2024 aa (Astronomy and Astrophysics) agu ads article report on 02/04/2025 13:54:02


cdaweb was referenced in 10 papers
spdf was referenced in 8 papers
space physics data facility was referenced in 8 papers
omni was referenced in 11 papers
omni2 was referenced in 0 papers
omni-2 was referenced in 0 papers
omniweb was referenced in 6 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
iri was referenced in 11 papers
international reference ionosphere was referenced in 0 papers
tipsod was referenced in 0 papers
hdp was referenced in 2 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
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40 of 3459 possible papers ( 1% ) contained references to SPDF keywords

Authors=Royer, P.; Merle, T.; Dsilva, K.; Sekaran, S.; Van Winckel, H.; Fremat, Y.; Van der Swaelmen, M.; Gebruers, S.; Tkachenko, A.; Laverick, M.; Dirickx, M.; Raskin, G.; Hensberge, H.; Abdul-Masih, M.; Acke, B.; Alonso, M. L.; Bandhu Mahato, S.; Beck, P. G.; Behara, N.; Bloemen, S.; Buysschaert, B.; Cox, N.; Debosscher, J.; De Cat, P.; Degroote, P.; De Nutte, R.; De Smedt, K.; de Vries, B.; Dumortier, L.; Escorza, A.; Exter, K.; Goriely, S.; Gorlova, N.; Hillen, M.; Homan, W.; Jorissen, A.; Kamath, D.; Karjalainen, M.; Karjalainen, R.; Lampens, P.; Lobel, A.; Lombaert, R.; Marcos-Arenal, P.; Menu, J.; Merges, F.; Moravveji, E.; Nemeth, P.; Neyskens, P.; Ostensen, R.; Papics, P. I.; Perez, J.; Prins, S.; Royer, S.; Samadi-Ghadim, A.; Sana, H.; Sans Fuentes, A.; Scaringi, S.; Schmid, V.; Siess, L.; Siopis, C.; Smolders, K.; Sodor, A.; Thoul, A.; Triana, S.; Vandenbussche, B.; Van de Sande, M.; Van De Steene, G.; Van Eck, S.; van Hoof, P. A. M.; Van Marle, A. J.; Van Reeth, T.; Vermeylen, L.; Volpi, D.; Vos, J.; Waelkens, C.
Title=MELCHIORS. The Mercator Library of High Resolution Stellar Spectroscopy, 2024, doi:10.1051/0004-6361/20234684710.48550/arXiv.2311.02705, ID=26672816
journal=Astronomy and Astrophysics
Keywords found:iri
Sample usage ( ACK ) =Acknowledgements This work is based on observations made with the Mercator Telescope, operated on the island of La Palma by the Flemmish Community, at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. Mercator operates thanks to the IRI-FWO project with code I000521N. This work is also based on observations obtained with the HERMES spectrograph, which is supported by the Research Foundation of Flanders (FWO), Belgium, the Research Council of KULeuven, Belgium, the Fonds National de la Recherche Scientifique (FNRS), Belgium, the Royal Observatory of Belgium, the Observatoire de Geneve, Switzerland and the Thuringer Landessternwarte Tautenburg, Germany.

Authors=Ding, Zheyi; Li, Gang; Mason, Glenn; Poedts, Stefaan; Kouloumvakos, Athanasios; Ho, George; Wijsen, Nicolas; Wimmer-Schweingruber, Robert F.; Rodriguez-Pacheco, Javier
Title=Modelling two energetic storm particle events observed by Solar Orbiter using the combined EUHFORIA and iPATH models, 2024, doi:10.1051/0004-6361/20234750610.48550/arXiv.2311.08346, ID=26672977
journal=Astronomy and Astrophysics
Keywords found:cdaweb
Sample usage ( ACK ) =SolO in-situ data are publicly available at NASA's Coordinated Data Analysis Web (CDAWeb) database ( https://cdaweb.gsfc.nasa.gov/index.html/ ). This work is supported in part by NASA grants 80NSSC19K0075, 80NSSC22K0268, 80NSSC21K1327, and NSF ANSWERS 2149771 at UAH-USA.

Authors=Zhuang, B.; Lugaz, N.; Al-Haddad, N.; Scolini, C.; Farrugia, C. J.; Regnault, F.; Davies, E. E.; Yu, W.; Winslow, R. M.; Galvin, A. B.
Title=Combining STEREO heliospheric imagers and Solar Orbiter to investigate the evolution of the 2022 March 10 CME, 2024, doi:10.1051/0004-6361/202347561, ID=26840452
journal=Astronomy and Astrophysics
Keywords found:cdaweb, space physics data facility
Sample usage ( ACK ) =We acknowledge NASA/GSFC's Space Physics Data Facility's CDAWeb service for the Solar Orbiter and Wind data. We thank the use of the data of SOHO LASCO, SDO AIA, and STEREO SECCHI from Virtual Solar Observatory.
Sample usage ( ACK ) =We acknowledge NASA/GSFC's Space Physics Data Facility's CDAWeb service for the Solar Orbiter and Wind data.

Authors=Bonfanti, A.; Brady, M.; Wilson, T. G.; Venturini, J.; Egger, J. A.; Brandeker, A.; Sousa, S. G.; Lendl, M.; Simon, A. E.; Queloz, D.; Olofsson, G.; Adibekyan, V.; Alibert, Y.; Fossati, L.; Hooton, M. J.; Kubyshkina, D.; Luque, R.; Murgas, F.; Mustill, A. J.; Santos, N. C.; Van Grootel, V.; Alonso, R.; Asquier, J.; Bandy, T.; Barczy, T.; Barrado Navascues, D.; Barros, S. C. C.; Baumjohann, W.; Bean, J.; Beck, M.; Beck, T.; Benz, W.; Bergomi, M.; Billot, N.; Borsato, L.; Broeg, C.; Collier Cameron, A.; Csizmadia, Sz.; Cubillos, P. E.; Davies, M. B.; Deleuil, M.; Deline, A.; Delrez, L.; Demangeon, O. D. S.; Demory, B. -O.; Ehrenreich, D.; Erikson, A.; Fortier, A.; Fridlund, M.; Gandolfi, D.; Gillon, M.; Gudel, M.; Gunther, M. N.; Heitzmann, A.; Helling, Ch.; Hoyer, S.; Isaak, K. G.; Kasper, D.; Kiss, L. L.; Lam, K. W. F.; Laskar, J.; Lecavelier des Etangs, A.; Magrin, D.; Maxted, P. F. L.; Mordasini, C.; Nascimbeni, V.; Ottensamer, R.; Pagano, I.; Palle, E.; Peter, G.; Piotto, G.; Pollacco, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Ribas, I.; Scandariato, G.; Segransan, D.; Seifahrt, A.; Smith, A. M. S.; Stalport, M.; Stefansson, G.; Steinberger, M.; Sturmer, J.; Szabo, Gy. M.; Thomas, N.; Udry, S.; Villaver, E.; Walton, N. A.; Westerdorff, K.; Zingales, T.
Title=Characterising TOI-732 b and c: New insights into the M-dwarf radius and density valley, 2024, doi:10.1051/0004-6361/20234818010.48550/arXiv.2311.12577, ID=26840563
journal=Astronomy and Astrophysics
Keywords found:

Authors=Pagano, I.; Scandariato, G.; Singh, V.; Lendl, M.; Queloz, D.; Simon, A. E.; Sousa, S. G.; Brandeker, A.; Cameron, A. Collier; Sulis, S.; Van Grootel, V.; Wilson, T. G.; Alibert, Y.; Alonso, R.; Anglada, G.; Barczy, T.; Navascues, D. Barrado; Barros, S. C. C.; Baumjohann, W.; Beck, M.; Beck, T.; Benz, W.; Billot, N.; Bonfils, X.; Borsato, L.; Broeg, C.; Bruno, G.; Carone, L.; Charnoz, S.; Corral van Damme, C.; Csizmadia, Sz.; Cubillos, P. E.; Davies, M. B.; Deleuil, M.; Deline, A.; Delrez, L.; Demangeon, O. D. S.; Demory, B. -O.; Ehrenreich, D.; Erikson, A.; Fortier, A.; Fossati, L.; Fridlund, M.; Gandolfi, D.; Gillon, M.; Gudel, M.; Gunther, M. N.; Helling, Ch.; Hoyer, S.; Isaak, K. G.; Kiss, L. L.; Kopp, E.; Lam, K. W. F.; Laskar, J.; Lecavelier des Etangs, A.; Magrin, D.; Maxted, P. F. L.; Mordasini, C.; Munari, M.; Nascimbeni, V.; Olofsson, G.; Ottensamer, R.; Palle, E.; Peter, G.; Piotto, G.; Pollacco, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Reimers, C.; Ribas, I.; Rieder, M.; Santos, N. C.; Segransan, D.; Smith, A. M. S.; Stalport, M.; Steller, M.; Szabo, Gy. M.; Thomas, N.; Udry, S.; Venturini, J.; Walton, N. A.
Title=Constraining the reflective properties of WASP-178 b using CHEOPS photometry, 2024, doi:10.1051/0004-6361/20234670510.48550/arXiv.2309.09037, ID=26840619
journal=Astronomy and Astrophysics
Keywords found:

Authors=Singh, V.; Scandariato, G.; Smith, A. M. S.; Cubillos, P. E.; Lendl, M.; Billot, N.; Fortier, A.; Queloz, D.; Sousa, S. G.; Csizmadia, Sz.; Brandeker, A.; Carone, L.; Wilson, T. G.; Akinsanmi, B.; Patel, J. A.; Krenn, A.; Demangeon, O. D. S.; Bruno, G.; Pagano, I.; Hooton, M. J.; Cabrera, J.; Santos, N. C.; Alibert, Y.; Alonso, R.; Asquier, J.; Barczy, T.; Navascues, D. Barrado; Barros, S. C. C.; Baumjohann, W.; Beck, M.; Beck, T.; Benz, W.; Bergomi, M.; Bonfanti, A.; Bonfils, X.; Borsato, L.; Broeg, C.; Charnoz, S.; Cameron, A. Collier; Davies, M. B.; Deleuil, M.; Deline, A.; Delrez, L.; Demory, B. -O.; Ehrenreich, D.; Erikson, A.; Fossati, L.; Fridlund, M.; Gandolfi, D.; Gillon, M.; Gudel, M.; Gunther, M. N.; Harre, J. -V.; Heitzmann, A.; Helling, Ch.; Hoyer, S.; Isaak, K. G.; Kiss, L. L.; Lam, K. W. F.; Laskar, J.; des Etangs, A. Lecavelier; Magrin, D.; Maxted, P. F. L.; Mischler, H.; Mordasini, C.; Nascimbeni, V.; Olofsson, G.; Ottensamer, R.; Palle, E.; Peter, G.; Piotto, G.; Pollacco, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Ribas, I.; Salmon, S.; Segransan, D.; Simon, A. E.; Stalport, M.; Steinberger, M.; Szabo, Gy. M.; Thomas, N.; Udry, S.; Ulmer, B.; Van Grootel, V.; Venturini, J.; Villaver, E.; Walton, N. A.; Zingales, T.
Title=CHEOPS observations of KELT-20 b/MASCARA-2 b: An aligned orbit and signs of variability from a reflective day side, 2024, doi:10.1051/0004-6361/20234753310.48550/arXiv.2311.03264, ID=27118025
journal=Astronomy and Astrophysics
Keywords found:

Authors=Baratashvili, T.; Poedts, S.
Title=The effect of adaptive mesh refinement and grid stretching on the magnetized coronal mass ejection model in Icarus, 2024, doi:10.1051/0004-6361/20234786410.48550/arXiv.2401.02504, ID=27299702
journal=Astronomy and Astrophysics
Keywords found:omni
Sample usage ( BODY ) =The arrival time is closer to the one in the OMNI data for the EUHFORIA simulation, but the strengths of the magnetic field components are slightly better modeled by Icarus AMR level 4 simulation. Overall, the profiles obtained in the Icarus simulations resemble the OMNI observed data slightly more closely, than with the EUHFORIA simulation.

Authors=Rojo, M.; Persson, M.; Sauvaud, J. -A.; Aizawa, S.; Nicolaou, G.; Penou, E.; Barthe, A.; Andre, N.; Mazelle, C.; Fedorov, A.; Yokota, S.; Saito, Y.; Heyner, D.; Richter, I.; Auster, U.; Schmid, D.; Fischer, D.; Horbury, T.; Owen, C. J.; Maksimovic, M.; Khotyaintsev, Y.; Louarn, P.; Murakami, G.
Title=Electron moments derived from the Mercury Electron Analyzer during the cruise phase of BepiColombo, 2024, doi:10.1051/0004-6361/202347843, ID=27299720
journal=Astronomy and Astrophysics
Keywords found:omni
Sample usage ( BODY ) =In order to derive Et-OMNI (hereafter OMNI), the count rates from all channels are simultaneously integrated for each energy bin.

Authors=Keppens, W.; Magyar, N.; Van Doorsselaere, T.
Title=Magnetic power spectrum variability with large-scale total magnetic field fluctuations, 2024, doi:10.1051/0004-6361/202347975, ID=27299736
journal=Astronomy and Astrophysics
Keywords found:cdaweb
Sample usage ( BODY ) =The magnetic field data were downloaded from the NASA Coordinated Data Analysis Web (CDAWeb). These data were measured by the fluxgate magnetometers (MAGs), which are part of the Electromagnetic Fields Investigation (FIELDS) instrument of PSP ( Fox et al. 2016 ).

Authors=Dumbovic, M.; Kramaric, L.; Benko, I.; Heber, B.; Vrsnak, B.
Title=A new method of measuring Forbush decreases, 2024, doi:10.1051/0004-6361/20234696910.48550/arXiv.2401.09000, ID=27316709
journal=Astronomy and Astrophysics
Keywords found:spdf, 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 ) =SOHO/EPHIN is supported by the Ministry of Economics via DLR grant 50OG1702. The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov .
Sample usage ( ACK ) =M.D. acknowledges support by the Croatian Science Foundation under the project IP-2020-02-9893 (ICOHOSS). We acknowledge the OMNIWeb database as the source of data used, as well as the SOHO/EPHIN.
Sample usage ( BODY ) =To analyse the in situ properties, we used one-minute plasma and magnetic field data in the geocentric solar ecliptic (GSE) system provided by the OMNIWeb 2 database ( King Papitashvili 2005 ). We identified ICME signatures using criteria described by (e.g.

Authors=Carcaboso, F.; Dumbovic, M.; Kay, C.; Lario, D.; Jian, L. K.; Wilson, L. B., III; Gomez-Herrero, R.; Temmer, M.; Heinemann, S. G.; Nieves-Chinchilla, T.; Veronig, A. M.
Title=Unveiling the journey of a highly inclined CME. Insights from the March 13, 2012, event with 110deg longitudinal separation, 2024, doi:10.1051/0004-6361/20234708310.48550/arXiv.2401.17501, ID=27534335
journal=Astronomy and Astrophysics
Keywords found:cdaweb, spdf, space physics data facility
Sample usage ( ACK ) =We acknowledge use of NASA/GSFC's Space Physics Data Facility's CDAWeb service. FC acknowledges the financial support by an appointment to the NASA Postdoctoral Program at NASA Goddard Space Flight Center, administered by Oak Ridge Associated Universities through a contract with NASA and the support of the Solar Orbiter mission.
Sample usage ( BODY ) =All the represented data have been acquired from the NASA's Coordinated Data Analysis Web (CDAWeb 4 ), part of the Space Physics Data Facility (SPDF). 3.1. Near-Earth observations Earth's surrounding ambient SW properties were measured by Wind, ACE and the four spacecraft of the Cluster mission.
Sample usage ( BODY ) =All the represented data have been acquired from the NASA's Coordinated Data Analysis Web (CDAWeb 4 ), part of the Space Physics Data Facility (SPDF). 3.1. Near-Earth observations Earth's surrounding ambient SW properties were measured by Wind, ACE and the four spacecraft of the Cluster mission.
Sample usage ( ACK ) =We acknowledge use of NASA/GSFC's Space Physics Data Facility's CDAWeb service. FC acknowledges the financial support by an appointment to the NASA Postdoctoral Program at NASA Goddard Space Flight Center, administered by Oak Ridge Associated Universities through a contract with NASA and the support of the Solar Orbiter mission.
Sample usage ( BODY ) =All the represented data have been acquired from the NASA's Coordinated Data Analysis Web (CDAWeb 4 ), part of the Space Physics Data Facility (SPDF). 3.1. Near-Earth observations Earth's surrounding ambient SW properties were measured by Wind, ACE and the four spacecraft of the Cluster mission.

Authors=Demangeon, O. D. S.; Cubillos, P. E.; Singh, V.; Wilson, T. G.; Carone, L.; Bekkelien, A.; Deline, A.; Ehrenreich, D.; Maxted, P. F. L.; Demory, B. -O.; Zingales, T.; Lendl, M.; Bonfanti, A.; Sousa, S. G.; Brandeker, A.; Alibert, Y.; Alonso, R.; Asquier, J.; Barczy, T.; Navascues, D. Barrado; Barros, S. C. C.; Baumjohann, W.; Beck, M.; Beck, T.; Benz, W.; Billot, N.; Biondi, F.; Borsato, L.; Broeg, Ch.; Buder, M.; Cameron, A. Collier; Csizmadia, Sz.; Davies, M. B.; Deleuil, M.; Delrez, L.; Erikson, A.; Fortier, A.; Fossati, L.; Fridlund, M.; Gandolfi, D.; Gillon, M.; Gudel, M.; Gunther, M. N.; Heitzmann, A.; Helling, Ch.; Hoyer, S.; Isaak, K. G.; Kiss, L. L.; Lam, K. W. F.; Laskar, J.; des Etangs, A. Lecavelier; Magrin, D.; Mecina, M.; Mordasini, Ch.; Nascimbeni, V.; Olofsson, G.; Ottensamer, R.; Pagano, I.; Palle, E.; Peter, G.; Piotto, G.; Pollacco, D.; Queloz, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Ribas, I.; Rieder, M.; Salmon, S.; Santos, N. C.; Scandariato, G.; Segransan, D.; Simon, A. E.; Smith, A. M. S.; Stalport, M.; Szabo, Gy. M.; Thomas, N.; Udry, S.; Van Grootel, V.; Venturini, J.; Villaver, E.; Walton, N. A.
Title=Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b, 2024, doi:10.1051/0004-6361/202348270, ID=27534377
journal=Astronomy and Astrophysics
Keywords found:

Authors=Wieser, M.; Williamson, H.; Wieser, G. Stenberg; Barabash, S.; Zhang, A.; Wang, C.; Wang, W.
Title=Energy spectra of energetic neutral hydrogen backscattered and sputtered from the lunar regolith by the solar wind, 2024, doi:10.1051/0004-6361/202348876, ID=27607294
journal=Astronomy and Astrophysics
Keywords found:cdaweb, space physics data facility, omni, omniweb
Sample usage ( ABSTRACT ) =We acknowledge use of NASA/GSFC's Space Physics Data Facility's OMNIWeb (or CDAWeb) service, and OMNI data.
Sample usage ( ABSTRACT ) =We acknowledge use of NASA/GSFC's Space Physics Data Facility's OMNIWeb (or CDAWeb) service, and OMNI data.
Sample usage ( BODY ) =The alpha to proton number density ratio, a sw , was obtained from the OMNI database ( King Papitashvili 2005 ). A histogram of values for this ratio is shown in Fig. 3 .
Sample usage ( ABSTRACT ) =We acknowledge use of NASA/GSFC's Space Physics Data Facility's OMNIWeb (or CDAWeb) service, and OMNI data.
Sample usage ( ABSTRACT ) =We acknowledge use of NASA/GSFC's Space Physics Data Facility's OMNIWeb (or CDAWeb) service, and OMNI data.

Authors=Colomban, L.; Kretzschmar, M.; Krasnoselkikh, V.; Agapitov, O. V.; Froment, C.; Maksimovic, M.; Berthomier, M.; Khotyaintsev, Yu. V.; Graham, D. B.; Bale, S.
Title=Quantifying the diffusion of suprathermal electrons by whistler waves between 0.2 and 1 AU with Solar Orbiter and Parker Solar Probe, 2024, doi:10.1051/0004-6361/20234748910.48550/arXiv.2402.06016, ID=27607304
journal=Astronomy and Astrophysics
Keywords found:cdaweb
Sample usage ( ACK ) =The data used in this work can be found in the Solar Orbiter archive ( http://soar.esac.esa.int/soar/ ) and NASA CDAWeb ( https://cdaweb.gsfc.nasa.gov/index.html ).

Authors=Akinsanmi, B.; Barros, S. C. C.; Lendl, M.; Carone, L.; Cubillos, P. E.; Bekkelien, A.; Fortier, A.; Floren, H. -G.; Collier Cameron, A.; Boue, G.; Bruno, G.; Demory, B. -O.; Brandeker, A.; Sousa, S. G.; Wilson, T. G.; Deline, A.; Bonfanti, A.; Scandariato, G.; Hooton, M. J.; Correia, A. C. M.; Demangeon, O. D. S.; Smith, A. M. S.; Singh, V.; Alibert, Y.; Alonso, R.; Asquier, J.; Barczy, T.; Barrado Navascues, D.; Baumjohann, W.; Beck, M.; Beck, T.; Benz, W.; Billot, N.; Bonfils, X.; Borsato, L.; Broeg, C.; Buder, M.; Charnoz, S.; Csizmadia, Sz.; Davies, M. B.; Deleuil, M.; Delrez, L.; Ehrenreich, D.; Erikson, A.; Farinato, J.; Fossati, L.; Fridlund, M.; Gandolfi, D.; Gillon, M.; Gudel, M.; Gunther, M. N.; Heitzmann, A.; Helling, Ch.; Hoyer, S.; Isaak, K. G.; Kiss, L. L.; Lam, K. W. F.; Laskar, J.; Lecavelier des Etangs, A.; Magrin, D.; Maxted, P. F. L.; Mecina, M.; Mordasini, C.; Nascimbeni, V.; Olofsson, G.; Ottensamer, R.; Pagano, I.; Palle, E.; Peter, G.; Piazza, D.; Piotto, G.; Pollacco, D.; Queloz, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Ribas, I.; Santos, N. C.; Segransan, D.; Simon, A. E.; Stalport, M.; Szabo, Gy. M.; Thomas, N.; Udry, S.; Van Grootel, V.; Venturini, J.; Villaver, E.; Walton, N. A.
Title=The tidal deformation and atmosphere of WASP-12 b from its phase curve, 2024, doi:10.1051/0004-6361/20234850210.48550/arXiv.2402.10486, ID=28150601
journal=Astronomy and Astrophysics
Keywords found:iri
Sample usage ( ACK ) =YAl acknowledges support from the Swiss National Science Foundation (SNSF) under grant 200020_192038. RAl, DBa, EPa, and IRi acknowledge financial support from the Agencia Estatal de Investigacion of the Ministerio de Ciencia e Innovacion MCIN/AEI/10.13039/501100011033 and the ERDF "A way of making Europe" through projects PID2019-107061GB-C61, PID2019-107061GB-C66, PID2021-125627OB-C31, and PID2021-125627OB-C32, from the Centre of Excellence "Severo Ochoa" award to the Instituto de Astrofisica de Canarias (CEX2019-000920-S), from the Centre of Excellence "Maria de Maeztu" award to the Institut de Ciencies de l'Espai (CEX2020-001058-M), and from the Generalitat de Catalunya/CERCA programme.

Authors=Larrodera, C.; Temmer, M.
Title=Evolution of coronal mass ejections with and without sheaths from the inner to the outer heliosphere: Statistical investigation for 1975 to 2022, 2024, doi:10.1051/0004-6361/20234864110.48550/arXiv.2402.16653, ID=28150617
journal=Astronomy and Astrophysics
Keywords found:omni
Sample usage ( BODY ) =Evolution with solar cycle Regarding the evolution with the solar cycle, Mitsakou Moussas (2014) , from the analysis of 325 ICMEs with sheaths obtained from a dataset of the OMNI near-Earth database and defined by their in situ plasma signatures during SC23 (between 1996 and 2008), obtained the average values of different magnitudes.

Authors=Soni, Shirsh Lata; Maharana, Anwesha; Guerrero, Antonio; Mishra, Wageesh; Poedts, Stefaan; Thampi, Smitha; Akhavan-Tafti, Mojtaba
Title=CMEs evolve in the interplanetary medium to double their predicted geo-effectiveness, 2024, doi:10.1051/0004-6361/202347552, ID=28997623
journal=Astronomy and Astrophysics
Keywords found:omniweb
Sample usage ( BODY ) =These data are obtained from the high-resolution data in OMNIweb (HRO) ( King Papitashvili 2005 ). Red and blue solid lines belong to the Run1 (only CME-3) and Run2 (all CMEs) respectively Fig. 12 , on the first and second plots for the solar-wind data and on the last plot for the predictions obtained from the respective solar-wind data from the simulations.

Authors=Katsavrias, C.; Nicolaou, G.; Di Matteo, S.; Kepko, L.; Viall, N. M.; Aminalragia-Giamini, S.; Livadiotis, G.
Title=Proton polytropic behavior of periodic density structures in the solar wind, 2024, doi:10.1051/0004-6361/202450217, ID=29031190
journal=Astronomy and Astrophysics
Keywords found:cdaweb
Sample usage ( ACK ) =The authors thank the National Space Science Data 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/ ).

Authors=Larosa, A.; Chen, C. H. K.; McIntyre, J. R.; Jagarlamudi, V. K.; Sorriso-Valvo, L.
Title=Evolution of the magnetic field rotation distributions in the inner heliosphere, 2024, doi:10.1051/0004-6361/202450030, ID=29071408
journal=Astronomy and Astrophysics
Keywords found:spdf
Sample usage ( ACK ) =We thank the members of the FIELDS/SWEAP teams and PSP community for helpful discussions. PSP data are available at the SPDF ( https://spdf.gsfc.nasa.gov ).

Authors=Rosario, N. M.; Demangeon, O. D. S.; Barros, S. C. C.; Gandolfi, D.; Egger, J. A.; Serrano, L. M.; Osborn, H. P.; Beck, M.; Benz, W.; Floren, H. -G.; Guterman, P.; Wilson, T. G.; Alibert, Y.; Fossati, L.; Hooton, M. J.; Delrez, L.; Santos, N. C.; Sousa, S. G.; Bonfanti, A.; Salmon, S.; Adibekyan, V.; Nigioni, A.; Venturini, J.; Alonso, R.; Anglada, G.; Asquier, J.; Barczy, T.; Barrado Navascues, D.; Barragan, O.; Baumjohann, W.; Beck, T.; Billot, N.; Biondi, F.; Bonfils, X.; Borsato, L.; Brandeker, A.; Broeg, C.; Cessa, V.; Charnoz, S.; Collier Cameron, A.; Csizmadia, Sz.; Cubillos, P. E.; Davies, M. B.; Deleuil, M.; Deline, A.; Demory, B. -O.; Ehrenreich, D.; Erikson, A.; Esposito, M.; Fortier, A.; Fridlund, M.; Gillon, M.; Gudel, M.; Gunther, M. N.; Helling, Ch.; Hoyer, S.; Isaak, K. G.; Kiss, L. L.; Lam, K. W. F.; Laskar, J.; Lecavelier des Etangs, A.; Lendl, M.; Luntzer, A.; Magrin, D.; Maxted, P. F. L.; Mordasini, C.; Nascimbeni, V.; Olofsson, G.; Osborne, H. L. M.; Ottensamer, R.; Pagano, I.; Palle, E.; Peter, G.; Piotto, G.; Pollacco, D.; Queloz, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Ribas, I.; Scandariato, G.; Segransan, D.; Simon, A. E.; Smith, A. M. S.; Stalport, M.; Szabo, Gy. M.; Thomas, N.; Udry, S.; Van Eylen, V.; Van Grootel, V.; Villaver, E.; Walter, I.; Walton, N. A.
Title=Precise characterisation of HD 15337 with CHEOPS: A laboratory for planet formation and evolution, 2024, doi:10.1051/0004-6361/20234775910.48550/arXiv.2403.16621, ID=29096814
journal=Astronomy and Astrophysics
Keywords found:iri
Sample usage ( ACK ) =V.A. is supported by FCT through national funds by the following grant: 2022.06962.PTDC ( http://doi.org/10.54499/2022.06962.PTDC ). RAl, DBa, EPa, and IRi acknowledge financial support from the Agencia Estatal de Investigacion of the Ministerio de Ciencia e Innovacion MCIN/AEI/10.13039/501100011033 and the ERDF "A way of making Europe" through projects PID2019-107061GB-C61, PID2019-107061GB-C66, PID2021-125627OB-C31, and PID2021-125627OB-C32, from the Centre of Excellence "Severo Ochoa" award to the Instituto de Astrofisica de Canarias (CEX2019-000920-S), from the Centre of Excellence "Maria de Maeztu" award to the Institut de Ciencies de l'Espai (CEX2020-001058-M), and from the Generalitat de Catalunya/CERCA programme.

Authors=Krenn, A. F.; Kubyshkina, D.; Fossati, L.; Egger, J. A.; Bonfanti, A.; Deline, A.; Ehrenreich, D.; Beck, M.; Benz, W.; Cabrera, J.; Wilson, T. G.; Leleu, A.; Sousa, S. G.; Adibekyan, V.; Correia, A. C. M.; Alibert, Y.; Delrez, L.; Lendl, M.; Patel, J. A.; Venturini, J.; Alonso, R.; Anglada, G.; Asquier, J.; Barczy, T.; Barrado Navascues, D.; Barros, S. C. C.; Baumjohann, W.; Beck, T.; Billot, N.; Bonfils, X.; Borsato, L.; Brandeker, A.; Broeg, C.; Charnoz, S.; Collier Cameron, A.; Csizmadia, Sz.; Cubillos, P. E.; Davies, M. B.; Deleuil, M.; Demangeon, O. D. S.; Demory, B. -O.; Erikson, A.; Fortier, A.; Fridlund, M.; Gandolfi, D.; Gillon, M.; Gudel, M.; Gunther, M. N.; Hasiba, J.; Heitzmann, A.; Helling, C.; Hoyer, S.; Isaak, K. G.; Kiss, L. L.; Lam, K. W. F.; Laskar, J.; Lecavelier des Etangs, A.; Lovis, C.; Magrin, D.; Maxted, P. F. L.; Mordasini, C.; Nascimbeni, V.; Olofsson, G.; Ottensamer, R.; Pagano, I.; Palle, E.; Peter, G.; Piotto, G.; Pollacco, D.; Queloz, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Ribas, I.; Rieder, M.; Santos, N. C.; Scandariato, G.; Segransan, D.; Simon, A. E.; Smith, A. M. S.; Stalport, M.; Steller, M.; Szabo, Gy. M.; Thomas, N.; Udry, S.; Ulmer, B.; Van Grootel, V.; Villaver, E.; Viotto, V.; Walton, N. A.; Zingales, T.
Title=Characterisation of the TOI-421 planetary system using CHEOPS, TESS, and archival radial velocity data, 2024, doi:10.1051/0004-6361/20234858410.48550/arXiv.2404.11074, ID=29096821
journal=Astronomy and Astrophysics
Keywords found:iri
Sample usage ( ACK ) =ML acknowledges support of the Swiss National Science Foundation under grant number PCEFP2_194576. RAl, DBa, EPa, and IRi acknowledge financial support from the Agencia Estatal de Investigacion of the Ministerio de Ciencia e Innovacion MCIN/AEI/10.13039/501100011033 and the ERDF "A way of making Europe" through projects PID2019-107061GB-C61, PID2019-107061GB-C66, PID2021-125627OB-C31, and PID2021-125627OB-C32, from the Centre of Excellence "Severo Ochoa" award to the Instituto de Astrofisica de Canarias (CEX2019-000920-S), from the Centre of Excellence "Mar a de Maeztu" award to the Institut de Ciencies de l'Espai (CEX2020-001058-M), and from the Generalitat de Catalunya/CERCA programme.

Authors=Dresing, N.; Yli-Laurila, A.; Valkila, S.; Gieseler, J.; Morosan, D. E.; Farwa, G. U.; Kartavykh, Y.; Palmroos, C.; Jebaraj, I.; Jensen, S.; Kuhl, P.; Heber, B.; Espinosa, F.; Gomez-Herrero, R.; Kilpua, E.; Linho, V. -V.; Oleynik, P.; Hayes, L. A.; Warmuth, A.; Schuller, F.; Collier, H.; Xiao, H.; Asvestari, E.; Trotta, D.; Mitchell, J. G.; Cohen, C. M. S.; Labrador, A. W.; Hill, M. E.; Vainio, R.
Title=The solar cycle 25 multi-spacecraft solar energetic particle event catalog of the SERPENTINE project, 2024, doi:10.1051/0004-6361/20244983110.48550/arXiv.2403.00658, ID=29163002
journal=Astronomy and Astrophysics
Keywords found:spdf, space physics data facility
Sample usage ( ACK ) =The ISOIS data are available to the community at https://spacephysics.princeton.edu/missions-instruments/isois ; data are also available via the NASA Space Physics Data Facility ( https://spdf.gsfc.nasa.gov/ ). BH, PK and SI thank the German Federal Mnistry for Economic Affairs and Energy and the German Space Agency (Deutsches Zentrum fur Luft- und Raum-fahrt, e.V., (DLR)) for their support of Solar Orbiter EPT and HET, STEREO SEPT and SOHO EPHIN under grants number 50OT2002 and 50OC2102.
Sample usage ( ACK ) =The ISOIS data are available to the community at https://spacephysics.princeton.edu/missions-instruments/isois ; data are also available via the NASA Space Physics Data Facility ( https://spdf.gsfc.nasa.gov/ ). BH, PK and SI thank the German Federal Mnistry for Economic Affairs and Energy and the German Space Agency (Deutsches Zentrum fur Luft- und Raum-fahrt, e.V., (DLR)) for their support of Solar Orbiter EPT and HET, STEREO SEPT and SOHO EPHIN under grants number 50OT2002 and 50OC2102.

Authors=Rojo, M.; Andre, N.; Aizawa, S.; Sauvaud, J. -A.; Saito, Y.; Harada, Y.; Fedorov, A.; Penou, E.; Barthe, A.; Persson, M.; Yokota, S.; Mazelle, C.; Hadid, L. Z.; Delcourt, D.; Fontaine, D.; Franz, M.; Katra, B.; Krupp, N.; Murakami, G.
Title=Structure and dynamics of the Hermean magnetosphere revealed by electron observations from the Mercury electron analyzer after the first three Mercury flybys of BepiColombo, 2024, doi:10.1051/0004-6361/202449450, ID=29246984
journal=Astronomy and Astrophysics
Keywords found:omni
Sample usage ( BODY ) =Hence, applying the same procedure to the OMNI count rate (solid green line), we should retrieve the same value of T e . On the other hand, estimates of n e from OMNI data products should be underestimated. We present in Fig. A.2 a and A.2 b a comparison between the densities and temperatures estimated from 3D and OMNI data, respectively.

Authors=Fortier, A.; Simon, A. E.; Broeg, C.; Olofsson, G.; Deline, A.; Wilson, T. G.; Maxted, P. F. L.; Brandeker, A.; Collier Cameron, A.; Beck, M.; Bekkelien, A.; Billot, N.; Bonfanti, A.; Bruno, G.; Cabrera, J.; Delrez, L.; Demory, B. -O.; Futyan, D.; Floren, H. -G.; Gunther, M. N.; Heitzmann, A.; Hoyer, S.; Isaak, K. G.; Sousa, S. G.; Stalport, M.; Turin, A.; Verhoeve, P.; Akinsanmi, B.; Alibert, Y.; Alonso, R.; Banhidi, D.; Barczy, T.; Barrado, D.; Barros, S. C. C.; Baumjohann, W.; Baycroft, T.; Beck, T.; Benz, W.; Biro, B. I.; Bodi, A.; Bonfils, X.; Borsato, L.; Charnoz, S.; Cseh, B.; Csizmadia, Sz.; Csanyi, I.; Cubillos, P. E.; Davies, M. B.; Davis, Y. T.; Deleuil, M.; Demangeon, O. D. S.; Derekas, A.; Dransfield, G.; Ducrot, E.; Ehrenreich, D.; Erikson, A.; Farina, C.; Fossati, L.; Fridlund, M.; Gandolfi, D.; Garai, Z.; Garcia, L.; Gillon, M.; Gomez Maqueo Chew, Y.; Gomez-Munoz, M. A.; Granata, V.; Gudel, M.; Guterman, P.; Hegedus, T.; Helling, Ch.; Jehin, E.; Kalup, Cs.; Kilkenny, D.; Kiss, L. L.; Kriskovics, L.; Lam, K. W. F.; Laskar, J.; Lecavelier des Etangs, A.; Lendl, M.; Lopez Pina, A.; Luntzer, A.; Magrin, D.; Miller, N. J.; Modrego Contreras, D.; Mordasini, C.; Munari, M.; Murray, C. A.; Nascimbeni, V.; Ottacher, H.; Ottensamer, R.; Pagano, I.; Pal, A.; Palle, E.; Pasetti, A.; Pedersen, P. P.; Peter, G.; Petrucci, R.; Piotto, G.; Pizarro-Rubio, A.; Pollacco, D.; Pribulla, T.; Queloz, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Ribas, I.; Sabin, L.; Santos, N. C.; Scandariato, G.; Schanche, N.; Schroffenegger, U.; Scutt, O. J.; Sebastian, D.; Segransan, D.; Seli, B.; Smith, A. M. S.; Southworth, R.; Standing, M. R.; Szabo, Gy. M.; Szakats, R.; Thomas, N.; Timmermans, M.; Triaud, A. H. M. J.; Udry, S.; Van Grootel, V.; Venturini, J.; Villaver, E.; Vinko, J.; Walton, N. A.; Wells, R.; Wolter, D.
Title=CHEOPS in-flight performance. A comprehensive look at the first 3.5 yr of operations, 2024, doi:10.1051/0004-6361/20234857610.48550/arXiv.2406.01716, ID=29247021
journal=Astronomy and Astrophysics
Keywords found:iri
Sample usage ( ACK ) =YAl acknowledges support from the Swiss National Science Foundation (SNSF) under grant 200020_192038. RAl, DBa, EPa, and IRi acknowledge financial support from the Agencia Estatal de Investigacion of the Ministerio de Ciencia e Innovacion MCIN/AEI/10.13039/501100011033 and the ERDF "A way of making Europe" through projects PID2019-107061GB-C61, PID2019-107061GB-C66, PID2021-125627OB-C31, and PID2021-125627OB-C32, from the Centre of Excellence "Severo Ochoa" award to the Instituto de Astrofisica de Canarias (CEX2019-000920-S), from the Centre of Excellence "Maria de Maeztu" award to the Institut de Ciencies de l'Espai (CEX2020-001058-M), and from the Generalitat de Catalunya/CERCA programme.

Authors=Magyar, N.; Verniero, J.; Szabo, A.; Zhang, J.; Van Doorsselaere, T.
Title=Solar wind data analysis aided by synthetic modeling: A better understanding of plasma frame variations from temporal data, 2024, doi:10.1051/0004-6361/20234807110.48550/arXiv.2405.12547, ID=30659077
journal=Astronomy and Astrophysics
Keywords found:cdaweb
Sample usage ( BODY ) =The data are publicly available from CDAWeb 2 . From the FIELDS instrument suite ( Bale et al. 2016 ), we used 3D fluxgate magnetometer data at four vectors/s in RTN coordinates, "mag_rtn_4_per_cycle", and electron density measured through quasi-thermal noise.

Authors=Rodriguez, L.; Shukhobodskaia, D.; Niemela, A.; Maharana, A.; Samara, E.; Verbeke, C.; Magdalenic, J.; Vansintjan, R.; Mierla, M.; Scolini, C.; Sarkar, R.; Kilpua, E.; Asvestari, E.; Herbst, K.; Lapenta, G.; Chaduteau, A. D.; Pomoell, J.; Poedts, S.
Title=Validation of EUHFORIA cone and spheromak coronal mass ejection models, 2024, doi:10.1051/0004-6361/20244953010.48550/arXiv.2405.04637, ID=30848674
journal=Astronomy and Astrophysics
Keywords found:spdf, omni, omniweb
Sample usage ( ACK ) =The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov . SOHO LASCO CME catalog is generated and maintained at the CDAW Data Center by NASA and The Catholic University of America in cooperation with the Naval Research Laboratory.
Sample usage ( ACK ) =The Royal Observatory of Belgium team thanks the Belgian Federal Science Policy Office (BELSPO) for the provision of financial support in the framework of the PRODEX Programme of the European Space Agency (ESA) under contract numbers 4000134088, 4000112292, 4000134474, and 4000136424. The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov .
Sample usage ( BODY ) =The arrival time estimates are compared with the observed arrival times, while the estimates of the ICME properties from the simulations are compared with measured in situ data obtained from the OMNI database. In particular, we focused on comparison of the solar wind bulk speed and magnetic field.
Sample usage ( ACK ) =The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov . SOHO LASCO CME catalog is generated and maintained at the CDAW Data Center by NASA and The Catholic University of America in cooperation with the Naval Research Laboratory.

Authors=Baalmann, L. R.; Hunziker, S.; Peronne, A.; Kirchner, J. W.; Glassmeier, K. -H.; Malaspina, D. M.; Wilson, L. B., III; Strahl, C.; Chadda, S.; Sterken, V. J.
Title=A solar rotation signature in cosmic dust: Frequency analysis of dust particle impacts on the Wind spacecraft, 2024, doi:10.1051/0004-6361/20245006910.48550/arXiv.2410.02351, ID=31167301
journal=Astronomy and Astrophysics
Keywords found:cdaweb
Sample usage ( BODY ) =In its current version, spanning the time period from 1995 until the end of August 2023, the dataset is publicly available on CDAWeb 2 . The dataset contains the millisecond-precise timestamp of each dust impact; the peak signal amplitudes of the x -antenna and of the y -antenna, which are also referred to as Channel 1 and Channel 2, respectively; the morphological type for each channel; and a location flag that denotes whether Wind was positioned within Earth's magnetosphere, the lunar wake, or neither.

Authors=Salmon, S. J. A. J.; Van Grootel, V.; Sulis, S.; Szabo, Gy. M.; Brandeker, A.; Broeg, C.; Ehrenreich, D.; Hoyer, S.; Sousa, S. G.; Kiefer, F.; Gandolfi, D.; Nardiello, D.; Charpinet, S.; Bonfanti, A.; Wilson, T. G.; Alibert, Y.; Alonso, R.; Anglada, G.; Barczy, T.; Barrado Navascues, D.; Barros, S. C. C.; Baumjohann, W.; Beck, M.; Beck, T.; Benz, W.; Billot, N.; Bonfils, X.; Borsato, L.; Cabrera, J.; Cessa, V.; Charnoz, S.; Collier Cameron, A.; Corral van Damme, C.; Csizmadia, Sz.; Cubillos, P. E.; Davies, M. B.; Deleuil, M.; Delrez, L.; Demangeon, O. D. S.; Demory, B. -O.; Erikson, A.; Fortier, A.; Fossati, L.; Fridlund, M.; Gillon, M.; Gudel, M.; Hasiba, J.; Isaak, K. G.; Kiss, L. L.; Laskar, J.; Lecavelier des Etangs, A.; Lendl, M.; Lovis, C.; Magrin, D.; Maxted, P. F. L.; Mordasini, C.; Nascimbeni, V.; Olofsson, G.; Ottensamer, R.; Pagano, I.; Palle, E.; Peter, G.; Piotto, G.; Pollacco, D.; Queloz, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Ribas, I.; Santos, N. C.; Scandariato, G.; Segransan, D.; Simon, A. E.; Smith, A. M. S.; Steller, M.; Thomas, N.; Udry, S.; Venturini, J.; Viotto, V.; Walter, I.; Walton, N. A.
Title=HR 10 as seen by CHEOPS and TESS: Revealing d Scuti pulsations, granulation-like signal and hint for transients, 2024, doi:10.1051/0004-6361/202346180, ID=31233909
journal=Astronomy and Astrophysics
Keywords found:iri
Sample usage ( ACK ) =This work was also partially supported by a grant from the Simons Foundation (PI Queloz, grant number 327127). IRI acknowledges support from the Spanish Ministry of Science and Innovation and the European Regional Development Fund through grant PGC2018-098153-B- C33, as well as the support of the Generalitat de Catalunya/CERCA programme.

Authors=Baratashvili, T.; Brchnelova, M.; Linan, L.; Lani, A.; Poedts, S.
Title=The operationally ready full 3D magnetohydrodynamic model from the Sun to Earth: COCONUT+Icarus, 2024, doi:10.1051/0004-6361/20244938910.48550/arXiv.2407.17903, ID=31281357
journal=Astronomy and Astrophysics
Keywords found:omni
Sample usage ( BODY ) =Therefore, the profiles obtained by COCONUT are compared to tomography data, white light images, and OMNI data at 1 AU to confirm their results. The paper is organised as follows.
Sample usage ( ABSTRACT ) =First, we compared the density data to the available tomography data near the Sun and then the modelled solar wind time series in Icarus was compared to OMNI 1-min data at 1 AU. Results. A range of approximated heating profiles were used in the full MHD coronal model to obtain a realistic solar wind configuration.

Authors=Nascimbeni, V.; Borsato, L.; Leonardi, P.; Sousa, S. G.; Wilson, T. G.; Fortier, A.; Heitzmann, A.; Mantovan, G.; Luque, R.; Zingales, T.; Piotto, G.; Alibert, Y.; Alonso, R.; Barczy, T.; Barrado Navascues, D.; Barros, S. C. C.; Baumjohann, W.; Beck, T.; Benz, W.; Billot, N.; Biondi, F.; Brandeker, A.; Broeg, C.; Busch, M. -D.; Collier Cameron, A.; Correia, A. C. M.; Csizmadia, Sz.; Cubillos, P. E.; Davies, M. B.; Deleuil, M.; Deline, A.; Delrez, L.; Demangeon, O. D. S.; Demory, B. -O.; Derekas, A.; Edwards, B.; Ehrenreich, D.; Erikson, A.; Fossati, L.; Fridlund, M.; Gandolfi, D.; Gazeas, K.; Gillon, M.; Gudel, M.; Gunther, M. N.; Helling, Ch.; Isaak, K. G.; Kerschbaum, F.; Kiss, L. L.; Korth, J.; Lam, K. W. F.; Laskar, J.; Lecavelier des Etangs, A.; Leleu, A.; Lendl, M.; Magrin, D.; Maxted, P. F. L.; Merin, B.; Mordasini, C.; Olofsson, G.; Ottensamer, R.; Pagano, I.; Palle, E.; Peter, G.; Pollacco, D.; Queloz, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Ribas, I.; Santos, N. C.; Scandariato, G.; Segransan, D.; Simon, A. E.; Smith, A. M. S.; Southworth, R.; Stalport, M.; Sulis, S.; Szabo, Gy. M.; Udry, S.; Ulmer, B.; Van Grootel, V.; Venturini, J.; Villaver, E.; Walton, N. A.
Title=The K2-24 planetary system revisited by CHEOPS, 2024, doi:10.1051/0004-6361/20245085210.48550/arXiv.2409.02995, ID=31521393
journal=Astronomy and Astrophysics
Keywords found:iri
Sample usage ( ACK ) =We acknowledge financial support from the Agencia Estatal de Investigacion of the Ministerio de Ciencia e Innovacion MCIN/AEI/10.13039/501100011033 and the ERDF "A way of making Europe" through projects PID2019-107061GB-C61, PID2019-107061GB- C66, PID2021-125627OB-C31, and PID2021-125627OB-C32, from the Centre of Excellence "Severo Ochoa" award to the Instituto de Astrofisica de Canarias (CEX2019-000920-S), from the Centre of Excellence "Maria de Maeztu" award to the Institut de Ciencies de l'Espai (CEX2020-001058-M), and from the Gen- eralitat de Catalunya/CERCA programme. DBa, EPa, and IRi acknowledge financial support from the Agencia Estatal de Investigacion of the Ministe- rio de Ciencia e Innovacion MCIN/AEI/10.13039/501100011033 and the ERDF "A way of making Europe" through projects PID2019-107061GB-C61, PID2019- 107061GB-C66, PID2021-125627OB-C31, and PID2021-125627OB-C32, from the Centre of Excellence "Severo Ochoa" award to the Instituto de Astrofisica de Canarias (CEX2019-000920-S), from the Centre of Excellence "Maria de Maeztu" award to the Institut de Ciencies de l'Espai (CEX2020-001058-M), and from the Generalitat de Catalunya/CERCA programme.

Authors=Belardinelli, Daniele; Benella, Simone; Stumpo, Mirko; Consolini, Giuseppe
Title=Derivation of a generalized Kappa distribution from the scaling properties of solar wind magnetic field fluctuations at kinetic scales, 2024, doi:10.1051/0004-6361/20245071410.48550/arXiv.2409.01775, ID=31521424
journal=Astronomy and Astrophysics
Keywords found:spdf, space physics data facility
Sample usage ( ACK ) =PSP, Wind and SO data used in this study are available at the NASA Space Physics Data Facility (SPDF), https://spdf.gsfc.nasa.gov/index.html . The authors acknowledge the contributions of the FIELDS team to the Parker Solar Probe mission, the Cluster FGM, STAFF P.I.s and teams, and the ESA-Cluster Science Archive for making available the data used in this work.
Sample usage ( ACK ) =PSP, Wind and SO data used in this study are available at the NASA Space Physics Data Facility (SPDF), https://spdf.gsfc.nasa.gov/index.html . The authors acknowledge the contributions of the FIELDS team to the Parker Solar Probe mission, the Cluster FGM, STAFF P.I.s and teams, and the ESA-Cluster Science Archive for making available the data used in this work.

Authors=Valentino, A.; Magdalenic, J.
Title=Modelling non-radially propagating coronal mass ejections and forecasting the time of their arrival at Earth, 2024, doi:10.1051/0004-6361/20244952110.48550/arXiv.2407.17295, ID=31521525
journal=Astronomy and Astrophysics
Keywords found:omni
Sample usage ( BODY ) =The CME arrival at Earth was inspected in a high-resolution in situ time series (1 min) of the ambient plasma characteristics obtained from the OMNI webpage, which compiles the in situ observations from several spacecraft, such as the Advanced Composition Explorer (ACE, Stone et al. 1998 ), WIND ( Harten Clark 1995 ), and the Deep Space Climate Observatory (DSCOVR).

Authors=Madar, A.; Opitz, A.; Erdos, G.; Timar, A.; Biro, N.; Koban, G.; Szabo, A.; Nemeth, Z.
Title=Directional discontinuities in the inner heliosphere from Parker Solar Probe and Solar Orbiter observations, 2024, doi:10.1051/0004-6361/202450684, ID=31521549
journal=Astronomy and Astrophysics
Keywords found:space physics data facility
Sample usage ( ACK ) =Data was obtained through ESA Solar Orbiter Archive, NASA Space Physics Data Facility ( https://nssdc.gsfc.nasa.gov ), and AMDA science analysis system provided by the Centre de Donnees de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Universite Paul Sabatier, Toulouse.

Authors=Wang, Yubao; Guo, Jingnan
Title=Statistical study of the peak and fluence spectra of solar energetic particles observed over four solar cycles, 2024, doi:10.1051/0004-6361/20245004610.48550/arXiv.2410.13186, ID=31607513
journal=Astronomy and Astrophysics
Keywords found:spdf, omniweb
Sample usage ( BODY ) =The solar wind speed data is obtained from GSFC/SPDF OMNIWeb interface 5 . We also obtained corresponding X-ray flare class for each SEP event from NOAA space environment services center 6 for further analysis in Sect. 4.4 .
Sample usage ( BODY ) =The solar wind speed data is obtained from GSFC/SPDF OMNIWeb interface 5 . We also obtained corresponding X-ray flare class for each SEP event from NOAA space environment services center 6 for further analysis in Sect. 4.4 .

Authors=Mohan, Atul; Gopalswamy, Natchimuthuk; Raju, Hemapriya; Akiyama, Sachiko
Title=Novel scaling laws to derive spatially resolved flare and CME parameters from sun-as-a-star observables, 2024, doi:10.1051/0004-6361/20245107210.48550/arXiv.2409.19145, ID=31639262
journal=Astronomy and Astrophysics
Keywords found:spdf, space physics data facility
Sample usage ( ACK ) =AM acknowledges Vratislav Krupar and NASA's Space Physics Data Facility (SPDF) ( https://spdf.gsfc.nasa.gov/ ) for the calibrated radio dynamic spectra.
Sample usage ( ACK ) =AM acknowledges Vratislav Krupar and NASA's Space Physics Data Facility (SPDF) ( https://spdf.gsfc.nasa.gov/ ) for the calibrated radio dynamic spectra.

Authors=Perottoni, Helio D.; Placco, Vinicius M.; Almeida-Fernandes, Felipe; Herpich, Fabio R.; Rossi, Silvia; Beers, Timothy C.; Smiljanic, Rodolfo; Amarante, Joao A. S.; Limberg, Guilherme; Werle, Ariel; Rocha-Pinto, Helio J.; Beraldo e Silva, Leandro; Daflon, Simone; Alvarez-Candal, Alvaro; Oliveira Schwarz, Gustavo B.; Schoenell, William; Ribeiro, Tiago; Kanaan, Antonio
Title=The S-PLUS Ultra-Short Survey: First data release, 2024, doi:10.1051/0004-6361/20234880110.48550/arXiv.2407.05004, ID=31639300
journal=Astronomy and Astrophysics
Keywords found:

Authors=Katsavrias, C.; Nicolaou, G.; Livadiotis, G.
Title=Dependence of the polytropic behaviour of solar wind protons on temperature anisotropy and plasma b near L1, 2024, doi:10.1051/0004-6361/202452168, ID=31664569
journal=Astronomy and Astrophysics
Keywords found:cdaweb
Sample usage ( ACK ) =The authors thank the National Space Science Data 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/ ).

Authors=Susarla, S. C.; Chalumeau, A.; Tiburzi, C.; Keane, E. F.; Verbiest, J. P. W.; Hazboun, J. S.; Krishnakumar, M. A.; Iraci, F.; Shaifullah, G. M.; Golden, A.; Bak Nielsen, A. -S.; Donner, J.; Griessmeier, J. -M.; Keith, M. J.; Oslowski, S.; Porayko, N. K.; Serylak, M.; Anderson, J. M.; Bruggen, M.; Ciardi, B.; Dettmar, R. -J.; Hoeft, M.; Kunsemoller, J.; Schwarz, D.; Vocks, C.
Title=Exploring the time variability of the solar wind using LOFAR pulsar data, 2024, doi:10.1051/0004-6361/20245068010.48550/arXiv.2409.09838, ID=32075366
journal=Astronomy and Astrophysics
Keywords found:omni
Sample usage ( BODY ) =Moreover, pulsars with intermediate-to-high ecliptic latitudes would be sensitive to the n e variability dictated by the solar cycle in this framework, as we expect the LoS to be passing through the fast wind during the periods of solar minima (causing the n e lows that we observe in Fig. 12 ), and during the solar maxima, the LoS possibly passes through a mixture of fast and slow wind (hence denser than the fast wind alone), causing the highs in n e shown in Fig. 12 . 5.3.1. Comparison with the OMNI data We compared the n e time series of a subset of pulsars with the proton density at 1 AU 12 provided by the OMNI database ( Papitashvili et al. 2014 ), as obtained with the in-situ spacecraft solar wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer ( ACE , see McComas et al. 1998 ) and DISCOVR .

Authors=Kreilgaard, Kimi C.; Mason, Charlotte A.; Cullen, Fergus; Begley, Ryan; McLure, Ross J.
Title=Inferring the distribution of the ionising photon escape fraction, 2024, doi:10.1051/0004-6361/20245074710.48550/arXiv.2405.10364, ID=32075417
journal=Astronomy and Astrophysics
Keywords found:hdp
Sample usage ( BODY ) =The posterior provides a lower limit on the escape fraction f esc > 0.38 from the 68 per cent HDP interval, consistent with previously reported values by Vanzella et al. (2010) , Ji et al. (2020) , where this source (Ion1) is extensively discussed (see also Saldana-Lopez et al. 2023 ).

Authors=Chadda, Shivank; Malaspina, David M.; Baalmann, Lennart R.; Sterken, Veerle J.; Hunziker, Silvan; Sternovsky, Zoltan
Title=A solar rotation signature in cosmic dust observed in STEREO spacecraft data, 2024, doi:10.1051/0004-6361/202451950, ID=32181199
journal=Astronomy and Astrophysics
Keywords found:space physics data facility, omni, omniweb
Sample usage ( ACK ) =We acknowledge use of NASA/GSFC's Space Physics Data Facility's OMNIWeb service, and OMNI data.
Sample usage ( ACK ) =We acknowledge use of NASA/GSFC's Space Physics Data Facility's OMNIWeb service, and OMNI data.
Sample usage ( BODY ) =Solar wind data measured near the L1 Sun-Earth Lagrange point from the OMNI database ( Papitashvili King 2020 ) are used to examine periodicities in solar wind properties, with the understanding that periodicities present in the solar wind at 1 AU propagate outward through the entire Solar System. One hour resolution OMNI data are used, then downsampled to 1 value per day by taking a median of the hourly data each day.
Sample usage ( ACK ) =We acknowledge use of NASA/GSFC's Space Physics Data Facility's OMNIWeb service, and OMNI data.