Zobrazeno 1 - 10
of 492
pro vyhledávání: '"DeRosa M"'
Autor:
Gopalswamy, N., Christe, S., Fung, S. F., Gong, Q., Gruesbeck, J. R., Jian, L. K., Kanekal, S. G., Kay, C., Kucera, T. A., Leake, J. E., Li, L., Makela, P., Nikulla, P., Reginald, N. L., Shih, A., Tadikonda, S. K., Viall, N., Wilson III, L. B., Yashiro, S., Golub, L., DeLuca, E., Reeves, K., Sterling, A. C., Winebarger, A. R., DeForest, C., Hassler, D. M., Seaton, D. B., Desai, M. I., Mokashi, P. S., Lazio, J., Jensen, E. A., Manchester, W. B., Sachdeva, N., Wood, B., Kooi, J., Hess, P., Wexler, D. B., Bale, S. D., Krucker, S., Hurlburt, N., DeRosa, M., Gosain, S., Jain, K., Kholikov, S., Petrie, G. J. D., Pevtsov, A., Tripathy, S. C., Zhao, J., Scherrer, P. H., Rajaguru, S. P., Woods, T., Kenney, M., Zhang, J., Scolini, C., Cho, K. S., Park, Y. D., Jackson, B. V.
We report on a study of the Multiview Observatory for Solar Terrestrial Science (MOST) mission that will provide comprehensive imagery and time series data needed to understand the magnetic connection between the solar interior and the solar atmosphe
Externí odkaz:
http://arxiv.org/abs/2303.02895
Autor:
Gopalswamy, N., Christe, S., Fung, S.F., Gong, Q., Gruesbeck, J.R., Jian, L.K., Kanekal, S.G., Kay, C., Kucera, T.A., Leake, J.E., Li, L., Mӓkelӓ, P., Nikulla, P., Reginald, N.L., Shih, A., Tadikonda, S.K., Viall, N., Wilson, L.B., III, Yashiro, S., Golub, L., DeLuca, E., Reeves, K., Sterling, A.C., Winebarger, A.R., DeForest, C., Hassler, D.M., Seaton, D.B., Desai, M.I., Mokashi, P.S., Lazio, J., Jensen, E.A., Manchester, W.B., Sachdeva, N., Wood, B., Kooi, J., Hess, P., Wexler, D.B., Bale, S.D., Krucker, S., Hurlburt, N., DeRosa, M., Gosain, S., Jain, K., Kholikov, S., Petrie, G.J.D., Pevtsov, A., Tripathy, S.C., Zhao, J., Scherrer, P.H., Rajaguru, S.P., Woods, T., Kenney, M., Zhang, J., Scolini, C., Cho, K.-S., Park, Y.-D., Jackson, B.V.
Publikováno v:
In Journal of Atmospheric and Solar-Terrestrial Physics January 2024 254
Publikováno v:
ApJ 900 136 (2020)
A physical magnetic field has a divergence of zero. Numerical error in constructing a model field and computing the divergence, however, introduces a finite divergence into these calculations. A popular metric for measuring divergence is the average
Externí odkaz:
http://arxiv.org/abs/2008.08863
Autor:
Linker, J. A., Caplan, R. M., Downs, C., Riley, P, Mikic, Z, Lionello, R., Henney, C. J., Arge, C. N., Liu, Y., Derosa, M. L., Yeates, A., Owens, M. J.
The heliospheric magnetic field is of pivotal importance in solar and space physics. The field is rooted in the Sun's photosphere, where it has been observed for many years. Global maps of the solar magnetic field based on full disk magnetograms are
Externí odkaz:
http://arxiv.org/abs/1708.02342
Akademický článek
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Publikováno v:
The Astrophysical Journal, Volume 820, Issue 1, article id. 16, 2016
With the global view and high-cadence observations from SDO/AIA and STEREO, many spatially separated solar eruptive events appear to be coupled. However, the mechanisms for "sympathetic" events are still largely unknown. In this study, we investigate
Externí odkaz:
http://arxiv.org/abs/1603.04900
Autor:
DeRosa, M. L., Wheatland, M. S., Leka, K. D., Barnes, G., Amari, T., Canou, A., Gilchrist, S. A., Thalmann, J. K., Valori, G., Wiegelmann, T., Schrijver, C. J., Malanushenko, A., Sun, X., Régnier, S.
The nonlinear force-free field (NLFFF) model is often used to describe the solar coronal magnetic field, however a series of earlier studies revealed difficulties in the numerical solution of the model in application to photospheric boundary data. We
Externí odkaz:
http://arxiv.org/abs/1508.05455
Autor:
Culhane, J. L., Brooks, D. H., van Driel-Gesztelyi, L., Demoulin, P., Baker, D., DeRosa, M. L., Mandrini, C. H., Zhao, L., Zurbuchen, T. H.
Seeking to establish whether active region upflow material contributes to the slow solar wind, we examine in detail the plasma upflows from Active Region (AR)10978, which crossed the Sun's disc in the interval 8 to 16 December, 2007 during Carrington
Externí odkaz:
http://arxiv.org/abs/1405.2949
Publikováno v:
The Astrophysical Journal, Volume 783, Issue 2, article id. 102, 15 pp. (2014)
The shapes of solar coronal loops are sensitive to the presence of electrical currents that are the carriers of the nonpotential energy available for impulsive activity. We use this information in a new method for modeling the coronal magnetic field
Externí odkaz:
http://arxiv.org/abs/1312.5389
The high-cadence, comprehensive view of the solar corona by SDO/AIA shows many events that are widely separated in space while occurring close together in time. In some cases, sets of coronal events are evidently causally related, while in many other
Externí odkaz:
http://arxiv.org/abs/1305.0801