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2025 Astrophysics and Space Science) Article

Report generated on 04/06/2026 12:31:30

cdaweb was referenced in 4 papers
spdf was referenced in 2 papers
space physics data facility was referenced in 4 papers
omni was referenced in 4 papers
omni2 was referenced in 0 papers
omni-2 was referenced in 0 papers
omniweb was referenced in 9 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

10 of 140 possible papers ( 7% ) contained references to SPDF keywords

Authors=Dugassa, Teshome; Habyarimana, Valence;
Title=Ionospheric disturbances in the African low-latitude region during the space weather event of September 2017, 2025, doi:10.1007/s10509-025-04407-w, ID:33014755.
Keywords: cdaweb, space physics data facility, omni, omniweb
Sample usage ( BODY ) =d by satellites missions in the upstream region, provided by OMNI database and available on CDAWeb ( https://cdaweb.gsfc.nasa.gov/index.html/ ). tream region, provided by OMNI database and available on CDAWeb ( https://cdaweb.gsfc.nasa.gov/index.html/ ).
Sample usage ( ACK ) =ng the TEC data at the IGS website ( ftp://cddis.gsfc.nasa.gov ), the NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service for providing OMNI data ( https://omniweb.gsfc.nasa.gov/form/dx
Sample usage ( ACK ) =gsfc.nasa.gov ), the NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service for providing OMNI data ( https://omniweb.gsfc.nasa.gov/form/dx1.html ), Instituto Geofisico del Peru, for supp
Sample usage ( BODY ) = wind (SW) parameters as measured by satellites missions in the upstream region, provided by OMNI database and available on CDAWeb ( https://cdaweb.gsfc.nasa.gov/index.html/ ).
Sample usage ( ACK ) =he IGS website ( ftp://cddis.gsfc.nasa.gov ), the NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service for providing OMNI data ( https://omniweb.gsfc.nasa.gov/form/dx1.html ), I ‘s Space Physics Data Facility’s OMNIWeb service for providing OMNI data ( https://omniweb.gsfc.nasa.gov/form/dx1.html ), Instituto Geofisico del Peru, for supporting its operation a

Authors=Data, Efrem Amanuel; Terefe, Dejene Ambisa; Gebino, Gebre Kalute;
Title=Performance evaluation of AfriTEC model during quiet and disturbed time over East African sector, 2025, doi:10.1007/s10509-025-04437-4, ID:34169208.
Keywords: space physics data facility, omniweb Sample usage ( ACK ) =te of Geomagnetism, India, for providing the GPS TEC analysis software. The NASA-Space Physics Data Facility, Goddard Space Flight Center ( https://omniweb.gsfc.nasa.gov/form/dx1.html ) is a
Sample usage ( ACK ) =The NASA-Space Physics Data Facility, Goddard Space Flight Center ( https://omniweb.gsfc.nasa.gov/form/dx1.html ) is acknowledged for the provision of the Kp and Dst index.

Authors=Data, Efrem Amanuel; Sulungu, Emmanuel Daudi; Okoh, Daniel Izuikedinachi; Terefe, Dejene Ambisa;
Title=Investigating the reliability of the AfriTEC model during the descending phase of Solar Cycle 24 across East Africa, 2025, doi:10.1007/s10509-025-04462-3, ID:35434217.
Keywords: space physics data facility, omniweb
Sample usage ( ACK ) =ional GNSS Service (IGS) team for data at ( https://arplsrv.ictp.it/ ). The NASA-Space Physics Data Facility, Goddard Space Flight Center ( https://omniweb.gsfc.nasa.gov/form/dx1.html ) is a
Sample usage ( ACK ) =The NASA-Space Physics Data Facility, Goddard Space Flight Center ( https://omniweb.gsfc.nasa.gov/form/dx1.html ) is acknowledged for the provision of the F10.7 and Dst index.
Sample usage ( BODY ) =), planetary Kp index, and the disturbance storm time (Dst) index, were sourced from NASA’s OMNIWeb service ( https://omniweb.gsfc.nasa.gov/form/dx1.html ). urbance storm time (Dst) index, were sourced from NASA’s OMNIWeb service ( https://omniweb.gsfc.nasa.gov/form/dx1.html ).

Authors=Ahmed, O.; Badruddin, B.; Derouich, M.;
Title=Forbush decreases during strong geomagnetic storms: time delays, rigidity effects, and ICME-driven modulation, 2025, doi:10.1007/s10509-025-04477-w, ID:36348446.
Keywords: spdf, omniweb
Sample usage ( ACK ) =Acknowledgements We used solar wind data from the GSFC/SPDF OMNIWeb interface, available at https://omniweb.gsfc.nasa.gov .
Sample usage ( ACK ) =Acknowledgements We used solar wind data from the GSFC/SPDF OMNIWeb interface, available at https://omniweb.gsfc.nasa.gov . We used solar wind data from the GSFC/SPDF OMNIWeb interface, available at https://omniweb.gsfc.nasa.gov .
Sample usage ( BODY ) = database, 4 while IP solar wind parameters and geomagnetic indices were retrieved from the OMNIWeb online tool. 5 These data were provided in the geocentric solar magnetospheric (GSM) coordi

Authors=Xu, Zifan; Ma, Guanyi; Wan, Qingtao; Li, Jinghua; Fan, Jiangtao; Dong, Chiyu;
Title=Regional ionospheric TEC modeling with BP neural network: a multi-station case study across East China, 2025, doi:10.1007/s10509-025-04481-0, ID:36602338.
Keywords: omniweb Sample usage ( ACK ) =The solar index and geomagnetic index were obtained from the OMNIWeb interface at https://omniweb.gsfc.nasa.gov ar index and geomagnetic index were obtained from the OMNIWeb interface at https://omniweb.gsfc.nasa.gov
Sample usage ( BODY ) =All these index data were downloaded from NASA’s OMNIWeb database ( https://omniweb.gsfc.nasa.gov ). All these index data were downloaded from NASA’s OMNIWeb database ( https://omniweb.gsfc.nasa.gov ).

Authors=Iswariya, S.; Panda, Sampad Kumar; Haralambous, Haris; Moses, Mefe; Paul, Krishnendu Sekhar; Okoh, Daniel;
Title=Geo-effectiveness of ICMES/MCs of different magnetic-polarity configurations, 2025, doi:10.1007/s10509-025-04487-8, ID:36900960.
Keywords: omni, omniweb
Sample usage ( ACK ) =Acknowledgements This research benefited significantly from OMNI/NASA’s data resources. We extend our appreciation to the valuable catalog contributions of Nieves-Chinchilla et al. ( 2019 )
Sample usage ( BODY ) =terval In this study, we analyzed 17 parameters using 1-hour averaged data obtained from the OMNI database ( https://omniweb.gsfc.nasa.gov/form/omni_min.html ). averaged data obtained from the OMNI database ( https://omniweb.gsfc.nasa.gov/form/omni_min.html ).
Sample usage ( ABSTRACT ) = employed correlation analysis and superposed epoch analysis on 17 parameters extracted from OMNI/NASA hourly datasets. The investigation focused on identifying how specific magnetic configu
Sample usage ( BODY ) =analyzed 17 parameters using 1-hour averaged data obtained from the OMNI database ( https://omniweb.gsfc.nasa.gov/form/omni_min.html ). These included parameters such as solar wind speed (V),

Authors=Shah, Asif;
Title=Non-Gaussian distributions in solar wind plasma: data analysis and source, 2025, doi:10.1007/s10509-025-04493-w, ID:36900961.
Keywords: cdaweb
Sample usage ( ACK ) =Acknowledgements The author is thankful to NASA CDAWEB and to J.H. King, N. Papitashvili for solar wind data.

Authors=Okike, O.; Nwuzor, O. C.; Rowland, P. I.; Ogunjobi, O.; Mtumela, Z.; Habarulema, J. B.; Menteso, F. M.; Ugwoke, R. E.; Ugwu, C. J.; Eya, I. O.; Alhassan, J. A.; Chukwude, A. E.; Iyida, E. U.; Nwofe, P. A.; Iburu, U.; Anekwe, F. N.; Onah, C. I.;
Title=Accurate cataloging of Forbush decreases: implications for space weather research, 2025, doi:10.1007/s10509-025-04507-7, ID:37336169.
Keywords: cdaweb, omniweb
Sample usage ( BODY ) =commonly available websites (e.g., https://omniweb.gsfc.nasa.gov/form/dx1.html , https://cdaweb.gsfc.nasa.gov/ ) and used with minimal or no data cleaning, the situation is different for FD d
Sample usage ( BODY ) =MF, D st , and ap index), can be downloaded from commonly available websites (e.g., https://omniweb.gsfc.nasa.gov/form/dx1.html , https://cdaweb.gsfc.nasa.gov/ ) and used with minimal or no d

Authors=Yeeram, Thana;
Title=Contribution of Alfven, Chorus, and ULF waves to high-energy electron flux at geostationary orbit in HILDCAA events during 2015 to 2017, 2025, doi:10.1007/s10509-025-04516-6, ID:38114904.
Keywords: cdaweb, spdf, omni, omniweb
Sample usage ( BODY ) =ck nose) and geomagnetic indices as obtained from OMNI database of NASA available at NASA’s CDAWeb ( http://cdaweb.gsfc.nasa.gov/ ). The data include the solar wind speed (), dynami ces as obtained from OMNI database of NASA available at NASA’s CDAWeb ( http://cdaweb.gsfc.nasa.gov/ ). The data include the solar wind speed (), dynamic pressure () and IMF in Geoc
Sample usage ( ACK ) =Acknowledgements The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface ( https://omniweb.gsfc.nasa.gov/ ).
Sample usage ( ACK ) =Acknowledgements The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface ( https://omniweb.gsfc.nasa.gov/ ).
Sample usage ( BODY ) =te-averaged (shifted to the Earth’s bow shock nose) and geomagnetic indices as obtained from OMNI database of NASA available at NASA’s CDAWeb ( http://cdaweb.gsfc.nasa.gov/ ).
Sample usage ( ACK ) =Acknowledgements The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface ( https://omniweb.gsfc.nasa.gov/ ). nts The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface ( https://omniweb.gsfc.nasa.gov/ ).
Sample usage ( BODY ) =ncluding remarks We have utilized the solar wind plasma and geomagnetic storm indices from OMNIweb, REF (E > 0.8 MeV and > 2 MeV) from GOES, trapped source and seed electron flux from POES,

Authors=Shakya, P. J.; Adhikari, B.; Calabia, A.; Panthi, A.;
Title=Magnetospheric Pc5 pulsation generated by interplanetary shocks during the geomagnetic storms, 2025, doi:10.1007/s10509-025-04521-9, ID:38256866.
Keywords: space physics data facility, omni, omniweb
Sample usage ( ACK ) =hors also want to thank OMNIWeb Data Explorer ( https://omniweb.gsfc.nasa.gov/ ), Space Physics Data Facility from NASA for providing the data of solar wind parameters.
Sample usage ( BODY ) =In (c-e) vertical dashed line indicates the interplanetary shock Figure 7 shows OMNI 1 min resolution IMF B and Bz in Geocentric Solar Ecliptic (GSE) coordinates, solar wind speed (Vsw) and e) vertical dashed lines indicate the first and second interplanetary shocks Figure 12 shows OMNI data of the solar wind and IMF parameters for the period from 00:00 UT 7 September to 24:00
Sample usage ( ACK ) =The authors also want to thank OMNIWeb Data Explorer ( https://omniweb.gsfc.nasa.gov/ ), Space Physics Data Facility from NASA for providing the data of solar wind parameters. The authors also want to thank OMNIWeb Data Explorer ( https://omniweb.gsfc.nasa.gov/ ), Space Physics Data Facility from NASA for providing the data of solar wind parameters.
Sample usage ( BODY ) =parameters and geomagnetic indices in geocentric solar ecliptic coordinates (GSE) from NASA OMNIweb ( http://omniweb.gsfc.nasa.gov ). We employ the interplanetary magnetic field (IMF indices in geocentric solar ecliptic coordinates (GSE) from NASA OMNIweb ( http://omniweb.gsfc.nasa.gov ). We employ the interplanetary magnetic field (IMF), the Bz component of the , we used data from SuperMAG, Kyoto’s World Data Center for Geomagnetism (WDC) database and OMNIWeb data, and we investigated ultra-low frequency (ULF) wave behavior during major geomagnetic