Variations in the geomagnetic dipole moment during the Holocene and the past 50 kyr

By M. Knudsen, P. Riisager, F. Donadini, I. Snowball, R. Muscheler, K. Korhonen, L. Pesonen. 2008

133 citations recorded by the source corpus.

Subfields: Atmospheric Science, Geophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/3071e6cb9d0662f2fc2f06491ad839360110c9f4

How researchers see this paper

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

In Atmospheric Science

1. I. Usoskin
2. Catherine Constable
3. Monika Korte
4. G. Kovaltsov
5. F. Donadini
6. G. Hulot
7. S. Solanki
8. R. Holme

In Geophysics

1. Monika Korte
2. Catherine Constable
3. F. Donadini
4. I. Usoskin
5. G. Kovaltsov
6. G. Hulot
7. R. Holme
8. S. Solanki

In Molecular Biology

1. I. Usoskin
2. G. Kovaltsov
3. S. Solanki
4. Catherine Constable
5. Monika Korte
6. N. Krivova
7. F. Donadini
8. G. Hulot

Citations in the corpus

• Solar activity during the Holocene: the Hallstatt cycle and its consequence for grand minima and maxima (2016, methodology): “Differences with the VADM variation curve of Knudsen et al. (2008) are larger.”
• 9,400 years of cosmic radiation and solar activity from ice cores and tree rings (2012, methodology): “The wavelet coherence between TSI of this study and two other recent TSI reconstructions (22, 25) based on single radionuclide records show agreement in the lowfrequency part (periods longer than 100 y) and differences in the high-frequency part (periods shorter than 100 y) (SI Appendix, Section S13”
• Reconstructing Holocene geomagnetic field variation: new methods, models and implications (2014, background): “Comparisons between dipole moment and dipole tilt reconstructions with more comprehensive spherical harmonic models highlight potential problems with recovering even the most basic (i.e. dipole) component of the field (Knudsen et al. 2008; Valet et al. 2008; Nilsson et al. 2010).”
• Geomagnetic field for 0–3 ka: 2. A new series of time‐varying global models (2009, methodology): “However, if most data come from a location with field intensity higher or lower than the average dipole intensity over the considered time interval, then even an averaged VADM is biased high or low, respectively.”
• Evolution of the solar irradiance during the Holocene (2011, methodology): “Figure 4 displays the reconstructions of the geomagnetic field intensity, including VADM reconstructions by Knudsen et al. (2008) and Genevey et al. (2008), and the VDM reconstructions by Genevey et al. (2008) and Korte & Constable (2005).”
• Solar Irradiance Variability and Climate (2013, background): “Hence, if the geomagnetic field is known from a previous reconstruction (e.g. Knudsen et al. 2008, Korte & Constable 2005), then the level of solar activity, primarily modulation potential, which depends mainly on the Sun’s open magnetic flux, can be determined using a simple model.”