Zobrazeno 1 - 10
of 74
pro vyhledávání: '"J. P. Wülser"'
Autor:
N. Schanche, C. A. Madsen, Steven H. Saar, J. Prchlik, Paul Bryans, R. Timmons, S. McKillop, P. Boerner, Charles C. Kankelborg, Samuel L. Freeland, B. De Pontieu, J. P. Wülser, M. Wiesmann, S. Jaeggli, S. Brannon, Wei Liu, Theodore D. Tarbell, Paola Testa
Publikováno v:
Solar Physics. 293
This work is supported by NASA contract NNG09FA40C (IRIS). The Interface Region Imaging Spectrograph (IRIS) is a NASA small explorer mission that provides high-resolution spectra and images of the Sun in the 133 – 141 nm and 278 – 283 nm waveleng
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::301d3538fe6f5a997b7c4f20d8e804d8
https://doi.org/10.1007/s11207-018-1364-8
https://doi.org/10.1007/s11207-018-1364-8
Publikováno v:
Solar Physics. 293
Using the 2016 Mercury transit of the Sun, we characterize on orbit spatial point spread functions (PSFs) for the Near- (NUV) and Far- (FUV) Ultra-Violet spectrograph channels of NASA’s Interface Region Imaging Spectrograph (IRIS). A semi-blind Ric
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::212ecbb393ab9984f9106eb78370198f
https://doi.org/10.1007/s11207-018-1347-9
https://doi.org/10.1007/s11207-018-1347-9
Autor:
J. P. Wülser, Nariaki Nitta, James R. Lemen, Dominic M. Zarro, Markus J. Aschwanden, Samuel L. Freeland
Publikováno v:
Solar Physics. 289:1257-1277
We study the association of solar flares with coronal mass ejections (CMEs) during the deep, extended solar minimum of 2007-2009, using extreme-ultraviolet (EUV) and white-light (coronagraph) images from the {\it Solar Terrestrial Relations Observato
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d206b03a2955a490bfcf477801cd4233
https://doi.org/10.1007/s11207-013-0388-3
https://doi.org/10.1007/s11207-013-0388-3
Autor:
Markus J. Aschwanden, J. P. Wülser
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 73:1082-1095
We review data analysis and physical modeling related to the 3-D reconstruction of active regions in the solar corona, using stereoscopic image pairs from the STEREO/EUVI instrument. This includes the 3-D geometry of coronal loops (with measurements
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a3d3853153fcbb548bd6c90a9e97162d
https://doi.org/10.1016/j.jastp.2010.09.008
https://doi.org/10.1016/j.jastp.2010.09.008
Autor:
J.-P. Wülser, O. Podladchikova, Angelos Vourlidas, Spiros Patsourakos, R. A. M. Van der Linden
Publikováno v:
The Astrophysical Journal. 709:369-376
The Solar Terrestrial Relations Observatory EUV telescopes have uncovered small-scale eruptive events, tentatively referred to as 'mini-CMEs' because they exhibit morphologies similar to large-scale coronal mass ejections (CMEs). Coronal waves and wi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::88e09a985621c6e4ccb1e9d94ef71fe8
https://doi.org/10.1088/0004-637x/709/1/369
https://doi.org/10.1088/0004-637x/709/1/369
Publikováno v:
Solar Physics. 259:1-11
The Solar Terrestrial Relations Observatory (STEREO) provides the first opportunity to triangulate the three-dimensional coordinates of active region loops simultaneously from two different vantage points in space. Three-dimensional coordinates of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1ff48403e68e8e0c0f9fb6c0d6367983
https://doi.org/10.1007/s11207-009-9383-0
https://doi.org/10.1007/s11207-009-9383-0
First Three‐Dimensional Reconstructions of Coronal Loops with theSTEREO AandBSpacecraft. I. Geometry
Publikováno v:
The Astrophysical Journal. 679:827-842
We present one of the first triangulations and 3D reconstructions of coronal loops, using the EUVI telescopes of the two STEREO A and B spacecraft. The first triangulation of coronal loops was performed in an active region, observed with STEREO A and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5b8d035fe0e1413ba5a7157470b1d79a
https://doi.org/10.1086/529542
https://doi.org/10.1086/529542
Autor:
Paola Testa, Juan Martinez-Sykora, James R. Lemen, Theodore D. Tarbell, Sarah A. Jaeggli, Alan M. Title, Neal E. Hurlburt, J. P. Wülser, Mats Carlsson, Viggo Hansteen, Katharine K. Reeves, Charles C. Kankelborg, B. De Pontieu, Tiago M. D. Pereira, Lucia Kleint, Hui Tian, Leon Golub, S. McKillop, P. Boerner, S. H. Saar
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd76cf3e1a52812a778eebfc680e16b5
http://hdl.handle.net/10852/56957
http://hdl.handle.net/10852/56957
Publikováno v:
Solar Physics. 180:361-375
The 20 August 1992 flare around 14:28 UT was observed in Hα, He and Ca ii H with the imaging spectrographs at Locarno-Monti, Switzerland, with the radiotelescopes in Bern, and in soft and hard X-rays by the Yohkoh satellite. In this paper we discuss
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::26903851fb0d9b28da364bdcbef28d3c
https://doi.org/10.1023/a:1005022327027
https://doi.org/10.1023/a:1005022327027
Publikováno v:
The Astrophysical Journal. 482:490-497
We examine the spatial relationship between solar hard X-ray sources observed with the Hard X-Ray Telescope aboard Yohkoh and photospheric electric currents observed at Mees Solar Observatory. In 1993, Canfield et al. concluded that energetic electro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::80e7fddc6ddcedfc258b90f4fd300413
https://doi.org/10.1086/304131
https://doi.org/10.1086/304131