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Report on 02/04/2025 13:54:02
cdaweb was referenced in 1 papers
spdf was referenced in 1 papers
space physics data facility was referenced in 1 papers
omni was referenced in 4 papers
gif_walk was referenced in 1 papers
iri was referenced in 2 papers
international reference ionosphere was referenced in 1 papers
heliophysics digital resource library was referenced in 1 papers
heliocloud was referenced in 1 papers
9 of 88 possible papers ( 10% ) contained references to SPDF keywords
Authors=Saha, Prasenjit; Sluse, Dominique; Wagner, Jenny; Williams, Liliya L. R.
Title=Essentials of Strong Gravitational Lensing, 2024, doi:10.1007/s11214-024-01041-w10.48550/arXiv.2401.04165, ID=26841301
journal=Space Science Reviews
Keywords found:omni
Sample usage ( BODY ) =Here, we imagine the source emitting an omni-directional light flash, and the wavefront shows how far that light flash has travelled in a given time in different directions.
Authors=Cardesin-Moinelo, A.; Godfrey, J.; Grotheer, E.; Blake, R.; Damiani, S.; Wood, S.; Dressler, T.; Bruno, M.; Johnstone, A.; Lucas, L.; Marin-Yaseli de la Parra, J.; Merritt, D.; Sierra, M.; Maattanen, A.; Antoja-Lleonart, G.; Breitfellner, M.; Muniz, C.; Nespoli, F.; Riu, L.; Ashman, M.; Escalante, A.; Geiger, B.; Heather, D.; Hepburn, A.; Pistone, V.; Raga, F.; Valles, R.; Companys, V.; Martin, P.; Wilson, C.
Title=Mars Express: 20 Years of Mission, Science Operations and Data Archiving, 2024, doi:10.1007/s11214-024-01059-0, ID=27300164
journal=Space Science Reviews
Keywords found:omni
Sample usage ( BODY ) =The X-band signal, amplified by a 65 W Traveling Wave Tube Amplifier (TWTA), allows downlink of science (and housekeeping) telemetry at high data rates, whereas the 5 W S-band signal is used in Safe Mode. Two omni-directional Low Gain S-band only antennas on the +/-Z-faces were used during Launch and Early Orbit Phase (LEOP) and could provide a ‘back-door’ for low bit rate (7.8125 bps) in case that the HGA was not correctly Earth-pointed.
Authors=Walsh, B. M.; Kuntz, K. D.; Busk, S.; Cameron, T.; Chornay, D.; Chuchra, A.; Collier, M. R.; Connor, C.; Connor, H. K.; Cravens, T. E.; Dobson, N.; Galeazzi, M.; Kim, H.; Kujawski, J.; Paw U, C. K.; Porter, F. S.; Naldoza, V.; Nutter, R.; Qudsi, R.; Sibeck, D. G.; Sembay, S.; Shoemaker, M.; Simms, K.; Thomas, N. E.; Atz, E.; Winkert, G.
Title=The Lunar Environment Heliophysics X-ray Imager (LEXI) Mission, 2024, doi:10.1007/s11214-024-01063-4, ID=28584993
journal=Space Science Reviews
Keywords found:cdaweb, spdf, space physics data facility
Sample usage ( BODY ) =Data will be stored and made publicly available in the Space Physics Data Facility (SPDF) Coordinated Data Analysis Web (CDAWeb) at NASA Goddard Space Flight Center.
Authors=McGranaghan, Ryan M.
Title=Complexity Heliophysics: A Lived and Living History of Systems and Complexity Science in Heliophysics, 2024, doi:10.1007/s11214-024-01081-210.48550/arXiv.2307.03287, ID=29247659
journal=Space Science Reviews
Keywords found:heliophysics digital resource library, heliocloud
Sample usage ( ACK ) =Thank you to the NASA Center for HelioAnalytics and Heliophysics Digital Resource Library for creating, maintaining, and making available HelioCloud, a cloud computing service for Heliophysicists.
Authors=Shearer, C. K.; McCubbin, F. M.; Eckley, S.; Simon, S. B.; Meshik, A.; McDonald, F.; Schmitt, H. H.; Zeigler, R. A.; Gross, J.; Mitchell, J.; Krysher, C.; Morris, R. V.; Parai, R.; Jolliff, B. L.; Gillis-Davis, J. J.; Joy, K. H.; Bell, S. K.; Lucey, P. G.; Sun, L.; Sharp, Z. D.; Dukes, C.; Sehlke, A.; Mosie, A.; Allton, J.; Amick, C.; Simon, J. I.; Erickson, T. M.; Barnes, J. J.; Dyar, M. D.; Burgess, K.; Petro, N.; Moriarty, D.; Curran, N. M.; Elsila, J. E.; Colina-Ruiz, R. A.; Kroll, T.; Sokaras, D.; Ishii, H. A.; Bradley, J. P.; Sears, D.; Cohen, B.; Pravdivseva, O.; Thompson, M. S.; Neal, C. R.; Hana, R.; Ketcham, R.; Welten, K.; the ANGSA science team
Title=Apollo Next Generation Sample Analysis (ANGSA): an Apollo Participating Scientist Program to Prepare the Lunar Sample Community for Artemis, 2024, doi:10.1007/s11214-024-01094-x, ID=30700046
journal=Space Science Reviews
Keywords found:
Authors=Hasegawa, H.; Argall, M. R.; Aunai, N.; Bandyopadhyay, R.; Bessho, N.; Cohen, I. J.; Denton, R. E.; Dorelli, J. C.; Egedal, J.; Fuselier, S. A.; Garnier, P.; Genot, V.; Graham, D. B.; Hwang, K. J.; Khotyaintsev, Y. V.; Korovinskiy, D. B.; Lavraud, B.; Lenouvel, Q.; Li, T. C.; Liu, Y. -H.; Michotte de Welle, B.; Nakamura, T. K. M.; Payne, D. S.; Petrinec, S. M.; Qi, Y.; Rager, A. C.; Reiff, P. H.; Schroeder, J. M.; Shuster, J. R.; Sitnov, M. I.; Stephens, G. K.; Swisdak, M.; Tian, A. M.; Torbert, R. B.; Trattner, K. J.; Zenitani, S.
Title=Advanced Methods for Analyzing in-Situ Observations of Magnetic Reconnection, 2024, doi:10.1007/s11214-024-01095-w10.48550/arXiv.2307.05867, ID=30806159
journal=Space Science Reviews
Keywords found:omni
Sample usage ( BODY ) =About 50 million measurements were extracted and then associated with a causal solar wind and IMF conditions from OMNI data using a solar wind propagation method (Safrankova et al. 2002 ).
Authors=Liu, Hang; Qin, Jianqi; Kamaci, Ulas; Kamalabadi, Farzad
Title=A Bayesian Framework for Accurate Determination of the Nighttime Ionospheric Parameters from the ICON FUV Observations, 2024, doi:10.1007/s11214-024-01106-w, ID=31169236
journal=Space Science Reviews
Keywords found:iri
Sample usage ( BODY ) =In Sect. 4 , we use the Bayesian method with prior distributions that are constructed based on the NRLMSIS 2.0 model (Emmert et al. 2021 ) and the IRI 2016 model (Bilitza et al. 2017 ) to resolve the bias in the ICON FUV L2.5 v05 data product.
Authors=Lugaz, Noe; Lee, Christina O.; Al-Haddad, Nada; Lillis, Robert J.; Jian, Lan K.; Curtis, David W.; Galvin, Antoinette B.; Whittlesey, Phyllis L.; Rahmati, Ali; Zesta, Eftyhia; Moldwin, Mark; Summerlin, Errol J.; Larson, Davin E.; Courtade, Sasha; French, Richard; Hunter, Richard; Covitti, Federico; Cosgrove, Daniel; Prall, J. D.; Allen, Robert C.; Zhuang, Bin; Winslow, Reka M.; Scolini, Camilla; Lynch, Benjamin J.; Filwett, Rachael J.; Palmerio, Erika; Farrugia, Charles J.; Smith, Charles W.; Mostl, Christian; Weiler, Eva; Janvier, Miho; Regnault, Florian; Livi, Roberto; Nieves-Chinchilla, Teresa
Title=The Need for Near-Earth Multi-Spacecraft Heliospheric Measurements and an Explorer Mission to Investigate Interplanetary Structures and Transients in the Near-Earth Heliosphere, 2024, doi:10.1007/s11214-024-01108-8, ID=31169242
journal=Space Science Reviews
Keywords found:omni
Sample usage ( BODY ) =For example, the highest solar wind speed ever measured near 1 au is about 2300 km s -1 for the 2012 July 23 CME measured by STEREO-A (Liu et al. 2014 ), which was associated with an IMF magnitude of ~110 nT. Based on OMNI data over the past 30 years, 99.9% of the 1-hour average of the measured proton velocity were below 820 km s -1 , 99.9% of the 1-hour average of the proton density were below 46 cm -3 , and 99.9% of the 1-hour dynamic pressure were below 18 nPa, while 99.9% of the 1-hour IMF magnitude were below 28 nT. 1-min measurements do reach higher extremes than those listed here.
Authors=Yamauchi, M.; Christon, S.; Dandouras, I.; Haaland, S.; Kastinen, D.; Kistler, L. M.; Mann, I.; Nozawa, S.; Plane, J. M. C.; Saito, Y.; Schulz, L.; Watababe, S.; Wurz, P.; Yau, A. W.
Title=Heavy Molecular and Metallic Ions in the Magnetosphere, 2024, doi:10.1007/s11214-024-01114-w, ID=31639866
journal=Space Science Reviews
Keywords found:iri, international reference ionosphere
Sample usage ( BODY ) =These models provide the distribution of the modeled species beyond what the empirical International Reference Ionosphere (IRI) model provides. Table 11 Models relevant to upflow of molecular and metallic ions reaching the exobase *1 Request to Juan Diego Carrillo Sanchez (juandiego.carrillosanchez@nasa.gov) For the ionospheric and mesospheric heavy ions to be lifted, a common model of the neutral convection and electromagnetic fields to estimate the dynamics of the atomic ions can be used for both the molecular and metallic ions.
