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Report on 02/04/2025 13:54:02
cdaweb was referenced in 1 papers
spdf was referenced in 3 papers
space physics data facility was referenced in 3 papers
omni was referenced in 15 papers
omni2 was referenced in 1 papers
omni-2 was referenced in 1 papers
omniweb was referenced in 10 papers
iri was referenced in 1 papers
20 of 169 possible papers ( 12% ) contained references to SPDF keywords
Authors=Owens, Mathew J.; Lockwood, Mike; Barnard, Luke A.; Usoskin, Ilya; Hayakawa, Hisashi; Pope, Benjamin J. S.; McCracken, Ken
Title=Reconstructing Sunspot Number by Forward-Modelling Open Solar Flux, 2024, doi:10.1007/s11207-023-02241-3, ID=26598393
journal=Solar Physics
Keywords found:spdf, omni
Sample usage ( ACK ) =Acknowledgments We have benefited from sunspot data provided by Royal Observatory of Belgium SILSO, sunspot latitude and area data collated by Mandal et al. and OMNI data provided by NASA/SPDF. We benefited from useful discussions as part of the International Space Science Institute (ISSI, Bern) team “Magnetic open flux and solar wind structuring in interplanetary space” (2019 - 2021), led by Manuela Temmer.
Sample usage ( BODY ) =The blue line in Figure 1 a shows OSF PS , the OSF estimate from annual OMNI and values, assuming an ideal Parker spiral to compute the equivalent .
Authors=Poluianov, Stepan; Batalla, Oscar; Mishev, Alexander; Koldobskiy, Sergey; Usoskin, Ilya
Title=Two New Sub-GLEs Found in Data of Neutron Monitors at South Pole and Vostok: On 09 June 1968 and 27 February 1969, 2024, doi:10.1007/s11207-023-02245-z, ID=26673643
journal=Solar Physics
Keywords found:omni, omniweb
Sample usage ( BODY ) =To complement the results in the lower energy range, we also used the OMNI database with data on the particle intensity from space-borne instruments to estimate fluence and .
Sample usage ( BODY ) =They are available in the database OMNI (Papitashvili and King, 2020 , https://omniweb.gsfc.nasa.gov), where one can find the integral proton intensities , , and with 1-hour resolution for the studied period from 1967 to 1969, as well as other data not relevant to this work.
Authors=Putri, Annisa Novia Indra; Herdiwijaya, Dhani; Hidayat, Taufiq
Title=On the Correlation of Cosmic-Ray Intensity with Solar Activity and Interplanetary Parameters, 2024, doi:10.1007/s11207-023-02249-9, ID=26673653
journal=Solar Physics
Keywords found:omniweb
Sample usage ( BODY ) =We therefore consider as another parameter the SPE flux data, which we took from the omniweb.gsfc.nasa.gov/ site. These SPEs data have the form of proton fluxes >10 MeV over the period 1967 - 2022, with an average temporal resolution of 27 days.
Authors=Takalo, Jouni
Title=The Instantaneous Response of the Geomagnetic Field, Near-Earth IMF, and Cosmic-Ray Intensity to Solar Flares, 2024, doi:10.1007/s11207-024-02257-310.48550/arXiv.2405.15340, ID=26871971
journal=Solar Physics
Keywords found:omni2, omni-2
Sample usage ( ACK ) =Definitive values of Ap are provided by GeoForschungs Zentrum (GFZ) Potsdam. The OMNI2 data are downloaded from https://spdf.gsfc.nasa.gov/pub/data/omni/low\_res\_omni/ .
Authors=Lockwood, Mike; Owens, Mat
Title=Reconstruction of Carrington Rotation Means of Open Solar Flux over the Past 154 Years, 2024, doi:10.1007/s11207-024-02268-0, ID=27300197
journal=Solar Physics
Keywords found:space physics data facility, omni
Sample usage ( ACK ) =We also thank the data centres that maintain and distribute the data, in particular British Geological Service, Edinburgh, the World Data Centre for Geomagnetism, Edinburgh, and NASA’s Space Physics Data Facility, Goddard Space Flight Center. We also thank the UK Science and Technology Facilities Council (STFC) for grant support.
Sample usage ( BODY ) =Figure 1 is a detailed look at the effects of averaging and then taking the modulus of one-minute or hourly Omni samples of the radial magnetic field in the near-Earth heliosphere, .
Authors=Melkumyan, A. A.; Belov, A. V.; Shlyk, N. S.; Abunina, M. A.; Abunin, A. A.; Oleneva, V. A.; Yanke, V. G.
Title=Forbush Decreases and Associated Geomagnetic Storms: Statistical Comparison in Solar Cycles 23 and 24, 2024, doi:10.1007/s11207-024-02281-3, ID=27502226
journal=Solar Physics
Keywords found:space physics data facility, omni, omniweb
Sample usage ( ACK ) =We are grateful also to the Space Physics Data Facility at NASA Goddard for providing the OMNI data.
Sample usage ( BODY ) =Lists of MCs are taken from published papers and online catalogues (Lynch et al., 2003 , 2005 ; Huttunen et al., 2005 ; Marubashi and Lepping, 2007 ; Yermolaev et al., 2009 ; Gopalswamy et al., 2010b ; Richardson and Cane, 2010 ; Kim et al., 2013 ; https://wind.nasa.gov/mfi/mag\_cloud\_pub1.html , https://wind.nasa.gov/mfi/mag\_cloud\_S1.html , https://cdaw.gsfc.nasa.gov/meetings/2010\_fluxrope/LWS\_CDAW2010\_ICMEtbl.html , http://www.srl.caltech.edu/ACE/ASC/DATA/level3/icmetable2.htm , http://www.iki.rssi.ru/**omni**/catalog/ ). The process of identification of FDs with solar and interplanetary sources is described in Melkumyan et al. ( 2018a , 2022 ).
Sample usage ( BODY ) =The FEID database contains information on variations of cosmic rays (VCR, http://spaceweather.izmiran.ru/dbs/kt/vcr.txt ), SW parameters (King and Papitashvili, 2005 ; http://omniweb.gsfc.nasa.gov/ow.html ), geomagnetic indices ( https://www.gfz-potsdam.de/en/kp-index/ , http://wdc.kugi.kyoto-u.ac.jp/dstdir/index.html ), solar flares ( http://www.swpc.noaa.gov/products/lgoes-x-ray ), and sunspot numbers ( https://www.sidc.be/silso/datafiles ).
Authors=Zhang, Kun; Zuo, Pingbing; Zou, Zhengyang; Feng, Xueshang; Huang, Yanshi; Wang, Shijin; Wei, Fengsi; Yang, Hao
Title=Forecasting Medium-Term F10.7 Using the Deep-Learning Informer Model, 2024, doi:10.1007/s11207-024-02284-0, ID=27607941
journal=Solar Physics
Keywords found:omniweb, iri
Sample usage ( BODY ) =Data Preparation The daily F10.7 indices used in this study are obtained from NASA OmniWeb, ranging from 1 January 1965 to 31 December 2021, which covers Solar Cycles 20 - 24.
Sample usage ( BODY ) =It has a wide range of applications in many middle- and upper-atmosphere and magnetosphere models (Su, Bailey, and Fukao, 1999 ), such as Nrlmsis-00 (Picone et al., 2002 ), JB2008 (Bowman et al., 2008 ), DTM (Bruinsma and Boniface, 2021 ), and IRI (Bilitza, 2018 ). Past research has devoted great effort to forecast F10.7 by using statistical approaches (e.g., Zhao and Han, 2008 ; Wang et al., 2018 ; Warren, Emmert, and Crump, 2017 ).
Authors=Wang, Y. -M.
Title=Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind, 2024, doi:10.1007/s11207-024-02300-3, ID=27828363
journal=Solar Physics
Keywords found:omni
Sample usage ( BODY ) =Relating Solar-Wind Properties to the Coronal Magnetic Field Figure 10 displays scatter plots constructed from near-Earth OMNI data, Advanced Composition Explorer (ACE) Solar Wind Ion Composition Spectrometer measurements, and PFSS-derived coronal-field parameters (see Wang, 2016 ).
Authors=Dumbovic, Mateja; Karbonini, Luci; Calogovic, Jasa; Matkovic, Filip; Martinic, Karmen; Remeshan, Akshay Kumar; Brajsa, Roman; Vrsnak, Bojan
Title=The Catalog of Hvar Observatory Solar Observations, 2024, doi:10.1007/s11207-024-02304-z10.48550/arXiv.2404.18576, ID=28832177
journal=Solar Physics
Keywords found:omniweb
Sample usage ( BODY ) =We use the 1-min plasma and magnetic-field data in the Geocentric solar ecliptic (GSE) system provided by the OMNIWeb database (King and Papitashvili, 2005 ). The shock arrival is observed 4 August 2011 around 22:00 UTC (DOY 216.9), followed by the highly turbulent compressed and heated plasma of the ICME sheath region.
Authors=Owens, Mathew J.; Barnard, Luke A.; Muscheler, Raimund; Herbst, Konstantin; Lockwood, Mike; Usoskin, Ilya; Asvestari, Eleanna
Title=A Geomagnetic Estimate of Heliospheric Modulation Potential over the Last 175 Years, 2024, doi:10.1007/s11207-024-02316-9, ID=29072752
journal=Solar Physics
Keywords found:spdf, omni
Sample usage ( ACK ) =Acknowledgments We have benefited from sunspot data provided by Royal Observatory of Belgium SILSO, OMNI data provided by NASA/SPDF, and WSO data provided by Standford University. We benefited from useful discussions as part of the International Space Science Institute (ISSI, Bern) team ‘Magnetic open flux and solar wind structuring in interplanetary space’ (2019 - 2021), led by Manuela Temmer.
Sample usage ( BODY ) =The red line shows the best estimate from in situ spacecraft observations in near-Earth space using the OMNI dataset (King and Papitashvili, 2005 ). This is computed by taking 20-hour averages of the radial magnetic field component and then computing , where is 1 AU.
Authors=Gil, Agnieszka; Asvestari, Eleanna; Mishev, Alexandar; Larsen, Nicholas; Usoskin, Ilya
Title=New Anisotropic Cosmic-Ray Enhancement (ACRE) Event on 5 November 2023 Due to Complex Heliospheric Conditions, 2024, doi:10.1007/s11207-024-02338-3, ID=30683262
journal=Solar Physics
Keywords found:spdf, omni, omniweb
Sample usage ( ACK ) =The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at omniweb.gsfc.nasa.gov . Data for the OTSO AC computations was obtained from the NASA and ESA co-owned SOHO database sohoftp.nascom.nasa.gov/ ) and, the Kyoto University-hosted World Data Center for Geomagnetism ( wdc.kugi.kyoto-u.ac.jp/ ), to whom we extend our thanks for the use of their publicly accessible databases.
Sample usage ( ACK ) =We acknowledge the Community Coordinated Modeling Center (CCMC) at Goddard Space Flight Center for the use of the StereoCAT tool, ccmc.gsfc.nasa.gov/tools/StereoCat/ . The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at omniweb.gsfc.nasa.gov .
Sample usage ( BODY ) =The red curves indicate the data from OMNI database (King and Papitashvili 2005 ) while the blue curves are based on the EUHFORIA output. Both OMNI and EUHFORIA time series are shifted by 62 min to bring them closer to near-Earth conditions.
Sample usage ( BODY ) =Panel a depicts the 10-min SymH geomagnetic data ( omniweb.gsfc.nasa.gov/ ) for the period of 4 - 6 November (DOY 308 - 310) 2023.
Authors=Liu, Junyan; Shen, Chenglong; Wang, Yang; Xu, Mengjiao; Chi, Yutian; Zhong, Zhihui; Mao, Dongwei; Zhang, Zhiyong; Wang, Can; Liu, Jiajia; Wang, Yuming
Title=Forecasting the Dst Index with Temporal Convolutional Network and Integrated Gradients, 2024, doi:10.1007/s11207-024-02340-9, ID=30683263
journal=Solar Physics
Keywords found:omni
Sample usage ( BODY ) =Dataset and Prediction Model Details The Dst-index data and solar-wind data used in this paper are obtained from NASA’s OMNI database (King and Papitashvili 2005 ). The data that we used contain the hourly Dst-index and solar-wind data from 00 UT on 1 January 1963 to 23 UT on 31 December 2016 since the final index with the final quality check is now available only up to 2016.
Authors=Elmhamdi, A.; Marassi, A.; Romano, P.; Contarino, L.; AlShehri, W.; Monstein, C.
Title=The Multifaceted M1.7 GOES-class Flare Event of 21 April 2023 in AR13283, 2024, doi:10.1007/s11207-024-02355-2, ID=30700048
journal=Solar Physics
Keywords found:space physics data facility, omni, omniweb
Sample usage ( BODY ) =To reveal the potential geomagnetic effects caused by the events under study, use is made of NASA/GSFC’s Space Physics Data Facility’s OMNIWeb service. In particular, four parameters are recovered from the OMNI database, 1 namely, the interplanetary magnetic fields (IMFs: Total and B z southward component), disturbance storm-time (Dst-index), plasma flow speed, and Kp (planetary K) index.
Sample usage ( ACK ) =We acknowledge the use of the different databases and tools appearing in our paper: OMNI database - ASSA CH detection tool and Solar-Demon dimming detection tool.
Sample usage ( BODY ) =In particular, four parameters are recovered from the OMNI database, 1 namely, the interplanetary magnetic fields (IMFs: Total and B z southward component), disturbance storm-time (Dst-index), plasma flow speed, and Kp (planetary K) index.
Authors=Reda, Raffaele; Giovannelli, Luca; Alberti, Tommaso
Title=Cross-Scale Phase Relationship of the Ca II K Index with Solar Wind Parameters: A Space Climate Focus, 2024, doi:10.1007/s11207-024-02346-3, ID=30806161
journal=Solar Physics
Keywords found:omni
Sample usage ( BODY ) =Such data have been downloaded at hourly resolution from the OMNI database 3 (accessed in May 2021) and later binned to obtain monthly averages. OMNI is a large database containing intercalibrated multisource data, both in low and high resolution (King and Papitashvili 2005 ).
Authors=Posner, A.; Richardson, I. G.; Strauss, R. D. -T.
Title=The “SEP Clock”: A Discussion of First Proton Arrival Times in Wide-Spread Solar Energetic Particle Events, 2024, doi:10.1007/s11207-024-02350-7, ID=31169278
journal=Solar Physics
Keywords found:cdaweb
Sample usage ( BODY ) =Data are publicly available from the NASA CDA Web (cdaweb.gsfc.nasa.gov). In one instance, we augmented the SOHO relativistic electron observations with Wind/3D Plasma Analyzer (3DP) data for the identification of relativistic electron arrival at the Earth.
Authors=Narock, Tom; Pal, Sanchita; Arsham, Aryana; Narock, Ayris; Nieves-Chinchilla, Teresa
Title=Classifying Different Types of Solar-Wind Plasma with Uncertainty Estimations Using Machine Learning, 2024, doi:10.1007/s11207-024-02379-810.48550/arXiv.2409.09230, ID=31169288
journal=Solar Physics
Keywords found:omni
Sample usage ( BODY ) =We then randomly sampled from solar minimum (years 2020 through 2022) and solar maximum (years 2012 through 2014) of OMNI one-minute data (King and Papitashvili 2020 ) collected at 1 au to obtain a comparable dataset of non-transient solar-wind plasma types. Each data point of our OMNI sample was classified as CH, SB, or SR following the categorization algorithm explained in Section 2.2 of Xu and Borovsky ( 2015 ). Any OMNI points classified as “ejecta” were discarded. Next, we averaged Wind and OMNI data to 10 minutes to remove small-scale fluctuations.
Authors=Giri, Ashutosh; Adhikari, Binod; Dahal, Subodh; Paula, K. S. S.; Bolzan, M. J. A.
Title=Multi-fractal Analysis of Cosmic Rays over Mid- and High-Latitude Stations During Severe Geomagnetic Storms, 2024, doi:10.1007/s11207-024-02393-w, ID=31522101
journal=Solar Physics
Keywords found:omni, omniweb
Sample usage ( ACK ) =The authors would like to acknowledge the space-weather data archive of the High-Resolution OMNI NASA, www.**omniweb**.gsfc.nasa.gov/ for providing solar parameters and geomagnetic indices and the Neutron Monitor Database www.nmdb.eu/nest/ for providing cosmic-ray data.
Sample usage ( BODY ) =The solar indices were obtained from NASA’s OmniWeb ( www.**omniweb**.gsfc.nasa.gov/ ). Methods The dynamics of the GS and CR counts are studied in this work using time-series analysis for pattern recognition, interruption detection, and forecasting in the frequency and time domains.
Authors=Papailiou, M.; Abunina, M.; Mavromichalaki, H.; Shlyk, N.; Belov, S.; Abunin, A.; Gerontidou, M.; Belov, A.; Yanke, V.
Title=Precursory Signs of Large Forbush Decreases: The Criterion of Anisotropy, 2024, doi:10.1007/s11207-024-02391-y, ID=31665594
journal=Solar Physics
Keywords found:omni, omniweb
Sample usage ( BODY ) =Data on solar-wind speed and interplanetary magnetic field (i.e., interplanetary conditions) and on geomagnetic indices Dst, , and Kp (i.e., geomagnetic activity) were provided by the OMNI database ( http://omniweb.gsfc.nasa.gov ). Data on SSCs ( http://isgi.unistra.fr/data\_download.php ) were also assessed.
Authors=Belov, S. M.; Shlyk, N. S.; Abunina, M. A.; Belov, A. V.; Abunin, A. A.; Oleneva, V. A.; Yanke, V. G.
Title=On the Most Interesting Solar-Wind and Cosmic-Ray Events in February-April 2023, 2024, doi:10.1007/s11207-024-02406-8, ID=32076116
journal=Solar Physics
Keywords found:omni, omniweb
Sample usage ( BODY ) =Hourly values of solar-wind parameters are taken from the OMNI database omniweb.gsfc.nasa.gov . Geomagnetic activity data are available at ftp://ftp.gfz-potsdam.de/pub/home/obs/kp-ap/wdc (Matzka et al. 2021 ) and wdc.kugi.kyoto-u.ac.jp/dstdir/index.html .
Authors=Wang, Jiaming; Matthaeus, William H.; Chhiber, Rohit; Roy, Sohom; Pradata, Rayta A.; Pecora, Francesco; Yang, Yan
Title=1/f Noise in the Heliosphere: A Target for PUNCH Science, 2024, doi:10.1007/s11207-024-02401-z10.48550/arXiv.2409.02255, ID=32524112
journal=Solar Physics
Keywords found:omni
Sample usage ( BODY ) =Figure 6 Compensated spectra of interplanetary magnetic field at 1 au using five intervals of data from ISEE 3 (panels a and b), IMP (panel c), and OMNI (panels d and e). behavior is observed between around and (Matthaeus and Goldstein 1986 , Figure 1).
