Abstract

Abstract An objective scheme is presented for estimating the lunar crustal magnetic field from the LMAG (Lunar MAGnetometer) data of the SELENE (“KAGUYA”) spacecraft. Our scheme improves the equivalent source method in three respects. The first improvement is that the source calculation is performed simultaneously with detrending. The second is that a great number of magnetic charges (magnetic monopoles) are used as the equivalent sources. The third is that the distribution of the magnetic charges is detremined by the damped least squares method, and the optimum smoothness is determined objectively by minimizing Akaike’s Bayesian Information Criterion (ABIC). For testing the scheme, we apply it to the Lunar Prospector magnetometer data in the region centered at the Reiner Gamma magnetic anomaly. The magnetic field map at an altitude of 20 km is stably drawn from datasets for different altitudes (18 km and 34 km). The ABIC minimizing criterion successfully controls the smoothness due to the numerical damping and extracts as much information as possible from the given data. This scheme will help produce a coherent lunar magnetic anomaly map by integrating the observations from various altitudes of the SELENE and previous missions.

Highlights

  • JAXA (Japan Aerospace Exploration Agency) has launched a lunar-orbiting satellite, SELENE (“KAGUYA”) on September 14, 2007 from the Tanegashima Space Center

  • We expect that the SELENE LMAG data will fill the gaps of the Lunar Prospector’s (LP) magnetometer data

  • In this study, we develop a new scheme for the 3-d estimation of the lunar crustal magnetic field from orbital measurements

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Summary

Introduction

JAXA (Japan Aerospace Exploration Agency) has launched a lunar-orbiting satellite, SELENE (“KAGUYA”) on September 14, 2007 from the Tanegashima Space Center. It was placed into a peripolar orbit at an altitude of about 100 km. It has a 3-component magnetometer (LMAG: Lunar MAGnetometer) primarily for mapping the crustal magnetic field of the Moon. Observations will continue for 1 year, and the LMAG investigator team is requesting optional observations at lower than 50 km altitude after the nominal mission. We expect that the SELENE LMAG data will fill the gaps of the Lunar Prospector’s (LP) magnetometer data

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