Validation of heliospheric modeling algorithms through pulsar observations I: Interplanetary scintillation-based tomography

Autor:	Tiburzi, C., Jackson, B. V., Cota, L., Shaifullah, G. M., Fallows, R. A., Tokumaru, M., Zucca, P.
Rok vydání:	2023
Předmět:	Astrophysics - Solar and Stellar Astrophysics Astrophysics - High Energy Astrophysical Phenomena Physics - Space Physics
Zdroj:	AdSpR (2022)
Druh dokumentu:	Working Paper
DOI:	10.1016/j.asr.2022.04.070
Popis:	Solar-wind 3-D reconstruction tomography based on interplanetary scintillation (IPS) studies provides fundamental information for space-weather forecasting models, and gives the possibility to determine heliospheric column densities. Here we compare the time series of Solar-wind column densities derived from long-term observations of pulsars, and the Solar-wind reconstruction provided by the UCSD IPS tomography. This work represents a completely independent comparison and validation of these techniques to provide this measurement, and it strengthens confidence in the use of both in space-weather analyses applications. Comment: Published in Journal of Advances in Space Research
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/2306.07451 Zobrazit plný text záznamu View this record from Arxiv