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Report generated on 04/06/2026 12:31:30
cdaweb was referenced in 11 papers
spdf was referenced in 5 papers
space physics data facility was referenced in 4 papers
omni was referenced in 5 papers
omni2 was referenced in 0 papers
omni-2 was referenced in 0 papers
omniweb was referenced in 3 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
20 of 3932 possible papers ( 1% ) contained references to SPDF keywords
Authors=Shaikh, Zubair I.; Nicolaou, Georgios; Raghav, Anil N.; Ghag, Kalpesh; Dhamane, Omkar;
Title=Revealing super-adiabatic features of interplanetary coronal mass ejections at 1 au, 2025, doi:10.1051/0004-6361/202451372, ID:32557802.
Keywords: cdaweb, space physics data facility
Sample usage ( ACK ) =ard Space Flight Center (GSFC) Space Physics Data Facility’s Coordinated Data Analysis Web (CDAWeb) to provide access to the data utilised in this study.
Sample usage ( ACK ) =We acknowledge the use of NASA’s Goddard Space Flight Center (GSFC) Space Physics Data Facility’s Coordinated Data Analysis Web (CDAWeb) to provide access to the data utilised in this study.
Authors=Linan, L.; Baratashvili, T.; Lani, A.; Schmieder, B.; Brchnelova, M.; Guo, J. H.; Poedts, S.;
Title=Coronal mass ejection propagation in the dynamically coupled space weather tool: COCONUT + EUHFORIA, 2025, doi:10.1051/0004-6361/202451854, ID:32600983.
Keywords: omni
Sample usage ( BODY ) =By comparing profiles at Earth with OMNI 1-min data, Baratashvili et al. (2024) found that the modelled heliosphere in ICARUS was more consistent with the OMNI data using the heatin ili et al. (2024) found that the modelled heliosphere in ICARUS was more consistent with the OMNI data using the heating introduced in Eq. ( 8 ) compared to the heating function in Eq. ( 6 )
Authors=Strugarek, A.; Garcia Munoz, A.; Brun, A. S.; Paul, A.;
Title=Tracing magnetic switchbacks to their source: An assessment of solar coronal jets as switchback precursors, 2025, doi:10.1051/0004-6361/202452140, ID:32710739.
Keywords: spdf, space physics data facility
Sample usage ( ACK ) =The PSP data used in this study are available at the NASA Space Physics Data Facility (SPDF), https://spdf.gsfc.nasa.gov . SDO is a mission for NASA’s LWS program. in this study are available at the NASA Space Physics Data Facility (SPDF), https://spdf.gsfc.nasa.gov . SDO is a mission for NASA’s LWS program.
Sample usage ( ACK ) =The PSP data used in this study are available at the NASA Space Physics Data Facility (SPDF), https://spdf.gsfc.nasa.gov .
Authors=Hyndman, R. A.; Dalla, S.; Laitinen, T.; Hutchinson, A.; Cohen, C. M. S.; Wimmer-Schweingruber, R. F.;
Title=Multi-spacecraft observations of the decay phase of solar energetic particle events, 2025, doi:10.1051/0004-6361/202453012, ID:32863873.
Keywords: cdaweb
Sample usage ( ACK ) =The use of the data made available via the NSSDC CDAWeb is acknowledged.
Sample usage ( BODY ) =V s w was taken from Coordinated Data Analysis Web (CDAWeb) 2 . The V s w value observed closest to the event start time, and within two hours of the start time was used.
Authors=Alterman, B. L.; Rivera, Y. J.; Lepri, S. T.; Raines, J. M.;
Title=The transition from slow to fast wind as observed in composition observations, 2025, doi:10.1051/0004-6361/202451550, ID:32863894.
Keywords: cdaweb
Sample usage ( BODY ) =These observations are provided by CDAWeb at the native ~92 s cadence. There are multiple SWE datasets, each utilizing nonlinear fitting to extract physical parameters, and each optimized fo
Authors=Temmer, M.; Dumbovic, M.; Martinic, K.; Cappello, G. M.; Remeshan, A. K.; Matkovic, F.; Milosic, D.; Koller, F.; Calogovic, J.; Susino, R.; Romoli, M.;
Title=Comparative analysis of two episodes of strongly geoeffective coronal mass ejection events in November and December 2023, 2025, doi:10.1051/0004-6361/202451479, ID:33461788.
Keywords: omni
Sample usage ( BODY ) =Data and methods The in situ measurements are from the OMNI_HRO_1MIN dataset, which was provided by the Coordinated Data Analysis Web 1 . is related to the first drop in Dst to -54 nT at November 4, 2023, around 24:00 UT. Fig. 5. OMNI in situ measurements and geomagnetic indices for each rotation ( x -axis shows time in UT). The shock arrival of CME2.2 is detected in OMNI on December 1, 2023, at 00:22 UT and for CME2.4+5 at 09:38 UT.
Authors=Calogovic, J.; Dumbovic, M.; Martinic, K.; Temmer, M.; Vrsnak, B.;
Title=Constraints to the drag-based reverse modeling, 2025, doi:10.1051/0004-6361/202346874, ID:33461795.
Keywords: omni
Sample usage ( BODY ) =The solar wind speed, w was obtained from in situ plasma measurements provided through the OMNI database ( King Papitashvili 2005 ). w was determined as the mean velocity of the solar wind o
Authors=Katsavrias, C.; Nicolaou, G.; Livadiotis, G.; Vourlidas, A.; Wilson, L. B., III; Sandberg, I.;
Title=The Polytropic Index of Interplanetary Coronal Mass Ejections near L1, 2025, doi:10.1051/0004-6361/202452984, ID:33632463.
Keywords: cdaweb
Sample usage ( ACK ) = Center of the Goddard Space Flight Center for the use permission of Wind data and the NASA CDAWeb team for making these data available at http://cdaweb.gsfc.nasa.gov/istp_public/ . data and the NASA CDAWeb team for making these data available at http://cdaweb.gsfc.nasa.gov/istp_public/ .
Authors=Katsavrias, C.; Di Matteo, S.; Kepko, L.; Viall, N. M.;
Title=The dependence of periodic density structures’ amplitude and length scale on solar wind density within stream interaction regions, 2025, doi:10.1051/0004-6361/202554483, ID:34107137.
Keywords: cdaweb
Sample usage ( ACK ) = Center of the Goddard Space Flight Center for the use permission of Wind data and the NASA CDAWeb team for making these data available ( http://cdaweb.gsfc.nasa.gov/istp_public ). ion of Wind data and the NASA CDAWeb team for making these data available ( http://cdaweb.gsfc.nasa.gov/istp_public ).
Authors=Kandekar, J.; Kumari, A.;
Title=On the limitations of using metric radio bursts as diagnostic tools for interplanetary coronal mass ejections, 2025, doi:10.1051/0004-6361/202553735, ID:34207547.
Keywords: cdaweb, omniweb
Sample usage ( BODY ) =The data was accessed through NASA’s Coordinated Data Analysis Web (CDAWeb 6 ). We utilized the 5 min high-resolution flow speed (km/s) and the magnetic field (nT) data.
Sample usage ( ACK ) =ric Observatory’s (SOHO) Large Angle and Spectrometric Coronagraph (LASCO), and NASA/GSFC’s OMNIweb database.
Sample usage ( BODY ) =We used the OMNI 5 min data from NASA/GSFC’s OMNIweb for the related ICMEs. The data was accessed through NASA’s Coordinated Data Analysis Web (CDAWeb 6 ). For this study we also explored the ICME parameters obtained from OMNIweb 7 (NASA/GSFC). The average strength of the B field vector (G) was obtained to be 9.4 x 10 -5 (G) (mean) with the mean
Authors=Khuntia, Soumyaranjan; Mishra, Wageesh; Agarwal, Anjali;
Title=Evolution of the interacting coronal mass ejections that drove the great geomagnetic storm of 10 May 2024, 2025, doi:10.1051/0004-6361/202452866, ID:34694300.
Keywords: cdaweb
Sample usage ( BODY ) =density and temperature, and the data were obtained from the Coordinated Data Analysis Web (CDAWeb). We selected an optimal subinterval duration of 6 data points (9.2 minutes) to fit the dens
Authors=Yoo, Ji-Hyeon; Lee, Dae-Young; Kim, Kyung-Chan;
Title=Response of energetic neutral atom flux in the heliosheath to fast variations in the solar wind and its dependence on pickup ion distribution models, 2025, doi:10.1051/0004-6361/202451747, ID:34996651.
Keywords: omni
Sample usage ( BODY ) =Initially, the solar wind at 1 AU was obtained from OMNI data 1 , representing the in situ measurements near heliolatitude 0deg. In (b) and (c), the data at 1 AU are available from OMNI data center, while those at 90 AU were obtained by considering differing transit times of solar wind parcels of different CRs using t
Authors=Milosic, D.; Temmer, M.; Heinemann, S. G.; Hofmeister, S.; Asvestari, E.;
Title=Case study on the evolution of corotating interaction regions for the “smiley coronal holes”: 0.3 to 1 AU, 2025, doi:10.1051/0004-6361/202453096, ID:35434915.
Keywords: spdf, space physics data facility
Sample usage ( BODY ) =All data were downloaded from the Space Physics Data Facility (SPDF) repository 1 . After reduction, we used a time cadence of 0.5 h for each instrument.
Sample usage ( BODY ) =All data were downloaded from the Space Physics Data Facility (SPDF) repository 1 . After reduction, we used a time cadence of 0.5 h for each instrument.
Authors=Zamora, Dario Javier; Abaca, Facundo; Zossi, Bruno S.; Elias, Ana G.;
Title=Evidence of nonlinear signatures in the solar wind proton density at the L1 Lagrange point, 2025, doi:10.1051/0004-6361/202555358, ID:36321370.
Keywords: spdf, omni, omniweb
Sample usage ( ACK ) =Ferri for support with the analysis code, and thank GSFC/SPDF and OMNIWeb for providing access to the data.
Sample usage ( BODY ) =The data we utilized in this study were taken from the OMNI directory 1 ( King Papitashvili 2005 ), which contains the hourly mean values of the interplanetary magnetic field and solar wind The data were taken from the OMNI directory. As can be seen, the fluctuations in N p are large during this interval, that is, the amplitudes of the fluctuations are larger than the mean.
Sample usage ( ACK ) =Ferri for support with the analysis code, and thank GSFC/SPDF and OMNIWeb for providing access to the data. This work was financially supported by CONICET (Argentina).
Authors=Katsavrias, C.; Nicolaou, G.; Verscharen, D.; Livadiotis, G.;
Title=Effective polytropic index in stream interaction regions near L1 and the effect of temperature anisotropy and plasma b, 2025, doi:10.1051/0004-6361/202556105, ID:36545049.
Keywords: cdaweb
Sample usage ( ACK ) = Center of the Goddard Space Flight Center for the use permission of Wind data and the NASA CDAWeb team for making these data available at http://cdaweb.gsfc.nasa.gov/istp_public/ . data and the NASA CDAWeb team for making these data available at http://cdaweb.gsfc.nasa.gov/istp_public/ .
Authors=Carella, Francesco; Lapenta, Giovanni; Bemporad, Alessandro; Eriksson, Stefan; Innocenti, Maria Elena; Kohne, Sophia; Magdalenic, Jasmina;
Title=Clustering Wind data at 1 AU to contextualize magnetic reconnection in the solar wind, 2025, doi:10.1051/0004-6361/202554265, ID:36602243.
Keywords: cdaweb
Sample usage ( BODY ) =Data were retrieved from the CDAWeb 1 Wind dataset using the SunPy Python library ( The SunPy Community 2020 ). the data gaps and the low-quality data using the data flags from WI_PM_3DP database on the CDAWeb; respectively, “GAP” to remove the gaps (0 is no gap and 1 is a gap) and “VALID” (1 is good-
Authors=Eyelade, Adetayo V.; Zenteno-Quinteros, Bea; Moya, Pablo S.; Silva, Javier I.; Urra, Benjamin A.; Lazar, Marian; Vinas, Adolfo F.;
Title=Characterizing solar wind electrons with the core-strahlo model: WIND-SWE-VEIS observations, 2025, doi:10.1051/0004-6361/202555368, ID:37335829.
Keywords: cdaweb
Sample usage ( ACK ) =We thank the Wind mission and NASA CDAWeb for the use of the Wind SWE VEIS electron data.
Authors=Pal, Sanchita; Mac Cormack, Cecilia; Kilpua, Emilia K. J.; Yogesh; Jian, Lan K.; Nieves-Chinchilla, Teresa;
Title=Magnetic interaction analysis of multiple interplanetary coronal mass ejections that led to a historic geomagnetic storm in May 2024, 2025, doi:10.1051/0004-6361/202555908, ID:37335979.
Keywords: cdaweb, spdf, space physics data facility
Sample usage ( BODY ) =We obtained science-level in situ data from NASA’s Coordinated Data Analysis Web (CDAWeb) with the highest available resolution. As the Level 2 IMPACT/MAG data had a significant data gap, we
Sample usage ( ACK ) =We acknowledge the data source Goddard Space Flight Center’s Space Physics Data Facility (SPDF) from where we downloaded the in situ solar wind data and use of JHelioviewer .
Sample usage ( ACK ) =We acknowledge the data source Goddard Space Flight Center’s Space Physics Data Facility (SPDF) from where we downloaded the in situ solar wind data and use of JHelioviewer .
Authors=Bruno, Alessandro; Pesce-Rollins, Melissa; Dalla, Silvia; Omodei, Nicola; Richardson, Ian G.; Ryan, James M.;
Title=The 2024 July 16 solar event: a challenge to the coronal mass ejection origin of long-duration gamma-ray flares, 2025, doi:10.1051/0004-6361/202556879, ID:38256357.
Keywords: omniweb
Sample usage ( BODY ) =ifically, by interpolating the solar-wind speed value (330 km/s) between the Wind (based on OmniWeb data 14 ) and STEREO-A measurements, the footpoint longitudinal separation DLon with respec
Authors=Deshpande, Ketaki; Magdalenic, Jasmina; Christopher Jebaraj, Immanuel; Pavai Valliappan, Senthamizh; Niemela, Antonio; Rodriguez, Luciano; Krupar, Vratislav;
Title=Coronal electron density: Insights from radio and in situ observations, and EUHFORIA modeling, 2025, doi:10.1051/0004-6361/202555142, ID:38256793.
Keywords: spdf
Sample usage ( ACK ) =The data are publicly available at https://spdf.gsfc.nasa.gov/ (PSP, STEREO, Wind). We would like to thank JHelioviewer for being able to browse LASCO, SECCHI, AIA and EUVI data ( http://jhel
