Figure 1 from Constraints on the Distances and Timescales of Solid Migration in the Early Solar System from Meteorite Magnetism

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Constraints on the Distances and Timescales of Solid Migration in the Early Solar System from Meteorite Magnetism

Authors: James F.J. Bryson, Benjamin P. Weiss, John B. Biersteker, Ashley J. King, and Sara S. Russell

2020 The Astrophysical Journal 896 103.

Provider: AAS Journals

Caption: Figure 1.

First-order reversal curve (FORC) diagram of WIS.2. The diagram shows a distinctive triangular shape. The FORC distribution extends vertically to interaction fields of ±∼100 mT at low coercivities and horizontally to a coercivity of ∼100 mT at near-zero interaction fields. The diagram contains a peak at H_c ≈ 10 mT and H_u ≈ 0 mT.

Other Images in This Article

Copyright and Terms & Conditions