Zobrazeno 1 - 10
of 372
pro vyhledávání: '"Nelson, C J"'
Autor:
Nelson, C. J., Hayes, L. A., Müller, D., Musset, S., Freij, N., Auchère, F., Cuadrado, R. Aznar, Barczynski, K., Buchlin, E., Harra, L., Long, D. M., Parenti, S., Peter, H., Schühle, U., Smith, P., Teriaca, L., Verbeeck, C., Zhukov, A. N., Berghmans, D.
The identification of large numbers of localised transient EUV brightenings, with small spatial scales, in the quiet-Sun corona has been one of the key early results from Solar Orbiter. However, much is still unknown about these events. Here, we aim
Externí odkaz:
http://arxiv.org/abs/2411.00467
Autor:
Nelson, C. J., Calchetti, D., Gandorfer, A., Hirzberger, J., Sinjan, J., Solanki, S. K., Berghmans, D., Strecker, H., Blanco, J.
The relationship between UV Bursts and solar surges is complex, with these events sometimes being observed together and sometimes being observed independently. Why this sporadic association exists is unknown, however, it likely relates to the physica
Externí odkaz:
http://arxiv.org/abs/2410.07770
Autor:
Nelson, C. J., Auchère, F., Cuadrado, R. Aznar, Barczynski, K., Buchlin, E., Harra, L., Long, D. M., Parenti, S., Peter, H., Schühle, U., Schwanitz, C., Smith, P., Teriaca, L., Verbeeck, C., Zhukov, A. N., Berghmans, D.
Publikováno v:
A&A 676, A64 (2023)
Localised transient EUV brightenings, sometimes named `campfires', occur throughout the quiet-Sun. However, there are still many open questions about such events, in particular regarding their temperature range and dynamics. In this article, we aim t
Externí odkaz:
http://arxiv.org/abs/2306.05190
Autor:
Nelson, C. J., Kleint, L.
Publikováno v:
A&A 668, A136 (2022)
Approximately 0.01 % of all Si IV 1394 A spectra sampled in 2013 and 2014 by the Interface Region Imaging Spectrograph (IRIS) have IRIS burst profiles. However, these events are not evenly distributed across datasets with 19.31 % of these spectra bei
Externí odkaz:
http://arxiv.org/abs/2211.13311
Solar active regions (ARs) play a fundamental role in driving many of the geo-effective eruptions which propagate into the Solar System. However, we are still unable to consistently predict where and when ARs will occur across the solar disk by ident
Externí odkaz:
http://arxiv.org/abs/2210.06276
Autor:
Nelson, C. J., Kleint, L.
Publikováno v:
A&A 666, A66 (2022)
Interface Region Imaging Spectrograph (IRIS) bursts are localised features thought to be driven by magnetic reconnection. Although these events are well-studied, it remains unknown whether their properties vary as their host active regions (ARs) evol
Externí odkaz:
http://arxiv.org/abs/2208.11013
Autor:
Noda, C. Quintero, Schlichenmaier, R., Rubio, L. R. Bellot, Löfdahl, M. G., Khomenko, E., Jurcak, J., Leenaarts, J., Kuckein, C., Manrique, S. J. González, Gunar, S., Nelson, C. J., Rodríguez, J. de la Cruz, Tziotziou, K., Tsiropoula, G., Aulanier, G., Collados, M., team, the EST
Publikováno v:
A&A 666, A21 (2022)
The European Solar Telescope (EST) is a project aimed at studying the magnetic connectivity of the solar atmosphere, from the deep photosphere to the upper chromosphere. Its design combines the knowledge and expertise gathered by the European solar p
Externí odkaz:
http://arxiv.org/abs/2207.10905
Publikováno v:
A&A 654, A50 (2021)
Numerous magnetohydrodynamic oscillations have been reported within solar pores over the past decades, including in line-of-sight (LOS) velocities, intensities, and magnetic field strengths. Our aim is to identify whether high-amplitude oscillations
Externí odkaz:
http://arxiv.org/abs/2107.10183
Publikováno v:
A&A 640, A120 (2020)
Downflows with high velocities occur in the transition region above many sunspots; however, how these signatures evolve over short time-scales in both spatial and spectral terms is still unknown. In this article, we investigate the evolution of downf
Externí odkaz:
http://arxiv.org/abs/2006.13617
Autor:
Korsos, M. B., Georgoulis, M. K., Gyenge, N., Bisoi, S. K., Yu, S., Poedts, S., Nelson, C. J., Liu, J., Yan, Y., Erdelyi, R.
In this article, we present the application of the weighted horizontal gradient of magnetic field (WGM) flare prediction method to 3-dimensional (3D) extrapolated magnetic configurations of 13 flaring solar active regions (ARs). The main aim is to id
Externí odkaz:
http://arxiv.org/abs/2005.12180