Visibility Analysis of the Sun as Viewed from Multiple Spacecraft at the Sun-Earth Lagrange Points
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Abstract
Beyond the Sun-Earth line, spacecraft equipped with various solar telescopes are intended to be deployed at several different vantage points in the heliosphere to carry out coordinated, multi-view observations of the Sun and its dynamic activities. In this context, we investigate solar visibility by imaging instruments onboard the spacecraft orbiting the Sun-Earth Lagrange points L1, L4 and L5, respectively. An optimal arrival time for vertical periodic orbits stationed at L4 and L5 is determined based on geometric considerations that ensure maximum visibility of solar poles or higher latitudes per year. For a different set of orbits around the three Lagrange points (L1, L4 and L5), we calculate the visibility of the solar surface (i.e., observation days per year) as a function of the solar latitude. We also analyze where the solar limb viewed from one of the three Sun-Earth Lagrange points under consideration is projected onto the solar surface visible to the other two. This analysis particularly aims at determining the feasibility of studying solar eruptions, such as flares and coronal mass ejections, with coordinated observations of off-limb erupting coronal structures and their on-disk magnetic footpoints. In addition, visibility analysis of a feature (such as sunspots) on the solar surface is made for multiple spacecraft in various types of orbits with different inclinations to quantify the improvement in continuous tracking of the target feature for studying its long-term evolution from emergence, growth and to decay. A comprehensive comparison of observations from single (L1), double (L1 and L4) and multi-space missions (L1, L4 and L5) is carried out through our solar visibility analysis, and this may help us to design future space missions of constructing multiple solar observatories at the Sun-Earth Lagrange points.Keywords
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This publication has 29 references indexed in Scilit:
- Manifold-Based Space Mission Design with Poincaré Filtering AlgorithmInternational Journal of Aeronautical and Space Sciences, 2023
- A Multi‐Purpose Heliophysics L4 MissionSpace Weather, 2021
- Space weather: the solar perspectiveLiving Reviews in Solar Physics, 2021
- Evolution of Active RegionsLiving Reviews in Solar Physics, 2015
- > 25 MeV Proton Events Observed by the High Energy Telescopes on the STEREO A and B Spacecraft and/or at Earth During the First ∼ Seven Years of the STEREO Mission2014
- Estimating the frequency of extremely energetic solar events, based on solar, stellar, lunar, and terrestrial recordsJournal of Geophysical Research, 2012
- Solar Cycle Predictions (Invited Review)Solar Physics, 2012
- On the theory of the oblateness of the SunSolar Physics, 2001
- The dynamical nature of coronal streamersJournal of Geophysical Research, 2000
- Using Dynamo Theory to predict the sunspot number during Solar Cycle 21Geophysical Research Letters, 1978