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Report generated on 04/06/2026 12:31:30
cdaweb was referenced in 2 papers
spdf was referenced in 1 papers
space physics data facility was referenced in 2 papers
omni was referenced in 7 papers
omni2 was referenced in 0 papers
omni-2 was referenced in 1 papers
omniweb was referenced in 4 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 212 possible papers ( 5% ) contained references to SPDF keywords
Authors=Ahmad, Nizam; Kilowasid, La Ode Muhammad Musafar; Fakhrurroja, Hanif; Neflia; Rachman, Abdul; Husin, Asnawi; Fathoni, Haries;
Title=How geomagnetic storms affect the loss of Starlink satellites in February 2022?, 2025, doi:10.1186/s40623-024-02124-2, ID:32558102.
Keywords: omniweb
Sample usage ( BODY ) = in the present study can be obtained from NASA’s Goddard Space Flight Center ( NASA GSFC ) OMNIweb data documentation at https://omniweb.gsfc.nasa.gov . ’s Goddard Space Flight Center ( NASA GSFC ) OMNIweb data documentation at https://omniweb.gsfc.nasa.gov .
Authors=Miyashita, Yukinaga; Ieda, Akimasa; Machida, Shinobu;
Title=Evolution of the near-Earth magnetotail associated with substorm onsets: revisiting the issues of onset timing and substorm triggering mechanism, 2025, doi:10.1186/s40623-025-02139-3, ID:32713184.
Keywords: omni
Sample usage ( ACK ) =E. Papitashvili for the OMNI solar wind and geomagnetic indices data. We thank M.
Sample usage ( BODY ) = 12 calculated using the T96 magnetic field model (Tsyganenko 1995 ) with the time series of OMNI data as the input parameters In Fig. 6 a, fast earthward flows possibly generated in the dis
Authors=Martinez-Calderon, Claudia; Shiokawa, Kazuo; Santolik, Ondrej; Kurita, Satoshi; Keika, Kunihiro; Connors, Martin; Schofield, Ian; Hanzelka, Miroslav; Kurth, William S.;
Title=Simultaneous ground-satellite observations of ELF/VLF emissions generated by a strong magnetospheric compression, 2025, doi:10.1186/s40623-025-02170-4, ID:33929155.
Keywords: omni
Sample usage ( BODY ) =Solar wind parameters and geomagnetic response indices were obtained from the OMNI Web database. Satellite-based observations were made by the Van Allen Probe B, also known as the Radiation
Authors=Kataoka, Ryuho; Nakano, Shinya; Uchino, Shiori; Reddy, Sachin A.;
Title=Extended red aurora associated with super substorm igniting the October 10, 2024 magnetic storm as revealed by citizen science, 2025, doi:10.1186/s40623-025-02178-w, ID:34169353.
Keywords: omni, omni-2
Sample usage ( BODY ) =igh solar wind density of 30/cc, and a high solar wind speed of ~ 700 km/s (Fig. 1 ). Fig. 1 OMNI-2 solar wind data (magnetic field, speed, and density), Dst index, and Kp index.
Sample usage ( BODY ) =gh solar wind density of 30/cc, and a high solar wind speed of ~ 700 km/s (Fig. 1 ). Fig. 1 OMNI-2 solar wind data (magnetic field, speed, and density), Dst index, and Kp index.
Authors=Iyemori, T.; Yokoyama, Y.; Aoyama, T.;
Title=A short period and compressional Pc3 magnetic pulsation possibly caused by a lamb wave and plasmaspheric cavity resonance, 2025, doi:10.1186/s40623-025-02205-w, ID:34694624.
Keywords: omni
Sample usage ( ACK ) =The solar wind data were provided by the NASA/OMNI data service. The ionospheric electron density of the IRI2020 model was calculated by the NASA/CCMC Instant Run service.
Sample usage ( BODY ) =The 1-min resolution solar wind data were downloaded from NASA/OMNI database to see the solar wind parameters, such as speed, plasma density, Alfven Mach number etc.
Authors=Buschmann, L. M.; Asamura, K.; Clausen, L. B. N.; Jin, Y.; Kojima, H.; Kumamoto, A.; Kurita, S.; Ogawa, Y.; Oksavik, K.; Saito, Y.; Spicher, A.; Yokota, S.; Miloch, W. J.;
Title=Plasma structuring within an expanded polar cap and cusp studied with the SS-520-3 sounding rocket, 2025, doi:10.1186/s40623-025-02189-7, ID:34694625.
Keywords: space physics data facility, omni, omniweb
Sample usage ( ACK ) =Acknowledgements The authors acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service, and OMNI data.
Sample usage ( ACK ) =he authors acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service, and OMNI data. EISCAT is an international association supported by research organizations in China (C
Sample usage ( BODY ) =el c) for the time between November 2nd throughout November 5th obtained from the 1-min NASA OMNI dataset through OMNIweb (Papitashvili et al. 2020 ). physical quantities for the time frame of 6:00 UT - 12:00 UT on November 4th. Note that the OMNI dataset is shifted to the bow shock. During the time of launch, a geomagnetic storm occurred
Sample usage ( ACK ) =Acknowledgements The authors acknowledge use of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service, and OMNI data. EISCAT is an international association supported by research organiza
Sample usage ( BODY ) =ween November 2nd throughout November 5th obtained from the 1-min NASA OMNI dataset through OMNIweb (Papitashvili et al. 2020 ). The launch time is indicated by a vertical turquoise line.
Authors=Shreedevi, P. R.; Nair, Achuthan S.; Miyoshi, Yoshizumi; Buchert, Stephan C.; Otsuka, Yuichi; Shinbori, Atsuki; Krishnan, Lalitha G.; Perwitasari, Septi; Nishioka, Michi;
Title=Superstorm-driven electron temperature (
Keywords: cdaweb, spdf, space physics data facility, omniweb
Sample usage ( ACK ) =The authors also thank the NASA/GSFC CDAWeb team for providing the interplanetary and geomagnetic activity data.
Sample usage ( BODY ) =agnetic parameters used in this study are sourced from the NASA Space Physics Data Facility (SPDF) OMNIWeb data center ( https://omniweb.gsfc.nasa.gov/ ).
Sample usage ( BODY ) =olar wind and geomagnetic parameters used in this study are sourced from the NASA Space Physics Data Facility (SPDF) OMNIWeb data center ( https://omniweb.gsfc.nasa.gov/ ).
Sample usage ( BODY ) = parameters used in this study are sourced from the NASA Space Physics Data Facility (SPDF) OMNIWeb data center ( https://omniweb.gsfc.nasa.gov/ ). from the NASA Space Physics Data Facility (SPDF) OMNIWeb data center ( https://omniweb.gsfc.nasa.gov/ ).
Authors=Shah, Trunali; Bhaskara, Veenadhari; Omura, Yoshiharu; Ojha, Biswajit; Singh, Satyavir; Bhanu, Remya; Ebihara, Yusuke;
Title=Magnetic field fluctuations coinciding with substorm events, 2025, doi:10.1186/s40623-025-02320-8, ID:38334558.
Keywords: omni
Sample usage ( BODY ) =instrument also provides plasma pressure data for ions, which is utilized in this study. The OMNI database is used to obtain the solar wind parameters and geomagnetic indices. Fig. 2 Geomagnetic indices and solar wind parameters observed on May 05, 2018, from the OMNI data set; a represent component of Interplanetary Magnetic Field (IMF in nT) in GSM coordinates,
Authors=Cha, Heechan; Goldstein, Jerry; Kataria, Dhirendra; Nishimura, Yukitoshi; Ogasawara, Keiichi;
Title=The spatiotemporal development of the midlatitude troughs and subauroral ion drift during a geomagnetic storm observed by multiple DMSP satellites, 2025, doi:10.1186/s40623-025-02349-9, ID:38475118.
Keywords: cdaweb
Sample usage ( BODY ) =We obtained DMSP data from CDAWeb (https://cdaweb.gsfc.nasa.gov) and Madrigal (http://cedar.openmadrigal.org) hosted by CEDAR. CDAWeb provides the data with Level 2 product We obtained DMSP data from CDAWeb (https://cdaweb.gsfc.nasa.gov) and Madrigal (http://cedar.openmadrigal.org) hosted by CEDAR. CDAWeb provides the data with Level 2 product ://cdaweb.gsfc.nasa.gov) and Madrigal (http://cedar.openmadrigal.org) hosted by CEDAR. CDAWeb provides the data with Level 2 product of the RPA data (ion temperature, ram velocity, and SSJ data were retrieved from Madrigal for F16 through F18, as some data were unavailable on CDAWeb. The IDM sensor measures both vertical (V) and horizontal (V) ion drift components with a bi
Authors=Watari, Shinichi; Ebihara, Yusuke; Nakamizo, Aoi;
Title=Statistical analysis of geomagnetically induced current data measured around Tokyo, Japan, 2025, doi:10.1186/s40623-025-02340-4, ID:38475129.
Keywords: omni, omniweb
Sample usage ( ACK ) =minute geomagnetic field data, K-index, and the lists of geomagnetic events, the NASA/GSFC’s OMNI data for solar wind parameters, the WDC for Geomagnetism, Kyoto for Dst index, the WDC-SILSO
Sample usage ( BODY ) =s associated with GMDs and GICs, we used the one-minute solar wind data from the NASA/GSFC’s OMNI data ( https://omniweb.gsfc.nasa.gov/ow_min.html ).
Sample usage ( BODY ) =s and GICs, we used the one-minute solar wind data from the NASA/GSFC’s OMNI data ( https://omniweb.gsfc.nasa.gov/ow_min.html ). Result and discussion GIC events and geomagnetic disturbances
