Search

Your search keyword '"Harra, L."' showing total 361 results
Start Over Author "Harra, L."
361 results on '"Harra, L."'

101. Coordination within the remote sensing payload on the Solar Orbiter mission

Author

Auchère, F., primary, Andretta, V., additional, Antonucci, E., additional, Bach, N., additional, Battaglia, M., additional, Bemporad, A., additional, Berghmans, D., additional, Buchlin, E., additional, Caminade, S., additional, Carlsson, M., additional, Carlyle, J., additional, Cerullo, J. J., additional, Chamberlin, P. C., additional, Colaninno, R. C., additional, Davila, J. M., additional, De Groof, A., additional, Etesi, L., additional, Fahmy, S., additional, Fineschi, S., additional, Fludra, A., additional, Gilbert, H. R., additional, Giunta, A., additional, Grundy, T., additional, Haberreiter, M., additional, Harra, L. K., additional, Hassler, D. M., additional, Hirzberger, J., additional, Howard, R. A., additional, Hurford, G., additional, Kleint, L., additional, Kolleck, M., additional, Krucker, S., additional, Lagg, A., additional, Landini, F., additional, Long, D. M., additional, Lefort, J., additional, Lodiot, S., additional, Mampaey, B., additional, Maloney, S., additional, Marliani, F., additional, Martinez-Pillet, V., additional, McMullin, D. R., additional, Müller, D., additional, Nicolini, G., additional, Orozco Suarez, D., additional, Pacros, A., additional, Pancrazzi, M., additional, Parenti, S., additional, Peter, H., additional, Philippon, A., additional, Plunkett, S., additional, Rich, N., additional, Rochus, P., additional, Rouillard, A., additional, Romoli, M., additional, Sanchez, L., additional, Schühle, U., additional, Sidher, S., additional, Solanki, S. K., additional, Spadaro, D., additional, St Cyr, O. C., additional, Straus, T., additional, Tanco, I., additional, Teriaca, L., additional, Thompson, W. T., additional, del Toro Iniesta, J. C., additional, Verbeeck, C., additional, Vourlidas, A., additional, Watson, C., additional, Wiegelmann, T., additional, Williams, D., additional, Woch, J., additional, Zhukov, A. N., additional, and Zouganelis, I., additional

Published
2020
Full Text
View/download PDF

102. Understanding the origins of the heliosphere: integrating observations and measurements from Parker Solar Probe, Solar Orbiter, and other space- and ground-based observatories

Author

Velli, M., primary, Harra, L. K., additional, Vourlidas, A., additional, Schwadron, N., additional, Panasenco, O., additional, Liewer, P. C., additional, Müller, D., additional, Zouganelis, I., additional, St Cyr, O. C., additional, Gilbert, H., additional, Nieves-Chinchilla, T., additional, Auchère, F., additional, Berghmans, D., additional, Fludra, A., additional, Horbury, T. S., additional, Howard, R. A., additional, Krucker, S., additional, Maksimovic, M., additional, Owen, C. J., additional, Rodríguez-Pacheco, J., additional, Romoli, M., additional, Solanki, S. K., additional, Wimmer-Schweingruber, R. F., additional, Bale, S., additional, Kasper, J., additional, McComas, D. J., additional, Raouafi, N., additional, Martinez-Pillet, V., additional, Walsh, A. P., additional, De Groof, A., additional, and Williams, D., additional

Published
2020
Full Text
View/download PDF

103. The Solar Orbiter EUI instrument: The Extreme Ultraviolet Imager

Author

Rochus, P., primary, Auchère, F., additional, Berghmans, D., additional, Harra, L., additional, Schmutz, W., additional, Schühle, U., additional, Addison, P., additional, Appourchaux, T., additional, Aznar Cuadrado, R., additional, Baker, D., additional, Barbay, J., additional, Bates, D., additional, BenMoussa, A., additional, Bergmann, M., additional, Beurthe, C., additional, Borgo, B., additional, Bonte, K., additional, Bouzit, M., additional, Bradley, L., additional, Büchel, V., additional, Buchlin, E., additional, Büchner, J., additional, Cabé, F., additional, Cadiergues, L., additional, Chaigneau, M., additional, Chares, B., additional, Choque Cortez, C., additional, Coker, P., additional, Condamin, M., additional, Coumar, S., additional, Curdt, W., additional, Cutler, J., additional, Davies, D., additional, Davison, G., additional, Defise, J.-M., additional, Del Zanna, G., additional, Delmotte, F., additional, Delouille, V., additional, Dolla, L., additional, Dumesnil, C., additional, Dürig, F., additional, Enge, R., additional, François, S., additional, Fourmond, J.-J., additional, Gillis, J.-M., additional, Giordanengo, B., additional, Gissot, S., additional, Green, L. M., additional, Guerreiro, N., additional, Guilbaud, A., additional, Gyo, M., additional, Haberreiter, M., additional, Hafiz, A., additional, Hailey, M., additional, Halain, J.-P., additional, Hansotte, J., additional, Hecquet, C., additional, Heerlein, K., additional, Hellin, M.-L., additional, Hemsley, S., additional, Hermans, A., additional, Hervier, V., additional, Hochedez, J.-F., additional, Houbrechts, Y., additional, Ihsan, K., additional, Jacques, L., additional, Jérôme, A., additional, Jones, J., additional, Kahle, M., additional, Kennedy, T., additional, Klaproth, M., additional, Kolleck, M., additional, Koller, S., additional, Kotsialos, E., additional, Kraaikamp, E., additional, Langer, P., additional, Lawrenson, A., additional, Le Clech’, J.-C., additional, Lenaerts, C., additional, Liebecq, S., additional, Linder, D., additional, Long, D. M., additional, Mampaey, B., additional, Markiewicz-Innes, D., additional, Marquet, B., additional, Marsch, E., additional, Matthews, S., additional, Mazy, E., additional, Mazzoli, A., additional, Meining, S., additional, Meltchakov, E., additional, Mercier, R., additional, Meyer, S., additional, Monecke, M., additional, Monfort, F., additional, Morinaud, G., additional, Moron, F., additional, Mountney, L., additional, Müller, R., additional, Nicula, B., additional, Parenti, S., additional, Peter, H., additional, Pfiffner, D., additional, Philippon, A., additional, Phillips, I., additional, Plesseria, J.-Y., additional, Pylyser, E., additional, Rabecki, F., additional, Ravet-Krill, M.-F., additional, Rebellato, J., additional, Renotte, E., additional, Rodriguez, L., additional, Roose, S., additional, Rosin, J., additional, Rossi, L., additional, Roth, P., additional, Rouesnel, F., additional, Roulliay, M., additional, Rousseau, A., additional, Ruane, K., additional, Scanlan, J., additional, Schlatter, P., additional, Seaton, D. B., additional, Silliman, K., additional, Smit, S., additional, Smith, P. J., additional, Solanki, S. K., additional, Spescha, M., additional, Spencer, A., additional, Stegen, K., additional, Stockman, Y., additional, Szwec, N., additional, Tamiatto, C., additional, Tandy, J., additional, Teriaca, L., additional, Theobald, C., additional, Tychon, I., additional, van Driel-Gesztelyi, L., additional, Verbeeck, C., additional, Vial, J.-C., additional, Werner, S., additional, West, M. J., additional, Westwood, D., additional, Wiegelmann, T., additional, Willis, G., additional, Winter, B., additional, Zerr, A., additional, Zhang, X., additional, and Zhukov, A. N., additional

Published
2020
Full Text
View/download PDF

104. The Hinode(Solar-B)Mission: An Overview

Author

Kosugi, T, Matsuzaki, K, Sakao, T, Shimizu, T, Sone, Y, Tachikawa, S, Minesugi, K, Ohnishi, A, Yamada, T, Tsuneta, S, Hara, H, Ichimoto, K, Suematsu, Y, Shimojo, M, Watanabe, T, Shimada, S, Davis, J. M, Hill, L. D, Owens, J. K, Title, A. M, Culhane, J. L, Harra, L. K, Doschek, G. A, and Golub, L

Subjects
Astronomy
Abstract

The Hinode satellite (formerly Solar-B) of the Japan Aerospace Exploration Agency's Institute of Space and Astronautical Science (ISAS/JAXA) was successfully launched in September 2006. As the successor to the Yohkoh mission, it aims to understand how magnetic energy is transferred from the photosphere to the upper atmospheres and resulting in explosive energy releases. Hinode is an observatory style mission, with all the instruments being designed and built to work together to address the science aims. There are three instruments onboard: the Solar Optical Telescope (SOT), the EUV Imaging Spectrometer (EIS), and the X-ray Telescope (XRT). This paper overviews the mission, including the satellite, the scientific payload and operations. It will conclude with discussions on how the international science community can participate in the analysis of the mission data.

Published
2007

105. Using SOHO to Understand CME-Producing Quiet-Region Filament Eruptions

Author

Sterling, A. C, Moore, R. L, and Harra, L. K

Subjects
Space Sciences (General)
Abstract

In recent years we have been studying solar eruptions in an attempt to determine their primary initiation mechanism. We have focused on events involving filaments, because motions of the filaments just prior to their violent eruption are indicative of changes in the entire magnetic field system involved in the eruption. When the pre-eruption filament resides in a quiet region, the motions leading up to eruption are slower than in similar eruptions in active regions due to the weaker magnetic field strength and correspondingly lower Alfven velocities. These early motions manifest themselves in a slow rise (a few km/s) of the filament, in some cases lasting several hours. After this the filament and associated magnetic structures erupt rapidly, accelerating to speeds of a few 10 kmh over a few minutes. Because of their slow evolution, quiet-region eruptions such as these can be effectively studied in EUV with SOHO/EIT, with its regular cadence of about 12 min. For several cases we have combined EIT images with SOHO/MDI magnetograms and data from other other instruments, and compared our observations with predictions from various eruption scenarios, in particular the "breakout" (Antiochos 1998), "tether cutting" (e.g., Moore et al. 2001), and MHD instability mechanisms. Here we present a representative example of a quiet-region eruption involving a filament ejection, that occurred on 2001 February 28 in a magnetically quadrupolar region and produced a halo CME in SOHO/LASCO images. In addition to EIT and MDI, we analyzed spectral data from SOHO/CDS and soft X-ray (SXR) images from Yohkoh/SXT. We found that flux emergence occurred near one end of the filament, and that both this emergence and resulting microflaring in SXRs and EUV were temporally and spatially closely related to the start of the filament's slow rise. Intensity changes (dimmings and brightenings) in the EIT and SXT images indicate that fields far removed from the erupting core were involved in the eruption, and that breakout-type reconnection did occur. Our observations allow us to investigate whether breakout was the trigger of the eruption, or merely a consequence of a more fundamental eruption process such as tether cutting or MHD instability occurring in a complex magnetic environment.

Published
2006

106. Initiation of the Slow-Rise and Fast-Rise Phases of an Erupting Solar Filament by Localized Emerging Magnetic Field via Microflaring

Author

Sterling, A. C, Moore, R. L, and Harra, L. K

Subjects
Solar Physics
Abstract

EUV data from EIT show that a filament of 2001 February 28 underwent a slow-rise phase lasting about 6 hrs, before rapidly erupting in a fast-rise phase. Concurrent images in soft X-rays (SXRs) from Yohkoh/SXT show that a series of three microflares, prominent in SXT images but weak in EIT approx.195 Ang EUV images, occurred near one end of the filament. The first and last microflares occurred respectively in conjunction with the start of the slow-rise phase and the start of the fast-rise phase, and the second microflare corresponded to a kink in the filament trajectory. Beginning within 10 hours of the start of the slow rise, new magnetic flux emerged at the location of the microflaring. This localized new flux emergence and the resulting microflares, consistent with reconnection between the emerging field and the sheared sigmoid core magnetic field holding the filament, apparently caused the slow rise of this field and the transition to explosive eruption. For the first time in such detail, the observations show this direct action of localized emerging flux in the progressive destabilization of a sheared core field in the onset of a coronal mass ejection (CME). Similar processes may have occurred in other recently-studied events, NASA supported this work through NASA SR&T and SEC GI grants.

Published
2006

111. The determination of electron densities in the solar atmosphere from the 1718.56 A/1486.51 A emission-line ratio in N IV

Author

Keenan, F. P, Harra, L. K, Doschek, G. A, and Cook, J. W

Subjects
Solar Physics
Abstract

The theoretical electron density sensitive emission-line ratio R = I(1718.56 a)/I(1486.51 A) in N IV is presented for a range of N(sub e)(approximately equals 10(exp 10) - 10(exp 12)/cu cm) applicable to higher density solar plasmas, such as active regions. A comparison of these calculations with the observed values of R of several solar features obtained with the Naval Research Laboratory's S082B spectrograph on board Skylab reveals general agreement between theory and observation at pointings just above the limb, where line blends with N IV 1718.56 A should be insignificant, which provides experimental support for the accuracy of the line ratio calculations.

Published
1994
Full Text
View/download PDF

112. Coronal electron density diagnostic from Fe XII

Author

Cook, J. W, Keenan, F. P, Harra, L. K, and Tayal, S. S

Subjects
Astrophysics
Abstract

We present observations of the forbidden coronal lines Fe XII 1242 A and 1349 A from active regions and from two flares, obtained by the SO82B slit spectrograph onboard Skylab. The line intensity ratio R = I(1242 A)/I(1349 A) is sensitive to electron density. We have calculated this ratio using recent atomic data, and obtained coronal electron densities at T = 1.5 x 10(exp 6) K for our observations. We find a range in N(sub e) of (0.5 to 7.2) x 10(exp 9)/cm(exp -3) for active regions, which is in good agreement with previous results from other diagnostic ratios in this temperature range, and of approximately (0.9 to 12) x 10(exp 9)/cm(exp -3) (or higher) for flares, which is generally low compared to previous flare results. The flare values employ particularly weak 1349 A observations and may not be reliable. From an observation of an active region just inside the solar limb, giving the best coverage in our data of both line profiles, we find a line width (FWHM) for both lines of 0.20 A, which corresponds to a nonthermal velocity of 18 km/sec.

Published
1994
Full Text
View/download PDF

113. Al II emission-line strengths in low-density astrophysical plasmas

Author

Keenan, F. P, Harra, L. K, Aggarwal, K. M, and Feibelman, W. A

Subjects
Astrophysics
Abstract

Theoretical values of the emission-line ratio R are derived for the transitions 3s2 1S-3s3p 3P2 and 3s2 1S-3s3p 3P1 in Al II, at 2660 and 2669 A, respectively. These ratios are compared with IUE observations of the planetary nebula NGC 7027 and the symbiotic star RR Tel, to illustrate the usefulness of the R as an electron density diagnostics. A value of R = 0.72 was deduced for NGC 7027, which implies log Ne = 4.2 for Te = 14,000 K. This is consistent with densities deduced earlier for this planetary nebula.

Published
1992
Full Text
View/download PDF

115. Production of High-Temperature Plasmas During the Early Phases of a C9.7 Flare. II. Bi-directional Flows Suggestive of Reconnection in a Pre-flare Brightening Region

Author

Sterling, Alphonse C., Harra, L. K., Watanabe, Tetsuya, and Hara, Hirohisa

Subjects
Physics, On board, Solar flare, Space and Planetary Science, law, Extreme ultraviolet lithography, Imaging spectrometer, Astronomy and Astrophysics, Magnetic reconnection, Plasma, Astrophysics, Flare, law.invention
Abstract

Accepted: 2012-07-17, 資料番号: SA1004351000

Published
2012

119. Evidence for Hot Fast Flow Above a Solar Flare Arcade

Author

Harra, L. K., Imada, Shinsuke, Aoki, Kuniya, Hara, Hirohisa, Watanabe, Tetsuya, and Shimizu, Toshifumi

Subjects
Physics, Sun: flares, Solar flare, Sun: corona, Astrophysics::High Energy Astrophysical Phenomena, Extreme ultraviolet lithography, Imaging spectrometer, Fast flow, FOS: Physical sciences, Astronomy and Astrophysics, Magnetic reconnection, Astrophysics, Space weather, Sun: UV radiation, law.invention, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, law, Physics::Space Physics, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Ultraviolet radiation, Solar and Stellar Astrophysics (astro-ph.SR), Flare
Abstract

Solar flares are one of the main forces behind space weather events. However the mechanism that drives such energetic phenomena is not fully understood. The standard eruptive flare model predicts that magnetic reconnection occurs high in the corona where hot fast flows are created. Some imaging or spectroscopic observations have indicated the presence of these hot fast flows but there have been no spectroscopic scanning observation to date to measure the two-dimensional structure quantitatively. We analyzed a flare that occurred on the west solar limb on 27 January 2012 observed by the Hinode EUV Imaging Spectrometer (EIS) and found that the hot (~30MK) fast (>500 km/s) component was located above the flare loop. This is consistent with magnetic reconnection taking place above the flare loop., 11 pages, 4 figures, accepted ApJL

Published
2013

120. The qualification campaign of the EUI instrument of Solar Orbiter

Author

Halain, J.-P., additional, Rochus, P., additional, Renotte, E., additional, Hermans, A., additional, Jacques, L., additional, Mazzoli, A., additional, Auchère, F., additional, Berghmans, D., additional, Harra, L., additional, Schühle, U., additional, Schmutz, W., additional, Aznar Cuadrado, R., additional, Dumesnil, C., additional, Gyo, M., additional, Kennedy, T., additional, Verbeeck, C., additional, and Smith, P., additional

Published
2016
Full Text
View/download PDF

124. The extreme UV imager telescope on-board the Solar Orbiter mission: overview of phase C and D

Author

Halain, J.-P., additional, Rochus, P., additional, Renotte, E., additional, Hermans, A., additional, Jacques, L., additional, Auchère, F., additional, Berghmans, D., additional, Harra, L., additional, Schühle, U., additional, Schmutz, W., additional, Zhukov, A., additional, Aznar Cuadrado, R., additional, Delmotte, F., additional, Dumesnil, C., additional, Gyo, M., additional, Kennedy, T., additional, Smith, P., additional, Tandy, J., additional, Mercier, R., additional, and Verbeeck, C., additional

Published
2015
Full Text
View/download PDF

128. Instrument for quantitative investigations on the physics of dynamics with UV/EUV high-throughput spectroscopy

Author

Shimizu, Toshifumi, Imada, Shinsuke, Watanabe, Tetsuya, Hara, Hirohisa, Ishobe, Hiroaki, Doschek, G., Korendyke, C., Teriaca, L., Schuehle, U., and Harra, L.

Abstract

第10回宇宙科学シンポジウム (2010年1月7日-8日. 宇宙航空研究開発機構宇宙科学研究本部), 10th Space Science Symposium (January 7-8, 2010. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)), Sagamihara, Kanagawa Japan, 「高スループットUV/EUV撮像分光望遠鏡」は、既存の分光望遠鏡に比べ１桁以上高いスループット(光子数)を持つUV-EUV域の分光観測を担う望遠鏡である。日本と欧米の研究者で組織されたHigh throughput UV/EUV spectroscopyサブワーキンググループ(chair 清水、co-chair: Doschek, メンバー：共著者)は、2009年3月から活動を始め、目指すサイエンスの検討やSOLAR-Cに搭載する雛形望遠鏡の検討を進めてきた。本ポスターにて望遠鏡の概要を紹介する。高スループットUV/EUV撮像分光望遠鏡は、定量的な物理診断(速度、温度、密度)を高解像度かつ高時間分解能で初めて可能とする画期的な望遠鏡であり、「ひので」が動画観測で明らかにした太陽大気でのダイナミックスや加熱など、太陽プラズマにおける物理素過程の理解を飛躍的に進めるものと期待されている。, 著者人数: 12人, 形態: カラー図版あり, 形態: CD-ROM1枚, Number of authors: 12, Physical characteristics: Original contains color illustrations, Note: One CD-ROM, 資料番号: AA0064742108

Published
2010

130. Erratum: 'Outflows at the edges of active regions: Contribution to solar wind formation?'

Author

Harra, L. K., Sakao, T., Mandrini, Cristina Hemilse, Hara, H., Imada, S., Young, P.R., van Driel Gesztelyi, Lidia, and Baker, D.

Subjects
Astronomía, Ciencias Físicas, SOLAR WIND [SUN], MAGNETIC FIELDS [SUN], CIENCIAS NATURALES Y EXACTAS
Abstract

Fil: Harra, L. K.. Mullard Space Science Laboratory; Reino Unido Fil: Sakao, T.. Institute of Space and Astronautical Science; Japón Fil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Hara, H.. National Astronomical Observatory of Japan; Japón Fil: Imada, S.. National Astronomical Observatory of Japan; Japón Fil: Young, P.R.. Rutherford Appleton Laboratory; Reino Unido Fil: van Driel Gesztelyi, Lidia. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia Fil: Baker, D.. Mullard Space Science Laboratory; Reino Unido

Published
2008

131. Using the Evolution of Coronal Dimming Regions to Probe the Global Magnetic Field Topology

Author

Attrill, G., Nakwacki, Maria Soledad, Harra, L. K., van Driel Gesztelyi, Lidia, Mandrini, Cristina Hemilse, Dasso, Sergio Ricardo, and Wang, J.

Subjects
Astronomía, CMES, purl.org/becyt/ford/1 [https], DIMMINGS, Ciencias Físicas, SUN, MAGNETIC CLOUDS, purl.org/becyt/ford/1.3 [https], CIENCIAS NATURALES Y EXACTAS
Abstract

We demonstrate that study of the evolving magnetic nature of coronal dimming regions can be used to probe the large-scale magnetic structure involved in the eruption of a coronal mass ejection (CME). We analyse the intensity evolution of coronal dimming regions using 195 Å data from the Extreme ultraviolet Imaging Telescope (EIT) on board the Solar and Heliospheric Observatory (SOHO). We measure the magnetic flux, using data from the SOHO/Michelson Doppler Imager (MDI), in the regions that seem most likely to be related to plasma removal. Then, we compare these magnetic flux measurements to the flux in the associated magnetic cloud (MC). Here, we present our analysis of the well-studied event on 12 May 1997 that took place just after solar minimum in a simple magnetic configuration. We present a synthesis of results already published and propose that driven “interchange reconnection” between the expanding CME structure with ‘`open’' field lines of the northern coronal hole region led to the asymmetric temporal and spatial evolution of the two main dimming regions, associated with this event. As a result of this reconnection process, we find the southern-most dimming region to be the principal foot-point of the MC. The magnetic flux from this dimming region and that of the MC are found to be in close agreement within the same order of magnitude, 1021 Mx. Fil: Attrill, G.. Mullard Space Science Laboratory; Reino Unido Fil: Nakwacki, Maria Soledad. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Harra, L. K.. Mullard Space Science Laboratory; Reino Unido Fil: van Driel Gesztelyi, Lidia. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia Fil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Wang, J.. National Astronomical Observatory; China

Published
2006

132. The EUV Imaging Spectrometer for Hinode

Author

Culhane, J. L., primary, Harra, L. K., additional, James, A. M., additional, Al-Janabi, K., additional, Bradley, L. J., additional, Chaudry, R. A., additional, Rees, K., additional, Tandy, J. A., additional, Thomas, P., additional, Whillock, M. C. R., additional, Winter, B., additional, Doschek, G. A., additional, Korendyke, C. M., additional, Brown, C. M., additional, Myers, S., additional, Mariska, J., additional, Seely, J., additional, Lang, J., additional, Kent, B. J., additional, Shaughnessy, B. M., additional, Young, P. R., additional, Simnett, G. M., additional, Castelli, C. M., additional, Mahmoud, S., additional, Mapson-Menard, H., additional, Probyn, B. J., additional, Thomas, R. J., additional, Davila, J., additional, Dere, K., additional, Windt, D., additional, Shea, J., additional, Hagood, R., additional, Moye, R., additional, Hara, H., additional, Watanabe, T., additional, Matsuzaki, K., additional, Kosugi, T., additional, Hansteen, V., additional, and Wikstol, Ø., additional

Full Text
View/download PDF

134. The Hinode (Solar-B) Mission: An Overview

Author

Kosugi, T., primary, Matsuzaki, K., additional, Sakao, T., additional, Shimizu, T., additional, Sone, Y., additional, Tachikawa, S., additional, Hashimoto, T., additional, Minesugi, K., additional, Ohnishi, A., additional, Yamada, T., additional, Tsuneta, S., additional, Hara, H., additional, Ichimoto, K., additional, Suematsu, Y., additional, Shimojo, M., additional, Watanabe, T., additional, Shimada, S., additional, Davis, J. M., additional, Hill, L. D., additional, Owens, J. K., additional, Title, A. M., additional, Culhane, J. L., additional, Harra, L. K., additional, Doschek, G. A., additional, and Golub, L., additional

Full Text
View/download PDF

136. The extreme UV imager of solar orbiter: from detailed design to flight model

Author

Halain, J.-P., additional, Rochus, P., additional, Renotte, E., additional, Auchère, F., additional, Berghmans, D., additional, Harra, L., additional, Schühle, U., additional, Schmutz, W., additional, Zhukov, A., additional, Aznar Cuadrado, R., additional, Delmotte, F., additional, Dumesnil, C., additional, Gyo, M., additional, Kennedy, T., additional, Mercier, R., additional, Verbeeck, F., additional, Thome, M., additional, Heerlein, K., additional, Hermans, A., additional, Jacques, L., additional, Mazzoli, A., additional, Meining, S., additional, Rossi, L., additional, Tandy, J., additional, Smith, P., additional, and Winter, B., additional

Published
2014
Full Text
View/download PDF

138. The EUI flight instrument of Solar Orbiter: from optical alignment to end-to-end calibration

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Halain, J.-P., Renotte, E., Auchère, F., Berghmans, D., Delmotte, F., Harra, L., Schmutz, W., Schühle, U., Aznar Cuadrado, R., Dumesnil, C., Gyo, M., Kennedy, T., Verbeeck, C., Barbay, J., Giordanengo, B., Gissot, S., Gottwald, A., Heerlein, K., Hellin, M.-L., Hermans, A., Hervier, V., Jacques, L., Laubis, C., Mazzoli, A., Meining, S., Mercier, R., Philippon, A., Roose, S., Rossi, L., Scholze, F., Smith, P., Teriaca, L., Zhang, X., and Rochus, P.

Published
2018
Full Text
View/download PDF

146. The EUI instrument on board the Solar Orbiter mission: from breadboard and prototypes to instrument model validation

Author

Halain, J.-P., primary, Rochus, P., additional, Renotte, E., additional, Appourchaux, T., additional, Berghmans, D., additional, Harra, L., additional, Schühle, U., additional, Schmutz, W., additional, Auchère, F., additional, Zhukov, A., additional, Dumesnil, C., additional, Delmotte, F., additional, Kennedy, T., additional, Mercier, R., additional, Pfiffner, D., additional, Rossi, L., additional, Tandy, J., additional, BenMoussa, A., additional, and Smith, P., additional

Published
2012
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results