Zobrazeno 1 - 10
of 29
pro vyhledávání: '"Extraterrestrial Physics, Space Sciences"'
Autor:
Alan Wood, Americo Gonzalez-Esparza, John M. Clover, Richard Fallows, M. S. Hamilton, Pete Riley, Andy Breen, Ernesto Aguilar-Rodriguez, Christopher J. Owen, E. A. Jensen, S. K. Glubokova, V. I. Shishov, Huw Morgan, Bernard V. Jackson, I. V. Chashei, P. K. Manoharan, Jon A. Linker, S. A. Tyul’bashev, A. S. Giunta, B. Pintér, G. Agalya, P. P. Hick, Andrew Walsh, Ken'ichi Fujiki, Munetoshi Tokumaru, Mathew J. Owens, Mario M. Bisi, Zoran Mikic
Publikováno v:
Bisi, M. M.; Breen, A. R.; Jackson, B. V.; Fallows, R. A.; Walsh, A. P.; Mikić, Z.; et al.(2010). From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection. Solar Physics: A Journal for Solar and Solar-Stellar Research and the Study of Solar Terrestrial Physics, 265(1), pp 49-127. doi: 10.1007/s11207-010-9602-8. Retrieved from: http://www.escholarship.org/uc/item/41x2g3rm
We report the results of a multi-instrument, multi-technique, coordinated study of the solar eruptive event of 13 May 2005. We discuss the resultant Earth-directed (halo) coronal mass ejection (CME), and the effects on the terrestrial space environme
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3d147acbf7217d8a1c96fb17dd5f0cad
https://doi.org/10.1007/s11207-010-9602-8
https://doi.org/10.1007/s11207-010-9602-8
Publikováno v:
Ulrich, R. K.; Parker, D.; Bertello, L.; & Boyden, J.(2010). Modeling Total Solar Irradiance Variations Using Automated Classification Software on Mount Wilson Data. Solar Physics: A Journal for Solar and Solar-Stellar Research and the Study of Solar Terrestrial Physics, 261(1), pp 11-34. doi: 10.1007/s11207-009-9460-4. Retrieved from: http://www.escholarship.org/uc/item/19t6w7c3
We present results using the AutoClass analysis application available at NASA/Ames Intelligent Systems Div. (2002) which is a Bayesian, finite mixture model classification system developed by Cheeseman and Stutz (1996). We apply this system to Mount
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e565fe9aa4e4138891acd971d23f4d59
https://doi.org/10.1007/s11207-009-9460-4
https://doi.org/10.1007/s11207-009-9460-4
Publikováno v:
Jian, L. K.; Russell, C. T.; Luhmann, J. G.; Galvin, A. B.; & MacNeice, P. J.(2009). Multi-Spacecraft Observations: Stream Interactions and Associated Structures. Solar Physics: A Journal for Solar and Solar-Stellar Research and the Study of Solar Terrestrial Physics, 259(1), pp 345-360. doi: 10.1007/s11207-009-9445-3. Retrieved from: http://www.escholarship.org/uc/item/08v2s8p7
The stream interaction region (SIR), formed when a fast stream overtakes a preceding slow stream, is the predominant large-scale solar wind structure at this early phase of the STEREO mission. Using multi-spacecraft observations from STEREO A and B,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7a052ff332caaaa19cf6404697f25a59
https://doi.org/10.1007/s11207-009-9445-3
https://doi.org/10.1007/s11207-009-9445-3
Autor:
Alan E. Rubin, Byeon-Gak Choi
Publikováno v:
Rubin, Alan E.; & Choi, Byeon-Gak. (2009). Origin of Halogens and Nitrogen in Enstatite Chondrites. Earth, Moon, and Planets: An International Journal of Solar System Science, 105(1), pp 41-53. doi: 10.1007/s11038-009-9316-9. Retrieved from: http://www.escholarship.org/uc/item/07h3r2cx
The EH and EL enstatite chondrites are the most reduced chondrite groups, having formed in nebular regions where the gas may have had high C/O and/or pH2/pH2O ratios. Enstatite chondrites (particularly EH) have higher CI- and Mg-normalized abundances
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::509f46bf0be384482f2ae2680eadb1c4
https://doi.org/10.1007/s11038-009-9316-9
https://doi.org/10.1007/s11038-009-9316-9
Autor:
Christopher T. Russell, Gordon Petrie, Kristin Simunac, Lan Jian, Emilia Kilpua, P. Schroeder, H. A. Elliott, Janet G. Luhmann, Yan Li, Davin Larson, Antoinette B. Galvin, J. T. Gosling
Publikováno v:
Kilpua, E. K.; Luhmann, J. G.; Gosling, J.; Li, Y.; Elliott, H.; Russell, C. T.; et al.(2009). Small Solar Wind Transients and Their Connection to the Large-Scale Coronal Structure. Solar Physics: A Journal for Solar and Solar-Stellar Research and the Study of Solar Terrestrial Physics, 256(1), pp 327-344. doi: 10.1007/s11207-009-9366-1. Retrieved from: http://www.escholarship.org/uc/item/0w40r9v8
It has been realized for some time that the slow solar wind with its embedded heliospheric current sheet often exhibits complex features suggesting at least partially transient origin. In this paper we investigate the structure of the slow solar wind
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e49dd09a990f80bb46186e9940b805c7
https://doi.org/10.1007/s11207-009-9366-1
https://doi.org/10.1007/s11207-009-9366-1
Autor:
Christopher T. Russell, Charles N. Arge, Y. Liu, I. de Pater, Christina O. Lee, Janet G. Luhmann, Xuepu Zhao, Pete Riley
Publikováno v:
Lee, C. O.; Luhmann, J. G.; Zhao, X. P.; Liu, Y.; Riley, P.; Arge, C. N.; et al.(2009). Effects of the Weak Polar Fields of Solar Cycle 23: Investigation Using OMNI for the STEREO Mission Period. Solar Physics: A Journal for Solar and Solar-Stellar Research and the Study of Solar Terrestrial Physics, 256(1), pp 345-363. doi: 10.1007/s11207-009-9345-6. Retrieved from: http://www.escholarship.org/uc/item/15v8k1wm
The current solar cycle minimum seems to have unusual properties that appear to be related to weak solar polar magnetic fields. We investigate signatures of this unusual polar field in the ecliptic near-Earth interplanetary magnetic field (IMF) for t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::083e634058e558b8a1e76b2ce7dc0c75
https://doi.org/10.1007/s11207-009-9345-6
https://doi.org/10.1007/s11207-009-9345-6
Autor:
Bernard V. Jackson, P. P. Hick, Gareth Dorrian, Mario M. Bisi, John M. Clover, Andy Breen, Richard Fallows
Publikováno v:
Bisi, M. M.; Jackson, B. V.; Breen, A. R.; Dorrian, G. D.; Fallows, R. A.; Clover, J. M.; et al.(2010). Three-Dimensional (3-D) Reconstructions of EISCAT IPS Velocity Data in the Declining Phase of Solar Cycle 23. Solar Physics: A Journal for Solar and Solar-Stellar Research and the Study of Solar Terrestrial Physics, 265(1), pp 233-244. doi: 10.1007/s11207-010-9594-4. Retrieved from: http://www.escholarship.org/uc/item/81d5t21s
The European Incoherent SCATter (EISCAT) radar has been used for remote-sensing observations of interplanetary scintillation (IPS) for a quarter of a century. During the April/May 2007 observing campaign, a large number of observations of IPS using E
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::224a6625a580b75c11795175a510d69a
http://www.escholarship.org/uc/item/81d5t21s
http://www.escholarship.org/uc/item/81d5t21s
Autor:
Yan Li, B. J. Lynch, George H. Fisher, Yang Liu, Janet G. Luhmann, Guillermo Stenborg, Brian T. Welsch, R. W. Nightingale
Publikováno v:
Li, Y.; Lynch, B. J.; Welsch, B. T.; Stenborg, G. A.; Luhmann, J. G.; Fisher, G. H.; et al.(2010). Sequential Coronal Mass Ejections from AR8038 in May 1997. Solar Physics: A Journal for Solar and Solar-Stellar Research and the Study of Solar Terrestrial Physics, 264(1), pp 149-164. doi: 10.1007/s11207-010-9547-y. Retrieved from: http://www.escholarship.org/uc/item/8d01c0tw
Three homologous coronal mass ejections (CMEs) occurred on 5, 12 and 16 May 1997 from the single magnetic polarity inversion line (PIL) of AR8038. The three events together provide STEREO-like quadrature views of the 12 May 1997 CME and EIT double di
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::505357b0a7922c9ff67612d8cc1ff27b
http://www.escholarship.org/uc/item/8d01c0tw
http://www.escholarship.org/uc/item/8d01c0tw
Autor:
Iannis Dandouras, Paul J. Kellogg, Andrei Fedorov, R. Karrer, C. Briand, Peter Wurz, Benoit Lavraud, Christopher T. Russell, Andrea Opitz, Emmanuel Penou, Philippe Louarn, Davin Larson, D. W. Curtis, David M. Malaspina, P. Schroeder, Antoinette B. Galvin, J. A. Sauvaud, Pierre Henri, Janet G. Luhmann
Publikováno v:
Solar Physics
Solar Physics, 2010, 266, pp.369-377. ⟨10.1007/s11207-010-9613-5⟩
Opitz, A.; Sauvaud, J.-A.; Fedorov, A.; Wurz, P.; Luhmann, J. G.; Lavraud, B.; Russell, C. T.; Kellogg, P.; Briand, C.; Henri, P.; Malaspina, D. M.; Louarn, P.; Curtis, D. W.; Penou, E.; Karrer, R.; Galvin, A. B.; Larson, D. E.; Dandouras, I.; Schroeder, P. (2010). Temporal Evolution of the Solar-Wind Electron Core Density at Solar Minimum by Correlating SWEA Measurements from STEREO A and B. Solar physics, 266(2), pp. 369-377. Springer 10.1007/s11207-010-9613-5
Opitz, A.; Sauvaud, J.-A.; Fedorov, A.; Wurz, P.; Luhmann, J. G.; Lavraud, B.; et al.(2010). Temporal Evolution of the Solar-Wind Electron Core Density at Solar Minimum by Correlating SWEA Measurements from STEREO A and B. Solar Physics: A Journal for Solar and Solar-Stellar Research and the Study of Solar Terrestrial Physics, 266(2), pp 369-377. doi: 10.1007/s11207-010-9613-5. Retrieved from: http://www.escholarship.org/uc/item/242227m2
Solar Physics, 2010, 266, pp.369-377. ⟨10.1007/s11207-010-9613-5⟩
Opitz, A.; Sauvaud, J.-A.; Fedorov, A.; Wurz, P.; Luhmann, J. G.; Lavraud, B.; Russell, C. T.; Kellogg, P.; Briand, C.; Henri, P.; Malaspina, D. M.; Louarn, P.; Curtis, D. W.; Penou, E.; Karrer, R.; Galvin, A. B.; Larson, D. E.; Dandouras, I.; Schroeder, P. (2010). Temporal Evolution of the Solar-Wind Electron Core Density at Solar Minimum by Correlating SWEA Measurements from STEREO A and B. Solar physics, 266(2), pp. 369-377. Springer 10.1007/s11207-010-9613-5
Opitz, A.; Sauvaud, J.-A.; Fedorov, A.; Wurz, P.; Luhmann, J. G.; Lavraud, B.; et al.(2010). Temporal Evolution of the Solar-Wind Electron Core Density at Solar Minimum by Correlating SWEA Measurements from STEREO A and B. Solar Physics: A Journal for Solar and Solar-Stellar Research and the Study of Solar Terrestrial Physics, 266(2), pp 369-377. doi: 10.1007/s11207-010-9613-5. Retrieved from: http://www.escholarship.org/uc/item/242227m2
International audience; The twin STEREO spacecraft provide a unique tool to study the temporal evolution of the solar-wind properties in the ecliptic since their longitudinal separation increases with time. We derive the characteristic temporal varia
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::21c2930112473246de45cc7ebf2fb85c
https://hal.science/hal-03732620
https://hal.science/hal-03732620
Autor:
Jean-Christophe Loison, Ian W. M. Smith, Wolf D. Geppert, Jürgen Troe, Karin I. Öberg, Harold Linnartz, Eric Herbst, Valentine Wakelam, Pascal Pernot, Marcelino Agúndez, Evelyne Roueff, Herma M. Cuppen, D. Talbi
Publikováno v:
Space Science Reviews
Space Science Reviews, Springer Verlag, 2010, 156 (1-4), pp.13-72
Space Science Reviews 2010
Space Science Reviews 2010, 2010, Online First, ⟨10.1007/s11214-010-9712-5⟩
Space Science Reviews, Springer Verlag, 2010, 156 (1-4), ⟨10.1007/s11214-010-9712-5⟩
Space Science Reviews, Springer Verlag, 2010, 156 (1-4), pp.13-72
Space Science Reviews 2010
Space Science Reviews 2010, 2010, Online First, ⟨10.1007/s11214-010-9712-5⟩
Space Science Reviews, Springer Verlag, 2010, 156 (1-4), ⟨10.1007/s11214-010-9712-5⟩
We survey the current situation regarding chemical modelling of the synthesis of molecules in the interstellar medium. The present state of knowledge concerning the rate coefficients and their uncertainties for the major gas-phase processes -- ion-ne
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5a6a5795613c7f54c6457d641ffd66a6
http://resolver.sub.uni-goettingen.de/purl?gs-1/7368
http://resolver.sub.uni-goettingen.de/purl?gs-1/7368