scispace - formally typeset
M

Mari Paz Miralles

Researcher at Harvard University

Publications -  35
Citations -  846

Mari Paz Miralles is an academic researcher from Harvard University. The author has contributed to research in topics: Coronal hole & Corona. The author has an hindex of 13, co-authored 35 publications receiving 768 citations. Previous affiliations of Mari Paz Miralles include University of Massachusetts Amherst & Smithsonian Institution.

Papers
More filters
Journal ArticleDOI

A Study of the Physics and Chemistry of L134N

TL;DR: In this paper, the authors carried out a comprehensive and self-consistent study of the physical and chemical state of the core of the dark cloud L134N (L183), whose molecular abundances provide a standard against which chemical models may be compared.
Journal ArticleDOI

Physical Conditions in a Coronal Mass Ejection from Hinode, Stereo, and SOHO Observations

TL;DR: In this paper, the early phases of a coronal mass ejection (CME) were analyzed using multi-wavelength observations from Hinode, Solar and Heliospheric Observatory (SOHO), and STEREO.
Journal ArticleDOI

The role of turbulence in coronal heating and solar wind expansion.

TL;DR: In this paper, the authors provide an overview of the current understanding of how the corona is heated and how the solar wind is accelerated, and review some key observational results from ultraviolet spectroscopy of the collisionless outer corona.
Journal ArticleDOI

Asymmetric magnetic reconnection in solar flare and coronal mass ejection current sheets

TL;DR: In this article, the authors present two-dimensional resistive magnetohydrodynamic simulations of line-tied asymmetric magnetic reconnection in the context of solar flare and coronal mass ejection current sheets.
Journal ArticleDOI

The Role of Turbulence in Coronal Heating and Solar Wind Expansion

TL;DR: This paper provides an overview of the current understanding of how the corona is heated and how the solar wind is accelerated, and some key observational results from ultraviolet spectroscopy of the collisionless outer corona.