Official websites use .gov
A
.gov website belongs to an official government
organization in the United States.
Secure .gov websites use HTTPS
A
lock (
) or https:// means you’ve safely connected to
the .gov website. Share sensitive information only on official,
secure websites.
Report generated on 04/06/2026 12:31:30
cdaweb was referenced in 5 papers
spdf was referenced in 2 papers
space physics data facility was referenced in 3 papers
omni was referenced in 3 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 1 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 1 papers
heliophysics digital resource library was referenced in 1 papers
heliocloud was referenced in 1 papers
14 of 181 possible papers ( 8% ) contained references to SPDF keywords
Authors=Mampaey, Benjamin; Delouille, Veronique; Vansintjan, Robbe;
Title=The SOLARNET Virtual Observatory: An Effective Way to Search Solar Datasets and Cross-Search with Solar Events, 2025, doi:10.1007/s11207-025-02424-0, ID:32713627.
Keywords: hdrl, heliophysics digital resource library, heliocloud
Sample usage ( BODY ) =The Heliophysics Digital Resource Library (HDRL) is presently working on linking research papers to the datasets they utilize.
Sample usage ( BODY ) =re, we could include a field ‘UAT_description’ in the dataset resources. The Heliophysics Digital Resource Library (HDRL) is presently working on linking research papers to the datasets they
Sample usage ( BODY ) =test the ease of access of the SVO API in a Cloud environment such as the one provided by HelioCloud or ESA Datalabs (Masson et al. 2024 ). By design, the SVO focuses on serving data in FITS
Authors=Yadav, Vipin K.; Vijaya, Y.; Krishnam Prasad, B.; Srikar, P. T.; Mahajan, Monika; Mallikarjun, K. V. L. N.; Zamani, Syeeda N.; Satyanarayana Kumari, B.; Lohar, K. A.; Kandpal, M. M.; Narendra, S.; Rai, Vijay S.; Adoni, Abhijit A.; Veeresha, D. R.; T. S., Smaran; Kalpana, A.; Srivastava, Nandita; Vichare, Geeta;
Title=The Fluxgate Magnetometer (MAG) on Board Aditya-L1 Spacecraft, 2025, doi:10.1007/s11207-025-02440-0, ID:33648688.
Keywords: omniweb
Sample usage ( BODY ) =(Image credit: NASA Omniweb). The magnetic field data from ACE spacecraft is not available since March 13, 2021 onwards as the spacecraft is in its fag end of life.
Authors=Goyal, Shiv Kumar; Tiwari, Neeraj Kumar; Patel, Arpit R.; Shanmugam, M.; Vadawale, Santosh V.; Chakrabarty, Dibyendu; Sebastian, Jacob; Dalal, Bijoy; Sharma, Piyush; Sarkar, Aveek; Sarda, Aaditya; Ladiya, Tinkal; Verma, Abhishek J.; Singh, Nishant; Kumar, Sushil; Painkra, Deepak Kumar; Kumar, Prashant; Shah, Manan S.; Adhyaru, Pranav R.; Adalja, Hiteshkumar L.; Banerjee, Swaroop B.; Subramanian, K. P.; Bapat, Bhas; Dadhania, M. B.; Kumar, Abhishek; Janardhan, P.; Bhardwaj, Anil;
Title=Aditya Solar Wind Particle Experiment on Board Aditya-L1: The Supra-Thermal and Energetic Particle Spectrometer, 2025, doi:10.1007/s11207-025-02441-z, ID:33648693.
Keywords: cdaweb
Sample usage ( ACK ) = fluxes obtained from the ACE-ULEIS and ACE-EPAM-LEMS120 instruments are taken from https://cdaweb.gsfc.nasa.gov/index.html . Last but not least, the authors are also thankful to the Editor
Authors=Kumar, Prashant; Bapat, Bhas; Shah, Manan S.; Adalja, Hiteshkumar L.; Patel, Arpit R.; Adhyaru, Pranav R.; Shanmugam, M.; Chakrabarty, Dibyendu; Banerjee, Swaroop B.; Subramanian, K. P.; Sarkar, Aveek; Ladiya, Tinkal; Sebastian, Jacob; Kumar, Abhishek; Kumar, Sushil; Singh, Nishant; Dadhania, M. B.; Vadawale, Santosh V.; Goyal, Shiv Kumar; Tiwari, Neeraj Kumar; Sarda, Aaditya; Painkra, Deepak Kumar; Sharma, Piyush; Verma, Abhishek J.; Yogesh; Janardhan, P.; Bhardwaj, Anil;
Title=Aditya Solar Wind Particle Experiment (ASPEX) on Board Aditya—L1: The Solar Wind Ion Spectrometer (SWIS), 2025, doi:10.1007/s11207-025-02443-x, ID:33648698.
Keywords: cdaweb
Sample usage ( ACK ) =thors also acknowledge the use of solar wind data from Wind spacecraft provided by the NASA CDAWeb ( https://cdaweb.gsfc.nasa.gov/ ). Last but not the least, the authors are gratefu e of solar wind data from Wind spacecraft provided by the NASA CDAWeb ( https://cdaweb.gsfc.nasa.gov/ ). Last but not the least, the authors are grateful to Prof.
Authors=Rakhmanova, Liudmila; Riazantseva, Maria; Yermolaev, Yuri; Khokhlachev, Alexander; Zastenker, Georgy;
Title=Turbulence Evolution Between 0.5 and 1 AU for the Solar Wind of Various Origins, 2025, doi:10.1007/s11207-025-02458-4, ID:33750055.
Keywords: cdaweb
Sample usage ( BODY ) =All data were obtained via the cdaweb.gsfc.nasa.gov/ web source. The two considered periods of the Wind and SolO alignments were analyzed previously by Volodin et al. ( 2024 ) who compared th
Authors=Siluszyk, M.; Iskra, K.;
Title=New Index Characterizing Magnetic Field Turbulence in Relation to the Galactic Cosmic Ray Intensity Variation in the Period 1968 - 2023, 2025, doi:10.1007/s11207-025-02453-9, ID:33829856.
Keywords: omniweb
Sample usage ( BODY ) =ransform We use data of the and components of the HMF for the period of 1968 - 2023 https://omniweb.gsfc.nasa.gov/form/dx1.html to calculate the PSD and exponent (Lyons 1996 ).
Authors=Tokumaru, Munetoshi; Nozaki, Nishiki; Fujiki, Ken’ichi;
Title=Linear Correlation Between Radial and Normal Component Fluctuations of the Interplanetary Magnetic Field, 2025, doi:10.1007/s11207-025-02475-3, ID:34695101.
Keywords: space physics data facility, omni, omniweb, cohoweb
Sample usage ( ACK ) =Acknowledgments We acknowledge the use of the COHOweb of the NASA/GSFC Space Physics Data Facility. We thank the Solar Influences Data Analysis Center of Royal Observatory of Belgium for pro
Sample usage ( BODY ) =The period covered by OMNI data spans over four and half solar cycles (SCs) from the SC 19/20 minimum to the SC 25 maximum. The distances of OMNI and PVO were virtually constant: 1 AU and 0.7 AU, respectively. For comparison, values of and derived from OMNI observations are indicated by dotted lines in the figure. Figure 17 Correlation plot between and derived from OMNI observations for (a) and (b) in 1986 and (c) and (d) in 1996.
Sample usage ( BODY ) =These data were obtained from the COHOweb ( omniweb.gsfc.nasa.gov/coho ). As shown in Table 1 , the IMF data used for this analysis include those from OMNI (King and Papitashvili 2005 ), Pion
Sample usage ( ACK ) =Acknowledgments We acknowledge the use of the COHOweb of the NASA/GSFC Space Physics Data Facility.
Sample usage ( BODY ) =These data were obtained from the COHOweb ( omniweb.gsfc.nasa.gov/coho ). As shown in Table 1 , the IMF data used for this analysis include those from OMNI (King and Papitashvili 2005 ), Pion
Authors=van der Merwe, F. H.; Engelbrecht, N. E.;
Title=Revisiting the Winding Angle of the Heliospheric Magnetic Field: Investigating the Influence of Turbulence, 2025, doi:10.1007/s11207-025-02490-4, ID:34811631.
Keywords: spdf, space physics data facility, omni, omniweb
Sample usage ( ACK ) =The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov .
Sample usage ( ACK ) =Acknowledgments The authors acknowledge the use of NASA/GSFC Space Physics Data Facility’s OMNIWeb service, and OMNI data.
Sample usage ( ACK ) = authors acknowledge the use of NASA/GSFC Space Physics Data Facility’s OMNIWeb service, and OMNI data. The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://o use of NASA/GSFC Space Physics Data Facility’s OMNIWeb service, and OMNI data. The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov .
Sample usage ( BODY ) =Data Analysis For this analysis the hourly-averaged Low Resolution OMNI (LRO) data set (King and Papitashvili 2005 ) available on the NASA OMNIWeb website 2 is used, spanning approximately 6
Sample usage ( ACK ) =Acknowledgments The authors acknowledge the use of NASA/GSFC Space Physics Data Facility’s OMNIWeb service, and OMNI data. The OMNI data were obtained from the GSFC/SPDF OMNIWeb inte y’s OMNIWeb service, and OMNI data. The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov . data. The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov .
Authors=Posner, Arik; Richardson, Ian G.; Zeitlin, Cary J.;
Title=Mars Ground Level Enhancements in the Context of the Solar Energetic Particle Clock, 2025, doi:10.1007/s11207-025-02482-4, ID:35893827.
Keywords: spdf, space physics data facility
Sample usage ( BODY ) =s total surface dose rate data publicly available from the NASA Space Physics Data Facility (SPDF). The time resolution of the RAD data is variable and changes over time, within a range of ei
Sample usage ( BODY ) =This work analyzes total surface dose rate data publicly available from the NASA Space Physics Data Facility (SPDF). The time resolution of the RAD data is variable and changes over time, wit
Authors=Illarionov, Egor; Tlatov, Andrey; Berezin, Ivan; Skorbezh, Nadezhda;
Title=Correlation of Coronal Hole Area Indices and Solar Wind Speed, 2025, doi:10.1007/s11207-025-02530-z, ID:36603215.
Keywords: omni, omniweb
Sample usage ( BODY ) =Solar Wind Data Daily solar wind speed data measured by ACE are obtained from the OMNI database https://omniweb.gsfc.nasa.gov . In this study we are interested in a correlation of high-speed
Sample usage ( BODY ) =ata Daily solar wind speed data measured by ACE are obtained from the OMNI database https://omniweb.gsfc.nasa.gov . In this study we are interested in a correlation of high-speed solar wind s
Authors=Zhao, Ming-Xian; Le, Gui-Ming;
Title=Direct Observational Evidence of Solar Wind Density Controlling the Evolution of the Ring Current During the 2024 October Major Storm, 2025, doi:10.1007/s11207-025-02539-4, ID:36603216.
Keywords: omniweb
Sample usage ( BODY ) = SYMH index with a 1-min time resolution were obtained from the website provided at https://omniweb.gsfc.nasa.gov/form/omnimin.html . Figure 1 illustrates the evolution of the Dst and SYMH in
Authors=McDougall, Emily; Poduval, Bala; Argall, Matthew;
Title=Observations of Switchback Chains in a Twin-CME Event, 2025, doi:10.1007/s11207-025-02541-w, ID:36901540.
Keywords: cdaweb
Sample usage ( ACK ) =Acknowledgements We would like to acknowledge David McComas at Princeton University, CDAWeb, and the FIELDS, and ISIS teams for providing the publicly available data for this study, as well
Authors=Wuttiya, Cherdchai; Yeeram, Thana;
Title=Study of North-South Asymmetric Corotating Solar Wind Structures and Rigidity Dependences of Galactic Cosmic Ray Unidirectional Latitudinal Gradient in
Keywords: omniweb
Sample usage ( ACK ) =CS tilt-angle data from the Wilcox Solar Observatory and the heliospheric data provided by OMNIWeb. Sunspot data are from the World Data Center SILSO, Royal Observatory of Belgium, Brussels.
Sample usage ( BODY ) =Interplanetary Plasma We use the one-hour averaged interplanetary plasma data from the OMNIWeb database. http://omniweb.gsfc.nasa.gov/ . one-hour averaged interplanetary plasma data from the OMNIWeb database. http://omniweb.gsfc.nasa.gov/ .
Authors=Zhao, Xinhua; Chai, Jiaqi; Feng, Shiwei; Xiang, Nanbin; Deng, Linhua; Liang, Yidan; Feng, Xueshang; Xu, Tingting; Wan, Miao;
Title=The Performance of a Blast Wave Model in Predicting Arrival Times of the Interplanetary Shocks from January 2013 to July 2023, 2025, doi:10.1007/s11207-025-02564-3, ID:37617307.
Keywords: cdaweb
Sample usage ( BODY ) =Here, we re-check the solar wind speed for each event from the CDAW website ( https://cdaweb.gsfc.nasa.gov/ ). Considering that our purpose is to develop a forecasting model, we should adopt
