Zobrazeno 1 - 10
of 21
pro vyhledávání: '"H. R. Gilbert"'
Autor:
T. A. Kucera, M. Luna, T. Török, K. Muglach, J. T. Karpen, C. Downs, X. Sun, B. J. Thompson, H. R. Gilbert
Publikováno v:
The Astrophysical Journal. 940:34
Understanding the magnetic structure of filament channels is difficult but essential for identifying the mechanism (s) responsible for solar eruptions. In this paper we characterize the magnetic field in a well-observed filament channel with two inde
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c014c0b419417119c9f5a68620b62234
https://doi.org/10.3847/1538-4357/ac9377
https://doi.org/10.3847/1538-4357/ac9377
Autor:
Manuel Luna, Jaume Terradas, Judith T. Karpen, Jose Luis Ballester, H. R. Gilbert, Therese A. Kucera, Karin Muglach
We have catalogued 196 filament oscillations from the GONG $H{\alpha}$ network data during several months near the maximum of solar cycle 24 (January - June 2014). Selected examples from the catalog are described in detail, along with our statistical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9b72065748d8efd22c1db321b101ee16
Autor:
Teimuraz V. Zaqarashvili, Manuel Collados, Turlough P. Downes, Jose Luis Ballester, H. R. Gilbert, Robert F. Pfaff, Igor Alexeev, Maxim L. Khodachenko, Enrique Vázquez-Semadeni, I. F. Shaikhislamov, Roberto Soler, Elena Khomenko
Partially ionized plasmas are found across the Universe in many different astrophysical environments. They constitute an essential ingredient of the solar atmosphere, molecular clouds, planetary ionospheres and protoplanetary disks, among other envir
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ae45cdf31c31b7ee41b460fda834ee2
The chromosphere is a complex region that acts as an intermediary between the magnetic flux emergence in the photosphere and the magnetic features seen in the corona. Large eruptions in the chromosphere of flares and filaments are often accompanied b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cca95617ca4a3151443acdbe4c48296e
Sequential chromospheric brightenings (SCBs) are often observed in the immediate vicinity of erupting flares and are associated with coronal mass ejections. Since their initial discovery in 2005, there have been several subsequent investigations of S
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3a5a95adf97327b26a223a5939e8a9a
Recent high-resolution and high-cadence EUV imaging has revealed a new phenomenon, impacting prominence debris, where prominence material from failed or partial eruptions can impact the lower atmosphere, releasing energy. We report a clear example of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cf013e7cb27fb3a61084d7c588057ac3
Autor:
Karin Muglach, Manuel Luna, Judith T. Karpen, Kalman J. Knizhnik, Therese A. Kucera, H. R. Gilbert
Publikováno v:
Proceedings of the International Astronomical Union
On 20 August 2010 an energetic disturbance triggered damped large-amplitude longitudinal (LAL) oscillations in almost an entire filament. In the present work we analyze this periodic motion in the filament to characterize the damping and restoring me
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd04b720513d0bd51b0931cdcb547bdb
Autor:
H. R. Gilbert, Andrew Inglis
Publikováno v:
The Astrophysical Journal. 797:72
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5a2b1943994b87327538773a372aab4c
https://doi.org/10.1088/0004-637x/797/1/72
https://doi.org/10.1088/0004-637x/797/1/72
Autor:
H. R. Gilbert, Karin Muglach, Manuel Luna, Kalman J. Knizhnik, Vadim M. Uritsky, Therese A. Kucera, Judith T. Karpen
Publikováno v:
The Astrophysical Journal
On 20 August 2010 an energetic disturbance triggered large-amplitude longitudinal oscillations in a nearby filament. The triggering mechanism appears to be episodic jets connecting the energetic event with the filament threads. In the present work we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::097d78257aa3325f0ee3242304dd572b
https://doi.org/10.1088/0004-637x/785/1/79
https://doi.org/10.1088/0004-637x/785/1/79
Publikováno v:
The Astrophysical Journal. 776:L12
Solar filaments exhibit a range of eruptive-like dynamic activity, ranging from the full or partial eruption of the filament mass and surrounding magnetic structure as a coronal mass ejection (CME), to a fully confined or 'failed' eruption. On 2011 J
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb51f15063e2312cc4e5fddd3d75c4c6
https://doi.org/10.1088/2041-8205/776/1/l12
https://doi.org/10.1088/2041-8205/776/1/l12