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Report generated on 02/04/2025 13:54:02
spdf was referenced in 2 papers
omni was referenced in 8 papers
omniweb was referenced in 8 papers
iri was referenced in 1 papers
9 of 126 possible papers ( 7% ) contained references to SPDF keywords
Authors=Rajana, Siva Sai Kumar; Panda, Sampad Kumar; Jade, Sridevi; Vivek, Chiranjeevi G.; Upadhayaya, A. K.; Bhardwaj, Arti; Jorphail, Sonam; Seemala, Gopi Krishna
Title=Impact of two severe geomagnetic storms on the ionosphere over Indian longitude sector during March-April 2023, 2024, doi:10.1007/s10509-024-04268-9, ID=26597763
journal=Astrophysics and Space Science
Keywords found:omni, omniweb
Sample usage ( ACK ) =Interplanetary and geomagnetic parameters are downloaded from the NASA-OMNI website ( https://omniweb.gsfc.nasa.gov/ ). Swarm TEC data is obtained from the European Space Agency (ESA) VIRES web platform ( https://vires.services/ ).
Authors=Mukesh, R.; Dass, Sarat C.; Vijay, M.; Kiruthiga, S.; Sagayam, Vijanth
Title=Prediction of ionospheric TEC by LSTM and OKSM during M class solar flares occurred during the year 2023, 2024, doi:10.1007/s10509-024-04290-x, ID=27299802
journal=Astrophysics and Space Science
Keywords found:omniweb, iri
Sample usage ( BODY ) =The TEC values for the Hyderabad GPS station located at 17.31degN latitude and 78.55degE longitude, designated as HYDE station in India, are collected from IONOLAB data servers, whereas the associated solar and geomagnetic parameters are collected from OMNIWEB data servers. The TEC data collected from IONOLAB is at a time resolution of 576 data per day i.e., the TEC is measured at every 2.5 minutes for the given location and the time resolution for the input parameters used in the model is hourly averaged.
Sample usage ( BODY ) =The prediction results were compared with BP and IRI models and found that the LSTM performed better. The authors investigated the significance of using multiple NN models to predict TEC values.
Authors=Ugwu, Chukwuebuka J.; Okike, Ogbonnaya; Menteso, Firew M.; Alhassan, Jibrin A.; Obiegbuna, Dominic C.; Chukwude, Augustine E.; Ugwoke, Romanus E.; Iyida, Evaristus U.; Eya, Innocent O.; Enwelum, Ugochukwu C.; Orji, Orji P.
Title=On the variation of small-amplitude Forbush decreases with solar-geomagnetic parameters, 2024, doi:10.1007/s10509-024-04310-w, ID=28584350
journal=Astrophysics and Space Science
Keywords found:omni, omniweb
Sample usage ( BODY ) =The daily interplanetary magnetic field (IMF), average solar wind speed (SWS), geomagnetic storm indices (Kp, Dst and Ap) data were obtained from the OMNI database 2 . Method The R-FD Location code used in the current work was developed by Paper I.
Sample usage ( ABSTRACT ) =The solar-geomagnetic variables were obtained from the OMNI database. A simple coincident R software code was employed in matching the related solar-geomagnetic variables with the weak Forbush events.
Sample usage ( ACK ) =Acknowledgements This paper makes use of the following websites: http://cr0.izmiran.rssi.ru/ and https://omniweb.gsfc.nasa.gov/html/owdata.html in sourcing our data. We appreciate the teams hosting these websites.
Authors=Yeeram, Thana
Title=The effects of solar radiation and geomagnetic disturbance during consecutive 27-day recurrent geomagnetic storms on variations of equatorial ionospheric parameters and spread F, 2024, doi:10.1007/s10509-024-04327-1, ID=29096854
journal=Astrophysics and Space Science
Keywords found:spdf, omni, omniweb
Sample usage ( ACK ) =The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface ( https://omniweb.gsfc.nasa.gov/ ). Geomagnetic indices are provided by the World Data Center for Geomagnetisms, Kyoto ( http://wdc.kugi.kyoto-u.ac.jp ).
Sample usage ( ACK ) =The ionograms were taken from Lowell Digisonde International. The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface ( https://omniweb.gsfc.nasa.gov/ ).
Authors=Kumar, R. Nirmalumar; Inbaseelan, C. Ranjith Dev; Karthikeyan, E.; Nithyasree, M.; Johnson, Jeyakumar H.
Title=Analysis of solar energetic particle (SEP) event on the geomagnetic environment during 24th solar cycle, 2024, doi:10.1007/s10509-024-04320-8, ID=29544206
journal=Astrophysics and Space Science
Keywords found:omni, omniweb
Sample usage ( BODY ) =Data and method of analysis The solar wind (SW) and interplanetary magnetic field (IMF) high-resolution (1 min) data and Dst index data were obtained from the OMNI database ( http://omniweb.gsfc.nasa.gov/ftpbrowser/wind_min_merge.html ).
Sample usage ( ACK ) =Acknowledgements The authors acknowledge Kyoto WDC ( http://wdc.kugi.kyoto-u.ac.jp/ ) for the AE and Kp index data as well as the Wind satellite team for the CME and IMF data ( http://omniweb.gsfc.nasa.gov/ ).
Authors=Ahmed, O.; Badruddin, B.; Derouich, M.
Title=Dynamics and solar wind control of the recovery of strong geomagnetic storms, 2024, doi:10.1007/s10509-024-04325-310.48550/arXiv.2407.02312, ID=29162978
journal=Astrophysics and Space Science
Keywords found:spdf, omni, omniweb
Sample usage ( ACK ) =Acknowledgements This study used data obtained from the GSFC/SPDF OMNIWeb interface, which can be found at https://omniweb.gsfc.nasa.gov .
Sample usage ( BODY ) =Observations and data analysis In this study, we identified 57 GS events Dst () with specified criteria (mentioned below) measured with 1-hour resolution data from 1995 to 2022, spanning three solar cycles. We used the NSSDC OMNI 1 database to retrieve averaged hourly geomagnetic index Dst, IP plasma, and field parameters.
Authors=Menteso, F. M.; Chukwude, A. E.; Okike, O.; Alhassan, J. A.
Title=The implications of the superposed effect of cosmic ray diurnal anisotropy on weak Forbush Events at Apatity and Moscow Neutron Monitors, 2024, doi:10.1007/s10509-024-04358-8, ID=30848739
journal=Astrophysics and Space Science
Keywords found:omni, omniweb
Sample usage ( BODY ) =Daily solar-geophysical parameters namely: solar wind speed (SWS), interplanetary magnetic field (IMF), geomagnetic storm indices (Dst and ap) data are downloaded from the OMNI database 2 . Table 1 Characteristics of APTY and MOSC NMs Event detection method FD magnitude and time of occurrence are the fundamental event properties required when seeking for solar emission agents that trigger CR reduction observed at Earth.
Sample usage ( ACK ) =Acknowledgements We are grateful to the teams that host the websites http://cr0.izmiran.rssi.ru/ and https://omniweb.gsfc.nasa.gov/html/ow data.html from where we sourced the data for this article.
Authors=Deng, Jingyu; Yuan, Guowu; Zhou, Hao; Wu, Hao; Tan, Chengming
Title=Real-time automated detection of multi-category solar radio bursts, 2024, doi:10.1007/s10509-024-04364-w, ID=31234056
journal=Astrophysics and Space Science
Keywords found:omni
Sample usage ( BODY ) =The YOLOv8n network structure comprises four modules: Input, Backbone, Neck, and Head, integrating several state-of-the-art (SOTA) technologies to improve flexibility and accuracy over many previous versions. Firstly, the Omni-Dimensional Dynamic Convolution (ODConv) algorithm is utilized to dynamically adjust the shape and size of the convolution kernel based on the input data features, enhancing the neural network’s feature extraction capability.
Authors=Gautam, Sujan Prasad; Muluye Tilahun, Atirsaw; Silwal, Ashok; Adhikari, Binod; Getachew Ejigu, Yohannes
Title=Ionospheric response to the 08 April 2024 total solar eclipse over United States: a case study, 2024, doi:10.1007/s10509-024-04372-w, ID=31607647
journal=Astrophysics and Space Science
Keywords found:omni, omniweb
Sample usage ( BODY ) =Thus, to determine the possible geomagnetic influence during the eclipse day, we use solar wind parameters and geomagnetic indices data downloaded from the Operating Mission as Nodes on the Internet Web (OMNI) system ( https://omniweb.gsfc.nasa.gov/ ). Fig. 1 Map of the United States.
Sample usage ( ACK ) =Acknowledgements We acknowledge University of NAVSTAR Consortium ( http://unavco.org/data/ ), OmniWeb Data Repository ( https://omniweb.gsfc.nasa.gov/ ), and Time and Date ( https://www.timeanddate.com/eclipse/ ) for providing publicly accessible dataset for this work.
Sample usage ( BODY ) =Thus, to determine the possible geomagnetic influence during the eclipse day, we use solar wind parameters and geomagnetic indices data downloaded from the Operating Mission as Nodes on the Internet Web (OMNI) system ( https://omniweb.gsfc.nasa.gov/ ). Fig. 1 Map of the United States. The red triangles represents the selected GPS stations.
