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Report generated on 04/06/2026 12:31:30
cdaweb was referenced in 1 papers
spdf was referenced in 4 papers
space physics data facility was referenced in 5 papers
omni was referenced in 6 papers
omni2 was referenced in 0 papers
omni-2 was referenced in 0 papers
omniweb was referenced in 3 papers
ftpbrowser was referenced in 0 papers
helioweb was referenced in 0 papers
atmoweb was referenced in 0 papers
modelweb was referenced in 0 papers
sscweb was referenced in 1 papers
cohoweb was referenced in 0 papers
gifwalk was referenced in 0 papers
gif_walk was referenced in 0 papers
tipsod was referenced in 0 papers
hdp was referenced in 0 papers
heliophysics data portal was referenced in 0 papers
vitmo was referenced in 0 papers
hdrl was referenced in 0 papers
heliophysics digital resource library was referenced in 0 papers
heliocloud was referenced in 0 papers
10 of 131 possible papers ( 8% ) contained references to SPDF keywords
Authors=Kramer, Eva; Koller, Florian; Suni, Jonas; LaMoury, Adrian T.; Poppelwerth, Adrian; Glebe, Georg; Mohammed-Amin, Tara; Raptis, Savvas; Vuorinen, Laura; Weiss, Stefan; Xirogiannopoulou, Niki; Archer, Martin; Blanco-Cano, Xochitl; Gunell, Herbert; Hietala, Heli; Karlsson, Tomas; Plaschke, Ferdinand; Preisser, Luis; Roberts, Owen; Simon Wedlund, Cyril; Temmer, Manuela; Voros, Zoltan;
Title=Jets Downstream of Collisionless Shocks: Recent Discoveries and Challenges, 2025, doi:10.1007/s11214-024-01129-3, ID:32524297.
Keywords: omni
Sample usage ( BODY ) =Vuorinen et al. ( 2019 ) used THEMIS and OMNI data between 2008 and 2011 in the subsolar magnetosheath. LaMoury et al. ( 2021 ) studied magnetosheath jets using THEMIS and OMNI data in the years 2008-2018 which include the data set of Plaschke et al. ( 2013 ) and Vuorinen et al. ( 2019 ). Koller et al. ( 2022 ) used data from THEMIS and OMNI between 2008 and 2020, and combined different lists and catalogues for CMEs, SIRs and HSSs. (a) MMS1 ion energy spectrogram, (b) OMNI IMF components (GSE), (c) MMS1 ion velocity (GSE), and (d) MMS1 electron density.
Authors=Wang, Chi; Branduardi-Raymont, Graziella; Escoubet, C. Philippe; Forsyth, Colin;
Title=Solar Wind Magnetosphere Ionosphere Link Explorer (SMILE): Science and Mission Overview, 2025, doi:10.1007/s11214-024-01126-6, ID:34169656.
Keywords: spdf, omni, omniweb, sscweb
Sample usage ( ACK ) =The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov . The orbit information was obtained from SPDF - Satellite Situation Center Web (SS b interface at https://omniweb.gsfc.nasa.gov . The orbit information was obtained from SPDF - Satellite Situation Center Web (SSCWeb) from the from the GSFC/SPDF interface. obtained from SPDF - Satellite Situation Center Web (SSCWeb) from the from the GSFC/SPDF interface.
Sample usage ( ACK ) =s Science and Technology Facilities Council (STFC) grants ST/Y003276/1 and ST/X004902/1. The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov .
Sample usage ( BODY ) =Fig. 6 Solar wind flux () from OMNI solar wind data (King and Papitashvili 2005 ) during the 2015-2017 timeframe. We use the AL index from OMNI database between 2015 and 2017 and use AL below -200 nT to define a substorm. Fig. 9 Number of events when AL index is below -200 nT during 2015-2017 from OMNI data (King and Papitashvili 2005 ). The total number of events is 4556 and the number when AL is below -200
Sample usage ( ACK ) =The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov . The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov .
Sample usage ( ACK ) =The orbit information was obtained from SPDF - Satellite Situation Center Web (SSCWeb) from the from the GSFC/SPDF interface. We acknowledge the CAS and ESA project managers LI Jing and Davi
Sample usage ( BODY ) =IS A, D, E and SMILE would be crossing the magnetopause within a distance of +/-1 R E using SSCweb ( https://sscweb.gsfc.nasa.gov ) orbit tools. be crossing the magnetopause within a distance of +/-1 R E using SSCweb ( https://sscweb.gsfc.nasa.gov ) orbit tools.
Authors=Turc, Lucile; Takahashi, Kazue; Kajdic, Primoz; Kilpua, Emilia K. J.; Sarris, Theodoros; Palmroth, Minna; Soucek, Jan; Pfau-Kempf, Yann; Dimmock, Andrew; Takahashi, Naoko;
Title=From Foreshock 30-Second Waves to Magnetospheric Pc3 Waves, 2025, doi:10.1007/s11214-025-01152-y, ID:33462456.
Keywords: omni
Sample usage ( BODY ) =(a) IMF cone angle according to the solar wind OMNI data. (b) Dynamic spectra of the magnetic field compressional component at Van Allen Probe A. (b) IMF components and cone angle upstream of the Earth’s bow shock from the OMNI data set. (c) Magnetic field strength measured by the THEMIS-A spacecraft and its associated dynamic power s 2014 ) explored the characteristics and occurrence of radial IMF events using the near-Earth OMNI data base for 1995-2011. The authors found that such periods of nearly radial field are asso
Authors=Zhang, Xiao-Xin; Wang, Yong-Mei; He, Fei; Liu, Xiao-Hong; Zhu, Bin; Du, Guo-Jun; Mao, Jing-Hua; Li, Peng-Da; Huang, Wei-Peng; Wang, Tian-Fang; Liu, Jiu; Yu, Shui; Wang, Zi-Yue; Wang, Hou-Mao; Shi, En-Tao; Du, Pei-Heng; Li, Jing; Li, Lei; Dai, Lei; Zheng, Jianhua; Shi, Xingjian; Vey, Sylvain; Agnolon, David; Runciman, Chris; Berlich, Rene; Palma, Javier Sanchez; Aguado, Sergio Moreno; Hubert, Benoit; Vandenrijt, Jean-Francois; Brisbois, Jeremy; Fleury-Frenette, Karl; Lenaerts, Cedric; Rabecki, Frederic; Rosin, Julien; Hardy, Cedric; Carter, Jennifer; Donovan, Eric; Spanswick, Emma; Liang, Jun; Enno, Greg; Li, Hua-Wang; Forsyth, Colin; Escoubet, Christophe Philippe; Wang, Chi;
Title=A Holistic Approach to the SMILE Mission and SMILE Public Engagement, 2025, doi:10.1007/s11214-025-01175-5, ID:34939316.
Keywords: omni, omniweb
Sample usage ( ACK ) =N data can be found via data repositories such as https://www.bas.ac.uk/project/superdarn/ . OMNI data used can be found at https://omniweb.gsfc.nasa.gov/ .
Sample usage ( ACK ) =OMNI data used can be found at https://omniweb.gsfc.nasa.gov/ . More information about the Orbyts public engagement programme can be found at https://www.orbyts.org/ .
Authors=Trattner, K. J.; LaBelle, J.; Santolik, O.; Kletzing, C. A.; Miles, D. M.; Fuselier, S. A.; Bonnell, J. W.; Bounds, S. R.; Kolmasova, I.; Petrinec, S. M.; Sawyer, R. P.; Vines, S. K.; Moser-Gauthier, C.; Cairns, I. H.; Yeoman, T. K.;
Title=The Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) Mission Design, 2025, doi:10.1007/s11214-025-01185-3, ID:35414745.
Keywords: cdaweb, space physics data facility, omni, omniweb
Sample usage ( ACK ) =cknowledgements We acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb (or CDAWeb or ftp) service, and OMNI data.
Sample usage ( ACK ) =Acknowledgements We acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb (or CDAWeb or ftp) service, and OMNI data.
Sample usage ( ACK ) =dge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb (or CDAWeb or ftp) service, and OMNI data.
Sample usage ( BODY ) =The cusp location is determined from the model described in Sect. 3 , parameterized by the OMNI solar wind data set advanced in time by one solar cycle (11 years) The top panel of Fig. 7 sho
Sample usage ( ACK ) =Acknowledgements We acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb (or CDAWeb or ftp) service, and OMNI data.
Authors=Christopher, I. W.; Kletzing, C. A.; Crawford, D.; Piker, C.; Wilkinson, D.; Steele, K.; Petrinec, S. M.; Bounds, S.; Vaclavik, S.; Omar, S.; Shults, E.; Winter, M.; Miles, D. M.;
Title=The Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) Science Operations Center, 2025, doi:10.1007/s11214-025-01199-x, ID:36266059.
Keywords: spdf, space physics data facility
Sample usage ( BODY ) =Archiving all TRACERS data at NASA’s Space Physics Data Facility (SPDF). The first two items comprise the bulk of the data transfer from the SOC to the MOC, and form the heart of the Operatio Archiving The archive for the TRACERS mission will be at NASA’s Space Physics Data Facility (SPDF): https://spdf.gsfc.nasa.gov It will contain all science data products generated dur r the TRACERS mission will be at NASA’s Space Physics Data Facility (SPDF): https://spdf.gsfc.nasa.gov It will contain all science data products generated during the lifetime of the The archiving process itself will be executed by the SPDF, as they will pull data from the TRACERS Portal as it becomes available.
Sample usage ( ABSTRACT ) =ssion, and second by preparing mission data for transfer to the Space Physics Data Facility (SPDF) for long-term archiving.
Sample usage ( BODY ) =Archiving all TRACERS data at NASA’s Space Physics Data Facility (SPDF). The first two items comprise the bulk of the data transfer from the SOC to the MOC, and form the heart of the Operatio Archiving The archive for the TRACERS mission will be at NASA’s Space Physics Data Facility (SPDF): https://spdf.gsfc.nasa.gov It will contain all science data products generated during the l
Sample usage ( ABSTRACT ) =ring the active mission, and second by preparing mission data for transfer to the Space Physics Data Facility (SPDF) for long-term archiving.
Authors=Lin, Yu; Wang, Xueyi; Fuselier, Stephen A.; Connor, Hyunju K.; Miles, David M.; Kletzing, Craig A.;
Title=Global Hybrid Modeling in TRACERS Mission, 2025, doi:10.1007/s11214-025-01213-2, ID:36603143.
Keywords: spdf, space physics data facility
Sample usage ( BODY ) = will be hosted on the same web server and archived at the NASA Space Physics Data Facility (SPDF) alongside other TRACERS mission data. These simulation data will be further processed to ge
Sample usage ( BODY ) = made public, they will be hosted on the same web server and archived at the NASA Space Physics Data Facility (SPDF) alongside other TRACERS mission data.
Authors=McComas, D. J.; Christian, E. R.; Schwadron, N. A.; Gkioulidou, M.; Allegrini, F.; Baker, D. N.; Bzowski, M.; Clark, G.; Cohen, C. M. S.; Cohen, I.; Collura, C.; Cully, M. J.; Dalla, S.; Desai, M. I.; Driesman, A.; Eng, D.; Fox, N. J.; Funsten, H. O.; Fuselier, S. A.; Galli, A.; Giacalone, J.; Hahn, J.; Hegarty, K. P.; Horbury, T.; Horanyi, M.; Kistler, L. M.; Kubiak, M. A.; Kubota, S.; Livi, S.; Lugaz, N.; Lee, C. O.; Luhmann, J.; Matthaeus, W.; Mitchell, D. G.; Mitchell, J. G.; Moebius, E.; Pope, S.; Provornikova, E.; Rankin, J. S.; Reisenfeld, D. B.; Reno, C.; Richardson, J. D.; Russell, C. T.; Shaw-Lecerf, M. M.; Scherrer, J.; Skoug, R. M.; Shen, M. M.; Spence, H. E.; Sternovsky, Z.; Strumik, M.; Szalay, J. R.; Tapley, M.; Tokumaru, M.; Turner, D. L.; Weidner, S.; Westlake, J.; Wurz, P.; Zank, G. P.;
Title=Interstellar Mapping And Acceleration Probe: The NASA IMAP Mission, 2025, doi:10.1007/s11214-025-01224-z, ID:37617483.
Keywords: omni
Sample usage ( BODY ) =tally driven instrument design decisions and forward modeling based on more than 50 years of OMNI data. The configuration of the solar wind-viewing sector enables 0.1% transmission while kee
Authors=Horanyi, Mihaly; Tucker, Scott; Sternovsky, Zoltan; Tyagi, Kush; Knappmiller, Scott; Ayari, Ethan; Mikula, Rebecca; Szalay, Jamey R.; Kempf, Sascha; Bollendonk, Chip; Gurnee, Reid; Fisher, Melanie; McCann, Delphine; Coakley, Luisa; Gurst, Scott; Davis, Kristina; Bramer, Shelley; Miller, Marc; Neher, Joel; Newcomb, Gregory; Oberg, Samuel; Sayler, Jeffrey; Wade, Stacy; Deaton, Teresa; Doner, Alex; Fontanese, John; Grun, Eberhard; Miller, Colin; Wing, Robyn; Holguin, Lee; Fowle, Max; Hellickson, Tim; Rhode, Asher; Brennan, Nat; Hansen, Doug; O’Connor, Darren; Kostovny, Alec; Shaver, Sam; Looney, Karen; Turner, Neal J.; Hillier, Jon; Postberg, Frank; Srama, Ralf; Christian, Eric; Gkioulidou, Matina; McComas, David J.; Schwadron, Nathan A.;
Title=Interstellar Dust Experiment (IDEX) Onboard NASA’s Interstellar Mapping And Acceleration Probe (IMAP), 2025, doi:10.1007/s11214-025-01230-1, ID:37617678.
Keywords: spdf, space physics data facility
Sample usage ( BODY ) =e publicly available through the SDC website or NASA’s Space Physics Data Facility ( https://spdf.gsfc.nasa.gov ) Fig. 24 IDEX science data pipeline.
Sample usage ( BODY ) =All data products will be publicly available through the SDC website or NASA’s Space Physics Data Facility ( https://spdf.gsfc.nasa.gov ) Fig. 24 IDEX science data pipeline.
Authors=Lee, Christina O.; Christian, Eric R.; Sandoval, Laura; Crabtree, Alastair; Desai, Mihir I.; Gkioulidou, Matina; Heber, Bernd; Horbury, Timothy; Kistler, Lynn; Knuth, Jenny; Larsen, Kristopher; Livi, Stefano; Lucas, Greg M.; Matlin, Daniel E.; Marbois, Tori; McComas, David J.; Grant Mitchell, J.; Mukherjee, Joey; Rankin, Jamie S.; Reno, Chelle; Schwadron, Nathan A.; Shrestha, Bishwas L.; Skoug, Ruth M.; Smith, Evan J.; Starkey, Michael J.; Turner, Drew L.; Williams, Bradley D.; Zirnstein, Eric J.;
Title=Space Weather Science to Enhance Forecasting with the NASA IMAP Active Link for Real-Time (I-ALiRT) System, 2025, doi:10.1007/s11214-025-01244-9, ID:38115848.
Keywords: space physics data facility
Sample usage ( BODY ) =provided in Sect. 4 regarding the archiving of the I-ALiRT data at the NASA GSFC Space Physics Data Facility. The summary and concluding remarks are provided in Sect. 5 . provided in the Common Data Format (CDF), which are archived by NASA at the GSFC Space Physics Data Facility website (see Sect. 4 for further details). of the I-ALiRT space weather data latencies I-ALiRT Data File Archive at the NASA Space Physics Data Facility The near real-time I-ALiRT data set generated during the IMAP mission will be arc g the IMAP mission will be archived and publicly accessible through the NASA GSFC Space Physics Data Facility (SPDF) website ( https://spdf.gsfc.nasa.gov/ ).
