Solar wind spatial scales in and comparisons of hourly Wind and ACE plasma and magnetic field data

By J. King, N. Papitashvili. 2005

1,284 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/ae0c85794f43af41e5962909d9c57d2afe5bd65a

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In Astronomy and Astrophysics

1. J. Borovsky
2. M. Denton
3. H. Cane
4. B. Lavraud
5. R. Forsyth
6. I. G. Richardson
7. M. Owens
8. V. Angelopoulos

In Molecular Biology

1. I. G. Richardson
2. H. Cane
3. V. Angelopoulos
4. J. Borovsky
5. M. Denton
6. M. Owens
7. B. Lavraud
8. S. Cranmer

Citations in the corpus

• Origins of the Ambient Solar Wind: Implications for Space Weather (2017, methodology): “For example, the half-century long OMNI database of plasma and field measurements at 1 AU has been shown to be useful for long-baseline studies of all kinds (e.g., O’Brien and McPherron 2000; King and Papitashvili 2005; Lee et al. 2009).”
• Altered solar wind-magnetosphere interaction at low Mach numbers: Coronal mass ejections (2008, methodology): “…work of Ridley et al. [2004]. ha l-0 03 77 24 0, v er si on 1 - 21 A pr 2 00 9 In section 3.1 we use the hourly-averaged OMNI-2 solar wind dataset [King and Papitashvili, 2005], together with lists of intervals of coronal mass ejections [Cane and Richardson, 2003], magnetic clouds [e.g.,…”
• Differences between CME‐driven storms and CIR‐driven storms (2006, methodology): “In Figure 10 the temperature-speed plot of the solar wind using the OMNI2 data set [King and Papitashvili, 2005] is shown (black points) and the data points wherein expression (2) is satisfied are plotted in red.”
• The Geomagnetic Kp Index and Derived Indices of Geomagnetic Activity (2021, methodology): “We used the OMNI 1-min solar wind data estimated for the Earth's bow shock nose (King & Papitashvili, 2005) for the years 1981–2019.”
• Statistics of whistler mode waves in the outer radiation belt: Cluster STAFF‐SA measurements (2013, methodology): “…from Cluster FGM measurements [Balogh et al., 2001]; geomagnetic activity indices and interplanetary magnetic field data were used as extracted from NASA/Goddard Space Flight Center’s OMNI (Operating Missions as a Node on the Internet) data set through OMNIWeb [King and Papitashvili, 2005].”
• The Heliospheric Magnetic Field (2013, methodology): “The OMNI dataset (e.g., King and Papitashvili, 2005, see also NSSDC: http: //omniweb.gsfc.nasa.gov/) collates the near-Earth solar wind measurements from numerous spacecraft, mostly recently IMP8, Wind and ACE.”
• Near-earth solar wind flows and related geomagnetic activity during more than four solar cycles (1963-2011) (2012, methodology): “These include 1-hour averages of near-Earth solar wind parameters obtained from the OMNI2 (formally OMNI) database (http:// omniweb.gsfc.nasa.gov/; King & Papitashvili 2005).”
• Multipoint observations of magnetospheric compression‐related EMIC Pc1 waves by THEMIS and CARISMA (2008, background): “The top panel of Figure 2 shows the OMNI [see King and Papitashvili, 2005 ] solar wind dynamic pressure time-shifted to the subsolar magnetopause, as well as the magnetic field magnitude observed by the geosynchronous GOES 12 satellite (10.24 magnetic latitude, 356.90 magnetic longitude).”
• Anti-sunward high-speed jets in the subsolar magnetosheath (2013, result): “Otherwise, typical reconnection outflow jet speeds on the order of the Alfvén velocity (less, if only taking into account the velocity component in GSE x direction) would be expected ( Priest and Forbes , 2000). In any case, the selection criteria would only allow for reconnection within the magneto”
• NEUTRAL INTERSTELLAR HELIUM PARAMETERS BASED ON IBEX-Lo OBSERVATIONS AND TEST PARTICLE CALCULATIONS (2012, background): “…typical abundance of solar wind alphas relative to protons, np(t)) is the local proton density taken from the OMNI-2 compilation of solar wind observations (King & Papitashvili 2005), and σHe,p, σHe,α are the charge exchange cross sections for the reaction given by Equation (2) and a sum of…”
• Catalog of large-scale solar wind phenomena during 1976–2000 (2009, methodology): “gsfc.nasa.gov/spacecraft_data/omni/old_hourly/ow_data. html [ 54 ].”