Zobrazeno 1 - 10
of 167
pro vyhledávání: '"McKillop S"'
Autor:
Acheson, J.G., Gallagher, E.A., Ward, J., McKillop, S., FitzGibbon, B., Boyd, A.R., Meenan, B.J., Lemoine, P., McGarry, J.P.
Publikováno v:
In Surface & Coatings Technology 15 January 2022 429
Autor:
Janvier, M., Savcheva, A., Pariat, E., Tassev, S., Millholland, S., Bommier, V., McCauley, P., McKillop, S., Dougan, F.
Publikováno v:
A&A 591, A141 (2016)
The standard model for eruptive flares has in the past few years been extended to 3D. It predicts typical J-shaped photospheric footprints of the coronal current layer, forming at similar locations as the Quasi-Separatrix Layers (QSLs). Such a morpho
Externí odkaz:
http://arxiv.org/abs/1604.07241
Autor:
Acheson, J.G., Robinson, L., McKillop, S., Wilson, S., McIvor, M.J., Meenan, B.J., Boyd, A.R.
Publikováno v:
In Materials Characterization January 2021 171
Autor:
Savcheva, A., Pariat, E., McKillop, S., McCauley, P., Hanson, E., Su, Y., Werner, E., DeLuca, E. E.
In this paper we present a topological magnetic field investigation of seven two-ribbon flares in sigmoidal active regions observed with Hinode, STEREO, and SDO. We first derive the 3D coronal magnetic field structure of all regions using marginally
Externí odkaz:
http://arxiv.org/abs/1506.03452
Autor:
Cheung, Mark C. M., De Pontieu, B., Tarbell, T. D., Fu, Y., Tian, H., Testa, P., Reeves, K. K., Martinez-Sykora, J., Boerner, P., Wuelser, J. P., Lemen, J., Title, A. M., Hurlburt, N., Kleint, L., Kankelborg, C., Jaeggli, S., Golub, L., McKillop, S., Saar, S., Carlsson, M., Hansteen, V.
We report on observations of recurrent jets by instruments onboard the Interface Region Imaging Spectrograph (IRIS), Solar Dynamics Observatory (SDO) and Hinode spacecrafts. Over a 4-hour period on July 21st 2013, recurrent coronal jets were observed
Externí odkaz:
http://arxiv.org/abs/1501.01593
Autor:
Hansteen, V., De Pontieu, B., Carlsson, M., Lemen, J., Title, A., Boerner, P., Hurlburt, N., Tarbell, T. D., Wuelser, J. P., Pereira, T. M. D., De Luca, E. E., Golub, L., McKillop, S., Reeves, K., Saar, S., Testa, P., Tian, H., Kankelborg, C., Jaeggli, S., Kleint, L., Martinez-Sykora, J.
Publikováno v:
Science, Volume 346, Issue 6207, id. 1255757 (2014)
The heating of the outer solar atmospheric layers, i.e., the transition region and corona, to high temperatures is a long standing problem in solar (and stellar) physics. Solutions have been hampered by an incomplete understanding of the magnetically
Externí odkaz:
http://arxiv.org/abs/1412.3611
Autor:
De Pontieu, B., van der Voort, L. Rouppe, McIntosh, S. W., Pereira, T. M. D., Carlsson, M., Hansteen, V., Skogsrud, H., Lemen, J., Title, A., Boerner, P., Hurlburt, N., Tarbell, T. D., Wuelser, J. P., De Luca, E. E., Golub, L., McKillop, S., Reeves, K., Saar, S., Testa, P., Tian, H., Kankelborg, C., Jaeggli, S., Kleint, L., Martinez-Sykora, J.
Publikováno v:
Science 17 October 2014, Vol. 346 no. 6207
The solar chromosphere and transition region (TR) form an interface between the Sun's surface and its hot outer atmosphere. Here most of the non-thermal energy that powers the solar atmosphere is transformed into heat, although the detailed mechanism
Externí odkaz:
http://arxiv.org/abs/1410.6862
Autor:
Tian, H., DeLuca, E. E., Cranmer, S. R., De Pontieu, B., Peter, H., Martínez-Sykora, J., Golub, L., McKillop, S., Reeves, K. K., Miralles, M. P., McCauley, P., Saar, S., Testa, P., Weber, M., Murphy, N., Lemen, J., Title, A., Boerner, P., Hurlburt, N., Tarbell, T. D., Wuelser, J. P., Kleint, L., Kankelborg, C., Jaeggli, S., Carlsson, M., Hansteen, V., McIntosh, S. W.
Publikováno v:
Science, 346, 1255711 (2014)
As the interface between the Sun's photosphere and corona, the chromosphere and transition region play a key role in the formation and acceleration of the solar wind. Observations from the Interface Region Imaging Spectrograph reveal the prevalence o
Externí odkaz:
http://arxiv.org/abs/1410.6143
Autor:
Peter, H., Tian, H., Curdt, W., Schmit, D., Innes, D., De Pontieu, B., Lemen, J., Title, A., Boerner, P., Hurlburt, N., Tarbell, T. D., Wuelser, J. P., Martínez-Sykora, J., Kleint, L., Golub, L., McKillop, S., Reeves, K. K., Saar, S., Testa, P., Kankelborg, C., Jaeggli, S., Carlsson, M., Hansteen, V.
Publikováno v:
Science 346, 1255726 (2014)
The solar atmosphere was traditionally represented with a simple one-dimensional model. Over the past few decades, this paradigm shifted for the chromosphere and corona that constitute the outer atmosphere, which is now considered a dynamic structure
Externí odkaz:
http://arxiv.org/abs/1410.5842
Autor:
Pereira, T. M. D., De Pontieu, B., Carlsson, M., Hansteen, V., Tarbell, T. D., Lemen, J., Title, A., Boerner, P., Hurlburt, N., Wülser, J. P., Martínez-Sykora, J., Kleint, L., Golub, L., McKillop, S., Reeves, K. K., Saar, S., Testa, P., Tian, H., Jaeggli, S., Kankelborg, C.
Solar spicules have eluded modelers and observers for decades. Since the discovery of the more energetic type II, spicules have become a heated topic but their contribution to the energy balance of the low solar atmosphere remains unknown. Here we gi
Externí odkaz:
http://arxiv.org/abs/1407.6360