Correction to “Localized gravity/topography admittance and correlation spectra on Mars: Implications for regional and global evolution”

By P. McGovern, Sean C. Solomon, David E. Smith, Maria T. Zuber, Mark Simons, Mark A. Wieczorek, Roger J. Phillips, G. Neumann, Oded Aharonson, James W. Head III. 2004

190 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/ab8a2d1fa90a07462dbae2256feeb4e6c4ffa08e

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Mark A. Wieczorek
2. Maria T. Zuber
3. F. Nimmo
4. G. Neumann
5. F. LeMoine
6. Philippe Lognonné
7. V. Belléguic
8. P. McGovern

In Geophysics

1. Mark A. Wieczorek
2. Maria T. Zuber
3. F. Nimmo
4. H. Dalton
5. Donald M. White
6. P. McGovern
7. Philippe Lognonné
8. A. Treiman

In Molecular Biology

1. William M. Folkner
2. Philippe Lognonné
3. Mark A. Wieczorek
4. F. Nimmo

Citations in the corpus

• Experimental petrology of the basaltic shergottite Yamato‐980459: Implications for the thermal structure of the Martian mantle (2006, result): “This produced a heat flux out of the mantle that is consistent with the mantle heat flux estimated by McGovern et al. (2002, 2004) on the basis of gravity modeling of the large volcanoes in Tharsis and Elysium.”
• Mars high resolution gravity fields from MRO, Mars seasonal gravity, and other dynamical parameters (2011, background): “These admittance spectral amplitude and shape are very similar to those found by McGovern et al. (2002, 2004) and especially Belleguic et al. (2005), but now extend to degree and order of 87 (the local degree strength value, 122 km) from less than 60 previously.”
• Constraints on the Martian lithosphere from gravity and topography data and implication for volcanism and possible mantle heterogeneities (2005, background): “Our elastic thickness estimates are found to be consistent with the revised values of McGovern et al. [2004] within their respective uncertainties (see Table 3). Nevertheless, we note that our best fit values are generally larger than those of McGovern et al. [2004] and our uncertainties are consi”
• EARLY CRUSTAL EVOLUTION OF MARS 1 (2005, background): “McGovern et al. (2004) investigated three areas of the southern highlands and found surface densities in the range of 2500 to 3000 kg m−3 and variable degrees of subsurface loading.”
• Crustal structure of Mars from gravity and topography (2004, background): “Elysium Mons and the Tharsis volcanos are assigned a value of 3300 kg m (cid:1) 3 [ McGovern et al. , 2004], in the manner given in Table 2.”