Zobrazeno 1 - 10
of 268
pro vyhledávání: '"Stenborg, G"'
Internal magnetic field structures observed by PSP/WISPR in a filament related coronal mass ejection
Autor:
Cappello, G. M., Temmer, M., Vourlidas, A., Braga, C., Liewer, P. C., Qiu, J., Stenborg, G., Kouloumvakos, A., Veronig, A. M., Bothmer, V.
Publikováno v:
A&A 688, A162 (2024)
We track and investigate from white-light data taken with the Wide-field Instrument for Solar PRobe (WISPR) aboard Parker Solar Probe (PSP), localized density enhancements, reflecting small-scale magnetic structures belonging to a filament-related co
Externí odkaz:
http://arxiv.org/abs/2402.14682
Autor:
Raouafi, N. E., Matteini, L., Squire, J., Badman, S. T., Velli, M., Klein, K. G., Chen, C. H. K., Matthaeus, W. H., Szabo, A., Linton, M., Allen, R. C., Szalay, J. R., Bruno, R., Decker, R. B., Akhavan-Tafti, M., Agapitov, O. V., Bale, S. D., Bandyopadhyay, R., Battams, K., Berčič, L., Bourouaine, S., Bowen, T., Cattell, C., Chandran, B. D. G., Chhiber, R., Cohen, C. M. S., D'Amicis, R., Giacalone, J., Hess, P., Howard, R. A., Horbury, T. S., Jagarlamudi, V. K., Joyce, C. J., Kasper, J. C., Kinnison, J., Laker, R., Liewer, P., Malaspina, D. M., Mann, I., McComas, D. J., Niembro-Hernandez, T., Panasenco, O., Pokorný, P., Pusack, A., Pulupa, M., Perez, J. C., Riley, P., Rouillard, A. P., Shi, C., Stenborg, G., Tenerani, A., Verniero, J. L., Viall, N., Vourlidas, A., Wood, B. E., Woodham, L. D., Woolley, T.
Publikováno v:
Space Science Reviews 2023
Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to determine the structure and dynamics of the Sun's coronal magnetic field, understand
Externí odkaz:
http://arxiv.org/abs/2301.02727
Autor:
Raouafi, Nour E., Stenborg, G., Seaton, D. B., Wang, H., Wang, J., DeForest, C. E., Bale, S. D., Drake, J. F., Uritsky, V. M., Karpen, J. T., DeVore, C. R., Sterling, A. C., Horbury, T. S., Harra, L. K., Bourouaine, S., Kasper, J. C., Kumar, P., Phan, T. D., Velli, M.
Publikováno v:
The Astrophysical Journal, 2023
We present EUV solar observations showing evidence for omnipresent jetting activity driven by small-scale magnetic reconnection at the base of the solar corona. We argue that the physical mechanism that heats and drives the solar wind at its source i
Externí odkaz:
http://arxiv.org/abs/2301.00903
Autor:
Liewer, P. C., Qiu, J., Ark, F., Penteado, P., Stenborg, G., Vourlidas, A., Hall, J. R., Riley, P.
The Wide-field Imager for Solar Probe (WISPR) onboard Parker Solar Probe (PSP), observing in white light, has a fixed angular field of view, extending from 13.5 degree to 108 degree from the Sun and approximately 50 degree in the transverse direction
Externí odkaz:
http://arxiv.org/abs/2209.02779
Autor:
Sieyra, M. V., Prasad, S. Krishna, Stenborg, G., Khomenko, E., Van Doorsselaere, T., Costa, A., Esquivel, A., Riedl, J. M.
Publikováno v:
A&A 667, A21 (2022)
Recurrent, arc-shaped intensity disturbances were detected by EUV channels in an active region. The fronts were observed to propagate along a coronal loop bundle rooted in a small area within a sunspot umbra. Previous works have linked these intensit
Externí odkaz:
http://arxiv.org/abs/2208.10857
Autor:
Sieyra, M. V., Cécere, M., Cremades, H., Iglesias, F. A., Sahade, A., Mierla, M., Stenborg, G., Costa, A., West, M., D'Huys, E.
Motivated by the need to improve the ability to forecast whether a certain coronal mass ejection (CME) is to impact Earth, and by the insufficiency of statistical studies that analyze the whole erupting system with the focus on the governing conditio
Externí odkaz:
http://arxiv.org/abs/2007.14317
Slow waves are commonly observed on the entire solar atmosphere. Assuming a thin flux tube approximation, the cut-off periods of slow-mode magneto-acoustic-gravity waves that travel from the photosphere to the corona were obtained in Costa et al. (20
Externí odkaz:
http://arxiv.org/abs/2004.09609
Publikováno v:
Journal of Geophysical Research (Space Physics), 120, 5329, 2015
High-quality white-light images from the SECCHI/HI-1 telescope onboard STEREO-B reveal high-velocity evanescent clumps [HVECs] expelled from the coma of the C/2011 L4 [Pan-STARRS] comet. Animated images provide evidence of highly dynamic ejecta movin
Externí odkaz:
http://arxiv.org/abs/1507.02579
Autor:
Cécere, M., Sieyra, M.V., Cremades, H., Mierla, M., Sahade, A., Stenborg, G., Costa, A., West, M.J., D’Huys, E.
Publikováno v:
In Advances in Space Research 15 March 2020 65(6):1654-1662
Autor:
Nieves-Chinchilla, T., Vourlidas, A., Stenborg, G., Savani, N. P., Koval, A., Szabo, A., Jian, L. K.
Coronal mass ejections (CMEs) are the main driver of Space Weather. Therefore, a precise forecasting of their likely geo-effectiveness relies on an accurate tracking of their morphological and kinematical evolution throughout the interplanetary mediu
Externí odkaz:
http://arxiv.org/abs/1311.6895