2024 mnras (Monthly Notices of the Royal Astronomical Society) agu ads article report on 02/04/2025 13:54:02


cdaweb was referenced in 2 papers
spdf was referenced in 0 papers
space physics data facility was referenced in 3 papers
omni was referenced in 6 papers
omni2 was referenced in 0 papers
omni-2 was referenced in 0 papers
omniweb was referenced in 2 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 1 papers
iri was referenced in 3 papers
international reference ionosphere 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

14 of 3659 possible papers ( 0% ) contained references to SPDF keywords

Authors=Vemareddy, P.; Ibrahim, M. Syed
Title=Eruption of prominence initiated by loss of equilibrium: multipoint observations, 2024, doi:10.1093/mnras/stad3323, ID=25568696
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:cdaweb
Sample usage ( ACK ) =The CME catalogue used in this study is generated and maintained by the Center for Solar Physics and Space Weather, the Catholic University of America, in cooperation with the Naval Research Laboratory and NASA. The data services from CDAWeb are also thankfully acknowledged. We gratefully acknowledge the anonymous referee's detailed comments and suggestions.

Authors=Tripathi, Anshuman; Datta, Abhirup; Choudhury, Madhurima; Majumdar, Suman
Title=Extracting the Global 21-cm signal from Cosmic Dawn and Epoch of Reionization in the presence of Foreground and Ionosphere, 2024, doi:10.1093/mnras/stae07810.48550/arXiv.2401.01935, ID=26810009
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:iri
Sample usage ( BODY ) =We used the International Reference Ionospheric (IRI) model to obtain the TEC value for the D-layer (Bilitza 2003 ).

Authors=Pezzi, O.; Blasi, P.
Title=Galactic cosmic ray transport in the absence of resonant scattering, 2024, doi:10.1093/mnrasl/slad19210.48550/arXiv.2305.02890, ID=26512564
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:omni
Sample usage ( BODY ) =The different role of d B res ( r ) and d B coh ( r ) can be appreciated from Fig. 1 that displays the magnetic field omni-directional energy spectrum E b ( k ) for different values of z.

Authors=Jain, Richa N.; Choudhary, R. K.; Imamura, T.
Title=Exploring the influence of the 'Smiley Sun' on the dynamics of inner solar corona and near-Earth space environment, 2024, doi:10.1093/mnrasl/slae008, ID=26810138
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:omniweb
Sample usage ( BODY ) =Solar wind bulk velocities as recorded by ACE spacecraft (from Omniweb), 5 min average, in the given experiment days. The smiley sun pattern of trio-coronal holes appeared on the solar disc on 26th October 2022 and it correctly fits the observation of the higher flow speeds after two to three days near the 1 au region, following the time expected by the Earth-directed particles accelerated in the inner region to take reaching 1 au.

Authors=Hayakawa, Hisashi; Carrasco, Victor M. S.; Aparicio, Alejandro J. P.; Villalba Alvarez, Joaquin; Vaquero, Jose M.
Title=An Overview of Sunspot Observations in the Early Maunder Minimum: 1645-1659, 2024, doi:10.1093/mnras/stad3922, ID=27108332
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:omni
Sample usage ( BODY ) =He stated as follows: 'We did not see any spots in the solar disc [Original Text: Nullae maculae in disco Solis a nobis conspectae fuerunt ]' on 1652 April 8 (Du Hamel 1660 , p. 11); and 'So, I have nothing more to say here about solar spots; indeed, no sunspots were observed, but the disc of the Sun was seen free from any spots, except for the clouds [Original Text: De maculis porro solaribus nil hic dicendum habeo; nullae enim tum observatae sunt, sed ab omni labe detersus si nubes excipias visus est Solis discus .]' on 1659 November 14 (Du Hamel 1660 , pp. 6-7)'.

Authors=Swayne, M. I.; Maxted, P. F. L.; Triaud, A. H. M. J.; Sousa, S. G.; Deline, A.; Ehrenreich, D.; Hoyer, S.; Olofsson, G.; Boisse, I.; Duck, A.; Gill, S.; Martin, D.; McCormac, J.; Persson, C. M.; Santerne, A.; Sebastian, D.; Standing, M. R.; Acuna, L.; Alibert, Y.; Alonso, R.; Anglada, G.; Barczy, T.; Barrado Navascues, D.; Barros, S. C. C.; Baumjohann, W.; Baycroft, T. A.; Beck, M.; Beck, T.; Benz, W.; Billot, N.; Bonfils, X.; Borsato, L.; Bourrier, V.; Brandeker, A.; Broeg, C.; Carmona, A.; Charnoz, S.; Collier Cameron, A.; Cortes-Zuleta, P.; Csizmadia, Sz; Cubillos, P. E.; Davies, M. B.; Deleuil, M.; Delfosse, X.; Delrez, L.; Demangeon, O. D. S.; Demory, B. -O.; Dransfield, G.; Erikson, A.; Fortier, A.; Forveille, T.; Fossati, L.; Fridlund, M.; Gandolfi, D.; Gillon, M.; Gudel, M.; Gunther, M. N.; Hara, N.; Hebrard, G.; Heidari, N.; Hellier, C.; Helling, Ch; Isaak, K. G.; Kerschbaum, F.; Kiefer, F.; Kiss, L. L.; Kunovac, V.; Lalitha, S.; Lam, K. W. F.; Laskar, J.; Lecavelier des Etangs, A.; Lendl, M.; Magrin, D.; Marafatto, L.; Martioli, E.; Miller, N. J.; Mordasini, C.; Moutou, C.; Nascimbeni, V.; 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.; Scandariato, G.; Segransan, D.; Simon, A. E.; Smith, A. M. S.; Southworth, R.; Stalport, M.; Szabo, Gy M.; Thomas, N.; Udry, S.; Ulmer, B.; Van Grootel, V.; Venturini, J.; Walton, N. A.; Willett, E.; Wilson, T. G.
Title=The EBLM Project- XI. Mass, radius, and effective temperature measurements for 23 M-dwarf companions to solar-type stars observed with CHEOPS, 2024, doi:10.1093/mnras/stad386610.48550/arXiv.2312.11339, ID=27108627
journal=Monthly Notices of the Royal Astronomical Society
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=Aguilar-Rodriguez, E.; Gonzalez-Aviles, J. J.; Riley, P.; Ben-Nun, M.; Rodriguez-Martinez, M.; Gonzalez, R. F.; Perez-Rivera, M. A.; Raga-Rasmussen, A. C.
Title=Numerical MHD models of stream interaction regions (SIRs) and corotating interaction regions (CIRs) using sunRunner3D: comparison with observations, 2024, doi:10.1093/mnras/stae640, ID=27299999
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:space physics data facility
Sample usage ( ACK ) =The authors also acknowledge the STEREO mission team and NASA's Space Physics Data Facility for providing the data needed for this study. EA-R acknowledges support from DGAPA/PAPIIT project IN106224, and CONAHCYT project CF-2023-G-364.

Authors=Dhandha, Jiten; Faes, Zoe; Smith, Rowan J.
Title=Decaying turbulence in molecular clouds: how does it affect filament networks and star formation?, 2024, doi:10.1093/mnras/stae86210.48550/arXiv.2307.12428, ID=27501881
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:omni
Sample usage ( BODY ) =In particular, the discovery of the omni-presence of these filaments in the ISM by Herschel (e.g. Men'shchikov et al. 2010 ) has brought a flurry of excitement and research on connecting the ISM geometry to the complex multiscale physics of star formation, especially that of massive stars (see Hacar et al. 2022 , and references therein).

Authors=Mishra, Wageesh; Sahani, Preity Sukla; Khuntia, Soumyaranjan; Chakrabarty, Dibyendu
Title=Distribution and recovery phase of geomagnetic storms during solar cycles 23 and 24, 2024, doi:10.1093/mnras/stae104510.48550/arXiv.2404.09234, ID=27841384
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:omni
Sample usage ( BODY ) =The availability of continuous observations of the near-Earth solar wind and interplanetary magnetic field as well the Dst index in the last two solar cycles adds an advantage to our study. 2 ANALYSIS OF DISTRIBUTION OF GEOMAGNETIC STORMS We take the 1-h Dst data sets from the OMNI Database at the National Space Science Data Center of NASA (King Papitashvili 2005 ), for which the source is the World Data Center for Geomagnetism, Kyoto, https://wdc.kugi.kyoto-u.ac.jp/wdc/Sec3.html .

Authors=Schaller, Matthieu; Borrow, Josh; Draper, Peter W.; Ivkovic, Mladen; McAlpine, Stuart; Vandenbroucke, Bert; Bahe, Yannick; Chaikin, Evgenii; Chalk, Aidan B. G.; Chan, Tsang Keung; Correa, Camila; van Daalen, Marcel; Elbers, Willem; Gonnet, Pedro; Hausammann, Loic; Helly, John; Husko, Filip; Kegerreis, Jacob A.; Nobels, Folkert S. J.; Ploeckinger, Sylvia; Revaz, Yves; Roper, William J.; Ruiz-Bonilla, Sergio; Sandnes, Thomas D.; Uyttenhove, Yolan; Willis, James S.; Xiang, Zhen
Title=SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications, 2024, doi:10.1093/mnras/stae92210.48550/arXiv.2305.13380, ID=28831949
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:

Authors=Watkins, A. E.; Mihos, J. C.; Harding, P.; Garner, R.
Title=Implications on star formation rate indicators from H II regions and diffuse ionized gas in the M101 Group, 2024, doi:10.1093/mnras/stae115310.48550/arXiv.2404.19003, ID=28151365
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:omni
Sample usage ( BODY ) =This does not mean that all radiation escaping from the H ii regions escapes the galaxy as a whole, of course: likely this escape is not omni-directional, and whether this escaping emission ionizes the galaxy's own ISM or leaves to ionize the IGM depends both on the directionality of the escape from the cloud and the location of the cloud within the galaxy itself (e.g.

Authors=Li, Huichao; Feng, Xueshang
Title=On the northward shift of the heliospheric current sheet at the end of solar cycle 24, 2024, doi:10.1093/mnras/stae169010.48550/arXiv.2407.06510, ID=29247471
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:cdaweb, space physics data facility, omni, omniweb
Sample usage ( BODY ) =The RT A ratios of each orbit and perihelion are calculated for PSP using the hourly averaged IMF data provided by the Coordinated Data Analysis Web (CDAWeb) service. These ratios are presented in Figure 3. The IMF data collected between two successive apogees are used to calculate RT A of each orbit.
Sample usage ( BODY ) =We acknowledge use of NASA/GSFC's Space Physics Data Facility's OMNIWeb and CDAWeb service for providing the observed in-situ data used in this paper.
Sample usage ( BODY ) =We first focus on the near-Earth data provided by the OMNI database. Following Mursula & Hiltula (2003), the polarity of the IMF data is defined by the plane division, where the toward (T) and away (A) polarity are defined by B x > B y and B x < B y respectively in the geocentric solar ecliptic (GSE) coordinate system.
Sample usage ( ABSTRACT ) =In this paper, we analyse the shift of the HCS by using information obtained from coronal model and in situ data provided by the near-Earth OMNI data base and the Parker Solar Probe (PSP). Coronal potential field source surface modelling results show that the northward shift is established at the beginning of 2018 and remains stable for about 2 yr.
Sample usage ( BODY ) =We acknowledge use of NASA/GSFC's Space Physics Data Facility's OMNIWeb and CDAWeb service for providing the observed in-situ data used in this paper.

Authors=Chhiber, Rohit; Pecora, Francesco; Usmanov, Arcadi V.; Matthaeus, William H.; Goldstein, Melvyn L.; Roy, Sohom; Wang, Jiaming; Thepthong, Panisara; Ruffolo, David
Title=The Alfven transition zone observed by the Parker Solar Probe in young solar wind - global properties and model comparisons, 2024, doi:10.1093/mnrasl/slae05110.48550/arXiv.2405.10437, ID=29200274
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:space physics data facility
Sample usage ( ACK ) =We acknowledge the PSP mission for use of the data, which are publicly available at NASA Space Physics Data Facility. PSP ephemeris was extracted from SPICE kernels obtained from PSP Science Gateway.

Authors=Alqasim, A.; Grieves, N.; Rosario, N. M.; Gandolfi, D.; Livingston, J. H.; Sousa, S.; Collins, K. A.; Teske, J. K.; Fridlund, M.; Egger, J. A.; Cabrera, J.; Hellier, C.; Lanza, A. F.; Van Eylen, V.; Bouchy, F.; Oelkers, R. J.; Srdoc, G.; Shectman, S.; Gunther, M.; Goffo, E.; Wilson, T.; Serrano, L. M.; Brandeker, A.; Wang, S. X.; Heitzmann, A.; Bonfanti, A.; Fossati, L.; Alibert, Y.; Delrez, L.; Sefako, R.; Barros, S.; Collins, K. I.; Demangeon, O. D. S.; Albrecht, S. H.; Alonso, R.; Asquier, J.; Barczy, T.; Barrado, D.; Baumjohann, W.; Beck, T.; Benz, W.; Billot, N.; Borsato, L.; Broeg, C.; Bryant, E. M.; Butler, R. P.; Cochran, W. D.; Cameron, A. Collier; Correia, A. C. M.; Crane, J. D.; Csizmadia, Sz; Cubillos, P. E.; Davies, M. B.; Daylan, T.; Deleuil, M.; Deline, A.; Demory, B. -O.; Derekas, A.; Edwards, B.; Ehrenreich, D.; Erikson, A.; Essack, Z.; Fortier, A.; Gazeas, K.; Gillon, M.; Gudel, M.; Hasiba, J.; Hatzes, A. P.; Helling, Ch; Hirano, T.; Howell, S. B.; Hoyer, S.; Isaak, K. G.; Jenkins, J. M.; Kanodia, S.; Kiss, L. L.; Korth, J.; Lam, K. W. F.; Laskar, J.; Etangs, A. Lecavelier des; Lendl, M.; Lund, M. B.; Luque, R.; Mann, A. W.; Magrin, D.; Maxted, P. F. L.; Mordasini, C.; Narita, N.; Nascimbeni, V.; Nowak, G.; Olofsson, G.; Osborn, H. P.; Osborne, H. L. M.; Osip, D.; Ottensamer, R.; Pagano, I.; Palle, E.; Peter, G.; Piotto, G.; Pollacco, D.; Queloz, D.; Ragazzoni, R.; Rando, N.; Rauer, H.; Redfield, S.; Ribas, I.; Rice, M.; Ricker, G. R.; Rieder, M.; Salmon, S.; Santos, N. C.; Scandariato, G.; Seager, S.; Segransan, D.; Shporer, A.; Simon, A. E.; Smith, A. M. S.; Stalport, M.; Szabo, Gy M.; Thompson, I.; Twicken, J. D.; Udry, S.; Vanderspek, R.; Van Grootel, V.; Venturini, J.; Villaver, E.; Villasenor, J.; Viotto, V.; Walter, I.; Walton, N. A.; Winn, J. N.; Yee, S. W.
Title=TOI-757 b: an eccentric transiting mini-Neptune on a 17.5-d orbit, 2024, doi:10.1093/mnras/stae176710.48550/arXiv.2407.20525, ID=30660569
journal=Monthly Notices of the Royal Astronomical Society
Keywords found:iri
Sample usage ( BODY ) =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 PID2019107061GB-C61, PID2019-107061GB-C66, PID2021-125627OBC31, 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 (CEX2020001058-M), and from the Generalitat de Catalunya/CERCA programme. DBa, EPa, and IRi acknowledge financial support from the Agencia Estatal de Investigacion of the Ministerio de CienMNRAS 000, 1-25 (2023) 21 cia e Innovacion MCIN/AEI/10.13039/501100011033 and the ERDF "A way of making Europe" through projects PID2019107061GB-C61, PID2019-107061GB-C66, PID2021-125627OBC31, 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 (CEX2020001058-M), and from the Generalitat de Catalunya/CERCA programme.