 papers
- Royal Observatory of BelgiumBE8 papers
- Goddard Space Flight CenterUS7 papers
- Marshall Space Flight CenterUS7 papers
- Institut d'Astrophysique SpatialeFR6 papers
- Southwest Research InstituteUS6 papers
- Instituto de Astrofísica de CanariasES5 papers
- National Astronomical Observatory of JapanJP5 papers
- NSF National Center for Atmospheric ResearchUS5 papers
- Center for Astrophysics Harvard & SmithsonianUS4 papers
5 papers · 1 filter
Causal Interaction between the subsurface rotation rate residuals and radial magnetic field in different timescales
Fadil Inceoglu, Rachel Howe, Paul T. M. Loto'aniu
We studied the presence and spatiotemporal characteristics and evolution of the variations in the differential rotation rates and radial magnetic fields in the Schwabe and Quasi-bi…
The QBO-type signals in the subsurface flow fields during solar cycles 23 and 24
Fadil Inceoglu, Rachel Howe, Paul T. M. Loto'aniu
We studied the presence and spatiotemporal evolution of the quasi-biennial oscillations (QBOs) in the rotation rate residuals at target depths of 0.90, 0.95,…
The Sun's Dynamic Extended Corona Observed in Extreme Ultraviolet
Daniel B. Seaton, J. Marcus Hughes, Sivakumara K. Tadikonda +6
The "middle corona" is a critical transition between the highly disparate physical regimes of the lower and outer solar corona. Nonetheless, it remains poorly understood due to the…
The Observational Uncertainty of Coronal Hole Boundaries in Automated Detection Schemes
Martin A. Reiss, Karin Muglach, Christian Möstl +16
Coronal holes are the observational manifestation of the solar magnetic field open to the heliosphere and are of pivotal importance for our understanding of the origin and accelera…
Mapping Solar Magnetic Fields from the Photosphere to the Base of the Corona
Ryohko Ishikawa, Javier Trujillo Bueno, Tanausu del Pino Aleman +25
Routine ultraviolet imaging of the Sun's upper atmosphere shows the spectacular manifestation of solar activity; yet we remain blind to its main driver, the magnetic field. Here we…