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pro vyhledávání: '"Hughes, J. Marcus"'
We present an extension of the Coronal Reconstruction Onto B-Aligned Regions (CROBAR) method to Linear Force Free Field (LFFF) extrapolations, and apply it to the reconstruction of a set of AIA, MDI, and STEREO EUVI data. The results demonstrate that
Externí odkaz:
http://arxiv.org/abs/2309.08053
Autor:
Caspi, Amir, Seaton, Daniel B., Casini, Roberto, Downs, Cooper, Gibson, Sarah E., Gilbert, Holly, Glesener, Lindsay, Guidoni, Silvina E., Hughes, J. Marcus, McKenzie, David, Plowman, Joseph, Reeves, Katharine K., Saint-Hilaire, Pascal, Shih, Albert Y., West, Matthew J.
Publikováno v:
Bulletin of the AAS, Vol. 55, Issue 3, Whitepaper #049 (16pp); 2023 July 31
The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poorly observed and understood. We highlight key questions related to mag
Externí odkaz:
http://arxiv.org/abs/2305.17146
Autor:
Seaton, Daniel B., Caspi, Amir, Casini, Roberto, Downs, Cooper, Gibson, Sarah E., Gilbert, Holly, Glesener, Lindsay, Guidoni, Silvina E., Hughes, J. Marcus, McKenzie, David, Plowman, Joseph, Reeves, Katharine K., Saint-Hilaire, Pascal, Shih, Albert Y., West, Matthew J.
Publikováno v:
Bulletin of the AAS, Vol. 55, Issue 3, Whitepaper #361 (9pp); 2023 July 31
Heliophysics image data largely relies on a forty-year-old ecosystem built on the venerable Flexible Image Transport System (FITS) data standard. While many in situ measurements use newer standards, they are difficult to integrate with multiple data
Externí odkaz:
http://arxiv.org/abs/2305.16535
Autor:
Caspi, Amir, Seaton, Daniel B., Casini, Roberto, Downs, Cooper, Gibson, Sarah E., Gilbert, Holly, Glesener, Lindsay, Guidoni, Silvina E., Hughes, J. Marcus, McKenzie, David, Plowman, Joseph, Reeves, Katharine K., Saint-Hilaire, Pascal, Shih, Albert Y., West, Matthew J.
Publikováno v:
Bulletin of the AAS, Vol. 55, Issue 3, Whitepaper #048 (10pp); 2023 July 31
COMPLETE is a flagship mission concept combining broadband spectroscopic imaging and comprehensive magnetography from multiple viewpoints around the Sun to enable tomographic reconstruction of 3D coronal magnetic fields and associated dynamic plasma
Externí odkaz:
http://arxiv.org/abs/2305.16533
Autor:
Seaton, Daniel B., Hughes, J. Marcus, Tadikonda, Sivakumara K., Caspi, Amir, DeForest, Craig, Krimchansky, Alexander, Hurlburt, Neal E., Seguin, Ralph, Slater, Gregory
Publikováno v:
Nature Astronomy, Vol. 5, pp. 1029-1035; 2021 August 02
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 difficulty of observing this faint region (1.5-3 solar radii). New ob
Externí odkaz:
http://arxiv.org/abs/2105.08028
Autor:
Hughes, J. Marcus, Hsu, Vicki W., Seaton, Daniel B., Bain, Hazel M., Darnel, Jonathan M., Krista, Larisza
In order to utilize solar imagery for real-time feature identification and large-scale data science investigations of solar structures, we need maps of the Sun where phenomena, or themes, are labeled. Since solar imagers produce observations every fe
Externí odkaz:
http://arxiv.org/abs/1910.00144
Autor:
Gibson, Steven J., Howard, Ward S., Jolly, Christian S., Newton, Jonathan H., Bell, Aaron C., Spraggs, Mary E., Hughes, J. Marcus, Tagliaboschi, Aaron M., Brunt, Christopher M., Taylor, A. Russell, Stil, Jeroen M., Dame, Thomas M.
We have mapped cold atomic gas in 21cm line HI self-absorption (HISA) at arcminute resolution over more than 90% of the Milky Way's disk. To probe the formation of H2 clouds, we have compared our HISA distribution with CO J=1-0 line emission. Few HIS
Externí odkaz:
http://arxiv.org/abs/1510.06784
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