Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Henney Carl J."'
Autor:
Heinemann, Stephan G., Owens, Mathew J., Temmer, Manuela, Turtle, James A., Arge, Charles N., Henney, Carl J., Pomoell, Jens, Asvestari, Eleanna, Linker, Jon A., Downs, Cooper, Caplan, Ronald M., Hofmeister, Stefan J., Scolini, Camilla, Pinto, Rui F., Madjarska, Maria S.
Coronal holes are recognized as the primary sources of heliospheric open magnetic flux (OMF). However, a noticeable gap exists between in-situ measured OMF and that derived from remote sensing observations of the Sun. In this study, we investigate th
Externí odkaz:
http://arxiv.org/abs/2402.12805
Autor:
Halford Alexa J., Kellerman Adam C., Garcia-Sage Katherine, Klenzing Jeffrey, Carter Brett A., McGranaghan Ryan M., Guild Timothy, Cid Consuelo, Henney Carl J., Ganushkina Natalia Yu., Burrell Angeline G., Terkildsen Mike, Welling Daniel T., Murray Sophie A., Leka K. D., McCollough James P., Thompson Barbara J., Pulkkinen Antti, Fung Shing F., Bingham Suzy, Bisi Mario M., Liemohn Michael W., Walsh Brian M., Morley Steven K.
Publikováno v:
Journal of Space Weather and Space Climate, Vol 9, p A34 (2019)
The space physics community continues to grow and become both more interdisciplinary and more intertwined with commercial and government operations. This has created a need for a framework to easily identify what projects can be used for specific app
Externí odkaz:
https://doaj.org/article/f4e7e2635ac64946b581cf30a63e3bed
Autor:
Asvestari, Eleanna, Temmer, Manuela, Caplan, Ronald M., Linker, Jon A., Heinemann, Stephan G., Pinto, Rui F., Henney, Carl J., Arge, Charles N., Owens, Mathew J., Madjarska, Maria S., Pomoell, Jens, Hofmeister, Stefan J., Scolini, Camilla, Samara, Evangelia
A plethora of coronal models, from empirical to more complex magnetohydrodynamic (MHD) ones, are being used for reconstructing the coronal magnetic field topology and estimating the open magnetic flux. However, no individual solution fully agrees wit
Externí odkaz:
http://arxiv.org/abs/2311.04024
The solar magnetic fields emerging from the photosphere into the chromosphere and corona are comprised of a combination of "closed" and "open" fields. The closed magnetic field lines are defined as those having both ends rooted in the solar surface,
Externí odkaz:
http://arxiv.org/abs/2304.07649
Autor:
Badman, Samuel T., Riley, Pete, Jones, Shaela I., Kim, Tae K., Allen, Robert C., Arge, C. Nick, Bale, Stuart D., Henney, Carl J., Kasper, Justin C., Mostafavi, Parisa, Pogorelov, Nikolai V., Raouafi, Nour E., Stevens, Michael L., Verniero, J. L.
Drawing connections between heliospheric spacecraft and solar wind sources is a vital step in understanding the evolution of the solar corona into the solar wind and contextualizing \textit{in situ} timeseries. Furthermore, making advanced prediction
Externí odkaz:
http://arxiv.org/abs/2303.04852
Autor:
Barnes, Graham, DeRosa, Marc L., Jones, Shaela I., Arge, Charles N., Henney, Carl J., Cheung, Mark C. M.
The concept of surface-flux transport (SFT) is commonly used in evolving models of the large-scale solar surface magnetic field. These photospheric models are used to determine the large-scale structure of the overlying coronal magnetic field, as wel
Externí odkaz:
http://arxiv.org/abs/2302.06496
Parker Solar Probes's (PSP)'s unique orbital path allows us to observe the solar wind closer to the Sun than ever before. Essential to advancing our knowledge of solar wind and energetic particle formation is identifying the sources of PSP observatio
Externí odkaz:
http://arxiv.org/abs/2205.13010
We explore the use of observed polar coronal holes (CHs) to constrain the flux distribution within the polar regions of global solar magnetic field maps in the absence of reliable quality polar field observations. Global magnetic maps, generated by t
Externí odkaz:
http://arxiv.org/abs/2204.13676
Autor:
Halford, Alexa J., Kellerman, Adam C., Garcia-Sage, Katherine, Klenzing, Jeffrey, Carter, Brett A., McGranaghan, Ryan M., Guild, Timothy, Cid, Consuelo, Henney, Carl J., Ganushkina, Natalia Y., Burrell, Angeline G., Terkildsen, Mike, Welling, Daniel T., Murray, Sophie A., Leka, K. D., McCollough, James P., Thompson, Barbara J., Pulkkinen, Antti, Fung, Shing F., Bingham, Suzy, Bisi, Mario M., Liemohn, Michael W., Walsh, Brian M., Morley, Steven K.
The space physics community continues to grow and become both more interdisciplinary and more intertwined with commercial and government operations. This has created a need for a framework to easily identify what projects can be used for specific app
Externí odkaz:
http://arxiv.org/abs/1907.08663
Autor:
Pillet, Valentin Martinez, Hill, Frank, Hammel, Heidi, de Wijn, Alfred G., Gosain, Sanjay, Burkepile, Joan, Henney, Carl J., McAteer, James R. T., Bain, Hazel M., Manchester IV, Ward B., Lin, Haosheng, Roth, Markus, Ichimoto, Kiyoshi, Suematsu, Yoshinori
Ground-based solar observations provide key contextual data (i.e., the 'big picture') to produce a complete description of the only astrosphere we can study in situ: our Sun's heliosphere. The next decade will see the beginning of operations of the D
Externí odkaz:
http://arxiv.org/abs/1903.06944