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Report generated on 04/06/2026 12:31:30
cdaweb was referenced in 6 papers
spdf was referenced in 2 papers
space physics data facility was referenced in 4 papers
omni was referenced in 8 papers
omni2 was referenced in 0 papers
omni-2 was referenced in 0 papers
omniweb was referenced in 7 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 0 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
17 of 288 possible papers ( 6% ) contained references to SPDF keywords
Authors=Kisvardai, Imre; Stempel, Filip; Randuska, Lukas; Mackovjak, Simon; Langer, Ronald; Strharsky, Igor; Kubancak, Jan;
Title=Analysis of 42 Years of Cosmic Ray Measurements by the Neutron Monitor at Lomnicky stit Observatory, 2025, doi:10.1029/2024EA003656, ID:32641156.
Keywords: space physics data facility, omni, omniweb
Sample usage ( BODY ) =We acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service and OMNI data (Papitashvili King, 2020).
Sample usage ( BODY ) =We acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service and OMNI data (Papitashvili King, 2020).
Sample usage ( BODY ) =The space weather indexes were downloaded from OMNIWeb https://omniweb.gsfc.nasa.gov/form/dx1.html (King Papitashvili, 2005). The space weather indexes were downloaded from OMNIWeb https://omniweb.gsfc.nasa.gov/form/dx1.html (King Papitashvili, 2005). We acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service and OMNI data (Papitashvili King, 2020).
Authors=Yu, Tingting; Cai, Xuguang; Ren, Zhipeng; Liu, Huixin; Qiu, Liuhui; Ma, Han; Li, Shaoyang; Wu, Kun;
Title=Local Time Variations of Quiet Time Meridional Winds During Solar Minimum Solstices Based on ICON Observations and Numerical Simulations, 2025, doi:10.1029/2024EA003880, ID:33014904.
Keywords: cdaweb
Sample usage ( BODY ) =F 10.7p , Kp, B y and B z indices are from https://cdaweb.gsfc.nasa.gov/cdaweb/sp_phys/ . AE and Kp indices were less than 1,000 nT and 4, respectively, except on DOY 356 and 358. F 10.7p , Kp, B y and B z indices are from https://cdaweb.gsfc.nasa.gov/cdaweb/sp_phys/ . AE and Kp indices were less than 1,000 nT and 4, respectively, except on DOY 356 and 358.
Authors=Majirsky, Adam; Mackovjak, Simon; Kostarova, Silvia; Amrich, Samuel;
Title=Extreme Space Weather Events of the Past 30 Years: Preparation for Data From Mission Vigil, 2025, doi:10.1029/2024EA003937, ID:33014908.
Keywords: space physics data facility, omni, omniweb
Sample usage ( BODY ) =We acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service and OMNI data (Papitashvili King, 2020).
Sample usage ( BODY ) =We acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service and OMNI data (Papitashvili King, 2020).
Sample usage ( BODY ) =The data source is the OMNIWeb database available at https://omniweb.gsfc.nasa.gov/form/dx1.html . 2 Figure Occurrence of great and severe geomagnetic storms, according to thresholds The data source is the OMNIWeb database available at https://omniweb.gsfc.nasa.gov/form/dx1.html . 2 Figure Occurrence of great and severe geomagnetic storms, according to thresholds We acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service and OMNI data (Papitashvili King, 2020).
Authors=Bernoux, Guillerme; Nguyen, Gautier; Sicard, Angelica; Maget, Vincent;
Title=Automatic Identification of Past Radiation Belts Electron Enhancement Events Using a Ground-Based Parameter, 2025, doi:10.1029/2024EA003945, ID:34100615.
Keywords: omni
Sample usage ( BODY ) =ates were removed after a visual inspection of their most appropriate begin and end dates in OMNI data (King Papitashvili, 2005). Reference Lists of Radiation Belts Electron Enhancement Even ates were removed after a visual inspection of their most appropriate begin and end dates in OMNI data (King Papitashvili, 2005). Reference Lists of Radiation Belts Electron Enhancement Even
Authors=Krishnan, Lalitha G.; Pant, Tarun Kumar; Manu, T.; Vineeth, C.; Jose, Lijo; Yaqub, Reuben Samson; Vishnupriya, K. S.; Sruthi, T. V.;
Title=Indian Equatorial Ionosphere Under the Influence of the May 2024 Geomagnetic Storm: Insights Into Electric Fields, Plasma Irregularities and F-Region Dynamics, 2025, doi:10.1029/2024EA004116, ID:34694576.
Keywords: cdaweb
Sample usage ( ACK ) =We gratefully acknowledge the CDAWeb team of NASA’s GSFC for the solar wind parameters and SYM-H index.
Sample usage ( BODY ) =observed from the L1 point and the geomagnetic index SYM-H were obtained from the NASA GSFC CDAWeb website. The SYM-H index derived based on the magnetic field observations from multiple loc olution data of the solar wind parameters and SYM-H index was downloaded from the NASA GSFC CDAWeb database available at https://cdaweb.gsfc.nasa.gov/ . -H index was downloaded from the NASA GSFC CDAWeb database available at https://cdaweb.gsfc.nasa.gov/ .
Authors=Liemohn, Michael W.; Rastatter, Lutz; Halford, Alexa J.; Zheng, Yihua; Garcia-Sage, Katherine S.; Redmon, Robert; Vines, Sarah K.;
Title=Guide for Conducting “Community Challenges” in Space Physics, 2025, doi:10.1029/2024EA004138, ID:34694580.
Keywords: cdaweb
Sample usage ( BODY ) =nd one-stop repository for space physics data, eventually leading to the creation of NASA’s CDAWeb ( https://cdaweb.gsfc.nasa.gov/ ). The analogous entity on the modeling side is th ace physics data, eventually leading to the creation of NASA’s CDAWeb ( https://cdaweb.gsfc.nasa.gov/ ). The analogous entity on the modeling side is the CCMC. nd one-stop repository for space physics data, eventually leading to the creation of NASA’s CDAWeb ( https://cdaweb.gsfc.nasa.gov/ ). The analogous entity on the modeling side is th ace physics data, eventually leading to the creation of NASA’s CDAWeb ( https://cdaweb.gsfc.nasa.gov/ ). The analogous entity on the modeling side is the CCMC.
Authors=Reddy, S. A.; Pi, X.; Forsyth, C.; Aruliah, A.; Smith, A.;
Title=Predictions of Equatorial Vertical Plasma Drift Using TEC Data and a Neural Network Model, 2025, doi:10.1029/2024EA004167, ID:34937621.
Keywords: cdaweb, omni
Sample usage ( BODY ) =asting System and OMNI data is freely available at: https://hapi-server.org/servers/#server=**CDAWeb** . The major Python packages used include: PyTorch, NumPy, Matplotlib, scikit-learn, and pan
Sample usage ( BODY ) =The Communication/Navigation Operations Forecasting System and OMNI data is freely available at: https://hapi-server.org/servers/#server=**CDAWeb** .
Authors=Jadhav, Ashish P.; Yamazaki, Yosuke; Gurubaran, S.; Sato, Kaoru; Koshin, Dai;
Title=2-Day Ionospheric Oscillations at Low Latitudes Due To an Ultra-Fast Kelvin Wave, 2025, doi:10.1029/2025EA004322, ID:34937648.
Keywords: spdf
Sample usage ( BODY ) =e obtained from the international GNSS service (IGS) and available at https://spdf.gsfc.nasa.gov/pub/data/gps/tec2hr_igs/ . The Hpo indices including Hp60 used in this study are available at
Authors=Akhavan-Tafti, M.; Soni, S. L.; Higgins, C.; Fung, S.; Lepri, S.; Lux, J.; Lazio, J.; Romero-Wolf, A.;
Title=SunRISE Ground Radio Lab: Monitoring Solar Radio Bursts With an Expansive Array of Antennae at High Schools Nationwide, 2025, doi:10.1029/2024EA004114, ID:34938425.
Keywords: cdaweb
Sample usage ( BODY ) =The data for CMEs and their associated flares, and Wind and are taken from http://cdaweb.gsfc.nasa.gov/istppub-lic/ and https://cdaw.gsfc.nasa.gov/CME_list/ .
Authors=Dodson-Robinson, Sarah E.; Haley, Charlotte;
Title=Multitaper Magnitude-Squared Coherence for Time Series With Missing Data: Understanding Oscillatory Processes Traced by Multiple Observables, 2025, doi:10.1029/2025EA004256, ID:34938546.
Keywords: omniweb
Sample usage ( BODY ) =Daily averaged Dst data were downloaded from NASA OMNIWeb ( https://omniweb.gsfc.nasa.gov ). Both downloads are archived at Dodson-Robinson and Haley ( 2025). Daily averaged Dst data were downloaded from NASA OMNIWeb ( https://omniweb.gsfc.nasa.gov ). Both downloads are archived at Dodson-Robinson and Haley ( 2025).
Authors=Dehvari, Masoud; Farzaneh, Saeed; Forootan, Ehsan;
Title=Dominant Longitudinal Wave-1 Pattern of the Equatorial Topside Ionosphere in the Early Morning Sector, 2025, doi:10.1029/2025EA004392, ID:36348646.
Keywords: omniweb
Sample usage ( BODY ) =The Ap index can be obtained from the OMNIWeb at https://omniweb.gsfc.nasa.gov/form/dx1.html . The Ap index can be obtained from the OMNIWeb at https://omniweb.gsfc.nasa.gov/form/dx1.html .
Authors=Khanal, Krishna; Zou, Ying; Zank, Gary P.;
Title=Suppression of Magnetopause Reconnection in the Presence of Cold Magnetospheric Plasma, 2025, doi:10.1029/2025EA004408, ID:38255947.
Keywords: spdf, omni, omniweb
Sample usage ( ACK ) =We acknowledge the use of ACE and WIND data from GSFC/SPDF OMNIWeb. Geotail magnetic field data were provided by T.
Sample usage ( BODY ) =ACE and WIND and OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov/form/omni_min.html .
Sample usage ( BODY ) =The dynamic pressure for ACE is based on 1 minute resolution time-shifted data from OMNI. For WIND, we used high resolution 3DP plasma data. el 2 data were obtained from https://themis.ssl.berkeley.edu/data/themis/ . ACE and WIND and OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov/for ata were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov/form/omni_min.html .
Sample usage ( ACK ) =We acknowledge the use of ACE and WIND data from GSFC/SPDF OMNIWeb. Geotail magnetic field data were provided by T.
Sample usage ( BODY ) =The geomagnetic conditions were obtained from OMNIWeb and the World Data Center (WDC) for Geomagnetism, Kyoto. The time shifted data sets from ACE and WIND were obtained from OMNIWeb. OMNIWeb uses a combination of Minimum Variance Analysis (MVA) (Sonnerup Scheible, 1998; Weimer et al., 2002) The time shifted data sets from ACE and WIND were obtained from OMNIWeb. OMNIWeb uses a combination of Minimum Variance Analysis (MVA) (Sonnerup Scheible, 1998; Weimer et al., 2002) high-resolution WIND data was time-shifted using the average of the time shifts provided by OMNIWeb (for one-minute resolution data) over the selected interval. ACE and WIND and OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov/form/omni_min.html . d WIND and OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov/form/omni_min.html .
Authors=Zhang, Kun; Wei, Fengsi; Huang, Yanshi; Zuo, Pingbing; Sun, Mengfei; Wang, Shijin; Yang, Hao; Ji, Jinlong; Shi, Huan; Lv, Liping; Chen, Zehao;
Title=Inversion of Global Thermospheric Density Map Based on Satellite Measurements Using Deep Learning RFR Network, 2025, doi:10.1029/2025EA004426, ID:38255964.
Keywords: omniweb
Sample usage ( BODY ) =Data Availability Statement The observed values of F10.7 are downloaded from OMNIWeb service (OMINI, 2015). The GOES-15 X-ray data can be acquired via NOAA website (NOAA, 2015).
Authors=Abdollahi, Danial; Alizadeh, M. Mahdi; Schuh, Harald; Tsai, Lung-Chih;
Title=Artificial Neural Network Model of High-Latitude Ionospheric Electric Potential: Hemispheric and Equinoctial Asymmetries, 2025, doi:10.1029/2025EA004331, ID:37562233.
Keywords: space physics data facility, omni
Sample usage ( ACK ) =We acknowledge the Space Physics Data Facility for the OMNI data (contact: Natalia Papitashvili Natalia.E.Papitashvili@nasa.gov ).
Sample usage ( ACK ) =We acknowledge the Space Physics Data Facility for the OMNI data (contact: Natalia Papitashvili Natalia.E.Papitashvili@nasa.gov ).
Sample usage ( BODY ) =iss.eo.esa.int/#swarm/Advanced/Plasma_Data/2Hz_TII_Cross-track_Dataset . The High resolution OMNI (HRO) IMF/solar wind data at 1-min are available at https://spdf.gsfc.nasa.gov/pub/data/**omni**
Authors=Sreekumar, Sreeba; Manju, G.; Pant, Tarun K.;
Title=Multi-Instrument Investigation of the Pre-Seismic Ionospheric Response to 2021 Haiti Earthquake, 2025, doi:10.1029/2025EA004394, ID:37562253.
Keywords: space physics data facility, omniweb
Sample usage ( ACK ) =The authors also acknowledge NASAs Space Physics Data Facility, United States Geological Survey (USGS), NOAA Physical Sciences Laboratory (NOAA PSL) for the various data sets used in the stu
Sample usage ( BODY ) = geomagnetic and solar indices such as Dst and F10.7 respectively are obtained from https://omniweb.gsfc.nasa.gov/form/dx1.html . The seismic event information may be obtained from USGS datab
Authors=Noh, Sung Jun; Morley, Steven K.; Cowee, Misa M.; Jordanova, Vania K.;
Title=A Probabilistic Model for Global EMIC Wave Activity Using Van Allen Probes Observations, 2025, doi:10.1029/2025EA004633, ID:38108690.
Keywords: cdaweb, omni
Sample usage ( BODY ) =Availability Statement Van Allen Probes magnetometer data is available at https://cdaweb.gsfc.nasa.gov/pub/data/rbsp/ . We obtained P dyn and F10.7 through OMNI data set that is available at . We obtained P dyn and F10.7 through OMNI data set that is available at https://cdaweb.gsfc.nasa.gov/pub/data/omni/ .
Sample usage ( BODY ) =P dyn and F10.7 are obtained from the OMNI data set (Papitashvili King, 2020). We particularly value the global activity estimation, which requires all the input parameters are available glo P dyn and F10.7 are obtained from the OMNI data set (Papitashvili King, 2020). We particularly value the global activity estimation, which requires all the input parameters are available glo We obtained P dyn and F10.7 through OMNI data set that is available at https://cdaweb.gsfc.nasa.gov/pub/data/omni/ . ained P dyn and F10.7 through OMNI data set that is available at https://cdaweb.gsfc.nasa.gov/pub/data/omni/ .
Authors=Tilahun, Atirsaw Muluye; Oljira, Asebe; Nigussie, Melessew; Gautam, Sujan Prasad; Ejigu, Yohannes Getachew;
Title=Equatorial Ionospheric VTEC Perturbations During the 21 June 2020 Solar Eclipse, 2025, doi:10.1029/2025EA004366, ID:38350518.
Keywords: omni
Sample usage ( ACK ) =Acknowledgments We would like to convey our sincere appreciation to UNAVCO and the OMNI Data Center for their free access to GPS, solar, and geomagnetic data.
